Magnetic Field Configuration of Flare Locations in NOAA10486

Details Magnetic Field Configuration of Flare Locations in NOAA10486 Magnetic Field Configuration of Flare Locations in NOAA10486

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh51c..11c&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SH51C-11

Other

7513 Coronal Mass Ejections, 7519 Flares, 7524 Magnetic Fields, 7529 Photosphere, 7536 Solar Activity Cycle (2162)

Scientific paper

The active region NOAA 10486 was the site of large solar flares that were associated with the coronal mass ejections. The initial trigger of these flares occurred at the sites where there was emergence of new flux in addition to the large magnetic shear. Several other large active regions also show that flux emergence is an essential property of such locations. In this paper, we present the magnetic field characteristics of NOAA10486 and compare them with similar active regions of past solar cycles.

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