The coronal transient of 16 June 1972
| Autor: | Shirley F. Hansen, Russell A. Howard, M. J. Koomen, Richard T. Hansen |
|---|---|
| Rok vydání: | 1974 |
| Předmět: |
Physics
Astrophysics::Instrumentation and Methods for Astrophysics Coronal cloud Coronal hole Astronomy Astronomy and Astrophysics Coronal loop Astrophysics Corona Coronal radiative losses Nanoflares Solar wind Space and Planetary Science Physics::Space Physics Coronal mass ejection Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics |
| Zdroj: | Solar Physics. 34:447-452 |
| ISSN: | 1573-093X 0038-0938 |
| DOI: | 10.1007/bf00153680 |
| Popis: | On 16 June 1972, the Naval Research Laboratory's coronagraph aboard OSO-7 tracked a huge coronal cloud moving outward from the Sun. Concurrent observations of the inner corona made by the High Altitude Observatory at Mauna Loa showed bifurcation of the underlying coronal structure. Together, these observations can be interpreted as evidence for the stretching of the closed fields into a ‘magnetic bottle’, extending to at least eight radii from the center of the Sun. |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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