Response of the Solar Atmosphere to Magnetic Flux Emergence from Hinode Observations

Details Response of the Solar Atmosphere to Magnetic Flux Emergence from Hinode Observations Response of the Solar Atmosphere to Magnetic Flux Emergence from Hinode Observations

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007pasj...59s.643l&link_type=abstract

Publications of the Astronomical Society of Japan, Vol.59, No.SP3, pp.S643--S648

Astronomy and Astrophysics

Astronomy

5

Sun: Magnetic Fields, Sun: Photosphere, Sun: X-Rays, Gamma Rays

Scientific paper

In the present work, we used optical and X-ray data from the Hinode satellite to study the response of the solar chromosphere and the corona to the emerging flux in the photosphere. In total, twelve emerging flux regions (EFRs) were selected to conduct this study. The average separation of the two polarities and the lifetime of these EFRs were 3.2'' and 40min, respectively. All of these regions showed corresponding enhanced emission in the CaII H line and soft X-rays with different filters, indicating that these small-scale and short-lived EFRs heat the chromosphere and the corona to some extent.

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