Elemental Abundances in the Inner Solar Corona Measured by SOHO/UVCS

Details Elemental Abundances in the Inner Solar Corona Measured by SOHO/UVCS Elemental Abundances in the Inner Solar Corona Measured by SOHO/UVCS

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh52c03k&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH52C-03 INVITED

Physics

2164 Solar Wind Plasma, 2169 Sources Of The Solar Wind, 7509 Corona, 7549 Ultraviolet Emissions

Scientific paper

The UVCS instrument aboard the SOHO spacecraft measures UV spectrum in the solar corona. The capability of observing Lyman lines of atomic hydrogen as well as lines from various elements, some with a range of ionization states, makes it possible to determine the absolute elemental abundances in both low and high FIP (First Ionization Potential) elements. We review UVCS observations of absolute abundances in various structures of the solar corona. These include streamers across its structure, at different latitudes and heights, as well as variations along the heliocentric heights above active regions.

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