[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 ...
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 ...
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 ...
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 ...
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 ...
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 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 ...
