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Geomagnetic Storm of March 8, 2012 [MAR0812_CME]
The sun erupted with one of the largest solar flares of this solar cycle on March 6, 2012 at 7PM EST. This flare was categorized as an X5.4, making it the second largest flare -- after an X6.9 on ...
Solar Magnetic Eruption Disturbances [ucar.scd.vets.vg.sme]
Solar 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 ...
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 ...
Observation of the nucleonic cosmic ray component at the Kerguelen and Terre-Adelie stations [227_0_IPEV_FR]
Observation de la composante nucléonique du rayonnement cosmique:
(1) comme participation française au réseau international des
moniteurs à neutrons,
(2) pour étudier laccélération ...
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 ...
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 ...
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 ...
Data from Neutron Monitor 6NM64 on King George Island [136-89_01]
LARC is an acronym, which stands for Laboratorio Antartico de Radiacion Cosmica
(Antarctic Laboratory for Cosmic Rays). LARC project started about ten years
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.
Advanced Composition Explorer (ACE) Real-Time Solar Wind Data from NOAA/SEC [ACE_RTSW]
Advanced Composition Explorer (ACE) Real-Time Solar Wind (RTSW) Data from
NOAA's Space Environment Center (SEC) provides up to an hour's advance warning
of unusual solar activity, such ...
Advanced Composition Explorer (ACE) Solar Isotope Spectrometer (SIS) Level 2 Data [ACE_SIS_LEVEL2]
The Solar Isotope Spectrometer (SIS) is designed to provide high
resolution measurements of the isotopic composition of energetic
nuclei from He to Ni (Z=2 to 28) over the energy range ...
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 ...
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 ...
SOHO/Comprehensive Suprathermal and Energetic Particle Analyzer (COSTEP) Data Archive [SOHO_COSTEP]
COSTEP addresses scientific objectives related to the following
* Steady state processes in the solar atmosphere
* Energy release and particle acceleration in the solar atmosphere
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 ...
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 ...
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 ...
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 ...
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 ...
Transition Region and Coronal Explorer (TRACE) Data Archive [TRACE]
The Transition Region and Coronal Explorer (TRACE) is a NASA Small Explorer
(SMEX) mission to image the solar corona and transition region at high angular
and temporal resolution. The TRACE project ...
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 ...
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 ...
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 ...
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 ...
X-ray Images of the Solar Corona from the Skylab S-054 Telescope [Skylab-05]
The X-ray telescope (experiment S-054) was a grazing incidence
instrument with a spatial resolution of approximately 2 arc seconds on
axis and had six broadband X-ray filters in the 2 - 60 Angstroem ...
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
Two databases containing the National Solar Observatory/Sacramento Peak
Fe XIV 530.3 nm and Ca XV 569.4 nm coronal ...
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 ...
Showing 1 through 27 of 27