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15 Titles Match Your Query
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1. 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 ...


2. 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/mission/about.php ] SDO: The Solar Dynamics Observatory is the first ...


3. Tomographic Imaging of the Velocity and Magnetic Fields in the Sun's Atmosphere [NSF-ANT06-32399]
The ultimate goal of this project is to determine the structure and dynamics of the Sun's atmosphere, assess the role of MHD waves in heating the chromosphere/corona and driving the solar wind, and ...


4. 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 ...


5. NOAA Space Environment Laboratory On-Line Solar and Geophysical Data [SEL-01]
The NOAA Space Environment Laboratory collects, evaluates, and distributes data relating to space plasma events, solar activity, and cosmic ray particle activity on a nearly real-time basis. Space ...


6. Solar Magnetic Flux Tubes [ucar.scd.vets.vg.mft]
Solar Magnetic Flux Tubes are magnetic field concentrations near the surface of the sun. Because of their close relation to their much larger cousins, sun spots, they are of great interest ...


7. 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 ...


8. Wilcox Solar Observatory Solar Data and Solar Magnetic Field Atlas [WILCOX_SOLAR_ATLAS]
The Wilcox Solar Observatory began daily observations of the Sun's global magnetic field in May 1975, with the goal of understanding changes in the Sun and how those changes affect the Earth; this ...


9. 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 ...


10. Solar Global Oscillation Network Group (GONG) [GONG]
The Global Oscillation Network Group ( GONG ) is a community-based project to conduct a detailed study of solar internal structure and dynamics using helioseismology. In order to exploit this new ...


11. Active Region UV Atlas [HRTS-II_ATLAS]
An ultraviolet spectral Atlas of a sunspot with high spectral and spatial resolution in the wavelength region 1190 - 1730 A is presented. The sunspot was observed with the High Resolution Telescope ...


12. On-line Solar Imaging Data Available from Big Bear Observatory [BBSO_ON_LINE]
Daily Big Bear Solar Observatory (BBSO) images are available from http://www.bbso.njit.edu/. Data available include: High-resolution H-alpha filtergram (usually center line) Dopplergram (usually ...


13. 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 ...


14. Solar Ultraviolet Data from Orbiting Solar Observatory (OSO 8) Space Mission [OSO-8-spectro-level1]
The LPSP multichannel High Resolution UV and visible spectometer was launched June 21, 1975 and was in operation until September 30, 1978 with 6 channels covering the most intense optically thick ...


15. High-cadence dual-height full disk solar dopplergrams and intensitygrams taken in January 2003 [MOTH_2003]
Simultaneous intensity and line-of-sight velocity data of the full solar disk as measured at the two heights probed by the K (770 nm) and Na (589 nm) Fraunhofer lines. Three sets of uninterrupted ...


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