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Microwave enhancement in coronal holes: Statistical properties

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Abstract

We report on the statistical properties of the microwave enhancement (brightness temperature, area, fine structure, life time and magnetic field strength) in coronal holes observed over a period of several solar rotations.

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Authors and Affiliations

  1. NASA/GSFC, Bldg 26, Room G-l, Code 682.3, Greenbelt, MD, USA

    N. Gopalswamy

  2. Nobeyama Radio Observatory, Minamisaku, 384-1305, Nagano, Japan

    K. Shibasaki

  3. Dept. of Physics, Case Western Reserve University, 44106, Cleveland, OH, USA

    M. Salem

Authors
  1. N. Gopalswamy
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  2. K. Shibasaki
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  3. M. Salem
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Corresponding author

Correspondence to N. Gopalswamy.

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Gopalswamy, N., Shibasaki, K. & Salem, M. Microwave enhancement in coronal holes: Statistical properties. J Astrophys Astron 21, 413–417 (2000). https://doi.org/10.1007/BF02702435

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  • DOI: https://doi.org/10.1007/BF02702435

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