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