Документ взят из кэша поисковой машины. Адрес оригинального документа : http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/100109/100109_01.pdf Дата изменения: Mon Jul 23 18:39:24 2012 Дата индексирования: Mon Feb 4 02:44:54 2013 Кодировка: Поисковые слова: annular solar eclipse

No. 1 Time (UT) 11:30 X-ray BP behaviour Magnetic fragment behaviour Note

A diffused A bipolar region is involved. Negative and Start of the data set. Both brightening region positive fragments are very close to each other. polarities in this region move is present. around, and the negative ones are more active. A bright stripe becomes very strong in the area. At the direction of the stripe, many activities, including cancellation and flux emergence, are going on. The locations of the fragments observed at the beginning of the data set have totally changed. The activity in this area is roughly responsible for the observed Xray behaviour. When cancellation is stronger, X-ray emission becomes stronger.

15:36

16:59

The stripe becomes faint. Another bright stripe becomes very strong to the north.

In some of the cancellation sites related to the End of the data set. bright strip, positive fragments are faint. A few other cancellation sites were formed. At the direction of the newly emerged bright stripe, an active site has been formed.