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1. Ulysses Heliospheric Data [ULYSSES]
The primary mission of the Ulysses spacecraft was to characterize the heliosphere as a function of solar latitude. The periods of primary scientific interest is when Ulysses was at or higher than ...


2. Interplanetary Monitoring Platform (IMP-8) Cosmic Ray Nuclear Composition (CRNC) Data [IMP8_UNH]
IMP-8 (IMP-J) was launched by NASA on October 26, 1973 to measure the magnetic fields, plasmas, and energetic charged particles (e.g., cosmic rays) of the Earth's magnetotail and magnetosheath and ...


3. The Student Nitric Oxide Explorer (SNOE) Data Archive at LASP and NSSDC [SNOE]
The 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 oxide in the ...


4. Solar Images and Spectra from the Yohkoh Spacecraft [Yohkoh-01]
This data set consists of data from all four instruments on board the Yohkoh spacecraft (formerly called Solar-A). Data are held as proprietary for two years after collection (although more recent ...


5. 3-D Plasma and Energetic Particle Investigation on WIND [WIND_3DP]
The main purpose of the Wind spacecraft is to measure the incoming solar wind, magnetic fields and particles, although early on it will also observe the Earth's foreshock region. Wind, together with ...


6. Energetic Particles: Acceleration, Composition and Transport (EPACT) Investigation on WIND [WIND_EPACT]
The main purpose of the Wind spacecraft is to measure the incoming solar wind, magnetic fields and particles, although early on it will also observe the Earth's foreshock region. Wind, together with ...


7. Fields and Particles Data from Explorers 33 and 35 [66-058A]
The Explorer 33 and 35 spacecraft, also referred to as Anchored IMP (AIMP) 1 and 2, were launched in 1966 and 1967 towards lunar-centric orbits. Explorer 35 achieved a 5 Rm lunar orbit, but Explorer ...


8. Gamma Ray Burst Detector (KONUS) on WIND [WIND_KONUS]
The main purpose of the Wind spacecraft is to measure the incoming solar wind, magnetic fields and particles, although early on it will also observe the Earth's foreshock region. Wind, together with ...


9. General Access to GRO/BATSE Solar Database Maintained at NASA/GSFC [GRO_BATSE_SOLAR_DB]
For the use of the solar physics and astronomy communities, a system that is available on-line for quick-look access to the solar flare data from the Gamma-Ray Observatory (GRO) has been established. ...


10. Geotail Data Archive at NASA/GSFC [NASA_GEOTAIL]
The GEOTAIL mission is a collaborative project undertaken by the Institute of Space and Astronautical Science (ISAS) and the National Aeronautics and Space Administration (NASA). Its primary objective ...


11. Interplanetary Monitoring Platform (IMP-8) Charged Particle Measurement Experiment (CPME) Data [IMP8_JHUCPME]
IMP-8 (IMP-J) was launched by NASA on October 26, 1973 to measure the magnetic fields, plasmas, and energetic charged particles (e.g., cosmic rays) of the Earth's magnetotail and magnetosheath and ...


12. Interplanetary Monitoring Platform (IMP-8) Electrostatic Energy-Charge Analyzer (EECA) Data [IMP8_UMD]
IMP-8 (IMP-J) was launched by NASA on October 26, 1973 to measure the magnetic fields, plasmas, and energetic charged particles (e.g., cosmic rays) of the Earth's magnetotail and magnetosheath ...


13. Interplanetary Monitoring Platform (IMP-8) Energetic Particle Experiment (EPE) Data [IMP8_JHUEPE]
IMP-8 (IMP-J) was launched by NASA on October 26, 1973 to measure the magnetic fields, plasmas, and energetic charged particles (e.g., cosmic rays) of the Earth's magnetotail and magnetosheath and ...


14. Interplanetary Monitoring Platform (IMP-8) Goddard Medium Energy (GME) Experiment Data [IMP8_GSFC]
IMP-8 (IMP-J) was launched by NASA on October 26, 1973 to measure the magnetic fields, plasmas, and energetic charged particles (e.g., cosmic rays) of the Earth's magnetotail and magnetosheath and ...


15. Interplanetary Monitoring Platform (IMP-8) Low-Energy Proton and Electron Differential Energy Analyzer (LEPEDEA) Data [IMP8_IOWA]
IMP-8 (IMP-J) was launched by NASA on October 26, 1973 to measure the magnetic fields, plasmas, and energetic charged particles (e.g., cosmic rays) of the Earth's magnetotail and magnetosheath and ...


16. Interplanetary Monitoring Platform (IMP-8) Magnetometer Experiment Data [IMP8_MAG]
IMP-8 (IMP-J) was launched by NASA on October 26, 1973 to measure the magnetic fields, plasmas, and energetic charged particles (e.g., cosmic rays) of the Earth's magnetotail and ...


17. Interplanetary Monitoring Platform (IMP-8) Solar Plasma Electrostatic Analyzer Data [IMP8_LANL]
IMP-8 (IMP-J) was launched by NASA on October 26, 1973 to measure the magnetic fields, plasmas, and energetic charged particles (e.g., cosmic rays) of the Earth's magnetotail ...


18. Interplanetary Monitoring Platform (IMP-8) Solar Plasma Faraday Cup Data [IMP8_MIT]
IMP-8 (IMP-J) was launched by NASA on October 26, 1973 to measure the magnetic fields, plasmas, and energetic charged particles (e.g., cosmic rays) of the Earth's magnetotail and magnetosheath and ...


19. Magnetic Field Investigation (MFI) on WIND [WIND_MFI]
The main purpose of the Wind spacecraft is to measure the incoming solar wind, magnetic fields and particles, although early on it will also observe the Earth's foreshock region. Wind, together with ...


20. NASA STEREO (Solar TErrestrial RElations Observatory) Data Products [NASA_STEREO_DATA_PLACEHOLDER]
[Source: NASA/GSFC Solar TErrestrial RElations Observatory (STEREO) home page, http://stereo.gsfc.nasa.gov/ ] STEREO (Solar ...


21. NASA Solar Dynamics Observatory (SDO) Science Data Products [SDO_DIF_PLACEHOLDER]
[Text Source: The Solar Dynamics Observatory (SDO) Project Home page, http://sdo.gsfc.nasa.gov/ ] SDO: The Solar Dynamics Observatory is the first mission to be launched for NASA's ...


22. Polar Sun-Earth Connection Mission Data Archive at NASA/GSFC [NASA_POLAR]
The Polar spacecraft was launched on February 24, 1996, to obtain data from both high- and low-altitude perspectives of this active region of geospace. High above the poles the particles of the solar ...


23. RHESSI Solar Flare Data: Light Curves, Spectra, and Images [RHESSI]
The primary mission of the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) is to explore the basic physics of particle acceleration and energy release in solar flares. RHESSI consists ...


24. Radio and Plasma Wave Investigation (WAVES) on WIND [WIND_WAVES]
The main purpose of the Wind spacecraft is to measure the incoming solar wind, magnetic fields and particles, although early on it will also observe the Earth's foreshock region. Wind, together with ...


25. SOHO/Charge, Element, and Isotope Analysis System (CELIAS) Data Archive [SOHO_CELIAS]
The CELIAS instrument is designed to study the composition of the solar wind (SW) and of solar and interplanetary energetic particles on SOHO. SOHO is a project of international cooperation between ...


26. SOHO/Comprehensive Suprathermal and Energetic Particle Analyzer (COSTEP) Data Archive [SOHO_COSTEP]
COSTEP addresses scientific objectives related to the following phenomena: * Steady state processes in the solar atmosphere * Energy release and particle acceleration in the solar atmosphere ...


27. SOHO/Coronal Diagnostics Spectrometer (CDS) Data Archive [SOHO_CDS]
The Coronal Diagnostics Spectrometer (CDS) onboard SOHO studies the emission line characteristics in the extreme ultraviolet (EUV) of the Sun. CDS observes the Sun's coronal properties and its interaction ...


28. SOHO/Energetic and Relativistic Nuclei and Electron (ERNE) Data Archive [SOHO_ERNE]
The Energetic and Relativistic Nuclei and Electron (ERNE) Sensor Unit (ESU) has two energetic particle sensors: LED and HED. ERNE will investigate the solar atmosphere by detecting charged particles ...


29. SOHO/Extreme Ultraviolet Imaging Telescope (EIT) Data Archive [SOHO_EIT]
The Extreme Ultraviolet Imaging Telescope (EIT) onboard the SOHO spacecraft observes the Sun over a 45 x 45 arcminute field of view in four emission line groups: FE IX, FE X, FE III, FE XV, and HE ...


30. SOHO/Global Oscillations at Low Frequencies (GOLF) Data Archive [SOHO_GOLF]
The GOLF experiment on the SOHO mission aims to study the internal structure of the sun by measuring the spectrum of global oscillations in the frequency range 10**-7 to 10**-2 Hz. Both p and g mode ...


31. SOHO/Large Angle and Spectrometric Coronagraph Experiment (LASCO) Data Archive [SOHO_LASCO]
The Large Angle and Spectrometric COronagraph (LASCO) instrument is one of 11 instruments included on the joint NASA/ESA SOHO (Solar and Heliospheric Observatory) spacecraft. The LASCO instrument ...


32. SOHO/Michelson Doppler Imager (MDI) and Solar Oscillations Investigation (SOI) Data Archive [SOHO_MDI_SOI]
MDI is a project of the Stanford-Lockheed Institute for Space Research and is a joint effort of the Solar Oscillations Investigation (SOI) in the W.W. Hansen Experimental Physics Laboratory of Stanford ...


33. SOHO/Solar Ultraviolet Measurements of Emitted Radiation (SUMER) Data Archive [SOHO_SUMER]
The Solar Ultraviolet Measurements of Emitted Radiation (SUMER) is a UV telescope and spectrometer that was designed and built at the Max-Planck-Institut fur Aeronomie (MPAe) with international ...


34. SOHO/Solar Wind Anisotropies (SWAN) Data Archive [SOHO_SWAN]
The SWAN (Solar Wind ANisotropies) instrument is one of twelve instruments onboard SOHO (SOlar Heliospheric Observatory) satellite. It is a collaboration between Finnish Meteorological Institute and ...


35. SOHO/UltraViolet Coronograph Spectrometer (UVCS) Data Archive [SOHO_UVCS]
The purpose of the UltraViolet Coronograph Spectrometer (UVCS) on the Solar and Heliospheric Observatory (SOHO) is to provide a detailed description of the extended solar corona that can be used to ...


36. SOHO/Variability of Solar Irradiance and Gravity Oscillations (VIRGO) Data Archive [SOHO_VIRGO]
The VIRGO Experiment on the ESA/NASA SOHO Mission has three types of instruments to measure total solar irradiance (TSI) with the absolute radiometers DIARAD and PMO6V, spectral solar irradiance at ...


37. Solar Images and Spectra from the Solar Maximum Mission (SMM) X-ray Polychromator [SMM-07]
Data from the X-ray Polychromator (XRP) consist of photon counting rates at selected X-ray wavelengths in the 1.4 - 22.5 A band from detectors which are used in a variety of modes to build up solar ...


38. Solar Images from the EUV and Soft X-ray Spectroheliographs on OSO-7 [71-083-01]
Two of the six instruments on board the OSO-7 were an EUV spectroheliograph (Neupert, Thames, and Chapman 1974) and a Hard X-ray Spectrometer (Datlowe, Elcan, and Hudson 1974). The spectroheliograph ...


39. Solar Maximum Mission (SMM) Coronagraph/Polarimeter Data [SMM-01]
The data from the Coronagraph/Polarimeter consist of digital images of the solar corona taken through various filters at visible wavelengths. The scientific objectives of the Coronagraph/Polarimeter ...


40. Solar Radio Observations from Space [SRO-01]
Many spacecraft were launched from 1962 thru 1973 to record solar and cosmic radio bursts. The spacecraft carried receivers for various frequency ranges, and collected data intermittently over those ...


41. Solar Ultraviolet Data from Orbiting Solar Observatory (OSO) Space Missions 1962 - 1978 [OSO-02]
The Orbiting Solar Observatory (OSO) series 1 & 3 - 8 collected solar UV data in the years 1962 - 1978. Many instruments were used to observe in various wavelength bands, tabulated below. The data ...


42. Solar Ultraviolet Observations from the Solar Maximum Mission/ Ultraviolet Spectrometer and Polarimeter (SMM/UVSP) [SMM-06]
Data from the Ultraviolet Spectrometer and Polarimeter (UVSP) consist of photon counts at selected UV wavelengths in the 1170 - 3500 A band from detectors which are used in a variety of modes to build ...


43. Solar Wind Experiment (SWE) on WIND [WIND_SWE]
The main purpose of the Wind spacecraft is to measure the incoming solar wind, magnetic fields and particles, although early on it will also observe the Earth's foreshock region. Wind, together with ...


44. Solar X-ray Data from Orbiting Solar Observatory (OSO) Space Missions 1962 - 1978 [OSO-01]
The Orbiting Solar Observatory (OSO) series 1 - 8 collected solar X-ray data in the years 1962 - 1978. Many instruments were used to observe in various photon energy ranges, tabulated below. The ...


45. Solar X-ray and Ultraviolet Data from SOLRAD Space Missions 1960 - 1973 [SOLRAD-01]
The Solar Radiation (SOLRAD) series 1, 4, 6 - 10 collected solar X-ray and ultraviolet data during numerous intervals in the years 1960 - 1973. The data consist of photon fluxes in various wavelength ...


46. Space Physics, Solar Physics and Astronomy Data from Space Physics Data System [SPDS-General]
The Space Physics Data System (SPDS) ( http://spdf.gsfc.nasa.gov/ ) serves the four science disciplines encompassed within the programs of the NASA Space Physics Division, namely: ...


47. The SWICS/MASS/STICS (SMS) Instrument Package on WIND [WIND_SMS]
The main purpose of the Wind spacecraft is to measure the incoming solar wind, magnetic fields and particles, although early on it will also observe the Earth's foreshock region. Wind, together with ...


48. Transient Gamma-Ray Spectrometer (TGRS) on WIND [WIND_TGRS]
The main purpose of the Wind spacecraft is to measure the incoming solar wind, magnetic fields and particles, although early on it will also observe the Earth's foreshock region. Wind, together with ...


49. X-ray Images of Solar Flares from the Solar Maximum Mission/Hard X-ray Burst Spectrometer (SMM/HXRBS) [SMM-05]
The HXRBS operated aboard the SMM spacecraft which was launched on February 14, 1980 and re-entered the Earth's atmosphere December 12, 1989. The duty cycle for the HXRBS was about 50% as a result ...


50. X-ray Images of Solar Flares from the Solar Maximum Mission/Hard X-ray Imaging Spectrometer (SMM/HXIS) [SMM-04]
The data from the Hard X-ray Imaging Spectrometer (HXIS) consist of solar flare images in X-rays, built up from simultaneous photon counting rates in each of 6 energy bands with boundaries at 3.5, ...


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