Corotating Interaction Regions: Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland
Saved in:
| Main Author: | |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
Dordrecht
Springer Netherlands
1999
|
| Series: | Space Sciences Series of ISSI
7 |
| Subjects: | |
| Online Access: | Volltext |
| Item Description: | 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 |
| Physical Description: | 1 Online-Ressource (XIV, 411 p) |
| ISBN: | 9789401711791 9789048153671 |
| ISSN: | 1385-7525 |
| DOI: | 10.1007/978-94-017-1179-1 |
Staff View
MARC
| LEADER | 00000nmm a2200000zcb4500 | ||
|---|---|---|---|
| 001 | BV042416273 | ||
| 003 | DE-604 | ||
| 005 | 00000000000000.0 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 150316s1999 |||| o||u| ||||||eng d | ||
| 020 | |a 9789401711791 |c Online |9 978-94-017-1179-1 | ||
| 020 | |a 9789048153671 |c Print |9 978-90-481-5367-1 | ||
| 024 | 7 | |a 10.1007/978-94-017-1179-1 |2 doi | |
| 035 | |a (OCoLC)864076143 | ||
| 035 | |a (DE-599)BVBBV042416273 | ||
| 040 | |a DE-604 |b ger |e aacr | ||
| 041 | 0 | |a eng | |
| 049 | |a DE-91 |a DE-83 | ||
| 082 | 0 | |a 523.01 |2 23 | |
| 084 | |a PHY 000 |2 stub | ||
| 100 | 1 | |a Balogh, A. |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a Corotating Interaction Regions |b Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland |c edited by A. Balogh, J. T. Gosling, J. R. Jokipii, R. Kallenbach, H. Kunow |
| 246 | 1 | 3 | |a Proceedings of an ISSI Workshop, 6-13 June 1998, Bern, Switzerland |
| 264 | 1 | |a Dordrecht |b Springer Netherlands |c 1999 | |
| 300 | |a 1 Online-Ressource (XIV, 411 p) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 490 | 0 | |a Space Sciences Series of ISSI |v 7 |x 1385-7525 | |
| 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 | ||
| 650 | 4 | |a Physics | |
| 650 | 4 | |a Astrophysics and Astroparticles | |
| 650 | 4 | |a Astronomy, Observations and Techniques | |
| 650 | 0 | 7 | |a Sonnenwind |0 (DE-588)4135572-6 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Heliosphäre |0 (DE-588)4243903-6 |2 gnd |9 rswk-swf |
| 655 | 7 | |8 1\p |0 (DE-588)1071861417 |a Konferenzschrift |2 gnd-content | |
| 689 | 0 | 0 | |a Sonnenwind |0 (DE-588)4135572-6 |D s |
| 689 | 0 | |8 2\p |5 DE-604 | |
| 689 | 1 | 0 | |a Heliosphäre |0 (DE-588)4243903-6 |D s |
| 689 | 1 | |8 3\p |5 DE-604 | |
| 700 | 1 | |a Gosling, J. T. |e Sonstige |4 oth | |
| 700 | 1 | |a Jokipii, J. R. |e Sonstige |4 oth | |
| 700 | 1 | |a Kallenbach, R. |e Sonstige |4 oth | |
| 700 | 1 | |a Kunow, H. |e Sonstige |4 oth | |
| 856 | 4 | 0 | |u https://doi.org/10.1007/978-94-017-1179-1 |x Verlag |3 Volltext |
| 912 | |a ZDB-2-PHA |a ZDB-2-BAE | ||
| 940 | 1 | |q ZDB-2-PHA_Archive | |
| 999 | |a oai:aleph.bib-bvb.de:BVB01-027851766 | ||
| 883 | 1 | |8 1\p |a cgwrk |d 20201028 |q DE-101 |u https://d-nb.info/provenance/plan#cgwrk | |
| 883 | 1 | |8 2\p |a cgwrk |d 20201028 |q DE-101 |u https://d-nb.info/provenance/plan#cgwrk | |
| 883 | 1 | |8 3\p |a cgwrk |d 20201028 |q DE-101 |u https://d-nb.info/provenance/plan#cgwrk | |
Record in the Search Index
| _version_ | 1804153084528558080 |
|---|---|
| any_adam_object | |
| author | Balogh, A. |
| author_facet | Balogh, A. |
| author_role | aut |
| author_sort | Balogh, A. |
| author_variant | a b ab |
| building | Verbundindex |
| bvnumber | BV042416273 |
| classification_tum | PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)864076143 (DE-599)BVBBV042416273 |
| dewey-full | 523.01 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.01 |
| dewey-search | 523.01 |
| dewey-sort | 3523.01 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-017-1179-1 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>03379nmm a2200577zcb4500</leader><controlfield tag="001">BV042416273</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">00000000000000.0</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">150316s1999 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789401711791</subfield><subfield code="c">Online</subfield><subfield code="9">978-94-017-1179-1</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789048153671</subfield><subfield code="c">Print</subfield><subfield code="9">978-90-481-5367-1</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-94-017-1179-1</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)864076143</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV042416273</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">aacr</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-91</subfield><subfield code="a">DE-83</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">523.01</subfield><subfield code="2">23</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">PHY 000</subfield><subfield code="2">stub</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Balogh, A.</subfield><subfield code="e">Verfasser</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Corotating Interaction Regions</subfield><subfield code="b">Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland</subfield><subfield code="c">edited by A. Balogh, J. T. Gosling, J. R. Jokipii, R. Kallenbach, H. Kunow</subfield></datafield><datafield tag="246" ind1="1" ind2="3"><subfield code="a">Proceedings of an ISSI Workshop, 6-13 June 1998, Bern, Switzerland</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Dordrecht</subfield><subfield code="b">Springer Netherlands</subfield><subfield code="c">1999</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (XIV, 411 p)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="490" ind1="0" ind2=" "><subfield code="a">Space Sciences Series of ISSI</subfield><subfield code="v">7</subfield><subfield code="x">1385-7525</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="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</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Physics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Astrophysics and Astroparticles</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Astronomy, Observations and Techniques</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Sonnenwind</subfield><subfield code="0">(DE-588)4135572-6</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Heliosphäre</subfield><subfield code="0">(DE-588)4243903-6</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="655" ind1=" " ind2="7"><subfield code="8">1\p</subfield><subfield code="0">(DE-588)1071861417</subfield><subfield code="a">Konferenzschrift</subfield><subfield code="2">gnd-content</subfield></datafield><datafield tag="689" ind1="0" ind2="0"><subfield code="a">Sonnenwind</subfield><subfield code="0">(DE-588)4135572-6</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2=" "><subfield code="8">2\p</subfield><subfield code="5">DE-604</subfield></datafield><datafield tag="689" ind1="1" ind2="0"><subfield code="a">Heliosphäre</subfield><subfield code="0">(DE-588)4243903-6</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="1" ind2=" "><subfield code="8">3\p</subfield><subfield code="5">DE-604</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Gosling, J. T.</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Jokipii, J. R.</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kallenbach, R.</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kunow, H.</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-94-017-1179-1</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-2-PHA</subfield><subfield code="a">ZDB-2-BAE</subfield></datafield><datafield tag="940" ind1="1" ind2=" "><subfield code="q">ZDB-2-PHA_Archive</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-027851766</subfield></datafield><datafield tag="883" ind1="1" ind2=" "><subfield code="8">1\p</subfield><subfield code="a">cgwrk</subfield><subfield code="d">20201028</subfield><subfield code="q">DE-101</subfield><subfield code="u">https://d-nb.info/provenance/plan#cgwrk</subfield></datafield><datafield tag="883" ind1="1" ind2=" "><subfield code="8">2\p</subfield><subfield code="a">cgwrk</subfield><subfield code="d">20201028</subfield><subfield code="q">DE-101</subfield><subfield code="u">https://d-nb.info/provenance/plan#cgwrk</subfield></datafield><datafield tag="883" ind1="1" ind2=" "><subfield code="8">3\p</subfield><subfield code="a">cgwrk</subfield><subfield code="d">20201028</subfield><subfield code="q">DE-101</subfield><subfield code="u">https://d-nb.info/provenance/plan#cgwrk</subfield></datafield></record></collection> |
| genre | 1\p (DE-588)1071861417 Konferenzschrift gnd-content |
| genre_facet | Konferenzschrift |
| id | DE-604.BV042416273 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:59Z |
| institution | BVB |
| isbn | 9789401711791 9789048153671 |
| issn | 1385-7525 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027851766 |
| oclc_num | 864076143 |
| open_access_boolean | |
| owner | DE-91 DE-BY-TUM DE-83 |
| owner_facet | DE-91 DE-BY-TUM DE-83 |
| physical | 1 Online-Ressource (XIV, 411 p) |
| psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
| publishDate | 1999 |
| publishDateSearch | 1999 |
| publishDateSort | 1999 |
| publisher | Springer Netherlands |
| record_format | marc |
| series2 | Space Sciences Series of ISSI |
| 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 |
| work_keys_str_mv | AT balogha corotatinginteractionregionsproceedingsofanissiworkshop613june1998bernswitzerland AT goslingjt corotatinginteractionregionsproceedingsofanissiworkshop613june1998bernswitzerland AT jokipiijr corotatinginteractionregionsproceedingsofanissiworkshop613june1998bernswitzerland AT kallenbachr corotatinginteractionregionsproceedingsofanissiworkshop613june1998bernswitzerland AT kunowh corotatinginteractionregionsproceedingsofanissiworkshop613june1998bernswitzerland AT balogha proceedingsofanissiworkshop613june1998bernswitzerland AT goslingjt proceedingsofanissiworkshop613june1998bernswitzerland AT jokipiijr proceedingsofanissiworkshop613june1998bernswitzerland AT kallenbachr proceedingsofanissiworkshop613june1998bernswitzerland AT kunowh proceedingsofanissiworkshop613june1998bernswitzerland |