Solar atmospheric heating and topology of solar magnetic field.

Details Solar atmospheric heating and topology of solar magnetic field. Solar atmospheric heating and topology of solar magnetic field.

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998arbes...4...54w&link_type=abstract

Astrophysics Reports, Special Issue, No. 4, p. 54 - 61

Astronomy and Astrophysics

Astrophysics

Solar Active Regions: Magnetograms, Solar Active Regions: Soft X Rays, Solar Active Regions: H Alpha, Solar Magnetic Fields: Topology

Scientific paper

The photospheric vector magnetic fields, Hα and soft X-ray images of AR 7321 were simultaneously observed with the Solar Flare Telescope at Mitaka and the Soft X-ray Telescope of Yohkoh on October 26, 1992, when there were no drastic activities in this region. Taking the observed photospheric vector magnetic fields as the boundary condition, 3D magnetic fields above the photosphere were computed with a new extrapolation method. Since Yohkoh data and Mitaka data were obtained in well arranged time sequences during the day, the evolution of 3D fields, Hα features and soft X-ray features in this region can be studied in detail.

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