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| Content Provider | Springer Nature Link |
|---|---|
| Author | Grigoryev, V. M. Ermakova, L. V. Salakhutdiva, I. I. Khlystova, A. I. |
| Copyright Year | 2009 |
| Abstract | The dynamics of the magnetic field and velocity field during the birth and an early development stage of a major active region is studied. SOHO MDI longitudinal-component magnetograms, Dopplergrams, and continuum images are used. The presence of an enhanced material upflow in the photosphere during the passing of the top of the magnetic flux loop, forming the active region, is revealed. The maximum upflow velosity is 2 km/s and the maximum size of the upflow area exceeds 20000 km. The lifetime of the upflow is about two hours. The undulating form of the magnetic flux tubes crossing the photosphere is confirmed. A structural-analysis technique is used to show that the trailing polarity field at the formation stage of the active region is more highly structured than the leading polarity field. |
| Starting Page | 823 |
| Ending Page | 829 |
| Page Count | 7 |
| File Format | |
| ISSN | 00167932 |
| Journal | Geomagnetism and Aeronomy |
| Volume Number | 49 |
| Issue Number | 7 |
| e-ISSN | 1555645X |
| Language | English |
| Publisher | SP MAIK Nauka/Interperiodica |
| Publisher Date | 2010-01-05 |
| Publisher Place | Dordrecht |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | Geophysics/Geodesy |
| Content Type | Text |
| Resource Type | Article |
| Subject | Geophysics Space and Planetary Science |
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