The initial trajectories of eruptive solar prominences
Trajectories of eruptive prominences are compared with the shapes of coronal neutral surfaces calculated in a potential approximation using photospheric measurements. Space-based Solar Dymamics Observatory and STEREO observations carried out at different viewing angles enable a precise determination...
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| Published in: | Astronomy reports Vol. 60; no. 3; pp. 356 - 365 |
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| Format: | Journal Article |
| Language: | English |
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Pleiades Publishing
01-03-2016
Springer Nature B.V |
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| Abstract | Trajectories of eruptive prominences are compared with the shapes of coronal neutral surfaces calculated in a potential approximation using photospheric measurements. Space-based Solar Dymamics Observatory and STEREO observations carried out at different viewing angles enable a precise determination of a prominence’s position at successive times during its eruption. In the initial segments of their trajectories, eruptive prominences move along neutral surfaces (
B
r
= 0) of the potential coronal magnetic field. This can be used to predict the directions of subsequent coronal mass ejections and to estimate their geoefficiency. |
|---|---|
| AbstractList | Trajectories of eruptive prominences are compared with the shapes of coronal neutral surfaces calculated in a potential approximation using photospheric measurements. Space-based Solar Dymamics Observatory and STEREO observations carried out at different viewing angles enable a precise determination of a prominence's position at successive times during its eruption. In the initial segments of their trajectories, eruptive prominences move along neutral surfaces (B sub(r) = 0) of the potential coronal magnetic field. This can be used to predict the directions of subsequent coronal mass ejections and to estimate their geoefficiency. Trajectories of eruptive prominences are compared with the shapes of coronal neutral surfaces calculated in a potential approximation using photospheric measurements. Space-based Solar Dymamics Observatory and STEREO observations carried out at different viewing angles enable a precise determination of a prominence’s position at successive times during its eruption. In the initial segments of their trajectories, eruptive prominences move along neutral surfaces ( B r = 0) of the potential coronal magnetic field. This can be used to predict the directions of subsequent coronal mass ejections and to estimate their geoefficiency. |
| Author | Filippov, B. P. |
| Author_xml | – sequence: 1 givenname: B. P. surname: Filippov fullname: Filippov, B. P. email: bfilip@izmiran.ru organization: Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, IZMIRAN |
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| CitedBy_id | crossref_primary_10_1017_pasa_2019_13 crossref_primary_10_3367_UFNe_2018_10_038467 |
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| Keywords | Astronomy Report Solar Dynamics Observatory Coronal Mass Ejection Solar Phys Neutral Surface |
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| Snippet | Trajectories of eruptive prominences are compared with the shapes of coronal neutral surfaces calculated in a potential approximation using photospheric... |
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| SubjectTerms | Approximation Astronomy Corona Coronal mass ejection Magnetic fields Mathematical analysis Observations and Techniques Physics Physics and Astronomy Prominences Segments Solar magnetic field Solar physics Sun Trajectories |
| Title | The initial trajectories of eruptive solar prominences |
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