Coronal temperatures, heating, and energy flow in a polar region of the sun at solar maximum

Journal Article · Tue Oct 01 00:00:00 EDT 1985 · Astrophys. J.; (United States)

DOI:https://doi.org/10.1086/163531· OSTI ID:5612615

Withbroe, G L; Kohl, J L; Weiser, H; Munro, R H

The profiles of resonantly scattered Lyman-alpha coronal radiation have been used to determine the hydrogen kinetic temperature from 1.5 to 4 solar radius from the center of the polar region of the corona observed in 1980 at solar maximum. Hydrogen temperatures derived from the line profiles were found to decrease with height from 1.2 million K at r = 1.5 solar radii to 600,000 K at r = 4 solar radius. Comparison of the measured kinetic temperatures with predictions from a semiempirical two-fluid model showed evidence of a small amount of heating or a nonthermal contribution to the motions of coronal protons between 1.5 and 4 solar radius. The widths of the profiles confirmed an upper limit of 110 + or - 15 km/s on the rms magnitude of the line-of-sight component of velocities between 1.5 and 4 solar radius. Density measurements obtained in situ in the solar wind in the ecliptic were used to locate the sources of low speed and high-speed winds in the polar region. An eclipse photograph of the corona at solar maximum is provided. 31 references.

• Research Organization: Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; High Altitude Observatory, Boulder, CO
• OSTI ID: 5612615
• Journal Information: Astrophys. J.; (United States), Vol. 297
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
SOLAR CORONA
PLASMA HEATING
TEMPERATURE MEASUREMENT
ENERGY SPECTRA
HYDROMAGNETIC WAVES
LYMAN LINES
SOLAR ACTIVITY
SOLAR RADIATION
SOLAR WIND
ATMOSPHERES
HEATING
RADIATIONS
SPECTRA
STELLAR ATMOSPHERES
STELLAR CORONAE
STELLAR RADIATION
640104* - Astrophysics & Cosmology- Solar Phenomena