Dynamics of line-of-sight velocities and magnetic field in the solar photosphere during the formation of the large active region NOAA 10488

Details Dynamics of line-of-sight velocities and magnetic field in the solar photosphere during the formation of the large active region NOAA 10488 Dynamics of line-of-sight velocities and magnetic field in the solar photosphere during the formation of the large active region NOAA 10488

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007astl...33..766g&link_type=abstract

Astronomy Letters, Volume 33, Issue 11, pp.766-770

Astronomy and Astrophysics

Astronomy

7

Scientific paper

Analysis of SOHO longitudinal magnetograms and Dopplergrams has revealed the appearance of a region of enhanced upflow of matter in the photosphere when the top of a loop-shaped magnetic flux tube forming a large active region passed through it. The maximum upflow velocity reached 2 km s-1, the maximum size exceeded 20 000 km, and the lifetime was about 2 h.

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