Global Change Master Directorygsfc-gcmduso@mail.nasa.gov502013-05-19T05:47:06Zesip Search: Parameters|SUN-EARTH INTERACTIONShttp://mddemo.gsfc.nasa.gov/KeywordSearch/OpenSearch.do 91 0 http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_OML1BIRR_V003OMI/Aura Level 1B Solar Irradiances V003 (OML1BIRR) at GES DISC-180.0,-90.0,180.0,90.02004-10-01T00:00:00ZT00:00:00Z2013-04-29T04:00:00ZThe Level-1B (L1B) Radiance Product OML1BIRR (Version-3) from the Aura-OMI is now available (http://disc.gsfc.nasa.gov/Aura/OMI/oml1birr_v003.shtml) to public from the NASA GSFC Earth Sciences Data ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_SOR3SOLFUVD_V012SORCE SOLSTICE FUV Level 3 Solar Spectral Irradiance Daily Means V012 SOR3SOLFUVD at GES DISC-180.0,-90.0,180.0,90.02003-05-14T00:00:00ZT00:00:00Z2012-10-09T04:00:00ZThe SORCE SOLSTICE Far-UV Solar Spectral Irradiance (SSI) data product SOR3SOLFUVD is constructed using measurements from the SOLSTICE FUV instrument, which are combined into merged daily solar spectra ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_SOR3SOLMUVD_V012SORCE SOLSTICE MUV Level 3 Solar Spectral Irradiance Daily Means V012 SOR3SOLMUVD at GES DISC-180.0,-90.0,180.0,90.02003-05-14T00:00:00ZT00:00:00Z2012-10-09T04:00:00ZThe SORCE SOLSTICE Mid-UV Solar Spectral Irradiance (SSI) data product SOR3SOLMUVD is constructed using measurements from the SOLSTICE MUV instrument, which are combined into merged daily solar spectra ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]ucar.scd.vets.vg.smeSolar Magnetic Eruption Disturbances2012-07-10T04:00:00ZSolar Magnetic Eruptions (SME), such as Coronal Mass Ejections and Solar
Flares, and their impact on Earth's space environment are the target of this
Space Weather research.Solar Magnetic Eruptions ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_SOR3TSI6_V013SORCE Level 3 Total Solar Irradiance 6-Hour Means V013 SOR3TSI6 at GES DISC-180.0,-90.0,180.0,90.02003-02-25T00:00:00ZT00:00:00Z2012-07-06T04:00:00ZThe Total Solar Irradiance (TSI) data set SOR3TSI6 contains the total solar irradiance (a.k.a solar constant) data collected by the Total Irradiance Monitor (TIM) instrument covering the full wavelength ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_SOR3TSID_V013SORCE Level 3 Total Solar Irradiance Daily Means V013 SOR3TSID at GES DISC-180.0,-90.0,180.0,90.02003-02-25T00:00:00ZT00:00:00Z2012-07-06T04:00:00ZThe Total Solar Irradiance (TSI) data set SOR3TSID contains the total solar irradiance (a.k.a solar constant) data collected by the Total Irradiance Monitor (TIM) instrument covering the full wavelength ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]NCL00121_122Daily, Monthly, Seasonal and Annual Climatic Data, Including Temperature and Wind Data for the Sachsen Region of Germany (1864-1890)5.0,45.0,15.0,55.01864-01-01T00:00:00Z1890-12-31T00:00:00Z2012-02-23T05:00:00ZClimatic data resides in 2 books, 'Das Klima des Konigreiches Sachsen'
(C/dc 320 L-wk), and 'Die Hauptsachlichsten Resultate aus den m den
Jahren 1864-1900 im Konigreich Sachsen Anstellten Meteorologischen ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]NCL00189_195Hourly, Daily, Monthly, and Yearly Surface Weather Data for Teddington and Richmond (Kew Observatory) England (1885-1910)-1.0,51.0,0.0,54.01885-01-01T00:00:00Z1910-12-31T00:00:00Z2012-02-23T05:00:00ZThe Teddington surface data resides in 2 books, 'Teddington, England, National
Physical Laboratory Report (1901-1910)' (C/de35 A1). Data contained in these
books are tables of hourly, daily, monthly ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]NCL00103_111_232_235Thunderstorms and Rainfall in Bayern, Germany and its High Altitude Regions (1833-1925), and Daily/Monthly Precipitation for Bayern (1891-1933)5.0,45.0,15.0,55.01833-01-01T00:00:00Z1933-12-31T00:00:00Z2012-02-23T05:00:00ZThe thunderstorm data resides in 1 book, 'Ueber Zundende Blitze im
Kongreich Bayern Wahrend Des Zeitraumes 1833 bis 1882' (C/dc 161 B)
written in German. The data contained in this book are tables ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]SDO_DIF_PLACEHOLDERNASA Solar Dynamics Observatory (SDO) Science Data Products2012-02-01T05:00:00Z[Text Source: The Solar Dynamics Observatory (SDO) Project Home page, http://sdo.gsfc.nasa.gov/mission/about.php ]
SDO: The Solar Dynamics Observatory is the first ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]SORCE_XPSSORCE Extreme Ultraviolet (XUV) Data from the XPS2003-02-25T00:00:00ZT00:00:00Z2012-02-01T05:00:00ZThis data set consists of SORCE Extreme Ultraviolet (XUV) data from the XPS
instrument on-board the SORCE spacecraft. The XPS instrument has 12 photodiodes
for measuring XUV and EUV irradiance. 7 ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]TIMED_SEESolar EUV Experiment (SEE) Data from the Thermosphere, Ionosphere, Mesosphere Energetics and Dynamics (TIMED) Mission2002-02-17T00:00:00ZT00:00:00Z2012-02-01T05:00:00ZThe Solar EUV Experiment (SEE) is one of four instruments that
constitute the TIMED spacecraft, the first mission of the NASA Solar
Connections program.
All SEE data products ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]SNOEThe Student Nitric Oxide Explorer (SNOE) Data Archive at LASP and NSSDC-180.0,-90.0,180.0,90.01998-03-11T00:00:00Z2003-09-30T00:00:00Z2012-02-01T05:00:00ZThe Student Nitric Oxide Explorer (SNOE or "snowy") is a small scientific
satellite that measured the effects of energy from the sun and from the
magnetosphere on the density of nitric ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]BOREAS_ECMWFBOREAS ECMWF 6-HOUR ANALYSIS AND FORECAST DATA-114.0,48.0,-92.0,62.01994-01-01T00:00:00Z1996-12-31T00:00:00Z2011-12-19T05:00:00ZIn cooperation with BOREAS atmospheric research efforts, the ECMWF agreed to provide BOREAS with a customized subset of its 6-hourly forecast data. This data set contains parameters from three ECMWF ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.class.GOME_L2Global Ozone Monitoring Experiment-2 (GOME-2) Total Ozone Level 2 Granules-180.0,-90.0,180.0,90.02007-10-01T00:00:00ZT00:00:00Z2011-11-29T05:00:00ZABSTRACT: The GOME-2 total ozone retrieval algorithm is based on OMI/TOMS (Ozone Monitoring Instrument / Total Ozone Mapping Spectrometer) V8 algorithm, which is a three-step process of successive ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_SOR3SIMD_V017SORCE SIM Level 3 Solar Spectral Irradiance Daily Means V017 SOR3SIMD at GES DISC-180.0,-90.0,180.0,90.02004-04-21T00:00:00ZT00:00:00Z2011-11-29T05:00:00ZThe SORCE SIM Solar Spectral Irradiance (SSI) data product SOR3SIMD is constructed using measurements from the SIM instruments, which are combined into merged daily solar spectra over the spectral ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_SOR3XPS6_V010SORCE XPS Level 3 Solar Spectral Irradiance 6-Hour Means V010 SOR3XPS6 at GES DISC-180.0,-90.0,180.0,90.02003-02-10T00:00:00ZT00:00:00Z2011-11-29T05:00:00ZThe SORCE XUV Photometer System (XPS) Solar Spectral Irradiance (SSI) 6-Hour Data Product SOR3XPS6 contains solar XUV irradiances in the 0.1 to 27 nm range, as well as Lyman-alpha, in broad bands ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_SOR3XPSD_V010SORCE XPS Level 3 Solar Spectral Irradiance Daily Means V010 SOR3XPSD at GES DISC-180.0,-90.0,180.0,90.02003-02-10T00:00:00ZT00:00:00Z2011-11-29T05:00:00ZThe SORCE XUV Photometer System (XPS) Solar Spectral Irradiance (SSI) Daily Data Product SOR3XPSD contains solar XUV irradiances in the 0.1 to 27 nm range, as well as Lyman-alpha, in broad bands (7-10 ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.class.GOMEMGIIGOME-2 Magnesium II Index-80.0,-90.0,180.0,90.02007-10-01T00:00:00ZT00:00:00Z2011-11-03T04:00:00ZABSTRACT: The Magnesium II information is extracted daily from the GOME-2 1B granules, as soon as new solar radiance measurements are available. The product includes a 61-wavelength subset of the ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.class.CORSNOAA CLASS archive: Continuously Operating Reference Stations (CORS)-180.0,-90.0,180.0,90.02010-10-01T00:00:00ZT00:00:00Z2011-11-02T04:00:00ZABSTRACT: The National Geodetic Survey (NGS), an office of NOAA's National Ocean Service (NOS), coordinates a network of geodetic-quality CORS stations that provide Global Positioning System (GPS) ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]ATMOS_SPACELAB3Atmospheric Trace Molecule Spectroscopy (ATMOS) Data From Spacelab-3-180.0,26.0,180.0,34.01985-04-29T00:00:00Z1985-05-05T00:00:00Z2011-07-29T04:00:00ZThe Atmospheric Trace Molecule Spectroscopy (ATMOS) experiment was flown on the Space Shuttle STS-51B as part of the Spacelab-3 laboratory to demonstrate the capability to monitor environmental quality ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]gov.noaa.ncdc.C00542U.S. Integrated Surface Irradiance Study (ISIS) Level 1 - 15 Minute Values and Statistics (DSI-9870)-123.0,30.0,-77.0,48.01995-01-01T00:00:00ZT00:00:00Z2011-07-21T04:00:00ZU.S. Integrated Surface Irradiance Study (ISIS) Level 1 - 15 Minute Values and Statistics is digital data set DSI-9870, archived at the National Climatic Data Center (NCDC).ISIS is a continuation ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]gov.noaa.ncdc.C00541U.S. Integrated Surface Irradiance Study (ISIS) Level 1 - Hourly Values (DSI-9871)-122.3,30.4,-77.7,47.51995-01-01T00:00:00ZT00:00:00Z2011-07-21T04:00:00ZU.S. Integrated Surface Irradiance Study (ISIS) Level 1 - Hourly Values is digital data set DSI-9871, archived at the National Climatic Data Center (NCDC).ISIS is a continuation of earlier National ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]gov.noaa.ncdc.C00540U.S. Integrated Surface Irradiance Study (ISIS) Level 2 (SURFRAD) (DSI-9872)-120.0,30.0,-74.0,49.01995-01-01T00:00:00ZT00:00:00Z2011-07-21T04:00:00ZU.S. Integrated Surface Irradiance Study (ISIS) Level 2 (SURFRAD) is digital
data set DSI-9872, archived at the National Climatic Data Center (NCDC).ISIS is a continuation
...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G01257Ionospheric Digital Database-180.0,-90.0,180.0,90.01957-01-01T00:00:00Z1990-01-01T00:00:00Z2011-04-19T04:00:00ZABSTRACT: The ionosphere is that part of the Earth's atmosphere that results mainly from the photo ionization of the upper atmosphere. Traditionally, the following ionospheric regions and their approximate ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G01119DMSP OLS - Operational Linescan System-180.0,-90.0,180.0,90.01975-04-01T00:00:00ZT00:00:00Z2011-03-10T05:00:00ZABSTRACT: Visible and infrared imagery from DMSP Operational Linescan System (OLS) instruments are used to monitor the global distribution of clouds and cloud top temperatures twice each day. The ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G01127DMSP SSIES - Ion Electron Scintillation Monitor-180.0,-90.0,180.0,90.01975-04-01T00:00:00ZT00:00:00Z2011-03-10T05:00:00ZABSTRACT: The SSIES measures the ambient electron density and temperatures, ambient ion density, the average ion temperature and molecular weight, the plasma drift and scintillation at the DMSP orbital ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G01122Information About Low Energy Particles That Cause the Aurora and Other High Latitude Phenomena-180.0,-90.0,180.0,90.01974-04-01T00:00:00ZT00:00:00Z2011-03-10T05:00:00ZABSTRACT: DMSP SSJ/4 data provide a complete energy spectrum of the low energy particles that cause the aurora and other high latitude phenomena. The data set consists of electron and ion particle ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00603Airglow Data-180.0,-90.0,180.0,90.01972-01-01T00:00:00ZT00:00:00Z2011-03-07T05:00:00ZABSTRACT: Airglow is a faint luminescence of the earth's upper atmosphere. The emitted electromagnetic radiation results mainly from photo-chemical reactions of upper atmospheric constituents. Although ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00599Measurement of the Low-Energy Portion of the Primary Cosmic Ray Spectrum-180.0,-90.0,180.0,90.01953-01-01T00:00:00ZT00:00:00Z2011-03-07T05:00:00ZABSTRACT: Most cosmic rays come from the galaxy, though some are produced by eruptive events on the Sun's surface. These high energy cosmic ray particles can affect satellites, causing single event ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00581Sudden Ionospheric Disturbances (SID)-180.0,-90.0,180.0,90.01958-01-01T00:00:00ZT00:00:00Z2011-03-07T05:00:00ZABSTRACT: Sudden ionospheric disturbances (SID) are caused by solar flare enhanced X-rays in the 1 to 10 angstrom range. Solar flares can produce large increases of ionization in the D-region of the ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00543Energetic Solar Protons and Electrons - Data from GOES Satellites-180.0,-90.0,180.0,90.01974-07-01T00:00:00Z1984-08-21T00:00:00Z2011-03-03T05:00:00ZABSTRACT: The Space Environment Monitor (SEM) instrument package on-board all GOES satellites has provided magnetometer, energetic particle, and soft X-ray data continuously since July 1974. Usually ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00563Ionospheric Oblique Incidence Soundings by Satellites-180.0,-90.0,180.0,90.01957-01-15T00:00:00Z1975-01-01T00:00:00Z2011-03-03T05:00:00ZABSTRACT: The oblique incidence sweep-frequency ionospheric sounding technique uses the same principle of operation as the vertical incidence sounder. The primary difference is that the transmitter ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00556Ionospheric Values (Daily Work Sheets), F-Plots, Tabulations, Booklets, Catalogs, and Log Books-180.0,-90.0,180.0,90.01944-03-01T00:00:00ZT00:00:00Z2011-03-03T05:00:00ZABSTRACT: These ionospheric data consist of scaling notes, equipment usage logs, and ionospheric values in the form of daily work sheets, F-Plots, tabulations, and booklets. The station notes list ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00569Measurements of the Absorptive Properties of the Ionosphere-180.0,-90.0,180.0,90.01963-01-01T00:00:00Z1990-12-31T00:00:00Z2011-03-03T05:00:00ZABSTRACT: Absorption of radio waves occurs when electrons responding to the wave fields collide with and transfer energy to the neutral particles. A study of ionospheric absorption yields information ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00551Photographic Records Showing the Variations of the Virtual Height of Reflection as a Function of the Radio Frequency-180.0,-90.0,180.0,90.01944-03-01T00:00:00ZT00:00:00Z2011-03-03T05:00:00ZABSTRACT: The standard (analog) ionosonde produces photographic records known as ionograms, which show the variations of the virtual height of reflection as a function of the radio frequency. The ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00533Solar Magnetic Field-180.0,-90.0,180.0,90.01931-01-01T00:00:00ZT00:00:00Z2011-03-03T05:00:00ZABSTRACT: The solar magnetic field is approximately a dipole at high latitudes and is highly irregular at middle and low latitudes. The field apparently gives rise to a coupling between solar differential ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00594Aurorae Data-180.0,-90.0,180.0,90.01957-01-01T00:00:00Z1984-11-20T00:00:00Z2011-03-02T05:00:00ZABSTRACT: An aurora involves emitted electromagnetic radiation that results primarily from the interaction of energetic, extra-atmospheric particles with the neutral gases of the upper atmosphere. ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00546Radio Emissions from Jupiter-180.0,-90.0,180.0,90.01966-07-01T00:00:00Z1979-08-01T00:00:00Z2011-03-02T05:00:00ZABSTRACT: The National Geophysical Data Center holds a published series of observations of Jovian Dekametric Emission bursts recorded on the University of Colorado's Boulder radio spectrograph. Between ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00582Satellite Environment-180.0,-90.0,180.0,90.01967-01-01T00:00:00ZT00:00:00Z2011-03-02T05:00:00ZABSTRACT: Satellites monitor in situ the effect of the Sun on the near-Earth environment. The GOES and SOLRAD satellites orbited at geostationary levels, about 22,000 miles above the Earth's surface. ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00538Solar Corona-180.0,-90.0,180.0,90.01939-01-01T00:00:00ZT00:00:00Z2011-03-02T05:00:00ZABSTRACT: The solar corona is the outermost layer of the sun's atmosphere--a very hot halo (millions of degrees), that, in the form of the solar wind, extends well past the Earth's orbit. The corona ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00547Solar Irradiance-180.0,-90.0,180.0,90.01978-08-01T00:00:00ZT00:00:00Z2011-03-02T05:00:00ZABSTRACT: The "solar constant" is, in fact, not constant. Recent satellite observations have found that the Total Solar Irradiance (TSI), the amount of solar radiation received at the top of the Earth's ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00534Solar Prominences and Filaments-180.0,-90.0,180.0,90.01919-03-01T00:00:00ZT00:00:00Z2011-03-02T05:00:00ZABSTRACT: Solar Prominences and Filaments appear as dark filamentary objects on the solar disk (filaments) and as protuberances on the edge of the solar disk (prominences). They generally sit above ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00542Solar Ultraviolet Data-180.0,-90.0,180.0,90.01978-11-01T00:00:00ZT00:00:00Z2011-03-02T05:00:00ZABSTRACT: The ultraviolet (UV) part of the electromagnetic spectrum ranges between 5 and 400 nanometers (nm). As the SORCE (Solar Radiation and Climate Experiment satellite) mission states, far UV ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00532Sunspot Numbers-180.0,-90.0,180.0,90.01700-01-01T00:00:00ZT00:00:00Z2011-03-02T05:00:00ZABSTRACT: In 1848 the Swiss astronomer Johann Rudolph Wolf introduced a daily measurement of sunspot number. His method, which is still used today, counts the total number of spots visible on the ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00146Electron Density Profile Data Contains Virtual Height/Frequency Pairs from a Profile or Profiles (Composite Months) of Ionograms-180.0,-90.0,180.0,90.01954-12-15T00:00:00Z1993-12-31T00:00:00Z2011-03-01T05:00:00ZABSTRACT: The Electron Density Profile, N(h), data set contains both individual profiles and composite months. The data consist of virtual height/frequency pairs from a profile or profiles (composite ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00145Measurement of Incoherent Scatter-180.0,-90.0,180.0,90.01965-11-15T00:00:00Z1977-12-15T00:00:00Z2011-03-01T05:00:00ZABSTRACT: For radio waves transmitted through the ionosphere with frequencies much larger (50 to 1300MHz) than the plasma frequency (up to 15MHz), very small-scale fluctuations of electron density ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00188POES Space Environment Monitor, Energetic Particles-180.0,-90.0,180.0,90.01978-11-01T00:00:00ZT00:00:00Z2011-03-01T05:00:00ZABSTRACT: The TIROS/NOAA satellite series, also known as POES, is designed to meet the National Oceanic and Atmospheric Administration's need for operational, remote sensing products for numerical ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00216Solar Radio Data-180.0,-90.0,180.0,90.01947-02-14T00:00:00ZT00:00:00Z2011-03-01T05:00:00ZABSTRACT: Scientists monitor the structure of the solar corona, the outer most regions of the Sun's atmosphere, using radio waves. The surface of the Sun is 6,000 degrees Kelvin, while the high corona ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00015DMSP SSJ/4 - Precipatating Electron and Ion Spectrometer-180.0,-90.0,180.0,90.01973-01-01T00:00:00Z1992-12-31T00:00:00Z2011-02-28T05:00:00ZABSTRACT: DMSP SSJ/4 data provide a complete energy spectrum of the low energy particles that cause the aurora and other high atitude phenomena. The data set consists of electron and ion particle ...