‎Administration‎

‎National Aeronautics and Space Administration‎

‎LAUNCH VEHICLES OF THE NATIONAL LAUNCH VEHICLE PROGRAM. NASA SP-10‎

‎Washington D. C.: National Aeronautics and Space Administration. VG. 1962. Paperback. Paperback in Very Good condition. . 8vo 8" - 9" tall. 31 pages. Quick Shipping All Books Mailed in Boxes Free Tracking Provided . National Aeronautics and Space Administration paperback‎

Bookseller reference : 39937

‎National Aeronautics and Space Administration [Compiler]‎

‎Leadership In Space: Selected Speeches of NASA Administrator Michael Griffin May 2005 - October 2008‎

‎U.S. National Aeronautics and Space Administration 2008-12-23. hardcover. New/New. 6x0x9. 2008 Book and DJ New and unread. U.S. National Aeronautics and Space Administration hardcover‎

Bookseller reference : SKU1021235 ISBN : 0160815657 9780160815652

‎National Aeronautics and Space Administration‎

‎Leadership in Space: Selected Speeches of NASA Administrator Michael Griffin May 2005 - October 2008‎

‎U.S. National Aeronautics and Space Admi 2008-12-23. First Edition. hardcover. New. 6.50x1.00x9.75. Buy with confidence. Excellent Customer Service & Return policy. U.S. National Aeronautics and Space Admi hardcover‎

Bookseller reference : DADAX0160815657 ISBN : 0160815657 9780160815652

‎National Aeronautics and Space Administration‎

‎Lifting Standard: NASA-STD-8719.9B‎

‎paperback. Good. Access codes and supplements are not guaranteed with used items. May be an ex-library book. paperback‎

Bookseller reference : 1731034903.G ISBN : 1731034903 9781731034908

‎National Aeronautics and Space Administration‎

‎Liquid Rocket Engine Turbopump Inducers‎

‎paperback. Good. Access codes and supplements are not guaranteed with used items. May be an ex-library book. paperback‎

Bookseller reference : 1499234732.G ISBN : 1499234732 9781499234732

‎National Aeronautics and Administration‎

‎Living Aloft: Human Requirements for Extended Spaceflight‎

‎Paperback / softback. New. paperback‎

Bookseller reference : B9781495327483 ISBN : 1495327485 9781495327483

‎National Aeronautics and Space Administration, Office of Public Affairs‎

‎Log of Apollo 11; EP-72‎

‎Washington DC: National Aeronautics and Space Administration Office of Public Affairs c1969. Presumed First Edition First printing. Pamphlet. Very good. The format is approximately 10.25 inches by 7.75 inches. 12 pages including covers. Illustrated front and back cover. Illustrations some in color. Presents key information by day and time of this historic lunar voyage. After being sent to the Moon by the Saturn V's third stage the astronauts separated the spacecraft from it and traveled for three days until they entered lunar orbit. Armstrong and Aldrin then moved into Eagle and landed in the Sea of Tranquility on July 20. The astronauts used Eagle's ascent stage to lift off from the lunar surface and rejoin Collins in the command module. They jettisoned Eagle before they performed the maneuvers that propelled Columbia out of the last of its 30 lunar orbits onto a trajectory back to Earth. They returned to Earth and splashed down in the Pacific Ocean on July 24 after more than eight days in space. Armstrong's first step onto the lunar surface was broadcast on live TV to a worldwide audience. He described the event as "one small step for a man one giant leap for mankind." Apollo 11 effectively proved U.S. victory in the Space Race to demonstrate spaceflight superiority by fulfilling a national goal proposed in 1961 by President John F. Kennedy "before this decade is out of landing a man on the Moon and returning him safely to the Earth." Apollo 11 July 16-24 1969 was the American spaceflight that first landed humans on the Moon. Commander Neil Armstrong and Lunar Module Pilot Buzz Aldrin landed the Apollo Lunar Module Eagle on July 20 1969 at 20:17 UTC and Armstrong became the first person to step onto the Moon's surface six hours and 39 minutes later on July 21 at 02:56 UTC. Aldrin joined him 19 minutes later and they spent about two and a quarter hours together exploring the site they had named Tranquility Base upon landing. Armstrong and Aldrin collected 47.5 pounds of lunar material to bring back to Earth as pilot Michael Collins flew the Command Module Columbia in lunar orbit and were on the Moon's surface for 21 hours 36 minutes before lifting off to rejoin Columbia. Apollo 11 was launched by a Saturn V rocket from Kennedy Space Center on Merritt Island Florida on July 16 at 13:32 UTC and it was the fifth crewed mission of NASA's Apollo program. The Apollo spacecraft had three parts: a command module CM with a cabin for the three astronauts the only part that returned to Earth; a service module SM which supported the command module with propulsion electrical power oxygen and water; and a lunar module LM that had two stages—a descent stage for landing on the Moon and an ascent stage to place the astronauts back into lunar orbit. National Aeronautics and Space Administration, Office of Public Affairs unknown‎

Bookseller reference : 86126

‎NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WASHINGTON DC‎

‎Lubrication Corrosion and Wear. A Continuing Bibliography‎

‎PN. New. 1965. Soft Cover. Date is original print. This is a reprint edition. . PN paperback‎

Bookseller reference : 727053

‎National Aeronautics and Space Administration‎

‎Lunar Reconnaissance Orbiter LRO: Leading NASA's Way Back to the Moon; Lunar Crater Observation and Sensing Satellite LCROSS: NASA's Mission to Search for Water on the Moon Press Kit/June 2009 NP-2009-05-88-MSFC‎

‎George C. Marshall Space Flight Center Huntsville A.: National Aeronautics and Space Administration George C. Marshall Space Flight Center 2009. Xerox-style reproduction. Assume only a few copies were made for medial representatives. Stapled at upper left corner. Good. Front cover i 1 36 2 pages. Illustrations. Three-hole punched. The top corner of some of the some of the back pages are bent/creased. Contents include Contacts; Media Services Information; LRO/LCROSS Executive Summary; Mission Quick Facts; LRO Quick Facts; LCROSS Quick Facts; Launch Vehicles Mated with LRO/LCROSS; LRO/LCROSS Mission Trajectory; Why the Moon; Historical Explorations of the Moon; LRO Mission Overview; LRO Mission at a Glance; LRO Instruments; LRO Across the Country; LRO Products and Benefits: LRO Spacecraft With Instruments; Treasure Hunting on the Moon: LRO and the Search for Water; Robot Scout: Fly Me Safely to the Moon; LCROSS Mission Overview; LCROSS Mission at a Glance; The Search for Water on the Moon; LCROSS Science Instruments; LCROSS Spacecraft; LCROSS Observation Campaign; Future NASA Lunar Missions; and Program/Project Oversight. The Lunar Reconnaissance Orbiter LRO is a NASA robotic spacecraft currently orbiting the Moon in an eccentric polar mapping orbit. Data collected by LRO have been described as essential for planning NASA's future human and robotic missions to the Moon. Its detailed mapping program is identifying safe landing sites locating potential resources on the Moon characterizing the radiation environment and demonstrating new technologies. Launched on June 18 2009 in conjunction with the Lunar Crater Observation and Sensing Satellite LCROSS as the vanguard of NASA's Lunar Precursor Robotic Program LRO was the first United States mission to the Moon in over ten years. LRO and LCROSS were launched as part of the United States's Vision for Space Exploration program. The probe has made a 3-D map of the Moon's surface at 100-meter resolution and 98.2% coverage excluding polar areas in deep shadow including 0.5-meter resolution images of Apollo landing sites. The first images from LRO were published on July 2 2009 showing a region in the lunar highlands south of Mare Nubium Sea of Clouds. The total cost of the mission is reported as US$583 million of which $504 million pertains to the main LRO probe and $79 million to the LCROSS satellite. As of 2019 LRO has enough fuel to continue operations for at least seven more years and NASA expects to continue utilizing LRO's reconnaissance capabilities to identify sites for lunar landers well into the 2020s. The Lunar Crater Observation and Sensing Satellite LCROSS was a robotic spacecraft operated by NASA. The mission was conceived as a low-cost means of determining the nature of hydrogen detected at the polar regions of the Moon. Launched immediately after discovery of lunar water by Chandrayaan-1 the main LCROSS mission objective was to further explore the presence of water in the form of ice in a permanently shadowed crater near a lunar polar region. It was successful in confirming water in the southern lunar crater Cabeus. It was launched together with the Lunar Reconnaissance Orbiter LRO on June 18 2009 as part of the shared Lunar Precursor Robotic Program the first American mission to the Moon in over ten years. LCROSS was designed to collect and relay data from the impact and debris plume resulting from the launch vehicle's spent Centaur upper stage and data-collecting Shepherding Spacecraft striking the crater Cabeus near the south pole of the Moon. Centaur had nominal impact mass of 5081 lb and an impact velocity of about 5600 mph releasing the kinetic energy equivalent of detonating approximately 2 tons of TNT. LCROSS suffered a malfunction on August 22 depleting half of its fuel and leaving very little fuel margin in the spacecraft. Centaur impacted successfully on October 9 2009 at 11:31 UTC. The Shepherding Spacecraft descended through Centaur's ejectate plume collected and relayed data impacting six minutes later at 11:37 UTC. Contrary to media reports at the time neither the impact nor its dust cloud could be seen from Earth using the naked eye or telescopes. National Aeronautics and Space Administration, George C. Marshall Space Flight Center unknown‎

Bookseller reference : 86122

‎National Astronautics and Space Administration Goddard Space Flight Center‎

‎M104: The Sombrero Galaxy NASA photograph; LG-2004-6-084-GSFC‎

‎Goddard Space Flight Center: National Astronautics and Space Administration Goddard Space Flight Center 2004. Presumed First Edition First printing this is one of multiple originals issued. Single sheet printed on both sides. Very good. The format is approximately 8 inches by 10 inches. This is a single sheet with printing/imagery on both sides in a plastic sleeve. On the front side is a large color photograph of the Sombrero Galaxy. The other side is in a two-column format. There are several images of the galaxy on the left side. NASA and the Hubble Heritage Team STScl/AURA is credited for this imagery. The text on the back side includes "Hats Off" to the Sombrero Galaxy Vocabulary Fast Facts and Looks are Deceiving. This galaxy's most striking feature is the dust lane that crosses in front of the bulge of the galaxy. This dust lane is actually a symmetrical ring that encloses the bulge of the galaxy. Most of the cold atomic hydrogen gas and the dust lie within this ring. The ring might also contain most of the Sombrero Galaxy's cold molecular gas although this is an inference based on observations with low resolution and weak detections. Additional observations are needed to confirm that the Sombrero galaxy's molecular gas is constrained to the ring. Based on infrared spectroscopy the dust ring is the primary site of star formation within this galaxy. The Sombrero Galaxy also known as Messier Object 104 M104 or NGC 4594 is a peculiar galaxy of unclear classification in the constellation borders of Virgo and Corvus being about 9.55 megaparsecs 31.1 million light-years from the Milky Way galaxy. It is a member of the Virgo II Groups a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster. It has an isophotal diameter of approximately 29.09 to 32.32 kiloparsecs 94900 to 105000 light-years making it slightly bigger in size than the Milky Way. It has a bright nucleus an unusually large central bulge and a prominent dust lane in its outer disk which is viewed almost edge-on. The dark dust lane and the bulge give it the appearance of a sombrero hat thus the name. Astronomers initially thought the halo was small and light indicative of a spiral galaxy; but the Spitzer Space Telescope found that the dust ring was larger and more massive than previously thought indicative of a giant elliptical galaxy. The galaxy has an apparent magnitude of 8.0 making it easily visible with amateur telescopes and is considered by some authors to be the galaxy with the highest absolute magnitude within a radius of 10 megaparsecs of the Milky Way. Its large bulge central supermassive black hole and dust lane all attract the attention of professional astronomers. The Sombrero Galaxy was discovered on May 11 1781 by Pierre Méchain who described the object in a May 1783 letter to J. Bernoulli that was later published in the Berliner Astronomisches Jahrbuch. Charles Messier made a handwritten note about this and five other objects now collectively recognized as M104 - M109 to his personal list of objects now known as the Messier Catalogue but it was not "officially" included until 1921. William Herschel independently discovered the object in 1784 and additionally noted the presence of a "dark stratum" in the galaxy's disc what is now called a dust lane Later astronomers were able to connect Méchain's and Herschel's observations. In 1921 Camille Flammarion found Messier's personal list of the Messier objects including the hand-written notes about the Sombrero Galaxy. This was identified with object 4594 in the New General Catalogue and Flammarion declared that it should be included in the Messier Catalogue. Since this time the Sombrero Galaxy has been known as M104. National Astronautics and Space Administration, Goddard Space Flight Center unknown‎

Bookseller reference : 86152

‎National Aeronautics and Space Administration‎

‎Managing Nasa in the Apollo Era‎

‎Hardcover. NEW/NEW. <br/> <br/> hardcover‎

Bookseller reference : Pazz185844 ISBN : 9798322279514 9798322279

‎National Aeronautics and Space Administration‎

‎Managing Nasa in the Apollo Era‎

‎NEW. unknown‎

Bookseller reference : BIB-NOV-15-2025-100987 ISBN : 9798321793750 9798321793

‎NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WASHINGTON DC‎

‎Manual for Users of the Unitary Plan Wind Tunnel Facilities of the National Advisory Committee for Aeronautics‎

‎PN. New. 1956. Soft Cover. Date is original print. This is a reprint edition. . PN paperback‎

Bookseller reference : 704912

‎National Aeronautics and Space Administration‎

‎Mars as Viewed By Mariner 9: a Pictorial Presentation By the Mariner 9 Television Team and the Planetology Program Principal Investigators‎

‎GPO. Used - Acceptable. Acceptable condition. No Dust Jacket Project Mariner Mars Space Photography A readable intact copy that may have noticeable tears and wear to the spine. All pages of text are present but they may include extensive notes and highlighting or be heavily stained. Includes reading copy only books. Bundled media such as CDs DVDs floppy disks or access codes may not be included. GPO unknown‎

Bookseller reference : SA15A-01046

‎National Aeronautics & Space Administration, Washington, DC. Scientific and Technical Information Office. Fletcher, J. D. C.‎

‎Mars as Viewed by Mariner 9. A Pictorial Presentation by the Mariner 9 Television Team and the Planetology Program Principal Investigators‎

‎Washington NASA SP-329 1974. Hard Cover. 225 p. photos maps. Contents include Foreword by James C. Fletcher; Giant Volcanoes of Mars; Mysterious Canyons; Channels; Fractures and Faults; Escarpments; Fretted and Chaotic Terrains; Craters; Wind-Shaped Features; Extensive Plains; Polar Regions; Clouds of Mars; Natural Satellites; Martian Enigmas; Similarities: Mars Earth and Moon; Shaded Relief Map of Mars. Black cloth stamped in gold; VG. Stock#27167. [Washington] NASA SP-329, 1974 hardcover‎

Bookseller reference : 27167

‎National Aeronautics and Space Administration‎

‎Mars as Viewed by Mariner 9: A Pictorial Presentation by the Mariner 9 Television Team & the Planetology Program. NASA SP-329‎

‎Washington DC: GPO 1976. Revised Edition. very good. Oversized 225 profusely illus. maps. GPO unknown‎

Bookseller reference : 27218

‎National Aeronautics and Space Administration‎

‎Mars Wars: The Rise and Fall of the Space Exploration Initiative‎

‎paperback. Good. Access codes and supplements are not guaranteed with used items. May be an ex-library book. paperback‎

Bookseller reference : 0160831571.G ISBN : 0160831571 9780160831577

‎NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WASHINGTON DC‎

‎Materials for Space Operations‎

‎PN. New. 1962. Soft Cover. Date is original print. This is a reprint edition. . PN paperback‎

Bookseller reference : 718151

‎National Aeronautics and Administration‎

‎Mercury Orbiter: Report of the Science Working Team‎

‎like new. unknown‎

Bookseller reference : 22145807 ISBN : 1502903180 9781502903181

‎National Aeronautics and Administration‎

‎Mercury Orbiter: Report of the Science Working Team‎

‎Paperback / softback. New. paperback‎

Bookseller reference : B9781502903181 ISBN : 1502903180 9781502903181

‎National Astronautics and Space Administration and Jet Propulsion Laboratory‎

‎Meteors and Meteorites NASA Poster; LG-2005-12-571-HQ -- JPL 400-1253J‎

‎Washington DC Pasadena CA: National Astronautics and Space Administration and Jet Propulsion Laboratory 2005. Presumed First Edition First printing. This is one of a presumed number of multiple originals issued. Poster. Very good. The format is approximately 8 inches by 10 inches. This is a single sheet with printing/imagery on both sides in a plastic sleeve. On the front side is a large color photograph of meteor and seven smaller images of meteorites a crater a meteor shower and meteor/meteorite examination. On the reverse there are three columns of text with the lower half of the right column describing the images on the front side. What's that flash of light streaking across the sky We call the objects that creates this brilliant effect by different names depending on where it is. Meteoroids are space rocks that range in size from dust grains to small asteroids. When meteoroids enter Earth's atmosphere or that of another planet at high speed and burn up they're called meteors. When you see lots if meteors you're watching a meteor shower. When a meteoroid survives its trip through the atmosphere and hits the ground it's called a meteorite. Meteorites typically range between the size of a pebble and a fist. Meteoroids are space rocks that range in size from dust grains to small asteroids. This term only applies when these rocks while they are still in space. Most meteoroids are pieces of other larger bodies that have been broken or blasted off. Some come from comets others from asteroids and some even come from the Moon and other planets. Some meteoroids are rocky while others are metallic or combinations of rock and metal. When meteoroids enter Earth's atmosphere or that of another planet at high speed and burn up they're called meteors. This is also when we refer to them as "shooting stars." Sometimes meteors can even appear brighter than Venus - that's when we call them "fireballs." Scientists estimate that about 48.5 tons of meteoritic material falls on Earth each day. Several meteors per hour can usually be seen on any clear night. When there are lots more meteors you're watching a meteor shower. Some meteor showers occur annually or at regular intervals as the Earth passes through the trail of dusty debris left by a comet and in a few cases asteroids. Meteor showers are usually named after a star or constellation that is close to where the meteors appear to originate in the sky. Perhaps the most famous are the Perseids which peak around August 12 every year. Every Perseid meteor is a tiny piece of the comet Swift-Tuttle which swings by the Sun every 135 years. Other notable meteor showers include the Leonids associated with comet Tempel-Tuttle; the Aquarids and Orionids linked to comet Halley and the Taurids associated with comet Encke. Most of this comet debris is between the size of a grain of sand and a pea and burns up in the atmosphere before reaching the ground. Sometimes meteor dust is captured by high-altitude aircraft and analyzed in NASA laboratories.<br /> Early Earth experienced many large meteor impacts that caused extensive destruction. While most craters left by ancient impacts on Earth have been erased by erosion and other geologic processes the Moon's craters are still largely intact and visible. Today we know of about 190 impact craters on Earth. A very large asteroid impact 65 million years ago is thought to have contributed to the extinction of about 75% of marine and land animals on Earth at the time including the dinosaurs. It created the 180-mile-wide Chicxulub Crater on the Yucatan Peninsula. One of the most intact impact craters is the Barringer Meteorite Crater also called Meteor Crater in Arizona. It's about 0.6 miles across and was formed by the impact of a piece of iron-nickel metal approximately 164 feet in diameter. It is only 50000 years old and it is so well preserved that it has been used to study impact processes. Geologists have studied the crater since the 1890s but its status as an impact crater wasn't confirmed until 1960. National Astronautics and Space Administration and Jet Propulsion Laboratory unknown‎

Bookseller reference : 86148

‎National Aeronautics and Space Administration‎

‎Microgravity Science and Applications: Program Tasks and Bibliography for FY 1992. NASA Technical Memorandum 4469‎

‎Washington DC: NASA 1993. good. 376 wraps bibliography stamp on front cover covers somewhat worn and soiled. NASA paperback‎

Bookseller reference : 46710

‎National Aeronautics and Space Administration Goddard Space Flight Center‎

‎Microwave Anisotropy Probe; FS-2001-3-018-GSFC‎

‎Greenbelt MD: National Aeronautics and Space Administration Goddard Space Flight Center 2001. Presumed First Edition First printing. Single sheet stiff card stock printed on both sides. Very good. The format is approximately 8.5 inches by 11 inches. Illustrations some in color on both sides. The WMAP objective was to measure the temperature differences in the Cosmic Microwave Background CMB radiation. The anisotropies then were used to measure the universe's geometry content and evolution; and to test the Big Bang model and the cosmic inflation theory. The mission created a full-sky map of the CMB with a 13 arcminutes resolution via multi-frequency observation. The map required the fewest systematic errors no correlated pixel noise and accurate calibration to ensure angular-scale accuracy greater than its resolution. The map contains 3145728 pixels and uses the HEALPix scheme to pixelize the sphere. The telescope also measured the CMB's E-mode polarization and foreground polarization. Its service life was 27 months; 3 to reach the L2 position and 2 years of observation. The MAP mission was proposed to NASA in 1995 selected for definition study in 1996 and approved for development in 1997. The WMAP was preceded by two missions to observe the CMB; i the Soviet RELIKT-1 that reported the upper-limit measurements of CMB anisotropies and ii the U.S. COBE satellite that first reported large-scale CMB fluctuations. The WMAP was 45 times more sensitive with 33 times the angular resolution of its COBE satellite predecessor. The European Planck mission operational 2009–2013 had a higher resolution and higher sensitivity than WMAP and observed in 9 frequency bands rather than WMAP's 5 allowing improved astrophysical foreground models. The Wilkinson Microwave Anisotropy Probe WMAP originally known as the Microwave Anisotropy Probe MAP and Explorer 80 was a NASA spacecraft operating from 2001 to 2010 which measured temperature differences across the sky in the cosmic microwave background CMB – the radiant heat remaining from the Big Bang. Headed by Professor Charles L. Bennett of Johns Hopkins University the mission was developed in a joint partnership between the NASA Goddard Space Flight Center and Princeton University. The WMAP spacecraft was launched on 30 June 2001 from Florida. The WMAP mission succeeded the COBE space mission and was the second medium-class MIDEX spacecraft in the NASA Explorer program. In 2003 MAP was renamed WMAP in honor of cosmologist David Todd Wilkinson 1935–2002 who had been a member of the mission's science team. After nine years of operations WMAP was switched off in 2010 following the launch of the more advanced Planck spacecraft by European Space Agency ESA in 2009. WMAP's measurements played a key role in establishing the current Standard Model of Cosmology: the Lambda-CDM model. The WMAP data are very well fit by a universe that is dominated by dark energy in the form of a cosmological constant. Other cosmological data are also consistent and together tightly constrain the Model. In the Lambda-CDM model of the universe the age of the universe is 13.772±0.059 billion years. The WMAP mission's determination of the age of the universe is to better than 1% precision. The current expansion rate of the universe is see Hubble constant 69.32±0.80 km·s 1·Mpc 1. The content of the universe currently consists of 4.628%±0.093% ordinary baryonic matter; 24.02%0.88% 0.87% cold dark matter CDM that neither emits nor absorbs light; and 71.35%0.95%<br /> 0.96% of dark energy in the form of a cosmological constant that accelerates the expansion of the universe. Less than 1% of the current content of the universe is in neutrinos but WMAP's measurements have found for the first time in 2008 that the data prefer the existence of a cosmic neutrino background with an effective number of neutrino species of 3.26±0.35. The contents point to a Euclidean flat geometry with curvature kdisplaystyle Omega _k of 0.00270.0039 0.0038. The WMAP measurements also support the cosmic inflation paradigm in several ways including the flatness measurement. The mission has won various awards: according to Science magazine the WMAP was the Breakthrough of the Year for 2003. This mission's results papers were first and second in the "Super Hot Papers in Science Since 2003" list. Of the all-time most referenced papers in physics and astronomy in the INSPIRE-HEP database only three have been published since 2000 and all three are WMAP publications. Bennett Lyman A. Page Jr. and David N. Spergel the latter both of Princeton University shared the 2010 Shaw Prize in astronomy for their work on WMAP. Bennett and the WMAP science team were awarded the 2012 Gruber Prize in cosmology. The 2018 Breakthrough Prize in Fundamental Physics was awarded to Bennett Gary Hinshaw Norman Jarosik Page Spergel and the WMAP science team. In October 2010 the WMAP spacecraft was derelict in a heliocentric graveyard orbit after completing nine years of operations. All WMAP data are released to the public and have been subject to careful scrutiny. The final official data release was the nine-year release in 2012. Some aspects of the data are statistically unusual for the Standard Model of Cosmology. For example the largest angular-scale measurement the quadrupole moment is somewhat smaller than the Model would predict but this discrepancy is not highly significant. A large cold spot and other features of the data are more statistically significant and research continues into these. National Aeronautics and Space Administration, Goddard Space Flight Center unknown‎

Bookseller reference : 86101

‎National Aeronautics and Administration‎

‎Middle Atmosphere Program - Handbook for MAP: Volume 15‎

‎like new. unknown‎

Bookseller reference : 21348629 ISBN : 1497451000 9781497451001

‎National Aeronautics and Administration‎

‎Middle Atmosphere Program - Handbook for Map: Volume 6‎

‎Paperback / softback. New. paperback‎

Bookseller reference : A9781497482982 ISBN : 1497482984 9781497482982