Large-Scale Shining Chains on the Solar Disk: Nobeyama Radioheliograph Data

Physics

Scientific paper

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Scientific paper

Consideration of the Nobeyama radioheliograms at 17 GHz with a restricted range of the brightness temperature (Tb≈ (5-20)× 103 K) revealed a novel phenomenon of the large-scale solar activity: long-living (days) and transient (hours) microwave shining chains of characteristic sizes comparable with the solar disk diameter and consisting of 30--60'' blobs.

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