Characteristics of intranetwork magnetic fields in a solar coronal hole.

Details Characteristics of intranetwork magnetic fields in a solar coronal hole. Characteristics of intranetwork magnetic fields in a solar coronal hole.

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997arbei..30...58l&link_type=abstract

Astrophysics Reports, Publications of the Beijing Astronomical Observatory, No. 30, p. 58 - 64

Astronomy and Astrophysics

Astrophysics

1

Solar Coronal Holes: Solar Magnetic Fields

Scientific paper

The magnetograms observed by the solar telescope magnetograph at the Beijing Astronomical Observatory for a solar coronal hole on June 23, 1993, which has a dominant magnetic field of N polarity, are used to investigate the characteristics of the intranetwork magnetic fields in the coronal hole. For the intranetwork magnetic hills with magnetic strengths between 10 Gs and 20 Gs conclusions are listed.

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