Corotating Interaction Regions: Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1999
|
| Schriftenreihe: | Space Sciences Series of ISSI
7 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. Until recently, however, CIRs could only be observed close to the ecliptic plane, and their three-dimensional structure was therefore not obvious to observers and theoreticians alike. Ulysses was the first spacecraft allowing direct exploration of the third dimen sion of the heliosphere. Since 1992, when it has entered a polar orbit that takes it 0 up to 80 latitude, the spacecraft's performance has been flawless and the mission has provided excellent data from a superbly matched set of instruments. Perhaps the most exciting observation during Ulysses' first passage towards the south pole of the Sun was a strong and long lasting CIR whose energetic particle effects were observed up to unexpectedly high latitudes. These observations, documented in a number of publications, stimulated considerable new theoretical work |
| Beschreibung: | 1 Online-Ressource (XIV, 411 p) |
| ISBN: | 9789401711791 9789048153671 |
| ISSN: | 1385-7525 |
| DOI: | 10.1007/978-94-017-1179-1 |
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| 500 | |a A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. Until recently, however, CIRs could only be observed close to the ecliptic plane, and their three-dimensional structure was therefore not obvious to observers and theoreticians alike. Ulysses was the first spacecraft allowing direct exploration of the third dimen sion of the heliosphere. Since 1992, when it has entered a polar orbit that takes it 0 up to 80 latitude, the spacecraft's performance has been flawless and the mission has provided excellent data from a superbly matched set of instruments. Perhaps the most exciting observation during Ulysses' first passage towards the south pole of the Sun was a strong and long lasting CIR whose energetic particle effects were observed up to unexpectedly high latitudes. These observations, documented in a number of publications, stimulated considerable new theoretical work | ||
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Datensatz im Suchindex
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| author | Balogh, A. |
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| dewey-ones | 523 - Specific celestial bodies and phenomena |
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| discipline | Physik |
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| spelling | Balogh, A. Verfasser aut Corotating Interaction Regions Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland edited by A. Balogh, J. T. Gosling, J. R. Jokipii, R. Kallenbach, H. Kunow Proceedings of an ISSI Workshop, 6-13 June 1998, Bern, Switzerland Dordrecht Springer Netherlands 1999 1 Online-Ressource (XIV, 411 p) txt rdacontent c rdamedia cr rdacarrier Space Sciences Series of ISSI 7 1385-7525 A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. Until recently, however, CIRs could only be observed close to the ecliptic plane, and their three-dimensional structure was therefore not obvious to observers and theoreticians alike. Ulysses was the first spacecraft allowing direct exploration of the third dimen sion of the heliosphere. Since 1992, when it has entered a polar orbit that takes it 0 up to 80 latitude, the spacecraft's performance has been flawless and the mission has provided excellent data from a superbly matched set of instruments. Perhaps the most exciting observation during Ulysses' first passage towards the south pole of the Sun was a strong and long lasting CIR whose energetic particle effects were observed up to unexpectedly high latitudes. These observations, documented in a number of publications, stimulated considerable new theoretical work Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Sonnenwind (DE-588)4135572-6 gnd rswk-swf Heliosphäre (DE-588)4243903-6 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift gnd-content Sonnenwind (DE-588)4135572-6 s 2\p DE-604 Heliosphäre (DE-588)4243903-6 s 3\p DE-604 Gosling, J. T. Sonstige oth Jokipii, J. R. Sonstige oth Kallenbach, R. Sonstige oth Kunow, H. Sonstige oth https://doi.org/10.1007/978-94-017-1179-1 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 3\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Balogh, A. Corotating Interaction Regions Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Sonnenwind (DE-588)4135572-6 gnd Heliosphäre (DE-588)4243903-6 gnd |
| subject_GND | (DE-588)4135572-6 (DE-588)4243903-6 (DE-588)1071861417 |
| title | Corotating Interaction Regions Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland |
| title_alt | Proceedings of an ISSI Workshop, 6-13 June 1998, Bern, Switzerland |
| title_auth | Corotating Interaction Regions Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland |
| title_exact_search | Corotating Interaction Regions Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland |
| title_full | Corotating Interaction Regions Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland edited by A. Balogh, J. T. Gosling, J. R. Jokipii, R. Kallenbach, H. Kunow |
| title_fullStr | Corotating Interaction Regions Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland edited by A. Balogh, J. T. Gosling, J. R. Jokipii, R. Kallenbach, H. Kunow |
| title_full_unstemmed | Corotating Interaction Regions Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland edited by A. Balogh, J. T. Gosling, J. R. Jokipii, R. Kallenbach, H. Kunow |
| title_short | Corotating Interaction Regions |
| title_sort | corotating interaction regions proceedings of an issi workshop 6 13 june 1998 bern switzerland |
| title_sub | Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland |
| topic | Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Sonnenwind (DE-588)4135572-6 gnd Heliosphäre (DE-588)4243903-6 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Sonnenwind Heliosphäre Konferenzschrift |
| url | https://doi.org/10.1007/978-94-017-1179-1 |
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