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Learn how NREL's Workforce Development and Education Programs inspire students, teachers, and executives to explore sustainable energy. The Office of Satellite and Product Operations (OSPO) is part of the National Environmental Satellite Data and Information Service (NESDIS). NESDIS is part of the. The methodology used by Lockwood and Frölish to smooth the lines was. Table (284) figure (152) graph (85) video (15) Expanded Table of Contents. PHYSICAL AND CHEMICAL PROPERTIES. Discussion introduction. Heat radiation (as opposed to particle radiation) is the transfer of internal energy in the form of electromagnetic waves. Chromium was discovered by the French chemist Nicholas Louis Vauquelin at Paris in1798. He was intrigued by a bright red mineral that had been discovered in a. Waveband: 16 bands in VIS, NIR and IR ranging from 0.47 µm to 13.3 µm VIS, NIR, SWIR, MWIR, TIR: Spatial resolution: 0.5 km in 0.64 µm band; 2.0 km in long wave IR. Ultraviolet - Wikipedia. Ultraviolet (UV) is an electromagnetic radiation with a wavelength from 1. PHz) to 4. 00 nm (7. THz), shorter than that of visible light but longer than X- rays. UV radiation constitutes about 1. Sun, and is thus present in sunlight. It is also produced by electric arcs and specialized lights, such as mercury- vapor lamps, tanning lamps, and black lights. The handouts and PowerPoint presentations below are resources to be used by any/all students and educators. It is appreciated if credit is given when. The 97th Edition of the Handbook of Chemistry and Physics print version is available for purchase at www.crcpress.com. ScienceDirect is the world's leading source for scientific, technical, and medical research. Explore journals, books and articles. 6 Statistical methods for the treatment of experimental data . 6.1 : Statistical methods for the treatment of experimental data. Installed Cost Benchmarks and Deployment Barriers for Residential Solar PV with Energy Storage: Q1 2016; Reducing Wind Curtailment through Transmission Expansion in a. Although it is not considered an ionizing radiation because its photons lack the energy to ionize atoms, long- wavelength ultraviolet radiation can cause chemical reactions and causes many substances to glow or fluoresce. Consequently, the biological effects of UV are greater than simple heating effects, and many practical applications of UV radiation derive from its interactions with organic molecules. Suntan, freckling and sunburn are familiar effects of over- exposure, along with higher risk of skin cancer. Living things on dry land would be severely damaged by ultraviolet radiation from the Sun if most of it were not filtered out by the Earth's atmosphere. The UV spectrum thus has effects both beneficial and harmful to human health. Ultraviolet rays are invisible to most humans: the lens in a human eye ordinarily filters out UVB frequencies or higher, and humans lack color receptor adaptations for ultraviolet rays. Near- UV radiation is visible to some insects, mammals, and birds. Small birds have a fourth color receptor for ultraviolet rays; this gives birds . UV also allows mammals to see urine trails, which is helpful for prey animals to find food in the wild. The males and females of some butterfly species look identical to the human eye but very different to UV- sensitive eyes—the males sport bright patterns in order to attract the females. Ultraviolet has a higher frequency than violet light. UV radiation was discovered in 1. German physicist Johann Wilhelm Ritter observed that invisible rays just beyond the violet end of the visible spectrum darkened silver chloride- soaked paper more quickly than violet light itself. The terms chemical and heat rays were eventually dropped in favour of ultraviolet and infraredradiation, respectively. By 1. 90. 3 it was known the most effective wavelengths were around 2. In 1. 96. 0, the effect of ultraviolet radiation on DNA was established. Ionizing radiation at shorter wavelengths. Vacuum ultraviolet. VUV1. 0–2. 00. 6. Strongly absorbed by atmospheric oxygen, though 1. Extreme ultraviolet. EUV1. 0–1. 21. 12. Entirely ionizing radiation by some definitions; completely absorbed by the atmosphere. A variety of solid- state and vacuum devices have been explored for use in different parts of the UV spectrum. Many approaches seek to adapt visible light- sensing devices, but these can suffer from unwanted response to visible light and various instabilities. Ultraviolet can be detected by suitable photodiodes and photocathodes, which can be tailored to be sensitive to different parts of the UV spectrum. Sensitive ultraviolet photomultipliers are available. Spectrometers and radiometers are made for measurement of UV radiation. Silicon detectors are used across the spectrum. Scientific instruments can therefore utilize this spectral range by operating in an oxygen- free atmosphere (commonly pure nitrogen), without the need for costly vacuum chambers. Significant examples include 1. Technology for VUV instrumentation was largely driven by solar astronomy for many decades. While optics can be used to remove unwanted visible light that contaminates the VUV, in general, detectors can be limited by their response to non- VUV radiation, and the development of . Wide- gap solid- state devices or vacuum devices with high- cutoff photocathodes can be attractive compared to silicon diodes. Extreme UV (EUV or sometimes XUV) is characterized by a transition in the physics of interaction with matter. Wavelengths longer than about 3. The long end of the EUV spectrum is set by a prominent He+ spectral line at 3. EUV is strongly absorbed by most known materials, but it is possible to synthesize multilayer optics that reflect up to about 5. EUV radiation at normal incidence. This technology was pioneered by the NIXT and MSSTA sounding rockets in the 1. In essence, all UVC is blocked by diatomic oxygen (1. The ozone layer then blocks most UVB. Meanwhile, UVA is hardly affected by ozone, and most of it reaches the ground. UVA makes up almost all of the ~ 2. Sun's total UV that penetrates the Earth's atmosphere. Solar ultraviolet. The Sun emits ultraviolet radiation at all wavelengths, including the extreme ultraviolet where it crosses into X- rays at 1. Extremely hot stars emit proportionally more UV radiation than the Sun. Sunlight in space at the top of Earth's atmosphere (see solar constant) is composed of about 5. W/m. 2 in vacuum. Of the ultraviolet radiation that reaches the Earth's surface, more than 9. UVA, with the small remainder UVB. There is essentially no UVC. Thick clouds block UVB effectively; but in . The ozone layer is especially important in blocking most UVB and the remaining part of UVC not already blocked by ordinary oxygen in air. Blockers and absorbers. The absorbers can themselves degrade over time, so monitoring of absorber levels in weathered materials is necessary. In sunscreen, ingredients that absorb UVA/UVB rays, such as avobenzone, oxybenzone. They are contrasted with inorganic absorbers/. Standard summer fabrics have UPF of approximately 6, which means that about 2. UV will pass through. Suspended nanoparticles in stained glass prevent UV rays from causing chemical reactions that change image colors. A set of stained glass color reference chips is planned to be used to calibrate the color cameras for the 2. ESA Mars rover mission, since they will remain unfaded by the high level of UV present at the surface of Mars. Ordinary window glass passes about 9. Other practical UV sources with more continuous emission spectra include xenon arc lamps (commonly used as sunlight simulators), deuterium arc lamps, mercury- xenon arc lamps, metal- halide arc lamps, and tungsten- halogen incandescent lamps. Fluorescent black light lamps use a phosphor on the inner tube surface, which emits UVA radiation instead of visible light. Some lamps use a deep- bluish- purple Wood's glass optical filter that blocks almost all visible light with wavelengths longer than 4. A black light may also be formed, very inefficiently, by using a layer of Wood's glass in the envelope for an incandescent bulb. Though cheaper than fluorescent UV lamps, only 0. Mercury- vapor black lights in ratings up to 1 k. W with UV- emitting phosphor and an envelope of Wood's glass are used for theatrical and concert displays. Black lights are used in applications in which extraneous visible light must be minimized; mainly to observe fluorescence, the colored glow that many substances give off when exposed to UV light. UVA/UVB emitting bulbs are also sold for other special purposes, such as tanning lamps and reptile- keeping. Short- wave ultraviolet lamps. These lamps emit ultraviolet light with two peaks in the UVC band at 2. From 8. 5% to 9. 0% of the UV produced by these lamps is at 2. The fused quartz glass tube passes the 2. Such tubes have two or three times the UVC power of a regular fluorescent lamp tube. These low- pressure lamps have a typical efficiency of approximately 3. UV output. Argon and deuterium arc lamps are often used as stable sources, either windowless or with various windows such as magnesium fluoride. It has the advantages of high- intensity, high efficiency, and operation at a variety of wavelength bands into the vacuum ultraviolet. Ultraviolet LEDs. LED efficiency at 3. UV wavelengths are also better. Such LED arrays are beginning to be used for UV curing applications, and are already successful in digital print applications and inert UV curing environments. Power densities approaching 3 W/cm. W/m. 2) are now possible, and this, coupled with recent developments by photoinitiator and resin formulators, makes the expansion of LED- cured UV materials likely. UVC LEDs are relatively new for use in disinfection. The nitrogen gas laser uses electronic excitation of nitrogen molecules to emit a beam that is mostly UV. The strongest ultraviolet lines are at 3. Another type of high power gas laser is the excimer laser. They are widely used lasers emitting in ultraviolet and vacuum ultraviolet wavelength ranges. Presently, UV argon- fluoride (Ar. F) excimer lasers operating at 1. The current wavelength limit of production of coherent UV is about 1. Ar. 2* excimer laser. Direct UV- emitting laser diodes are available at 3. Ultraviolet lasers can also be made by applying frequency conversion to lower- frequency lasers. Ultraviolet lasers have applications in industry (laser engraving), medicine (dermatology, and keratectomy), chemistry (MALDI), free air secure communications, computing (optical storage) and manufacture of integrated circuits. Tunable vacuum ultraviolet (VUV) via sum and difference frequency mixing. The generation is generally done in gasses (e. By making one of the lasers tunable, the VUV can be tuned. If one of the lasers is resonant with a transition in the gas or vapor then the VUV production is intensified. However, resonances also generate wavelength dispersion, and thus the phase matching can limit the tunable range of the 4 wave mixing. Difference frequency mixing (lambda. The EUV is not emitted by the laser, but rather by electron transitions in an extremely hot tin or xenon plasma, which is excited by an excimer laser. Synchrotron light sources can also produce all wavelengths of UV, including those at the boundary of the UV and X- ray spectra at 1. Human health- related effects. Getting too much sun exposure can be harmful, but in moderation is beneficial. UV light causes the body to produce vitamin D, which is essential for life. The human body needs some UV radiation in order for one to maintain adequate vitamin D levels. One minimal erythemal dose of sunlight UV radiation provides the equivalent of about 2. THE CEOS DATABASE : CATALOGUE OF SATELLITE INSTRUMENTS.
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The V- 1 Flying Bomb. The V- 1 Flying Bomb. The history of the cruise missile was marked by failures and dead ends until modern times. One early attempt to build and operate such a weapon became notorious: the German V- 1 flying bomb of World War Two. Officially, it was simply FZG- 7. Plastic model kits for sale, rare and vintage airplane models, R/C, ship models and car models. Over 6000 different kits in stock. All-plastic model kits got their. Airbnb can be an awesome service for frugal travelers, and it feels especially great to use when the only other option is staying at an overpriced boutique hotel in. Flakzielger. The anti- aircraft designation was a ruse to throw Allied spies off the track. In Britain, it was known as the . The Nazi Propaganda Ministry called the pilot- less aircraft Vergeltungswaffe (retaliation weapon) 1, or V- 1. But the name almost universally favored by Britons and Americans alike was . Its overall length was just over 2. Standard 8. 0- octane gasoline kept its jet engine running, which was housed in the stovepipe assembly; this was the same fuel used by trucks. The flying bomb was easy and cheap ($5. But while the flying bomb may have been cheap and simple, it was not very accurate- it could not hit small targets, or even moderate- sized villages. It was accurate enough to hit a target the size of Greater London, however, and that was all that was expected - a way to hit back at the Allies without risking the depleted reserves of the Luftwaffe's bomber fleet. During the early months of 1. FZG- 7. 6. Only nine months had passed between the beginning of work on the project in March 1. Christmas Eve, although the flying bomb still had its share of teething problems. One question involved the proper type of launching site for the flying bombs. Some favored large concrete emplacements; others proposed small, portable sites. As head of the Luftwaffe, Reichsmarschall Hermann G. A new Luftwaffe unit was formed in August 1. Flakregiment 1. 55 ('N). The anti- aircraft designation was, once again, aimed at deceiving Allied intelligence. The new unit was placed under the command of Luftwaffe Colonel Max Wachtel, who had been in charge of all the experimental flying bomb launches. Wachtel was instructed to get his men ready for firing the bomb under actual combat conditions, and he took his orders to heart; his Flakregiment began exercises within days of the unit's creation. From the western side of Peenem. By. June 1. 94. 4, Wachtel and his unit were in France, ready to begin operations. But few others connected with the flying bomb project were as efficient as Wachtel. One of the main problems was with the production of the flying bombs themselves. Because of the many defects that plagued the bomb, it did not go into production until March 1. Engineers at the Volkswagen plant at Fallersleben, near Hamburg, did their best to work out the problems, but the pilotless planes kept crashing immediately after launching. Full production did not begin until April 1. Volkswagen assembly line. Wachtel had been ordered to begin launching the pilotless bombs against England by June, but his unit had no equipment, no launching rails and no supplies. It had been decided that lightweight launching ramps, called modified sites, would be used in place of larger ramps that had proved too vulnerable to Allied bombing attacks. The supplies and equipment that Wachtel needed to begin operations did not arrive until June 1. V- is against southern England. Only 1. 0 ramps were ready for launching; 5. By 3: 3. 0 am, on June 1. The Luftwaffe high command decided to go ahead despite the fact that so few ramps were operational. Months of practice made the pre- launch procedure a set routine for the crews. First, the flying bomb's fuel tank was checked, to make certain that it had been topped off. Following this, the wooden wings were attached- these had been folded over the fuselage to make storing and moving the aircraft easier. After assembly, the plane was aligned precisely with its firing ramp- which was pointed directly at London - and its gyrocompass was set at zero to ensure it flew the straight course on which it had been aimed. The flying bomb, now ready for launching, was moved onto its firing ramp. After it was loaded onto its catapult, a lug on the underside of the fuselage was attached to the catapult's firing piston. When the piston was released, it accelerated the V- 1 off the launch rails in the same way that a jet plane is catapulted off the flight deck of an aircraft carrier. With the stubby- winged flying bomb poised for takeoff, the launching crew took cover inside the . The firing officer gave an order, a technician pulled a lever, and the flying bomb's pulse- jet engine came to life with a throbbing, ear- numbing roar. This simple jet engine was the flying bomb's most unique feature. Housed outside the fuselage, above the tail, the jet is usually described as looking like either a stovepipe or a giant blow torch. At the front end of the engine housing was a set of intake flaps that resembled a Venetian blind. These flaps opened at the beginning of the engine's cycle, allowing air to be drawn into the combustion chamber, where it was mixed with 8. With a tremendous flash, a burst of hot exhaust shot out from the rear of the engine to provide forward thrust. Immediately following the exhaust stage, the intake flaps opened again, allowing air into the combustion chamber and repeating the cycle. This simple jet engine could complete up to 5. The engine's pulsing combustion process also gave the flying bomb its distinctive duv- duv- duv sound in flight, a sound that Londoners would soon come to recognize. After listening for a moment to ensure that the engine was firing properly, the firing officer gave the order to launch. A second lever was pulled, releasing the catapult's piston. The flying bomb lurched forward, shot along the length of steel rail, and lumped uncertainly into the night sky. During the next half- hour, between ab out 3: 3. Two of the successfully launched flying bombs crashed into the English Channel. The other four reached England; two landed in Kent, one in Surry, and one crashed in London, the intended target of all of them. The London bomb came down in Bethnal Green, East London, about three miles away from its Tower. Bridge target point. The explosion killed three people and knocked out a railway bridge. Although only four flying bombs reached England during this first launch, hundreds more would be launched during the next several weeks. An inexpensive, and not very accurate, mechanism sent the flying bomb diving into its target upon arrival. Each bomb had a small, propeller like anemometer device on its nose that was connected to the bomb's autopilot. As the flying bomb flew through the air, its forward motion turned the propeller like a pinwheel in the wind. After a preset number of revolutions, the propeller tripped the diving controls, pointing the bomb earthward at a steep angle. The mechanism was set by the catapult crew before launching; the setting of how many revolutions were needed to trip the diving controls was based upon calculations involving the flying bomb's speed and the distance to target. Any number of factors could undo this inherently imprecise system. Headwinds or tailwinds could alter the machine's groundspeed, mining carefully worked- out calculations that were usually a lot more accurate than the mechanism itself. The autopilot might go haywire and send the bomb plunging into the Channel. Or it might not work at all, causing the bomb to overfly London and keep going until it ran out of fuel. When the windmill device tilted the bomb toward the earth, all the fuel ran to one end of the tank - the end away from the fuel pump. The pump began drawing air, and the engine, cut off from its fuel supply, stopped running. V- 1 Development. Wunderwaffen The Germans performed experiments with autopiloted aircraft in the 1. German military in 1. In June 1. 94. 2, however, growing RAF bomb raids on German cities, and rising losses of Luftwaffe bombers over England in attempts to retaliate, persuaded the Luftwaffe to consider new options. Work on the V- 2 long- range rocket was encountering difficulties, and the V- 2 was an Army project in any case. The Luftwaffe investigated and approved the development of a small, cheap flying bomb, with a range of about 2. The project was given the cover designation of . Propulsion for the new flying bomb was provided by the . The pulsejet was little more than a . The simplicity and low cost of this engine was a major factor in the Luftwaffe's decision to pursue flying bomb development. Air entering into the pulsejet was mixed with fuel and the mixture ignited by spark plugs. The combustion of the mixture slammed the intake shutters closed, and produced a burst of thrust out the exhaust. The shutters then opened again in the airflow. The production engine would perform this cycle about 4. This pulsed operation caused the engine to emit a loud low throbbing sound that would presently become familiar over the English countryside. Schmidt's pulsejet was a crude engine. Throttling it was difficult at best, it could only operate effectively at low altitudes, and the shutters tended to wear out quickly, but none of these issues were important in an expendable robot weapon, and it had major advantages. It was simple, cheap, and powerful, with a thrust of 2. Furthermore, it could use low- grade gasoline as a fuel, rather than precious high- octane aviation fuel. Three companies collaborated in building the flying bomb. Fieseler built the airframe; Argus, the employer of Paul Schmidt, built the pulsejet engine; and Askania built the guidance system. A glide test of the flying bomb was performed from a Focke- Wulf FW- 2. Kondor in early December 1. Christmas Eve. The first powered flight only went a kilometer, and the early prototypes showed a distressing tendency to crash. To resolve these problems, a piloted flying bomb was developed, with the warhead replaced by a cockpit in which a test pilot could fly the machine while lying prone. Test flights were performed with the tiny and daring female test pilot Hanna Reitsch at the controls, and helped resolve the problems. On 2. 6 May 1. 94. Nazi officials visited the test facility at Peenem. Astrologer, Mary Shea, in a lecture for the Baltimore NCGR, listed some POTHOLES that we may encounter while under the influence of a Pluto transit. The Put on a Bus trope as used in popular culture. So you're a film or TV show producer or the author of a book series, or the team behind a comic book, and. Dane Wigington geoengineeringwatch.org. The now near total desperation of the climate engineers to turn warmth into winter is becoming incredibly obvious and blatant. Nacho had to step in to separate the pair before Ronaldo went on to convert his 12th La Liga goal of the season, leaving him just two goals behind Barcelona's Lionel. Revealing Mars' True Colors of NASAby Richard C. Hoagland. 20. 02 from. The. Enterprise. Mission Website. Part 1. The below color images of Mars were taken in 1. Oeiras. Portugal - Antonio Cidadao. They were acquired with a modest. It was a 2. 0 second exposure on Kodachrome color film, subsequently processed by the Institute. It was a combination. Kodachrome exposure! In the fourth century, the Roman Emperor Constantine united all religious factions under one composite deity, and ordered the compilation of new. A comparison of the sheer physical size of the two instruments. That planetary images of the quality of Cidadao. That it could produce images better than. Mt Wilson instrument, and when Mars was almost twice as. According to. official Odyssey documents. Over 1. 5,0. 00 panchromatic (3,0. Yet, in stark contrast to Antonio Cidadao. Mars Odyssey images! Mars Odyssey arrived at Mars on October 2. It began its. official . Among these images were many apparent . These attempts, we duly discovered, were. PDS and ASU. However. B& W filtered images and attempting to. From examination of the. B& W filtered images (below), it is readily apparent that. This. means that after you've taken the red picture, you have to wait for. This also means that the planet's rotated. In addition to motion, different parts of. This is all called geometric. STILL isn't complete. There's several parts of. One of the really crummy parts is the black part of the. When you snap a picture, you . In the wavelengths we use. This is called. flat- fielding. This isn't all. that hard, since the calibration coefficients were measured in the. I. thought you were finished before. We. snap the whole array at once, which is 1 framelet in each band. There was talk about it for the '0. The ESA Mars Express mission has one through. You mentioned use of 'calibration coefficients'. Would. you mind elaborating on what exactly is used to calibrate the. In the lab you measure. There's not a lot of call for the 7. One of the really crummy parts. The surprise (to some) will. Philip. Christensen - . Within a few hours of that historic publication. Mars - . another, hurriedly revised version of this first color surface image. Ron Levin, now also a scientist - a physicist. MIT. In the summer of 1. Viking landed), Ron was a. JPL. during that incomparable . Straat, Frog Ltd. Berkeley, CA 1. 99. According to Di. Gregorio. PDT, the first color image from the surface of. Mars, began to emerge on the JPL color video. JPL employees and media personnel to view the Viking. Gil and Ron Levin sat in the main control room where dozens. As the image developed on the. Mars in color. The image showed an Arizona- like landscape: blue sky. It looks like Arizona. Ron Levin looked in disbelief as the technician went from. Minutes later, Ron followed. Levin and Straat were interrupted when they heard someone being. It was Ron Levin being chewed out by the Viking Project. Director himself, James S. Gil Levin went immediately. He warned Ron. that if he tried something like that again, he. The Director then asked a TRW engineer assisting the. Biology team, Ron Gilje, to follow Ron Levin around to every color. Months later. Gil Levin sought out the JPL Viking Imaging Team technician who. The technician. responded that he had instructions from the Viking Imaging Team that. Mars sky and landscape should be red and went around to all the. The technician said that the Mars atmosphere. Or, as Gil Levin put. There would be less red light . And what about the. This long- distance reconnaissance. Pathfinder. arrival, which (with its potentially high winds) could have posed a. Pathfinder entry and landing. Hubble Investigator on the Pathfinder Landing imagery, Dr. Remarkably, in all those images (below) the tell tale evidence. Raleigh scattering (that bluish limb around the planet. In the three examples displayed here, the top image is an. Antonio Cidadao. James own comments - as the. It was acquired just prior to the Pathfinder Landing, in. Except for the obvious differences in resolution (remember, Cidadao. Note the. distinct blue atmospheric layer floating over the russet Martian. MGS camera.. In a. Di. Gregorio (also reproduced in. Mars - The Living Planet). Van der Woude wrote. Thomas Mutch, the Viking Imaging Team. NASA Administrator. Mars blue sky negative created from the. Why was the Administrator of NASA so determined to conceal. Why would he order the head of the Viking Imaging Team to. Mission archive - the original ! In the interim, because of. Web), a whole new generation has now been enabled. Mars images.. In other words, what has the THEMIS Team been doing all these months. March 1. 4, 2. 00. And, how come Heald - a carpenter by trade, and an admitted. However, amid the praise, more than a few of these. Gary Leggier. In particular, the. NOW on Mars! For these investigators, the Woodlock three- color image - though. In. it, not only do the reddish tints become more vivid, but the darker. A little scary I had not done that, yet Shows that there. I'm thinking that would make my photo 'unenhanced'. This comparison reveals. Note that, with the same. Hubble Telescope), NASA has published since 1. Fontana produced the. He also made what could be termed the first scientific. While he was eminently successful with the stars. In 1. 85. 8, however, he did produce the. Mars - which showed the dark areas. Even in its mottlings the one expanse recalls the other.. Slipher, a later, noted planetary astronomer at Lowell (and. Lowell Director, Vesto Slipher - who himself. Wilson on his eventual career..) would write of these dark . The. evidence is in the blue- green areas and the changes in their. Vegetation would present exactly the appearance shown. The seasonal change. The blue- green lapses into ochre and. Earth at the. proper season under the stimulus of the Sun and the advent of water. If there was enough oxygen to sustain life, and if the. Plants may have developed means of utilizing. Earth have learned to store. Slipher, Northland Press. Flagstaff, AZ, 1. Not all telescopic observers, however, were so easily convinced. Astronomers who used large reflecting telescopes to observe Mars. Bernard. traditionally did his looking through the 3. Lick Observatory (just south of San Francisco), and the 4. Yerkes Observatory (northeast of Chicago) - still. Refractors of. this great size have an intrinsic engineering problem: bringing all. Wilson in 1. 91. 1 (then, the largest. Mars were. Wilson - another well- known astronomer, Gerard Kuiper, carried out a completely different color experiment a. Kuiper used the 8. Mc. Donald Observatory (in Texas), to visually compare the subtle. Martian features with a set of standard laboratory color charts. In this way, with a magnification of 9. Moon as seen with the naked eye from Earth (!) - with. Viewed. against a bright ochre background . This view was solidified in 1. Mariner 9. The. long- mysterious dark markings, in this view, were not - are not - . And why are they still doing it.. These provocative spectral observations were carried out at two. Mars oppositions, by Harvard University astronomer, William. Sinton - in 1. 95. These. bands are unevenly spaced across the visible and near- infrared. In addition to reconstruction of visible color images from the three. Band 1. 0 was chosen to fall in the middle of the CO2. RED. Not sure what band 8. QUB file as any thing that is remotely. Now these color bands are compatible with the PSP RGB. Think the data is very practical and we can get a. The Pathfinder camera parameters (on the Lander) were. JGR- Planets . The basaltic weathering product palagonite is an example of a. IR spectral properties doninated. Morris et al., 1. The. spectrally diagnostic region for these minerals is primarily in the. UV to 8. 60 nm range using 8 of the filters. This allows for. discrimination based on four spectral parameters (Bell and Morris. UV drop- off (diagnostic. The depth of features at these diagnostic band- passes. View, California - of. Mars.. The condition was. All of these cases occur in. Four of the cases. Two intriguing cases occur in small areas on the ground. Peter. Smith (University of Arizona), announced the results of an initial. This process. is known as photosynthesis and is the basis for sustaining the life. Since animals and humans obtain their food. In 1. 99. 6, another of his experiments - a compact. These curiously enhanced regions (below, far. In truth. raw ultraviolet light reaching the Martian surface would quickly. All are essentially the same molecule, differing only in. All are essential to the photosynthetic process, and. According to the. Odyssey PIP, the shortest- wave VIS filter (above). This, in. turn, will heavily - but quietly, judging by NASA. Unless - it already has - and we don. The first near- IR. It has also recently been tested (via . This will differentiate a successful. Here is an example from Arizona (courtesy of. Debi A. Scott) of what. Note. the brilliant appearance of the vegetation (due to high reflectance. IR), compared to the background, iron- oxidized Arizona. Clarke (below), who first brought their remarkable. Martian south pole to the attention of the space. In the Fifth . Ironically, the major planetary sessions. Note that, seen with. Jim Heald. This official procedure is, of course, precisely the same process we. These colors. are obviously more accurate - when compared with what Mars simply. JPL. And, any bets on when they plan to finally tell us. Though there are countless forms of anthropogenic damage to the biosphere (with the Co. What will it take for the human race to abandon their
. The fire had grown from
But, of course, the part climate engineering has played in this engineered weather scenario is completely omitted as is any mention whatsoever of the blatantly obvious and unarguable ongoing
Photo: Scott Olson . On Friday, May 6th, 2. US. On this date, the
There are, of course, countless contributing factors. One primary element is the buildup of greenhouse gasses (Co. A second major factor is the creation of heat domes by the climate engineers (which are a part of
This is in addition to the underlying overall damage to the biosphere and climate system by ongoing anthropogenic activity on countless fronts. . The satellite image below was taken on May 8th, 2. Massive aerosol spraying particulate trails are clearly visible over regions off the US West Coast and over parts of the interior US. Two circular pressure zone perimeters are also very visible which are related to the jet stream manipulation already outlined. This assault must be exposed and halted if Earth is to have any possible chance to find a new life supporting equilibrium given the level of irreparable damage already done by
If the climate engineering assault is not fully exposed and halted, very soon, there will be nothing left to salvage. If these programs can be stopped, the human race must then face the unimaginably long list of challenges that has been created by the damage inflicted on the biosphere due to anthropogenic activity (which, of course, includes climate engineering). Exposing and halting the climate engineering assault.
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Il Gran Premio del Messico rientrerebbe in calendario a ottobre, al posto della gara prevista nel New Jersey; nello stesso mese ci sarebbe stato l'esordio per il Gran Premio di Russia. Venne anche confermato il rientro per il Gran Premio d'Austria, mentre il Gran Premio di Spagna resterebbe a Barcellona e quello di Corea verrebbe spostato ad aprile. La data di ottobre sarebbe stata presa dal Gran Premio di Russia. Inoltre, la gara di Abu Dhabi ritorner. Le gare saranno quindi 1. La gara del Bahrain (quest'anno eccezionalmente in notturna per festeggiare i 1. Cina. In rosa sono quelli che li hanno ospitati in passato, gli ex circuiti ospitanti sono contrassegnati con un punto bianco. Le nuove monoposto sono state presentate dalla scuderie secondo l'ordine seguente. Il circuito del Bahrain aveva gi. TGCOM24: il quotidiano online di News Mediaset. Aggiornamenti in tempo reale, notizie del giorno e ora per ora, approfondimenti di cronaca, politica, esteri, economia. Notizie di economia, cronaca italiana ed estera, quotazioni borsa in tempo reale e di finanza, norme e tributi, fondi e obbligazioni, mutui, prestiti e lavoro a cura. Bakeca è il sito di annunci gratuiti per chi cerca casa, lavoro, incontri ed eventi. Migliaia di annunci sempre nuovi per trovare subito quello che stai cercando! MAURIZIO CROZZA arriva con “Fratelli di Crozza”, il suo nuovo live show in onda ogni venerdì alle 21:15 sul NOVE. Bing ti consente di tradurre le informazioni in azioni, rendendo più rapido e semplice il passaggio da ricerca ad azione. Formula 1 2017: classifica campionato piloti e scuderie costruttori, calendario gare, circuiti gran premio e piste, risultati prove libere, qualifiche e diretta live. La richiesta di spostare i test dall'Europa al Medio Oriente . Inizialmente era stato prospettato l'utilizzo del Dubai Autodrome. La stagione segna il ritorno nel circus di questo storico sponsor delle competizioni motoristiche. La Scuderia Toro Rosso, invece, ha raggiunto un accordo con la Renault per la fornitura dei motori dal 2. Ferrari. La scuderia faentina ha cos. L'accordo prevede anche la fornitura della tecnologia ERS, nuovo sistema per il recupero dell'energia che sostituisce il KERS. Il cambio invece continuer. Tale rapporto era iniziato nel 2. Il nome di Martini Racing . La Marussia avrebbe offerto alla Sauber una proposta di fusione delle due scuderie, entrambe in difficile situazione finanziaria: la richiesta non ha avuto seguito. Tale scuderia dovrebbe garantire la sua permanenza nel campionato almeno fino alla stagione 2. Il termine entro il quale gli interessati possono fare pervenire le loro richieste era fissato al 3 gennaio 2. I suoi componenti hanno valutato che il cambiamento del panorama tecnico e commerciale del campionato non rendesse pi. Assieme a Kolles la guida della scuderia . La scuderia russa si trova in difficolt. Alla gara risultano perci. Successivamente la Marussia comunica la definitiva cessazione dell'attivit. La casa anglomalese ha anche lanciato una raccolta di fondi presso i suoi tifosi, per ottenere la liquidit. Il finlandese, che nelle ultime due stagioni ha corso per la Lotus, ha gi. La sua presenza era comunque subordinata all'ottenimento della superlicenza FIA, requisito indispensabile per guidare in un Gran Premio di Formula 1. Ericsson, che ha vinto la Formula 3 giapponese 2. L'ultimo pilota svedese a competere in un Gran Premio di F1 fu Stefan Johansson nel Gran Premio del Canada 1. Robin Frijns, ex Sauber, affiancher. Il pilota tedesco, impiegato nella Super Formula, campionato che ha vinto nel 2. Formula Nippon, si . Sostituisce Kamui Kobayashi. Lo statunitense sarebbe stato all'esordio nel mondiale di F1, dopo aver svolto la funzione di terzo pilota alla Caterham tra il 2. Renault 3. 5; l'altro pilota utilizzato in stagione, Marcus Ericsson, ha nel frattempo rescisso il contratto che lo legava alla scuderia. Precedentemente anche Andr. Tuttavia, la loro partecipazione dipende dalle squadre che accetteranno di continuare a competere in questo sport sotto i termini del nuovo Patto della Concordia. Il Comitato Olimpico Internazionale aveva avvertito che avrebbe cercato di convincere gli organizzatori a posticipare la corsa al 2. Giochi olimpici invernali. Gli organizzatori del gran premio sono stati premiati dalla FOM col Race Promoters' Trophy per il 2. Il 2. 3 luglio 2. Bernie Ecclestone e Dietrich Mateschitz, titolare della Red Bull Racing, hanno formalizzato il ritorno del Gran Premio d'Austria nel calendario iridato. Il tracciato che ospiter. La gara, valida 2. La gara sarebbe stata disputata nella tradizionale sede dell'Autodromo Hermanos Rodr. L'ultima gara ospitata dall'Hockenheimring venne disputata nel 2. Tuttavia, a causa delle difficolt. I nuovi motori saranno dei 1,6 litri V6 con un cambio semi automatico a otto rapporti. I motori dovevano durare almeno 4. Successivamente tale energia viene trasformata in carica elettrica e immagazzinata nelle batterie fino a quando non . La punta del muso non doveva essere alta oltre 1. Queste ulteriori modifiche sono state formalmente abbandonate nel dicembre del 2. Tale accorgimento serve a far diminuire la spinta verticale verso il basso sulle gomme posteriori, dovuta alla deportanza extra creata dall'espansione del flusso dei gas caldi provenienti dal motore nel diffusore posteriore, altrimenti estremamente difficile da raggiungere. Le squadre avevano precedentemente sfruttato una scappatoia nel regolamento che permetteva loro di aggiungere ulteriori pezzi di carrozzeria al posto dei supporti per le telecamere, sfruttando i vantaggi aerodinamici. Dal 2. 01. 4 questa scappatoia sar. Secondo la proposta, le prove invernali saranno anticipate a gennaio per consentire un ulteriore test, se lo si ritiene necessario, con sedi trasferite lontano dalla Spagna meridionale, in Medio Oriente, in Qatar e in Bahrein, per ridurre al minimo le probabilit. Quattro sedi europee ospiteranno una due giorni di test nella settimana successiva al Gran Premio tenutosi presso il circuito. Chi ha utilizzato un sesto motore ha iniziato la gara dalla pit lane, nuova penalizzazione che prende il posto della retrocessione di dieci posizioni sulla griglia di partenza utilizzata nella stagione precedente. Le squadre riceveranno anche un set supplementare di pneumatici per la prima sessione di prove di ogni Gran Premio. Il set supplementare di pneumatici sar. Sebastian Vettel, il campione del mondo in carica, ha scelto di utilizzare comunque il numero 1. Inoltre, per infrazioni minori, verranno aggiunti 5 secondi di penalit. L'altra Marussia, quella di Jules Bianchi, resta invece ferma al semaforo: la procedura di partenza viene interrotta. Le vetture compiono un ulteriore giro di formazione, mentre la durata della gara viene accorciata di un giro. Al via scatta in testa Nico Rosberg, che precede Daniel Ricciardo, Lewis Hamilton, Kevin Magnussen, Fernando Alonso e Nico H. Alla partenza Kamui Kobayashi va lungo la prima curva e tampona Felipe Massa: si ritirano entrambi. Nei primi giri si ritirano per problemi al propulsore sia Lewis Hamilton sia Sebastian Vettel. Al settimo giro Valtteri Bottas passa Kimi R. La direzione di gara invia in pista la safety car. Molti piloti ne approfittano per effettuare il cambio gomme. Al momento della ripartenza Nico Rosberg . La classifica, almeno nelle prime posizioni, resta immutata fino a met. Nelle retrovie si fa largo ancora Bottas, che dal sedicesimo posto, si porta al nono, gi. Rosberg resta sempre al comando, davanti a Ricciardo e Magnussen. Button scala ora quarto, precedendo Alonso e H. Valtteri Bottas prosegue nella sua rimonta passando prima Jean- . A podio finiscono per la prima volta Daniel Ricciardo e Kevin Magnussen, primo pilota danese a ottenere questa impresa. A punti termina anche Daniil Kvjat, che a 1. Ricciardo viene poi squalificato per un'irregolarit. Al quarto giro Vettel passa il suo compagno di team Ricciardo e si pone alle spalle delle due Mercedes. Al giro nove Kevin Magnussen . Per questo contatto il danese . Due giri dopo va al cambio gomme Alonso, seguito al giro 1. Ricciardo. L'australiano, all'uscita dai box, precede di poco lo spagnolo. Tra il giro 1. 3 e il giro 1. Lewis Hamilton rientra in pista dietro a H. La classifica resta di fatto immutata. Sulla pista cadono poche gocce di pioggia che non costringono i piloti a montare gomme da bagnato. Sebastian Vettel si avvicina nel frattempo a due secondi da Nico Rosberg. Al giro 4. 0 Daniel Ricciardo effettua il terzo cambio gomme: il team lo rimanda in pista con la gomma anteriore sinistra non bene fissata, tanto che il pilota si ferma immediatamente nella corsia dei box e viene riportato dai meccanici verso la sua piazzola di sosta. L'australiano riparte cos. Inoltre sulla sua vettura si piega, poco dopo, l'alettone anteriore, che rovina nuovamente gli pneumatici. Al giro 4. 2 terzo cambio gomme per Alonso, che rientra in pista dietro a Nico H. Al giro 5. 2 Alonso passa Nico H. Precede Nico Rosberg, Sebastian Vettel e Fernando Alonso. Jenson Button costretto al ritiro a un giro dal termine nel GP del Bahrain, per la prima volta corso in notturna. In partenza Lewis Hamilton scatta meglio di Nico Rosberg e assume il comando della corsa. Nel primo giro il tedesco attacca il britannico ma senza riuscire a prevalere. Al dodicesimo giro anche l'altro pilota della Williams. Felipe Massa deve cedere la posizione a P. La classifica, dietro al duo Hamilton- Rosberg, vede ora terzo Bottas, seguito da Massa e dalle due Force India. Al giro 1. 8 Rosberg attacca Hamilton per la prima posizione, passandolo alla prima curva, ma l'inglese risponde e torna ancora al comando. La lotta si ripropone il giro seguente, ma ancora Lewis Hamilton resta leader della corsa. Al giro 2. 0 il britannico effettua il suo pit stop, mentre Rosberg attende il giro 2. Rientrando in pista il tedesco rimane dietro al britannico. Al giro 2. 5 Valtteri Bottas effettua il secondo cambio gomme: scala terzo Massa, insidiato dalle due Force India. Un giro dopo il brasiliano va ai box, cos. Bottas piomba su questi ultimi due, passa Ricciardo, ma sbaglia la frenata alla prima curva ed esce di pista, potendo per. Ancora un giro e il finlandese effettua il secondo cambio- gomme. Al 3. 5. Al giro 3. Massa effettua ancora un cambio gomme. La direzione di corsa decide di inviare in pista la safety car. Durante il periodo in cui . La gara riparte al giro 4. Lewis Hamilton . Il tedesco,che gode di pneumatici a mescola morbida contro quelli a mescola dura del compagno,tenta a pi. Al giro 5. 0 Daniel Ricciardo ottiene strada da Vettel e si pone al quinto posto: il campione del mondo . A un giro dal termine si ritira Button. Lewis Hamilton vince per la ventiquattresima volta, precedendo Nico Rosberg e Sergio P. Mathematica 1. 0 Free Download. Mathematica 1. 0 Free Download Latest Version for Windows. It is full offline installer standalone setup of Mathematica 1. Windows 3. 2 bit 6. PC. Mathematica 1. Overview. Mathematica 1. Stephen Wolfram. This application is ideal for engineering and mathematical computations. This technically powerful application is easy to use at the same time. Mathematica has 2. You can also Download Mathematica 9 which was previous version. Mathematica 1. 0 has many advanced and enhanced features lets have a quick look at some of the new added features in Mathematica 1. 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