The density structure of a solar polar coronal hole

Details The density structure of a solar polar coronal hole The density structure of a solar polar coronal hole

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jgr...104.9781w&link_type=abstract

Journal of Geophysical Research, Volume 104, Issue A5, p. 9781-9790

Astronomy and Astrophysics

Astrophysics

9

Solar Physics, Astrophysics, And Astronomy: Ultraviolet Emissions, And Astronomy: Transition Region, And Astronomy: Corona, And Astronomy: Coronal Holes

Scientific paper

Electron densities derived from Si III, Ne VII, Mg VIII, Si VIII, and Mg IX line ratios observed above the limb of a polar coronal hole with the Solar Ultraviolet Measurements of Emitted Radiation (SUMER) spectrometer on the Solar and Heliospheric Observatory (SoHO) are presented. The electron densities are consistent with a constant pressure of 1.6×1014cm-3K (logPe=14.2).

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