FY91 AASERT: Implications of the Small Scale Structure in the Quiet Sun for the Solar Wind Flow

Details FY91 AASERT: Implications of the Small Scale Structure in the Quiet Sun for the Solar Wind Flow FY91 AASERT: Implications of the Small Scale Structure in the Quiet Sun for the Solar Wind Flow

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996sao..reptt....h&link_type=abstract

Technical Report, Smithsonian Astrophysical Observatory Cambridge, MA United States

Astronomy and Astrophysics

Astrophysics

Solar Wind, Solar Activity, Magnetic Field Configurations, Research Management, Solar Spectra, Solar Corona, Coronal Holes

Scientific paper

The AASERT Program was established to provide training for graduate and undergraduate student in the field of research complementing a program sponsored by the Department of Defense.The main focus of this program was to explore the physical characteristics of the fine scale magnetic structure in coronal holes which a believe to be the source region of the fast solar wind.

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