Coronal Thick Target Hard X-Ray Emissions and Radio Emissions

ASTROPHYSICAL JOURNAL LETTERS, no. 1 (2013)

Cited by: 3|Views1

Abstract:

A distinctive class of hard X-ray (HXR) sources located in the corona was recently found, which implies that the collisionally thick target model (CTTM) applies even to the corona. We investigated whether this idea can be independently verified by microwave radiations which have been known as the best companion to HXRs. This study is cond...More

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