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51. 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 ...


52. Measurement of Cosmic Ray Response Functions for an Ice Cherenkov Detector [NSF-ANT08-38838]
We determined a set of cosmic ray response functions for the ice Cherenkov detector used by the surface air shower IceTop, part of the IceCube Neutrino Observatory at the South Pole. At the same time ...


53. 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 ...


54. 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 ...


55. 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 ...


56. National Solar Observatory (NSO) Sacramento Peak Fe XIV and Ca XV Coronal Maps [NSO_DATA_02]
The National Solar Observatory has made data accessible on-line via the networks. Two databases containing the National Solar Observatory/Sacramento Peak Fe XIV 530.3 nm and Ca XV 569.4 nm coronal ...


57. National Solar Observatory/ Kitt Peak Synoptic Solar Data [NSO_DATA_01]
The National Solar Observatories have made data available on-line. The data are produced with the NSO Vacuum Telescope located on Kitt Peak, Arizona. There are several types of data derived from ...


58. 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 ...


59. Ottawa/Penticton 2800 MHz Solar Radio Flux [FE00216]
Solar radio flux is measured from the undisturbed solar surface, developing active regions on the sun and from short-lived enhancements above the daily level. Radio ...


60. PENGUIn - A High-Latitude Window to Geospace Dynamics [NSF-ANT08-40398]
This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5). The PENGUIn team will continue investigating in depth a multi-scale electrodynamic system that comprises ...


61. Polar Experimantal Network for Geospace Upper-atmosphere Investigations (PENGUIn): Interhemispheric Investigations along the 40 Degree Magnetic Meridian [NSF-ANT08-39858]
'This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).' The solar wind - magnetosphere - ionosphere system and the space weather phenomena it controls ...


62. 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 ...


63. Preliminary Data from the Solar Optical Universal Polarimeter (SOUP) on Spacelab2 [SOUP-01]
The Solar Optical Universal Polarimeter (SOUP) experiment was flown in July and August, 1985, on board the STS-51F/Spacelab II shuttle mission. Images of solar features observed in white light were ...


64. Pumping of Magnetic Fields by PTCC [ucar.scd.vets.vg.pumping]
This research explores the transport of magnetic fields on the Solar surface by Penetrative Turbulent Compressible Convection (PTCC).This research attempts to better understand the process ...


65. 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 ...


66. RIOMETER DATA, IONOSPHERIC ABSORPTION [RIO-01]
Cosmic noise is received at 38.2 MHz by a solid state Riometer and dual dipole antenna at Terra Nova Bay, Italian Antarctic Base. These kind of measurements are useful to determine the ionospheric ...


67. 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 ...


68. Research in Aurorae from Belgrano I Station, Antarctica [JCADM_CDA_DNA_AURORAE]
The location of the Belgrano Station in the auroral zone facilitates the observation of auroral activity and its correlation with other geophysical events. The data was acquired continuously through ...


69. Research in Geomagnetism from Direccion Nacional del Antartico [JCADM_DNA_CDA_GEOMAG]
Geomagnetic storm activity is being monitored using high sensitivity magnetometers at the Belgrano and San Martin Antarctic Stations. Geomagnetic pulsations are digitally filtered and recorded. ...


70. 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 ...


71. 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 ...


72. 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 ...


73. 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 ...


74. 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 ...


75. 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 ...


76. 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 ...


77. 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 ...


78. 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 ...


79. 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 ...


80. 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 ...


81. SORCE Extreme Ultraviolet (XUV) Data from the XPS [SORCE_XPS]
This 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 ...


82. Search coil magnetometer data from BAS AGOs in Antarctica [JCADM_US_MAG_AGO]
Search coil magnetometer data are primarily used to study waves and transient variations in Earth's magnetic field in the ULF (Ultra-Low-Frequency) range, from ~0.001 Hz to ...


83. Server of Early Ground Magnetometer Data [BRUNET_GROUND]
Magnetic data from chains of ground stations are currently available at UCLA for 1977 through 1987. They are available at one minute resolution in either HDZ or XYZ coordinates. Data from the following ...


84. Solar Chromospheric Variability from the National Solar Observatory (NSO) [NSO_CA2]
Observations of the disk-integrated solar Ca II K-line are made using the Evans Coronal Facility at The National Solar Observatory/ Sacramento Peak. A coelostat is used to feed the horizontal Littrow ...


85. Solar Data from the University of Hawaii Mees Solar Observatory (MSO) [MEES_SOLAR_OBS_DATA]
The Mees Solar Observatory of the University of Hawaii regularly observes the Sun and archives the following data on-line: - solar active region maps - white light telescope images - imaging vector ...


86. Solar EUV Experiment (SEE) Data from the Thermosphere, Ionosphere, Mesosphere Energetics and Dynamics (TIMED) Mission [TIMED_SEE]
The 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 ...


87. Solar Features [gov.noaa.ngdc.stp.solar.solar-features]
Collection includes a variety of solar feature datasets contributed by a number of national and private solar observatories located worldwide.


88. Solar Features - Prominences and Filaments [gov.noaa.ngdc.stp.solar.solar-features_prominences-filaments]
Prominences and filaments are two manifestations of the same phenomenon. Both prominences and filaments are features formed above the chromosphere by cool dense gases held in place by solar magnetic ...


89. Solar Features - Prominences and Filaments - Filaments [gov.noaa.ngdc.stp.solar.solar-features_prominences-filaments_filaments]
Filaments are formed in magnetic loops that hold relatively cool, dense gas suspended above the surface of the Sun (David Hathaway/NASA)


90. Solar Features - Prominences and Filaments - Prominences [gov.noaa.ngdc.stp.solar.solar-features_prominences-filaments_prominences]
A prominence is a large, bright features extending outward from the sun's surface, often in a loop shape (Wikipedia)


91. Solar Features - Solar Flares [gov.noaa.ngdc.stp.solar.solar-features_solar-flares]
A solar flare is a short-lived sudden increase in the intensity of radiation emitted in the neighborhood of sunspots. For many years it was best monitored in the H-alpha wavelength and occurs in the ...


92. Solar Features - Solar Flares - H-Alpha [gov.noaa.ngdc.stp.solar.solar-features_solar-flares_h-alpha]
A short-lived sudden increase in the intensity or radiation emitted in the neighborhood of sunspots monitored in H-alpha.


93. Solar Features - Solar Flares - Index [gov.noaa.ngdc.stp.solar.solar-features_solar-flares_index]
Daily index of solar flare activity.


94. Solar Features - Solar Flares - Patrol [gov.noaa.ngdc.stp.solar.solar-features_solar-flares_patrol]
The H-alpha Flare Patrol identifies time periods each day when the sun is being continuously monitored by select ground-based solar observatories.


95. Solar Features - Solar Flares - X-rays [gov.noaa.ngdc.stp.solar.solar-features_solar-flares_x-rays]
Listings and characterizations of solar x-ray flares


96. Solar Flare Data from the Berkeley-Illinois-Maryland Array [BIMA]
The BIMA array is a 3-element radio interferometer. Flare observations at 86 GHz with high spatial resolution were obtained during the Flares 22/MAX'91 campaign of December 1991/Jnauary 1992. Times ...


97. Solar Geophysical Data (SGD) Reports (1955-2009) [gov.noaa.ngdc.stp.solar.solar_geophysical_data]
Solar-Geophysical Data (SGD) reports were a comprehensive compilation of many different kinds of observational data of the sun's activity and its effects on the Earth. Data from the worldwide network ...


98. 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 ...


99. Solar Ground-Based Data from the Base de donnees Solaire Sol (BASS) 2000 Project [SOLAR_BASS2000]
BASS 2000 has been initiated by the Institut National des Sciences de l'Univers together with the Midi-Pyrenees Observatory, the research group "solar and stellar magnetodynamic", the ...


100. Solar Imagery [gov.noaa.ngdc.stp.solar.solar-imagery]
Collection includes a variety of solar photographic and illustrated datasets contributed by a number of national and private solar observatories located worldwide. Daily solar observations range from ...


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