Structure of convective flows on supergranular scales in the solar photosphere
The exploration of the velocity field of the real solar convection was performed using neutral iron line λ ≈ 639.3 nm profile from the observations with high spatial resolution. The inverse procedure was applied for each profile to reproduce the velocity field in the solar photosphere. Acoustic wave...
Gespeichert in:
| Veröffentlicht in: | Advances in Astronomy and Space Physics |
|---|---|
| Datum: | 2012 |
| 1. Verfasser: | |
| Format: | Artikel |
| Sprache: | English |
| Veröffentlicht: |
Головна астрономічна обсерваторія НАН України
2012
|
| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/119189 |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | Structure of convective flows on supergranular scales in the solar photosphere / O.A. Baran // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 153-156. — Бібліогр.: 14 назв. — англ. |