SOHO/UltraViolet Coronograph Spectrometer (UVCS) Data Archive

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 address a broad range of scientific
questions regarding the nature of the solar corona and the generation of the
solar wind.

UVCS makes measurements of the solar corona between 2 and 10 solar radii from
sun center with high spectral and spatial resolution. From the spectroscopic
measurements at ultraviolet wavelengths, the
- proton velocity distribution,
- proton outflow velocity,
- electron temperature, and
- O VI, Si XII, and Mg X outflow velocities and densities

can be determined. Information about the

- O VI, Si XII, and Mg X velocity distributions,
- electron density, and
- minor ions densities

can also be learned.

All SOHO/UVCS data are available from the public SOHO data archive:
http://sohowww.nascom.nasa.gov/data/data.html

Mirror archives are available at:
SOHO Archive at Rutherford Appleton Laboratory, UK.:
http://trace.solararchive.rl.ac.uk/soho/

SOHO Archive at the Institut d'Astrophysique Spatiale, France:
http://idc-medoc.ias.u-psud.fr/

SOHO Archive at Osservatorio Astronomico di Torino, Torino, Italy:
http://solar.to.astro.it/