Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976
| ISSN: |
1573-093X
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|---|---|
| Source: |
Springer Online Journal Archives 1860-2000
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| Topics: |
Physics
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| Notes: |
Abstract Observations of coronal holes, solar wind streams, and geomagnetic disturbances during 1973–1976 are compared in a 27-day pictorial format which shows their long-term evolution. The results leave little doubt that coronal holes are related to the high-speed streams and their associated recurrent geomagnetic disturbances. In particular, these observations strongly support the hypothesis that coronal holes are the solar origin of the high-speed streams observed in the solar wind near the ecliptic plane.
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| Type of Medium: |
Electronic Resource
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| URL: |
| _version_ | 1798296581735186432 |
|---|---|
| autor | Sheeley, N. R. Harvey, J. W. Feldman, W. C. |
| autorsonst | Sheeley, N. R. Harvey, J. W. Feldman, W. C. |
| book_url | http://dx.doi.org/10.1007/BF00162451 |
| datenlieferant | nat_lic_papers |
| hauptsatz | hsatz_simple |
| identnr | NLM195887220 |
| issn | 1573-093X |
| journal_name | Solar physics |
| materialart | 1 |
| notes | Abstract Observations of coronal holes, solar wind streams, and geomagnetic disturbances during 1973–1976 are compared in a 27-day pictorial format which shows their long-term evolution. The results leave little doubt that coronal holes are related to the high-speed streams and their associated recurrent geomagnetic disturbances. In particular, these observations strongly support the hypothesis that coronal holes are the solar origin of the high-speed streams observed in the solar wind near the ecliptic plane. |
| package_name | Springer |
| publikationsjahr_anzeige | 1976 |
| publikationsjahr_facette | 1976 |
| publikationsjahr_intervall | 8024:1975-1979 |
| publikationsjahr_sort | 1976 |
| publisher | Springer |
| reference | 49 (1976), S. 271-278 |
| search_space | articles |
| shingle_author_1 | Sheeley, N. R. Harvey, J. W. Feldman, W. C. |
| shingle_author_2 | Sheeley, N. R. Harvey, J. W. Feldman, W. C. |
| shingle_author_3 | Sheeley, N. R. Harvey, J. W. Feldman, W. C. |
| shingle_author_4 | Sheeley, N. R. Harvey, J. W. Feldman, W. C. |
| shingle_catch_all_1 | Sheeley, N. R. Harvey, J. W. Feldman, W. C. Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976 Abstract Observations of coronal holes, solar wind streams, and geomagnetic disturbances during 1973–1976 are compared in a 27-day pictorial format which shows their long-term evolution. The results leave little doubt that coronal holes are related to the high-speed streams and their associated recurrent geomagnetic disturbances. In particular, these observations strongly support the hypothesis that coronal holes are the solar origin of the high-speed streams observed in the solar wind near the ecliptic plane. 1573-093X 1573093X Springer |
| shingle_catch_all_2 | Sheeley, N. R. Harvey, J. W. Feldman, W. C. Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976 Abstract Observations of coronal holes, solar wind streams, and geomagnetic disturbances during 1973–1976 are compared in a 27-day pictorial format which shows their long-term evolution. The results leave little doubt that coronal holes are related to the high-speed streams and their associated recurrent geomagnetic disturbances. In particular, these observations strongly support the hypothesis that coronal holes are the solar origin of the high-speed streams observed in the solar wind near the ecliptic plane. 1573-093X 1573093X Springer |
| shingle_catch_all_3 | Sheeley, N. R. Harvey, J. W. Feldman, W. C. Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976 Abstract Observations of coronal holes, solar wind streams, and geomagnetic disturbances during 1973–1976 are compared in a 27-day pictorial format which shows their long-term evolution. The results leave little doubt that coronal holes are related to the high-speed streams and their associated recurrent geomagnetic disturbances. In particular, these observations strongly support the hypothesis that coronal holes are the solar origin of the high-speed streams observed in the solar wind near the ecliptic plane. 1573-093X 1573093X Springer |
| shingle_catch_all_4 | Sheeley, N. R. Harvey, J. W. Feldman, W. C. Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976 Abstract Observations of coronal holes, solar wind streams, and geomagnetic disturbances during 1973–1976 are compared in a 27-day pictorial format which shows their long-term evolution. The results leave little doubt that coronal holes are related to the high-speed streams and their associated recurrent geomagnetic disturbances. In particular, these observations strongly support the hypothesis that coronal holes are the solar origin of the high-speed streams observed in the solar wind near the ecliptic plane. 1573-093X 1573093X Springer |
| shingle_title_1 | Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976 |
| shingle_title_2 | Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976 |
| shingle_title_3 | Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976 |
| shingle_title_4 | Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976 |
| sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
| source_archive | Springer Online Journal Archives 1860-2000 |
| timestamp | 2024-05-06T09:54:23.115Z |
| titel | Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976 |
| titel_suche | Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976 |
| topic | U |
| uid | nat_lic_papers_NLM195887220 |