The Radial and Angular Variation of the Electron Density in the Solar Corona

Details The Radial and Angular Variation of the Electron Density in the Solar Corona The Radial and Angular Variation of the Electron Density in the Solar Corona

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999apj...524l.133g&link_type=abstract

The Astrophysical Journal, Volume 524, Issue 2, pp. L133-L137.

Astronomy and Astrophysics

Astronomy

26

Magnetohydrodynamics: Mhd, Sun: Solar Wind, Sun: Corona, Sun: Uv Radiation, Techniques: Spectroscopic

Scientific paper

We derive, for the first time, electron densities as a function of both radius (R) and position angle (θ) for the southwest quadrant of the off-limb corona, using the density-sensitive Si IX λ349.9/λ341.9 and Si X λ356.0/λ347.7 extreme-ultraviolet line ratios. The observations were made with the coronal diagnostic spectrometer on board the Solar and Heliospheric Observatory over the ranges of 1.00 R_solar

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