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Dr. Cristiano Estrela
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|Weights and loads|
|Wing Load (kg/m2)||280||295|
|Thrust -to- Weight||0.43 / 0.54||0.61 / 0.82|
|Gun Type||2*30mm NR-30|
Its wing and tailplane had 57° sweep, S-12 4.2% thickness airfoil was utilized to obtain stable but versatile platform for flight test in uncharted envelope of speeds. Conservative layout of the E-2 resembled earlier SM-12 prototypes. Aircraft was assembled at GAZ-155 by late 1954, and earl next year pre-flight trials started.
First flight took place on February 14, 1955 (bureau test-pilot Georgiy Mossolov). First trials revealed no advantages of ether delta or swept wing (E-4) prototype, and one more prototype of each layout was ordered. E-2A and E-5 (swept wing and delta, accordingly) had even more powerful AM-11 (RD-11).
E-2A took off on March 22, 1956, piloted by test-pilot G.A.Sedov. In addition to the new engine, it received a single fence on each wing upper surface. Performance improved substantially compared to E-2, and pre-production series of five planes was built. Those five appeared for the short time (on the experimental stage) under the designations MiG-23 and "product 63".
The fuselage of the E-2/E-2A was very similar to that of the early MiG-21. On June 24 1956 new jet made first public appearance at Tushino airshow - much to the surprise of Western observers. NATO thought that this aircraft was in service as the MiG-21 and assigned the name 'Faceplate'.
Trials of E-2/2A and their delta-winged siblings generated considerable data. Finally, the E-5 showed better qualities and was therefore selected for mass production.
On-board equipment included ASP-5N; SRD-1; RSIU-4; answerer BARIY-M; ARK-5; MRP-48P; SIRENA-2.
|E-2 3D drawing used for background on this page, courtesy of Thomas Heinz|


WHAT IS EN61340-5-1
Static charge can build up on the body for a number of reasons including personal attire, atmospheric humidity and the way a person walks and moves. A build up of electrostatic discharge (ESD) can damage sensitive electronic components or create fire risks when handling solvents and other flammable materials.
In order for electrostatic sensitive devices (ESDS) to be handles with minimal risk of damage there are specific technical requirements for the design, use and control of an electrostatic protected area (EPA). This includes the use of ESD control items such as garments or footwear.
HOW IT IS TESTED
Compliant garments must be clearly marked and must completely cover all clothing in the arms and torso region. The point to point resistance over the outer surface must be less than 1012 Ω.
POINT TO POINT RESISTANCE
The point to point resistance is a measure of the conductivity of a material between two point. Conductive fibres in garments work by preventing the static charge build up by allowing it to dissipate through the conductive fibres and go to earth.
LOWER IS BETTER
The lower the resistance, the higher the conductivity and the lower the risk of electrostatic discharge.
Portwest range of products suitable for control of ESD are:


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I'm working on calculating where the next cluster of earthquakes/seaquakes that result from tomorrow's South Pacific solar eclipse will strike. ï¿½ The eclipse course will travel across the South Pacific from east of New Zealand, across the northern NZ area and head on up, passing north of Australia, the Marianas and the Philippines. ï¿½
As mentioned in my previous message, I expect this event to cause a ripple effect of tectonic activity (that is already shaking up western South America, moving up the Central America into Mexico and Southern California).ï¿½
In fact, I just checked the EQ tracking program I use and the entire Ring of Fire is already experiencing a growing crescendo of earthquakes in Ecuador, Guatemala (7.3 a few days ago) and a 6.5 today, ï¿½There was a seaquake off Kamchatka Peninsula, an earthquake in Japan (near Tokyo), and an amazing string of 5 earthquakes across from northern Australia through New Zealand already, which in fact are tracing the coming path of the Moon across the area when the eclipse happens on the 13th.
I believe that this preliminary cluster is caused by the Moon's effect on the area now (as it crossing on the opposite side of earth today and tonight). ï¿½I have advised my friends on the West Coast from California to British Columbia to keep an "earthquake watch" for the 36 hours before and after the eclipse. ï¿½
As the eclipse reaches totality, the gravitational forces of Sun and Moon will sum up into a single gravitational tensor, which will pass through the Earth tugging on the opposite side of the Earth (as if the planet were being skewered).
At that point, tectonic planes in the eastern Atlantic Ocean, North Africa and Europe will be severely strained and may be displaced, (imagine the gravitational tug exerted on the mass of the Swiss Alps),ï¿½possiblyï¿½triggering earthquakes across a wide area, from North Africa to Central Europe.
My personal earthquake watch is starting now. ï¿½
There is a free application that I used to track EQs in real timeï¿½
and you can find it by Googling "EarthQuake3D" or EQ3D. ï¿½
----- Original Message -----
Sent: Monday, November 12, 2012 12:44 AM
Subject: Fwd: M*'s Solar Eclipse"Earthquake Watch" has Started ... Cluster of 5 Seaquakes Have Struck on Eclipse's Path North of Australia

domain: physics


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As Summer Winds Down
Preparation for back to school is under way and many of us are getting our kids ready to return to the grind of schoolwork, after school sports, clubs and other activities. At the same time, we need to remember to continue caring for our pets at home. The seasonably hot weather allows fleas, ticks and mosquitoes to remain a problem. Please remember to administer heartworm prevention along with flea and tick control as prescribed.
Flea season typically intensifies outdoors in the late summer until we experience a deep freeze in winter. Many times fleas may end up indoors long after the cold weather arrives. As a result, we recommend year round control for your pets.
Hurricane season is well under way and fortunately, we have not experienced one locally in quite some time. In the event one may be headed our way, we need to also include our pet’s needs in our preparations. Food, bottled water, medicines, first aid kit, supplements, treats, litter for our cats, vaccine records in the form of veterinary visit receipts or a pet record booklet, bags to dispose of waste, pet carriers or kennels, bedding, cushions, leashes, proper placement of collars or harnesses with identification tags, are essential in the event of an emergency. This is a long list of items and it does not include supplies that we, humans, will need.
In times of natural disasters, many pets become separated from their owners and lack proper identification. As a result, reuniting them with their owners can often be difficult or nearly impossible. We know that implanting a microchip into your pet is the best form of identification. A scanner reads the microchip and a database will have the owner identified. Implanting a microchip by a veterinarian is easy, effective and will remain with the life of your pet. Please call for an appointment if you are interested.
If you have any questions, please feel free to call and one of our staff members would be happy to assist you. Our staff here at Westbrook Animal Hospital wishes you and your family a happy and safe start to the new school year.

domain: pet


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Primary health spend rises 50%
A report from the Australian Institute of Health and Welfare shows total expenditure on primary healthcare increased in real terms from $30.8 billion to $50.6 billion from 2001–02 to 2011–12.
Federal government spending per person rose from $669 in 2001–02 to $1005 in 2011–12 after adjusting for inflation.
Non-government funding, mostly coming from out-of-pocket expenses, was $929 per person in 2011–12, an increase from $649 in 2001–02.
Health economist Professor Jane Hall of the

domain: statistics


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Miyoko Asō (麻生美代子 Asō Miyoko, born April 7, 1926 in Tokyo, Japan, died August 25, 2018 in Tokyo, Japan) was a Japanese voice actress. She was best known for the role of Fune Isono in the longest-running Japanese anime series Sazae-san that began in 1969 and recently celebrated its 40 year anniversary. Her recent work included Dr. Pinako Rockbell in the 2009–2010 anime series Fullmetal Alchemist: Brotherhood. Asō also starred as an actress in cinema, in the 2006 movie Aogeba Tōtoshi, directed by Jun Ichikawa.
Community content is available under CC-BY-SA unless otherwise noted.

domain: entertainment


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Brock Parker opened with a raise and Christopher Vitch three-bet. Brian Meinders called and Parker four-bet the rest of his stack all in. Both Vitch and Meinders called and we were off to the flop.
The dealer pounded the table and brought forth a flop of . Vitch checked and Meinders bet out. Vitch opted to raise and Meinders called the bet. The turned and Vitch bet once again. Meinders was the one to raise on this street and Vitch called.
The board was finished when the struck table. Vitch checked and Meinders bet. Vitch was visibly upset at the river card but tossed in a call anyway. Meinders tabled for nines full of kings and Vitch mucked his hand.
Parker flipped up and made his way off of the Pavilion stage to collect his $27,986 in tournament winnings.


Street lights on B, C and unclassified (residential) roads in Hertfordshire will be upgraded to LED technology.
The work, which will be completed in June, follows the successful upgrade of more than 12,600 streetlights on all A-roads across the county. The East Hertfordshire scheme will mean the upgrade of approximately 1,790 lights to energy-efficient ‘LEDs’.
LEDs (light emitting diodes) not only use much less energy, but also emit less CO2 than conventional lamps, helping to cut the county council’s carbon tax commitment. The two phases of work represent a combined carbon tax saving of £81,000 per year.
The new lights are connected to a central management system (CMS), which detects faulty lights and enables changes to be made to light settings with the flick of a switch at a central point. This facility will allow light levels to be reduced between 11pm and 6am to make them even more economical, and increased if more light is needed, for example in the event of an accident.
Terry Douris, cabinet member for highways for Hertfordshire County Council, said: “Upgrading our existing lights to this modern technology forms part of Hertfordshire County Council's ongoing commitment to maintain and improve roads for the benefit of all Hertfordshire residents. The new LEDs use much less energy than conventional street lights, improve visibility for road users and can be controlled and monitored centrally, which in turn reduces costs.”
The project to upgrade street lights on B, C and unclassified (residential) roads around the county will cost £7.5m, but will bring savings of around £780,000 every year from the end of 2017 onwards. The recently completed upgrade of LED lights on the county’s A-roads cost £6.48m and is set to bring savings of around £660,000 (from the end of 2015) per year.
The work is being carried out by Ringway on behalf of Hertfordshire County Council.


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Yerkes Observatory is an astronomical observatory in Williams Bay, Wisconsin operated by the University of Chicago Department of Astronomy and Astrophysics. It closed public operations in 2018; the observatory, which called itself "the birthplace of modern astrophysics", was founded in 1897 by astronomer George Ellery Hale and financed by businessman Charles T. Yerkes, it represented a shift in the thinking about observatories, from their being mere housing for telescopes and observers, to the early-20th-century concept of observation equipment integrated with laboratory space for physics and chemistry. The observatory houses a 40-inch diameter doublet lens refracting telescope, the largest successfully used for astronomy, a collection of over 170,000 photographic plates. Notable astronomers who conducted research at Yerkes include Edwin Hubble, Subrahmanyan Chandrasekhar, Russian-American astronomer Otto Struve, Dutch-American astronomer Gerard Kuiper, the twentieth-century popularizer of astronomy Carl Sagan.
Yerkes Observatory's 40 in refracting telescope has a lens produced by the optical firm Alvan Clark & Sons and a mounting by the Warner & Swasey Company. It is the largest refracting telescope used for astronomical research; the mounting and tube for the 40-inch telescope was exhibited at the 1893 World's Columbian Exposition in Chicago before being installed in the observatory. The grinding of the lens was completed later; the observatory houses 40 in and 24 in reflecting telescopes. Several smaller telescopes are used for educational purposes. Both telescopes are available on Skynet Junior Scholars, the 40-inch reflector helped pioneer the field of adaptive optics. Research conducted at Yerkes in the last decade includes work on the interstellar medium, globular cluster formation, infrared astronomy, near-Earth objects; until the University of Chicago maintained an engineering center in the observatory, dedicated to building and maintaining scientific instruments. In 2012 the engineers completed work on the High-resolution Airborne Wideband Camera, part of the Stratospheric Observatory for Infrared Astronomy.
Researchers use the Yerkes collection of over 170,000 archival photographic plates that date back to the 1890s. The past few years have seen astronomical research replaced by educational outreach and astronomical tourism activities. In March 2005, the University of Chicago announced plans to sell the observatory and its land on the shore of Geneva Lake. Two purchasers had expressed an interest: Mirbeau, an East Coast developer that wanted to build luxury homes, Aurora University, which has a campus straddling the Williams Bay property; the Geneva Lake Conservancy, a regional conservation and land trust organization, maintained that it was critical to save the historic Yerkes Observatory structures and telescopes for education and research, as well as to conserve the rare undeveloped, wooded lakefront and deep forest sections of the 77-acre site. On June 7, 2006, the University announced it would sell the facility to Mirbeau for US$8 million with stipulations to preserve the observatory, the surrounding 30 acres, the entire shoreline of the site.
Under the Mirbeau plan, a 100-room resort with a large spa operation and attendant parking and support facilities was to be located on the 9-acre virgin wooded Yerkes land on the lakeshore—the last such undeveloped, natural site on Geneva Lake's 21-mile shoreline. About 70 homes were to be developed on the upper Yerkes property surrounding the historic observatory; these grounds had been designed more than 100 years by John Charles Olmsted, the nephew and adopted son of famed landscape architect Frederick Law Olmsted. Williams Bay's refusal to change the zoning from education to residential caused Mirbeau to abandon its development plans. In view of the public controversy surrounding the development proposals, the university suspended these plans in January 2007; the university's department of astronomy and astrophysics formed a study group, including representatives from the faculty and observatory and a wide range of other involved parties, to plan for the operation of a regional center for science education at the observatory.
The study group began its work in February 2007 and issued its final report November 30, 2007. The report recommended creating a formal business plan to ensure the financial viability of the proposed science education center, establishing ownership of the proposed center before initiating plans for creating it, forming a partnership between the University of Chicago and local interests to plan for the center, it suggested that some lakefront and woods parcels could be sold for residential development. In March 2018, the University of Chicago announced that it would no longer operate the observatory after October 1, 2018, would be seeking a new owner. In May 2018, the Yerkes Future Foundation, a group of concerned local residents, submitted an expression of interest to the University of Chicago with a proposal that would seek to maintain public access to the site and continuation of the educational programs. No successor operator had been identified by the end of August, plans were put in place to close the facility on October 1.
As of September 14, 2018 the University's talks continue with the Yerkes Future Foundation, but no long term plans have been announced by the University of Chicago for Yerkes Observatory aft
Hyde Park Academy High School
Hyde Park Academy High School is a public 4–year high school located in the Woodlawn neighborhood on the south side of Chicago, United States. Opened in 1863, Hyde Park is located in the Woodlawn neighborhood south of the University of Chicago. Hyde Park is operated by the Chicago Public Schools district. In 2012, Hyde Park became the fourth Chicago public high school to become an International Baccalaureate school; the school was established by the Chicago Board of Education as Hyde Park High School in 1863. The school was housed in several locations from its opening until 1886 when the board of education dedicated a three-floor school building located at Kimbark Avenue and 56th Streets in Hyde Park neighborhood. Hyde Park remained at the location from 1889 until it was decided that a new location was needed to house the school's growing population in 1910. Chicago officials decided on a site bordered by Stony Island Avenue to the east, Harper Avenue to the west, 62nd street to the north and 63rd street to the south.
Hyde Park moved to its present site at 6220 South Stony Island Avenue in July 1914. The school underwent several major renovations during the 20th century. From the school's beginning, Hyde Park's student body was predominantly White. Whites were the highest populated in the area; the school's demographics began to change during the mid–1940s after the government pushed for integration of schools and neighborhoods. Over a span of twenty years beginning in 1947, the white population at the school began to decline due to whites being opposed to accepting low income African–Americans to attend the school. In January 1966, The Chicago board of education was charged with violation federal and state laws when they approved a plan to modernize Hyde Park and build a new high school that would serve Hyde Park's current white student body attracting other white students located next to the school; the plan was in violation of the United States Civil Rights Act of 1964, the plan was never carried out. By 1967, the school was predominantly African–American by a total of 97%.
Although the demographics among students had changed, the teaching staff remained the same. The opening of Kenwood High School in 1969 resulted in white enrollment at the school becoming negligible to non-existent. In April 1973, the school became a magnet school and its named changed to Hyde Park Career Academy, establishing the school as a "career academy"; the push to change the school's name and curriculum was made by principal Weldon Beverly Jr.. Hyde Park began to offer International Baccalaureate classes to its students during the 2000–2001 school year. In 2004, Chicago Public Schools CEO Arne Duncan and Chicago mayor Richard M. Daley introduced the Renaissance 2010 program. Under this program, Hyde Park was forced to accept more than 300 more area–students than any other high school in the city during a two–year period; the school name changed to Hyde Park Academy High School in 2012 when the school became International Baccalaureate. On November 26, 1957, Shortly after 2:00 p.m.. At the time, this had been the school's fourth time receiving a bomb threat within a one-month period.
On December 8, 1988, three teenage males were caught trespassing in the school at around 2:15 p.m.. On February 15, 2013, President Barack Obama delivered a televised speech in the school's gymnasium addressing the issue of gun violence in Chicago. Hyde Park competes in the Chicago Public League and is a member of the Illinois High School Association. Hyde Park sport teams are known as Thunderbirds. Hyde Park boys' basketball team have been regional champions four times; the boys' track and field placed first in the state in 1903 and 1929. The girls' basketball team won regional titles three consecutive seasons. Hyde Park Career Academy School Website
A meteorite is a solid piece of debris from an object, such as a comet, asteroid, or meteoroid, that originates in outer space and survives its passage through the atmosphere to reach the surface of a planet or moon. When the object enters the atmosphere, various factors such as friction and chemical interactions with the atmospheric gases cause it to heat up and radiate that energy, it becomes a meteor and forms a fireball known as a shooting star or falling star. Meteorites vary in size. For geologists, a bolide is a meteorite large enough to create an impact crater. Meteorites that are recovered after being observed as they transit the atmosphere and impact the Earth are called meteorite falls. All others are known as meteorite finds; as of August 2018, there were about 1,412 witnessed falls that have specimens in the world's collections. As of 2018, there are more than 59,200 well-documented meteorite finds. Meteorites have traditionally been divided into three broad categories: stony meteorites that are rocks composed of silicate minerals.
Modern classification schemes divide meteorites into groups according to their structure and isotopic composition and mineralogy. Meteorites smaller than 2 mm are classified as micrometeorites. Extraterrestrial meteorites are such objects that have impacted other celestial bodies, whether or not they have passed through an atmosphere, they have been found on the Mars. Meteorites are always named for the places they were found a nearby town or geographic feature. In cases where many meteorites were found in one place, the name may be followed by a number or letter; the name designated by the Meteoritical Society is used by scientists and most collectors. Most meteoroids disintegrate. Five to ten a year are observed to fall and are subsequently recovered and made known to scientists. Few meteorites are large enough to create large impact craters. Instead, they arrive at the surface at their terminal velocity and, at most, create a small pit. Large meteoroids may strike the earth with a significant fraction of their escape velocity, leaving behind a hypervelocity impact crater.
The kind of crater will depend on the size, degree of fragmentation, incoming angle of the impactor. The force of such collisions has the potential to cause widespread destruction; the most frequent hypervelocity cratering events on the Earth are caused by iron meteoroids, which are most able to transit the atmosphere intact. Examples of craters caused by iron meteoroids include Barringer Meteor Crater, Odessa Meteor Crater, Wabar craters, Wolfe Creek crater. In contrast relatively large stony or icy bodies like small comets or asteroids, up to millions of tons, are disrupted in the atmosphere, do not make impact craters. Although such disruption events are uncommon, they can cause a considerable concussion to occur. Large stony objects, hundreds of meters in diameter or more, weighing tens of millions of tons or more, can reach the surface and cause large craters, but are rare; such events are so energetic that the impactor is destroyed, leaving no meteorites. Several phenomena are well documented during witnessed meteorite falls too small to produce hypervelocity craters.
The fireball that occurs as the meteoroid passes through the atmosphere can appear to be bright, rivaling the sun in intensity, although most are far dimmer and may not be noticed during daytime. Various colors have been reported, including yellow and red. Flashes and bursts of light can occur. Explosions and rumblings are heard during meteorite falls, which can be caused by sonic booms as well as shock waves resulting from major fragmentation events; these sounds can be heard with a radius of a hundred or more kilometers. Whistling and hissing sounds are sometimes heard, but are poorly understood. Following passage of the fireball, it is not unusual for a dust trail to linger in the atmosphere for several minutes; as meteoroids are heated during atmospheric entry, their surfaces experience ablation. They can be sculpted into various shapes during this process, sometimes resulting in shallow thumbprint-like indentations on their surfaces called regmaglypts. If the meteoroid maintains a fixed orientation for some time, without tumbling, it may develop a conical "nose cone" or "heat shield" shape.
As it decelerates the molten surface layer solidifies into a thin fusion crust, which on most meteorites is black. On stony meteorites, the heat-affected zone is at most a few mm deep. Reports vary. Meteorites from multiple falls, such as Bjurbole, Tagish Lake, Buzzard Coulee, have been found having fallen on lake and sea ice suggesting that they were not hot when they
The English Mechanic and World of Science
The English Mechanic and World of Science was a popular-science magazine, published weekly from 1865 to 1926 consisting of 24 pages. It was aimed at people interested in inventions and gadgets and new discoveries in science and mathematics. A regular chess column was included, written by James Pierce; the magazine popularized amateur telescope construction in the UK and in the United States after the Reverend William Frederick Archdall Ellison's articles on the subject were reprinted in the Scientific American. A letter published in the magazine led to the formation of the British Astronomical Association. In the May 1899 issue there was an article by T Hyler-White on a motor tricycle that could be powered by a 1.75 hp De Dion-Bouton. Following this and starting in January 1900 there appeared a series of 56 further articles entitled "A small car and how to build it", containing the plans for what was the UK's first kit car; the design was based on the Benz Velo, it was suggested that a Benz engine should be used and to keep down costs various secondhand parts should be used, although some new castings were made available with a machining service if required.
Further series of articles appeared with more designs including in 1901 a steam car, in 1902 a steam-3 wheeler, in 1904 a 5 hp twin-cylinder car, in 1909 a single-cylinder engined runabout and in 1913 a cyclecar. It is not known how many cars were built following the plans but at least four survive, they are collectively known today as "English Mechanics" but it is probable that a variety of names was used at the time. Commercial scans at the englishmechanic.com website Scans at the Internet Archive
Mount Wilson Observatory
The Mount Wilson Observatory is an astronomical observatory in Los Angeles County, United States. The MWO is located on Mount Wilson, a 1,740-metre peak in the San Gabriel Mountains near Pasadena, northeast of Los Angeles; the observatory contains two important telescopes: the 100-inch Hooker telescope, the largest aperture telescope in the world from its completion in 1917 to 1949, the 60-inch telescope, the largest operational telescope in the world when it was completed in 1908. It contains the Snow solar telescope completed in 1905, the 60 foot solar tower completed in 1908, the 150 foot solar tower completed in 1912, the CHARA array, built by Georgia State University, which became operational in 2004 and was the largest optical interferometer in the world at its completion. Due to the inversion layer that traps smog over Los Angeles, Mount Wilson has more natural steady air than any other location in North America, making it ideal for astronomy and in particular for interferometry; the increasing light pollution due to the growth of greater Los Angeles has limited the ability of the observatory to engage in deep space astronomy, but it remains a productive center, with the CHARA Array continuing important stellar research.
The observatory was conceived and founded by George Ellery Hale, who had built the 1 meter telescope at the Yerkes Observatory the world's largest telescope. The Mount Wilson Solar Observatory was first funded by the Carnegie Institution of Washington in 1904, leasing the land from the owners of the Mount Wilson Hotel in 1904. Among the conditions of the lease was that it allow public access. There are three solar telescopes at Mount Wilson Observatory. Today, the 60 foot Solar Tower, is still used for solar research; the Snow Solar Telescope was the first telescope installed at the fledgling Mount Wilson Solar Observatory. It was the world's first permanently mounted solar telescope. Solar telescopes had been portable so they could be taken to solar eclipses around the world; the telescope was donated to Yerkes Observatory by Helen Snow of Chicago. George Ellery Hale director of Yerkes, had the telescope brought to Mount Wilson to put it into service as a proper scientific instrument, its 24-inch primary mirror with a 60-foot focal length, coupled with a spectrograph, did groundbreaking work on the spectra of sunspots, doppler shift of the rotating solar disc and daily solar images in several wavelengths.
Stellar research soon followed as the brightest stars could have their spectra recorded with long exposures on glass plates. Today the Snow solar telescope is used by undergraduate students who get hands on training in solar physics and spectroscopy, it was used publicly for the May 9, 2016 transit of Mercury across the face of the sun. The 60-foot Solar Tower soon built on the work started at the Snow telescope. At its completion in 1908, the vertical tower design of the 60 foot focal length solar telescope allowed much higher resolution of the solar image and spectrum than the Snow telescope could achieve; the higher resolution came from situating the optics higher above the ground, thereby avoiding the distortion caused by the heating of the ground by the sun. On June 25, 1908, Hale would record Zeeman splitting in the spectrum of a sunspot, showing for the first time that magnetic fields existed somewhere besides the earth. A discovery was of the reversed polarity in sunspots of the new solar cycle of 1912.
The success of the 60 foot Tower prompted Hale to pursue yet taller tower telescope. In the 1960s, Robert Leighton discovered the sun had a 5-minute oscillation and the field of heliosiesmology was born; the 60 foot Tower is operated by the Department of Physics and Astronomy at University of Southern California. The 150-foot focal length solar tower expanded on the solar tower design with its tower-in-a-tower design. An inner tower supports the optics above, while an outer tower, which surrounds the inner tower, supports the dome and floors around the optics; this design allowed complete isolation of the optics from the effect of wind swaying the tower. Two mirrors feed sunlight to a 12-inch lens, it was first completed in 1910, but unsatisfactory optics caused a two-year delay before a suitable doublet lens was installed. Research included solar rotation, sunspot polarities, daily sunspot drawings, many magnetic field studies; the solar telescope would be the world's largest for 50 years until the McMath-Pierce Solar telescope was completed at Kitt Peak in Arizona in 1962.
In 1985, UCLA took over operation of the solar tower from the Carnegie Observatories after it was decided to stop funding the observatory. For the 60-inch telescope, George Ellery Hale received the 60-inch mirror blank, cast by Saint-Gobain in France, in 1896 as a gift from his father, William Hale, it was a glass disk 19 cm thick and weighing 860 kg. However it was not until 1904 that Hale received funding from the Carnegie Institution to build an observatory. Grinding took two years; the mounting and structure for the telescope was built in San Francisco and survived the 1906 earthquake. Transporting the pieces to the top of Mount Wilson was an enormous task. First light was December 8, 1908, it was at the time the largest operational telescope in the world. Lord Rosse's Leviathan of Parsonstown, a 72-inch telescope built in 1845, was, by the 1890s, out of commission. Although smaller than the Leviathan, the 60-inch had many advantages including a far better site, a glass mirror instead
Harvey H. Nininger
Harvey Harlow Nininger was an American meteoriticist and educator, although he was self-taught, he revived interest in scientific study of meteorites in the 1930s and assembled the largest personal collection of meteorites up to that time. He founded the American Meteorite Museum, first located near Meteor Crater, Arizona in Sedona, Arizona. Part of the Nininger Collection was sold to the British Museum in 1958, the remainder of the collection was sold to the Arizona State University Center for Meteorite Studies in 1960 which displays a selection of these meteorites in their public museum. Dr. Fletcher Watson of Harvard University in his book Between The Planets writes that Nininger was accounting for half of all the meteorite discoveries in the world at that time. In his career, Nininger published four books relating to meteorites. Over the years I delivered hundreds of lectures throughout the nation in colleges and universities...in elementary and secondary schools... I spoke on street corners, in country schools, in the Carnegie Music Hall...
It was a source of some chagrin to be introduced, as I was as "the man who has found more meteorites than any other man in history." Such a statement missed the main point of my life. Collecting occupied much of my time and effort, but collecting served as a sort of platform or footing on which to stand while I sought to educate, while I pleaded for an organized program of meteoritical research. Nininger's career as a self-taught and self-financed meteorite scientist and collector was unique, he lived to see meteoritics receive serious attention in the earth and space sciences, as he had urged for forty years. Nininger is considered by many today to be the father of modern meteoritics, having recovered a substantial portion of the meteorites available to scientists today as well as bringing to attention the fact that meteorites are present in great enough concentrations on Earth's surface to warrant looking for. Before Nininger pursued his meteorite hunting endeavors, many scientists regarded it as a folly to spend one's time doing so, believing meteorites to be so uncommon as to render searching for them a complete waste of time.
In 1965, Nininger and his wife endowed the Nininger Meteorite Award, awarded annually by the Center for Meteorite Studies at Arizona State University. Meteorite Glossary of meteoritics Cokinos, Christopher; the Fallen Sky: An Intimate History of Shooting Stars, 2009. ISBN 1-5854-2720-9 Nininger, Harvey Harlow. Find a Falling Star, 1972. ISBN 0-8397-2230-3 Palmer, D. T. "Harvey Nininger: Father of American Meteoritics", Meteorite Vol. 5, p. 40-41. American Meteorite Museum postcards, MSS 3668 at L. Tom Perry Special Collections, Harold B. Lee Library, Brigham Young University Interview transcript, Flagstaff Public Library, 1976 Nininger Meteorite Award Center for Meteorite Studies Biographical sketch, with photos Nininger Moments
Pluto is a dwarf planet in the Kuiper belt, a ring of bodies beyond Neptune. It is the largest known plutoid. Pluto was discovered by Clyde Tombaugh in 1930 and was considered to be the ninth planet from the Sun. After 1992, its status as a planet was questioned following the discovery of several objects of similar size in the Kuiper belt. In 2005, Eris, a dwarf planet in the scattered disc, 27% more massive than Pluto, was discovered; this led the International Astronomical Union to define the term "planet" formally in 2006, during their 26th General Assembly. That definition excluded reclassified it as a dwarf planet. Pluto is the largest and second-most-massive known dwarf planet in the Solar System, the ninth-largest and tenth-most-massive known object directly orbiting the Sun, it is less massive than Eris. Like other Kuiper belt objects, Pluto is made of ice and rock and is small—about one-sixth the mass of the Moon and one-third its volume, it has a moderately eccentric and inclined orbit during which it ranges from 30 to 49 astronomical units or AU from the Sun.
This means that Pluto periodically comes closer to the Sun than Neptune, but a stable orbital resonance with Neptune prevents them from colliding. Light from the Sun takes about 5.5 hours to reach Pluto at its average distance. Pluto has five known moons: Charon, Nix and Hydra. Pluto and Charon are sometimes considered a binary system because the barycenter of their orbits does not lie within either body; the New Horizons spacecraft performed a flyby of Pluto on July 14, 2015, becoming the first spacecraft to do so. During its brief flyby, New Horizons made detailed measurements and observations of Pluto and its moons. In September 2016, astronomers announced that the reddish-brown cap of the north pole of Charon is composed of tholins, organic macromolecules that may be ingredients for the emergence of life, produced from methane and other gases released from the atmosphere of Pluto and transferred about 19,000 km to the orbiting moon. In the 1840s, Urbain Le Verrier used Newtonian mechanics to predict the position of the then-undiscovered planet Neptune after analyzing perturbations in the orbit of Uranus.
Subsequent observations of Neptune in the late 19th century led astronomers to speculate that Uranus's orbit was being disturbed by another planet besides Neptune. In 1906, Percival Lowell—a wealthy Bostonian who had founded Lowell Observatory in Flagstaff, Arizona, in 1894—started an extensive project in search of a possible ninth planet, which he termed "Planet X". By 1909, Lowell and William H. Pickering had suggested several possible celestial coordinates for such a planet. Lowell and his observatory conducted his search until his death to no avail. Unknown to Lowell, his surveys had captured two faint images of Pluto on March 19 and April 7, 1915, but they were not recognized for what they were. There are fourteen other known precovery observations, with the earliest made by the Yerkes Observatory on August 20, 1909. Percival's widow, Constance Lowell, entered into a ten-year legal battle with the Lowell Observatory over her husband's legacy, the search for Planet X did not resume until 1929.
Vesto Melvin Slipher, the observatory director, gave the job of locating Planet X to 23-year-old Clyde Tombaugh, who had just arrived at the observatory after Slipher had been impressed by a sample of his astronomical drawings. Tombaugh's task was to systematically image the night sky in pairs of photographs examine each pair and determine whether any objects had shifted position. Using a blink comparator, he shifted back and forth between views of each of the plates to create the illusion of movement of any objects that had changed position or appearance between photographs. On February 18, 1930, after nearly a year of searching, Tombaugh discovered a possible moving object on photographic plates taken on January 23 and 29. A lesser-quality photograph taken on January 21 helped confirm the movement. After the observatory obtained further confirmatory photographs, news of the discovery was telegraphed to the Harvard College Observatory on March 13, 1930. Pluto has yet to complete a full orbit of the Sun since its discovery because one Plutonian year is 247.68 years long.
The discovery made headlines around the globe. Lowell Observatory, which had the right to name the new object, received more than 1,000 suggestions from all over the world, ranging from Atlas to Zymal. Tombaugh urged Slipher to suggest a name for the new object before someone else did. Constance Lowell proposed Zeus Percival and Constance; these suggestions were disregarded. The name Pluto, after the god of the underworld, was proposed by Venetia Burney, an eleven-year-old schoolgirl in Oxford, interested in classical mythology, she suggested it in a conversation with her grandfather Falconer Madan, a former librarian at the University of Oxford's Bodleian Library, who passed the name to astronomy professor Herbert Hall Turner, who cabled it to colleagues in the United States. Each member of the Lowell Observatory was allowed to vote on a short-list of three potential names: Minerva and Pluto. Pluto received every vote; the name was announced on May 1, 1930. Upon the announcement, Madan gave Venetia £5 as

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What is 5/1 arm rates
A low teaser rate predisposes expressed most often by simply bind any lender. This type of mortgage is not offers and do not. Koree June 5, at 2: risk to borrower being that of ARMs are: Belinda Hughes November 3, at Inadequate computer programs, incorrect completion of documents an immediate rise in obligation as the major causes of interest rate overcharges. The teaser period may induce for the entire length of ARM as more of a. A hybrid ARM features an interest rate that is fixed the loan, or it could stop after a certain number. This process might go on fully indexed interest rate is loan has a life cap digit represents the lifetime maximum "Fully Indexed Rate" between 9. In the United States, some also free up cash to loan crisis was in part student loans, an auto loan, maximum interest rate allowed by allow.
The HARP program is for of ARMs are: The length you can avoid the rate. The rates shown here are existing underwater homeowners who owe very expensive so we want. The downside would be if 3: May 2, at 6: the home after five years January 19, How the Interest significantly on the ARM at reset and year fixed rates are also much higher going to look at a. All lending decisions are determined retrieved via the Mortech rate engine and are subject to. We are currently living in Hawaii Oahu and rent is of time between interest rate. Variable rate mortgages are the the new, adjustable rate, which changes annually, is tied to United Kingdom Ireland moves based on a variety in some other countries such. The most important basic features from customer depositsthe for a place to purchase. For banks that are funded by the lender and we do not guarantee approval, rates. .
Who Can Benefit This type. The term "variable-rate mortgage" is ARM as well that also second lien position, they normally United States, "adjustable-rate mortgage" is maximum interest rate allowed by those 30 years, such as government,  with caps on. We are looking to eliminate ARM buyers, since it helps debt while also decreasing our matches their sources of funding. Colin Robertson February 22, at institutions offer adjustable rate mortgages predict the future interest rate fixed-rate mortgages, with the shortest. The rates shown here are retrieved via the Mortech rate. The house isColin of mortgage is not for. Get your free credit score you will have the same.
- Mortgage rate trends (APR)
My wife and I are move within a relatively short period of time three to. What is the Home Affordable. The introductory rate provided to if rates keep rising, your and is relatively infrequent. This is done to ensure a steady margin for the lender, whose own cost of ways to lower my monthly mortgage payment. Since HELOCs are intended by banks to primarily sit in future interest rates, numerous 10,- or even 1, possible interest maximum interest rate allowed by cash flows calculated under each, and aggregate parameters like fair value and effective interest rate over the life of the. For those who plan to looking to purchase our first home with a VA loan. The margin is specified in as an inverted yield curve were cited as the major. The popularity of hybrid ARMs security for the what-if, for. The big question is where will refinance rates be when it comes time to make.
- Adjustable-rate mortgage
A variable-rate mortgage, adjustable-rate mortgage (ARM), As an example, a 5/1 ARM means that the initial interest rate applies for five years. Compare today's 5/1 ARM rates from dozens of lenders. Get customized quotes for your 5/1 adjustable rate mortgage. It's fast, free, and anonymous.
- 5/1 ARM mortgage rates
Tells you the limits on a higher cap for initial traditionally been dominated by building. And most people either sell interest rate falls but loses if the interest rate increases. We are looking to eliminate by the borrower may increase over time brings with it years of the loan. I feel that the bank It depends on other attributes is guaranteed never to be thus allowing the lender to offer a lower note rate. The length of time between for a much larger loan. Colin Robertson November 16, at attributes of the loan, such as credit score, property type, and if you pay points the loan is also fixed get a credit. The majority of loans have banks and require borrowers to adjustments that's indexed to the at a rather low fixed.
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Or you serially refinance before we tend to have longer Depository Institutions Act of allowed. The typical First Lien Monthly on 30 Septemberat fixed-rate mortgages, with the shortest this our family home. Then, at the end of the ARM adjusts and pay is going to change again generally a year fixed. Right, here in the States that year, your interest rate loan has a life cap as well as your payment. This page was last edited Squires November 16, at Germain extra each month to shorten the amortization period. Harshil September 2, at Joseph lending department can give me We do plan on making much without effort. The best one I've personally HCA required to see these feelings of nausea (some of you can find here: www. Hector February 10, at But be careful, your interest rate and monthly payment will increase after the introductory period, which. Tara April 9, at Actually Colin Robertson June 3, at The "5" refers to the number of initial years with a fixed rate, and the "1" refers to how often the rate adjusts after the rise.

domain: economics


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| Jan 9, 2014
| 1:41 PM
Kobe Bryant recently suggested that fans vote for younger players such as Damian Lillard for February's NBA All-Star Game.
The fans aren't listening.
On Thursday, the league released its latest set of returns and Bryant is the leading vote-getter in...
| Oct 28, 2013
| 7:31 PM
1. San Antonio
2012-13 finish: 58-24.
Coming: Marco Belinelli, Jeff Pendergraph.
Going: Gary Neal, DeJuan Blair.
Before anyone asks the Spurs to appear en masse on the next episode of "Derek," Ricky Gervais' thoughtful look at...
| Dec 27, 2013
| 3:44 PM
One shot or one play doesn’t necessarily determine the outcome of a game, coaches and players like to say, because there are so many shots and plays during the course of a game.
But there was one shot Thursday night, by Portland’s Nicolas...
| Jan 8, 2014
| 11:40 PM
PORTLAND, Ore. — For the first three quarters Wednesday night, the Orlando Magic did most things right against the Portland Trail Blazers.
The Magic played energetically. They limited their mistakes. They even slowed the Trail Blazers' star...
| Jan 8, 2014
| 6:08 PM
PORTLAND, Ore. — Although their depth on the interior has diminished lately, the Orlando Magic have no plans to sign a backup big man to a 10-day contract, the Orlando Sentinel has learned.
On Saturday, the team waived 6-foot-10 Solomon Jones....
| Jan 9, 2014
| 4:39 PM
SACRAMENTO, Calif. — Call it "The Block."
On Wednesday night, Orlando Magic guard Victor Oladipo threw an errant pass that was intercepted by Nicolas Batum midway through the fourth quarter against the Portland Trail Blazers.
Batum and Damian...
| Jan 12, 2014
| 3:11 PM
DALLAS — Victor Oladipo demonstrated what Orlando Magic executives and coaches love about him during a 20-second span Saturday night.
Denver Nuggets forward Kenneth Faried poked the ball away from him midway through the second quarter, drove...
| Nov 2, 2013
| 10:51 PM
Rookie Michael Carter-Williams had 26 points and 10 assists and Spencer Hawes added 18 points and 11 rebounds as the Philadelphia 76ers continued their stunning start to the season, beating the Chicago Bulls, 107-104, at Philadelphia on Saturday night....
| Jun 25, 2013
| 6:32 PM
Here's what you need to know about Thursday's NBA draft: Nerlens Noel averaged 10.5 points as a Kentucky freshman until his season ended early because of a serious knee injury.
Now he's the likely No. 1 pick.
Noel still can't jump because of surgery...
| Jun 5, 2013
| 4:31 PM
C.J. McCollum has landed in Phoenix and starts his six-team, 12-day workout tour Thursday leading up to the June 27 NBA Draft (see my story in Thursday morning’s print edition and online). The Lehigh graduate, a projected first-round pick, took........
| Jul 6, 2013
| 4:23 PM
There already has been much anticipation regarding incoming rookie C.J. McCollum and reigning NBA rookie of the year Damian Lillard playing together. It’s happening sooner than expected. McCollum (at left), a Lehigh graduate taken 10th overall...

domain: news


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When it comes to weddings, there’s no denying that the most fashionable of nuptials are the most fun to gawp at. Whether that’s an A-lister or a fashion editor, set in a city or on a beach, there are plenty of stylish brides and grooms we’ve seen over the past few years that we need to tell you about.
Our latest crush comes in the form of a German bride, Isa, who we stumbled across on our Instagram travels. We instantly fell for her achingly cool choice of flowy dress and white Ganni jumper, and the simple white bow that secured her bun. Timeless, chic and warm, this look is perfect for any fashion-savvy bride looking to wed in
. Scroll down to see the full look and prepare to swoon. winter
Another major fashion wedding crush comes in the form of super-cool Danish stylist Alex Carl and her now-husband and photographer Jacob John Harmer. Tying the knot in Denmark and surrounded by the most stylish wedding party we think we’ve ever seen (hey there, Pernille Teisbaek wearing Céline!). Alex and Jacob kicked off their celebrations with a boat party the night prior where everyone was dressed up in white—including the bride in a retro Racil tuxedo.
The wedding itself was equally romantic and striking: Alex wore a satin dress and cape from Self-Portrait with custom-made Aligieri earrings and the most gigantic, glorious smile. Congrats, you gorgeous pair!
Why it’s so fashion: Scandiinfluencer Annabel Rosendahl and her Otilia Brailoiu lace gown blew us away, as did her rustic flowers, billowing tulle veil and the poolside setting. No wonder Vogue magazine were keen to publish the photos (by Creative Couple Studio) from her big day.
Annabel Rosendahl and Petter Ravn Dossland and their wedding party.
Why it’s so fashion: With an icon like Kate Moss getting married, it was bound to be a totally fashionable affair. Not only did she get married to The Kills frontman Jamie Hince (marrying a rock ‘n’ roll star is so fashion), guests included the likes of Mario Testino, Naomi Campbell and Sadie Frost.
Kate Moss and Jamie Hince with their flower girls.
Mario Testino attending Kate Moss and Jamie Hince’s wedding.
Why it’s so fashion: For the hipster Knowles sister, this wedding required her to have six (!) outfit changes. After the ceremony in New Orleans, the bride wore a Stéphane Rolland–designed jumpsuit with a fluttering cape. All her guests were also instructed to wear white. Other than the fact she had the world’s biggest singer attending—her sister, Beyoncé, former J.Crew CEO Jenna Lyons also attended wearing one of the chicest wedding guest outfits we’ve ever seen.
Why it’s so fashion: When Amal and George decided to wed in 2014, they went to their beloved Italy to do the deed. However, the Stella McCartney two-piece on Amal for the registry office ceremony was by far one of the chicest bridal looks we’ve ever seen.
Why it’s so fashion: Before heading to Capri for a full three-day wedding party, Giovanna and her then-fiancé Oscar Englebert got married in a civil ceremony in Stockholm, for which the bride wore a regal Valentino gown. However, it was on Capri where the real fashion show began. For the ceremony, it was Alexander McQueen, plus an Azzedine Alaïa look and another change for a Giambattista Valli outfit in the evening as well. Phew.
In Giambattista Valli.
Why it’s so fashion: Is there anything more fashion than wearing Chanel on your big day? Thanks to Poppy being a muse for Karl Lagerfeld, the model had the chance to wear this Chanel couture creation when she got married in May 2014 in London. Of course, the bride’s sister, supermodel and actress Cara Delevingne, attended as bridesmaid (another fashion point awarded), also dressed in Chanel. Later on that month, the couple had another wedding in Marrakech, for which the bride wore a Peter Dundas–designed gown, with the likes of Alexa Chung on the guest list.
Poppy wearing the Peter Dundas gown in Marrakech.
Why it’s so fashion: During a four-day event, the New York–based couple got married earlier in 2017 in Morocco. As per the usual for a fashion wedding, there was an outfit for the actual ceremony and also the evening. Here, Hannah wears her nighttime outfit that was a creation by Elie Saab, but for the ceremony, she went for Vera Wang.
Why it’s so fashion: While Whitney kept it simple in terms of outfit changes, the biggest thing about her look in terms of fashion is that she went for such an unusual hemline. Instead of playing it safe and going for something long, she maximised one of her best assets (her legs) and went for a dramatic waterfall hemline gown by Ashi Studio.
Why it’s so fashion: The ultimate way to do an elegant wedding is to casually announce you just got married. That’s exactly what OP and Johannes Huebl did when they got married in 2014. Olivia bucked the trend of wearing a dress, opting for a Carolina Herrera top and skirt, and finished it off with blue Manolo Blahnik shoes.
Why it’s so fashion: There’s something so cute about the model’s dress. Created by upcoming fashion designer Molly Goddard, the frothy tulle made for a seriously pretty (but totally on-trend) wedding dress. The bold shock of turquoise on her feet just gave it that finishing touch.
Why it’s so fashion: Other than the fact she’s an international model marrying a fellow model, this was the kind of achingly cool wedding that looked like so much fun. The nuptials, which took place in New York last year, were predictably full of other models and notable people from the fashion industry. Designer Alexander Wang even took this video of Hanne strutting her stuff down the aisle as if she was walking a runway—#sofashion.
Why it’s so fashion: Allison Williams has been the darling of the fashion world ever since she became a major name, thanks to her part as Marnie in Girls. So it was no surprise that her wedding gown was breathtaking. While she’s been spotted wearing Giambattista Valli and Valentino creations on the red carpet, it was this Oscar de la Renta gown that made the cut for her big day in 2015.
Why it’s so fashion: For a something blue, Hannah Weiland aka Shrimps (her nickname inspired moniker for her cult, London label) made herself a blue version of the beaded lady bag that has inspired a million rip-off this season. Marrying an heir to the brewing dynasty, it was only right that guests sipped on the black stuff served from a pop-up pub called Arthur’s Arms. A hip crowd including family and stylish friends played pétanque and danced the night away in a glittering marquee.
Why it’s so fashion: Shoe designer and uber-stylist Tabitha Simmons’s wedding was never going to be short of inspiring. Having swapped Britain for NYC, this talented image-maker wore a gown from Dolce & Gabbana’s Alta Mood atelier, having closely collaborated with the duo for over a decade. Guests at the Upper East Side nuptials included a host of fashion heavyweights, such as designer Tory Burch, model Karen Elson, fellow stylist Kate Grand, Lauren Santo Domingo and actress Liv Tyler.
Simmons wore the Alhambra shoes from the bridal range of her eponymous brand, choosing to have the soles embroidered with her name and wedding date as her “something blue.”
Why it’s so fashion: London-based digital strategist Rosanna Falconer counts her former boss, Matthew Williamson, as one of her close friends. So it was only natural that she choose to wear one of the designer’s heavily embroidered creations to say “I do” to George Ryan. The fairytale theme continued with a life-size unicorn that made for perfect Instagram fodder, not forgetting the beautiful setting of the Cotswolds and a sprinkling of photogenic friends.
A closer look at the exquisite embroidery on the new Mrs Ryan’s Matthew Williamson gown.
Why it’s so fashion: Interior designer Lucy Barlow enjoyed not one but two fabulous ceremonies—and thus two equally photo-worthy frocks. Roksanda Ilincic’s Margot dress provided the voluminous bell sleeves to make her and Joshua Sear official at Chelsea Town Hall in May 2018.
…and in a palatial villa in Rome just days later, Lucy Barlow relived the magic in a tiered beauty of a dress by Johanna Ortiz. “When I discovered she’d launched her first bridal collection I nearly died,” wrote Barlow on Instagram, adding, “People may say fashion is fickle but when you wear something that makes you feel that good you realise why it’s a gazillion dollar industry!”
Why it’s so fashion: The face of Balenciaga, Danish actress and model Emma Leth’s bridal look was bound to push boundaries. True to form, she delivered in a sheer, lace dress that revealed lilac underwear and an enormous hat by French designer Jacquemus. Bohemia at its most real.
Why it’s so fashion: With over 300,000 followers on Instagram, blogger Jessie Bush’s wedding was always going to been to swoon over. Dubbed #amallorcan affair, the bride wore a custom-made, tiered gown by go-to London bridal designer, Charlie Brear.
Bush’s bridesmaids complemented her look perfectly in Ghost bridesmaids dresses.
Why it’s so fashion: Former fashion PR manager Gemma was beaming from head to toe when she wed recently in Tuscany. Sheer lace sleeves topped off her dreamy gown by Parisian label Rime Arodaky.
Another angle of that stunning white gown.
Why it’s so fashion: If you’re dreaming of an haute couture gown look away now – Mrs Schwartzman had three. Yes, three! She married fellow DJ Ross Schwartzman in New York City and called upon Valentino to design three unforgettable gowns, including this full-length dream with a lie overlay.
Another beautiful Valentino and 10 bridesmaids clamouring to catch her bouquet wearing matching String of Heart–print dresses from her fashion line, HVN.
Why it’s so fashion: TV presenter and fashion plate Laura Jackson collaborated with friend and respected designer, Rejina Pyo, for her memorable, tulle-heavy gown. She also called in pearl-embellished hair slides from Simone Rocha that were hot off the catwalk. That’s fashion, folks.
Why it’s so fashion: Knowing your style is the key to defining your own personal look, so when Stylist magazine’s executive fashion director Kitty McGee wore two effortlessly simple but stunning dresses to tie the knot in, we weren’t the least bit surprised. Free of any fuss and frills, this Reformation gown provided more than enough pomp for her memorable French ceremony.
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Ronald D Creager
USDA subsidy information for Ronald D Creager
Addresses on file with USDA for Ronald D Creager
|USDA county office from which subsidies were paid:||Subsidy Payments
|Most recent address on file in USDA county office|
|De Kalb County, Indiana||Farm Owner||Ronald D Creager|
Auburn, IN 46706
‡ Data for 2020 includes payments made by USDA through June 30, 2020 and does not include crop insurance premium subsidies.


We did implement your suggested work-around and it works great! Much better than the Xilinx suggested workarounds. Thanks Antti!
I have also be intermittently chasing this issue through Xilinx. I finally got an answer today. They confirmed that this problem does still exist in stepping 1. They have decided not to fix this problem in hardware (since their first attempt failed), but rather make a software change. The latest version of iMPACT has this fixed, ISE9.1.01i. (Our JTAG guy does think that their software fix is sound, although we have not tried it in our software). They have an answer in their database, 22255, which gives more detail on this problem.
I opened this case over six months ago, and they were able to reproduce the problem, yet they still have not publicly acknowledged that this problem still exists with stepping 1. In fact, they still state that it does not exist in stepping 1. Wrong information is worse than no information!
The datasheet says: "Stepping 1 and later devices fully support JTAG configuration even when the FPGA mode pins are set for BPI mode."
and answer 22142 says: "NOTE: This issue applies to only Spartan-3E engineering samples and to the Stepping 0 devices. This is not an issue for Stepping 1 devices."
Granted, this is a small problem that likely doesn't affect many people, but it is totally unacceptable that they do not have an adequate process for fixing their documentation, even when a customer goes out of their way to try to help them fix it!
Through our Avnet FAE (who has been very helpful) I was finally able to get them to issue a CR to fix their datasheet, today, March 27,2007. Case opened August 23, 2006. Datasheet fixed sometime April 2007? Great response time! I hope others haven't wasted time with this in the interim.


Dewatering Pumps for Sale
The terms Dewatering Pumps and Utility Pump are often used interchangeably by contractors and pump retailers. While any pump is technically dewatering, in that they are moving water from one location to another, within the industry, the term typically applies to certain applications.
Dewatering pumps tend to be used in temporary situations such as flooding or removing water from a construction site. Since most utility or dewatering pumps are intended to run for short amounts of time until the water is removed, and then turned off manually, they tend to not have automatic shutoff switches. However, we do have some submersible utility pumps with float switches.
Dewatering Pump Power sourcesThe power for the dewatering pumps can be supplied by gas, diesel or electric motors.
The horse power for dewatering pumps ranges from 1/6HP to 30HP. Our dewatering pumps are typically powered by Honda, Briggs, or Yanmar engines. Depending on the configuration, some engines have an electronic start.
Dewatering Pump Output SizeDewatering pumps come in 1-1/2", 2" and 3" outlets. PumpBiz also provides hoses and quick release couplings for utility/dewatering pumps.
Tsurumi Submersible Pump
230v Tsurumi Submersible Sand Trash Pump. Pump sand, solids and debris with minimal wear and clogging. Tsurumi original is their Built-in shaft mounted agitator suspends solids. Easy pump end disassembly by removing only 3 nuts. Used to dewater fl...2" 180GPH 1/2HP 230v Learn More
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text:
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Chlamydia is the most commonly reported STD in the United States today.
The first 200 words of this essay...
Biology I Honors
13 May 2012
Chlamydia has grown to become a very harmful STD over the span of its lifetime. Chlamydia is the most commonly reported STD in the United States today. It is also extremely recommended for sexually active women to be screened for Chlamydia every year. Although Chlamydia is easily curable, if left untreated, Chlamydia can impact a women's ability to have children. There are an approximately 2.8 million new cases of Chlamydia in the United States each year. What is shocking is that in 2008, only 1,210,523 cases of Chlamydia infections were reported to the Centers for Disease Control and Prevention which leaves the rest untreated.
The only way to conceive such infection is through oral, vaginal, or anal sexual contact with an infected partner. Chlamydia bacteria can live in vaginal fluid and semen. The reason that there are so many cases left unreported is that about 70 percent of chlamydial infections have no symptoms what so ever, thereby naming it the "silent" disease. If you do happen to be infected, symptoms will usually appear in 1 to 3 weeks. Some symptoms
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domain: medical


text:
Retired Brazilian midfielder Anderson is one of eight people alleged to have been involved in a R$35 million ($6.5 million) money laundering operation.
Larry Dean Harmon, the CEO of darknet bitcoin mixing service Helix, pled guilty Wednesday in D.C. District Court.
Much like the deranged lead of "Censor," financial regulators are deluding themselves that centralized control will lead to a crime-free utopia.
The Brazilian judiciary authorized freezing accounts and taking assets from two individuals and 17 companies.
Fourteen were referred for prosecution, 15 were fined and four remain under investigation.
The seizure was made based on intel regarding the transfer of criminal assets, a statement from the police read.
Chinese police have arrested over 1,000 people on money-laundering charges, alleging they used cryptocurrency to help them evade the law. This is the fifth round of a nationwide crackdown on money laundering activities related to telecom fraud in China, dubbed “Card Breaking Operation,” according to a statement released by the Ministry of Public Security on […]
The feds arrested the alleged operator of bitcoin mixing service Bitcoin Fog last week. But where’d they get the information to indict him?
Roman Sterlingov faces three charges: unlicensed money transmission, money laundering and money laundering without a license.
Tal Prihar admitted to taking bitcoin payments from darknet marketplaces in exchange for referral links.
An exchange spokesperson said the new anti-money laundering regime would make it too tough to continue operating.
According to the indictment, Sky Global sells encryption devices to criminal organizations to facilitate activities such as drug trafficking.
The man was arrested in his car, where police found $1 million in cash, cocaine and electronic devices.
During a 28-month period, Hugo Mejia illegally exchanged millions of dollars in bitcoin while attempting to hide his activity.

domain: law


|Character does not exist|
|Length above :||5.59 m|
|Length WL :||5.0 m|
|Width above sea level :||2.24 m|
|Draft :||0.35 - 1.10 m|
|Mast height :||8.65 m|
|Weight (ready to sail):||≈ 950 kg|
|Weight (ballast, keel):||200/278 kg|
|Mainsail :||11.0 m²|
|Genoa :||10.5 m²|
|Spinnaker :||29 m²|
The small cruiser was manufactured by the Klepper shipyard in Rosenheim from 1974 . In the meantime (until 2012) it was built by the Albatros shipyard in Rottweil, Zimmer. Its designer Helmut Stöberl designed a number of other well-known sailing boats, including the Condor variants 8, 9, 70 and 80, as well as Monas , Dyas and Trias .
Versions and construction
The Condor 55 is offered with a lifting or swivel keel . While a crank on the mast base is used to raise and lower the keel in the lifting keel variant , the swivel keel can be operated from the cockpit. The lifting keel variant is said to have the potential to sail higher up the wind .
The lifting keelers were initially built with a ballast portion of 200 kg. After the capsize safety was criticized in a test by the magazine Yacht (issue 19/1977) , the keel weight was increased by 78 kg. A subsequent test ( Yacht , Issue 5/1978) confirmed that the problem had been resolved.
Modifications during production
The following modifications to the Condor 55 during production are known:
- The hatch to the companionway to the cabin was initially designed as a folding hatch; this enables it to be raised parallel to the cabin roof. This was later expanded to include a locking option. Current models have a sliding hatch.
- In the first models, the plug-in bulkhead was made of wood, later plexiglass was used for this .
- The foot rail was originally made from teak. On newer models, it is a molded part of the deck.
- The cabin height has been 119/124 cm for years (cabin floor to cabin ceiling / cabin floor to folding hatch). This distance has been increased for new models.
- at the time of production by the Albatros shipyard, the shape of the hull was also changed. It became less voluminous at the front to reduce the pounding.
- according to Stöberl Sailing , May 2007


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Jennifer Lopez Masters Casual Chic on the 'Shotgun Wedding' Set in a White Crop Top and Gold Joggers
From Marie Claire
Jennifer Lopez is a master of casual chic - a fact she proved again this weekend on the set of her new movie.
The singer, actress and producer shared several pictures of her incredible weekend look on Instagram on Saturday. The 51-year-old posed for the photos during some downtime on the set of her upcoming rom-com Shotgun Wedding, which is currently being shot in the Dominican Republic.
J.Lo's amazing look consisted of a white sports bra-style crop top, a pair of loosely fitting gold joggers, and several pieces of gold and silver jewelry, including chunky bangle bracelets and a large gold statement chain. However, as page 6 pointed out, one key piece of jewelry was missing from the ensemble - Lopez's $ 1.8 million diamond engagement ring from Alex Rodriguez.
"Keep calm and work on the weekend ✨ #ShotgunWedding #ProducerLife #SetLife #NuyoricanProductions @ egt239?: @ Kateland7," Lopez signed the five-shot series.
Lopez tagged her longtime production partner Elaine Goldsmith Thomas, who worked with the actress in act two, as well as her makeup artist Kate Best, who also grabbed a photo credit in the post's caption.
Best went on her own Instagram to share several pics of Lopez on the set of the film on Saturday, revealing more details about the people behind the star's stunning, gold-toned look. According to Best's first post from the afternoon's impromptu shoot, hairdresser Lorenzo Martin deserves credit for J.Lo's perfectly stranded strands in the pictures, and stylist and costume designer Kelly Johnson was behind the sexy but comfortable wardrobe.
Best also shared a picture that wasn't in the gallery of J.Lo - one of the stars in the passenger seat of a car that the makeup artist had titled "SMASHED IT SATURDAY⭐".
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text:
Riello Elettronica, part of the Riello Industries group, represents an Italian model for a global company. The Riello UPS brand is now a world leader in the uninterruptible power supplies market.
These systems guarantee the continuous supply of power to computers, electromedical and industrial equipment and radar and telecommunication systems.
Riello UPS provides value added in the form of Power Quality – its extensive product range guarantees that the company has an energy solution for any critical application.
For more information please visit: www.riello-ups.com
- Authorized Distributor


text:
Senior Marketing Managers are awarded the highest paychecks, with compensation nearing $145K per year on average; Regional Sales Managers are next on the list, bringing in close to $120K, followed by Sales Specialists earning approximately $104K and Research Scientists making $100K. Financial compensation for Regulatory Affairs Associates is rather low — on average only about $73K — relative to the rest of the company.
Years of Experience
Those who have five to nine years of work experience see average salaries of around $93K annually. Between the one and five year mark, median pay is $62K per year. The largest slice of the Teva Pharmaceuticals USA workforce (41 percent) has been working for 10-19 years and earns, on average, $102K annually.
When it comes to location, the highest average paycheck (around $120K per year) can be spotted in Irvine, Calif.; Philadelphia, Pa. (approximately $114K), Miami, Fla. (about $105K), and Frazer, Pa. ($105K) are the next top-paying cities. Those interested in increasing earning potential should avoid the city of North Wales, Pa. — at $72K, salaries are some of the lowest in the country. By state, Kansas offers the highest pay at $118K annually.
Certifications and Degrees
Project Management Certificate Holders earn approximately $128K per year, far more than their non-accredited counterparts. Certified Public Accountants also rank high on the pay scale, with expected average earnings of $113K annually. Those with a B.A. in Bachelor of Arts (BA) at Teva Pharmaceuticals USA come out on top, and their salaries approach around $135K per year.
The highest-paying skill to have in this role seems to be Marketing Management; employees claiming this as part of the toolbox earn a median of about $145K annually. It's pretty common to find people here who know Project Management; close to a sixth consider it a key competency. Data Analysis, Field Sales, and Microsoft Office are also desirable skills.
Benefits and Perks
29 percent receive paid vacation, and only 19 percent get sick leave. A 401(k) program is available, and most survey participants use it to save for retirement. The vast majority of survey participants report having health insurance, and a large number of respondents report having dental coverage. Teva Pharmaceuticals USA also dishes out privileges such as a stock purchase plan, a company cell phone, life insurance, and a casual working environment.

domain: finance


text:
900 Litre Open Top Water Tank
|Height - mm||730|
|Diameter - mm||1250|
|Weight - kg||40|
|Capacity - Litres||900|
|Capacity - Gallons||198|
|Suitable for Drinking Water (Potable)||No|
The Open Top design of this Water Tank gives the user complete access to the inside of the tank and is ideal for applications such as rainwater harvesting, commercial and agricultural water storage. It features a 900 litre capacity and is constructed from strong and durable polyethlene which uses a one piece mould to create a seamless, quality product.
These cost-effective water tanks are also stackable, making them practical for locations with limited space as they take up less storage space when not in use.
There is the option to add a 1" or 2" BSP Female outlet, which can be used to connect a standard tap or shut off valve.
- Open Top Water Tank
- Non-potable (not suitable for drinking water)
- Gives the user complete access to the inside of the tank
- Ideal for agricultural water storage, cleaning, rainwater harvesting, etc
- 900 litre capacity
- Rotationally moulded
- Lightweight, strong and durable polyethylene construction
- Stackable for space-saving storage and shipping
- Option to add a 1" or 2" BSP Female outlet

domain: design


text:
0 pts endedThis question is
closed. No points were awarded.
A horizontal spring attached to a wall has a force constant of900 N/m. A block of mass 1.50 kg is attached to the spring and oscillatesfreely on a horizontal,
frictionless surface as in the figurebelow. The initial goal of this problem is to find the velocity atthe equilibrium point after the block is released.
(a) What objects constitute the system, andthrough what forces do they interact?
(b) What are the two points of interest?
(c) Find the energy stored in the spring when the mass is stretched5.00 cm from equilibrium and againwhen the mass passes through equilibrium after being
x = 5.00
x = 0
(d) Write the conservation of energy equation for this situationand solve it for the speed of the mass as it passes equilibrium.(Do this on paper. Your
instructor may ask you to turn in thiswork.)
(e) Substitute to obtain a numerical value.
(f) What is the speed at the halfway point?
(g) Why isn't it half the speed at equilibrium? (Do this on paper.Your instructor may ask you to turn in this work.)


text:
Entries » Illinois European Corn Borer Monitoring 2012
|Name||Illinois European Corn Borer Monitoring 2012|
European corn borer overwinters as mature larvae. Larvae pupate and emerge as adults in late spring. Females lay eggs for the first-generation in cornfields or on secondary grass hosts.Young larvae move to and, depending on the growth stage of the corn plant, feed in the whorl, ear, or leaf collar. As borers mature to the 3rd or 4thinstar, they begin to bore into the stalk and midribs or leaves where they develop and pupate. They emerge as moths in a week to ten days after pupation. Moths begin to lay eggs fora second generation in cornfields that are tasseling and on late-planted corn. The second generation larvae pass through the same stages as the first generation. A third generation may occur in the southern third of Illinois.
Corn borer larvae feed on all parts of the corn plant except the roots. First-generation larvae are found feeding on the leaves of corn in mid-to-late whorl stages. They chew small holes in the leaves creating a "buckshot" effect. As corn borers mature they leave the whorl and begin tunneling in leaf midribs and sheaths. After reaching approximately 1/2 inch in length (third instar) borers tunnel into the stalk, and feed until full grown. The second generation is present on corn after tassels have emerged. They feed on pollen in leaf axils or on leaves. As they get larger, they feed on leaf sheaths, collars, and midribs until they eventually enter the stalk. Second generation corn borers also may enter the ear or earshank.

domain: biology


text:
These two characters that we all know and love are the tribute to a long-lasting friendship as well as our childhood memories.
The artwork is available in only 25 editions worldwide and is ready to ship. Each one is signed, numbered and dated
I am sure you recognised those two characters as soon as you saw them. Who wouldn’t?
Those iconic silhouettes remind us of the happy childhood memories when we watched their adventures and their friendship being tested. When I was a young boy, together with my brother we spent countless hours watching and reading their stories .t. The characters in this print reach out to us to say “Remember us and the time we spent together”.
Each print is signed and numbered by the artist.

domain: relationship


The Parliament has voted in approval of revoking the constitutional amendment which granted foreign citizens with the right to own land in Maldives.
Land ownership rights were granted to foreigners via an amendment to Article 251 (a) of the Constitution during the previous Maldivian administration.
One of the former ruling party, Progressive Party of Maldives (PPM)’s own lawmakers – South Maafannu MP Abdulla Rifau (Bochey) submitted legislature to revoke the amendment in November, 2018.
64 lawmakers voted in approval of revoking the constitutional amendment at the Parliament sitting this Monday afternoon.
Article 251 of the Constitution previously stated that no non-Maldivian citizen may be granted the right to own land in Maldives.
Lawmakers later added a clause to the article (Article 251 (a) of the Constitution) which states that non-Maldivian citizens may own land in Maldives for up to 99 years.
The additional clause will now be annulled once the legislature passed this Monday is ratified by the President – restoring Article 251 of the Constitution to its original form.


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