The Cosmic Dynamo: Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992
Gespeichert in:
| Weitere Verfasser: | , , |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1993
|
| Schriftenreihe: | International Astronomical Union Symposia Union Astronomique Internationale
157 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | This IAU-symposium was the first which was entirely dedicated to dynamo processes, which are fundamental on all cosmical scales. Dynamo theory concerns one of the few truly key questions of recent cosmic physics. There is increasing evidence for the magnetic character of most short-term activity phenomena in astrophysics. Obviously, the triangle "gravity, nuclear power, magnetism" dictates cosmic evolution over a very broad scale of magnitudes. A complicated interplay of rotation, magnetism and turbulence, that is hard to resolve, determines stellar and galactic activity for almost all the short and medium timescales. Behind these multiform phenomena, the cosmic dynamo works in various guise. . "I, all involving inductive and dissipative equilibria in rotating turbulent cosmic plasmas. The Sun, representing the cosmic dynamo par excellence, stands from the beginning at the centre of interest for those who followed the dynamo idea. Even the first models were able to present an explanation of the typical structural appearance of the solar magnetic field, i. e. a 22 year cycle, activity belts and their zonal migration, antisymmetry of t. he magnetic polarity. However, the solar dynamo still provides topics of further discussions, since confrontation with recent observational data raised and still raises new questions, non of which have yet found a plausible answer. These questions represent a challenge for the development of the basic theories: Understanding of turbulence, especially using methods of modern nonlinear physics. Numerical simulations are promising in the near future |
| Beschreibung: | 1 Online-Ressource (XXXII, 499 p) |
| ISBN: | 9789401107723 9780792325475 |
| DOI: | 10.1007/978-94-011-0772-3 |
Internformat
MARC
| LEADER | 00000nmm a2200000zcb4500 | ||
|---|---|---|---|
| 001 | BV042415759 | ||
| 003 | DE-604 | ||
| 005 | 20171019 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 150316s1993 |||| o||u| ||||||eng d | ||
| 020 | |a 9789401107723 |c Online |9 978-94-011-0772-3 | ||
| 020 | |a 9780792325475 |c Print |9 978-0-7923-2547-5 | ||
| 024 | 7 | |a 10.1007/978-94-011-0772-3 |2 doi | |
| 035 | |a (OCoLC)905375161 | ||
| 035 | |a (DE-599)BVBBV042415759 | ||
| 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 | ||
| 245 | 1 | 0 | |a The Cosmic Dynamo |b Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992 |c edited by F. Krause, K.-H. Rädler, G. Rüdiger |
| 246 | 1 | 3 | |a Proceedings of the 157th Symposium of the International Astronomical Union held in Potsdam, Germany, September 7--11, 1992 |
| 264 | 1 | |a Dordrecht |b Springer Netherlands |c 1993 | |
| 300 | |a 1 Online-Ressource (XXXII, 499 p) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 490 | 1 | |a International Astronomical Union Symposia / Union Astronomique Internationale |v 157 | |
| 500 | |a This IAU-symposium was the first which was entirely dedicated to dynamo processes, which are fundamental on all cosmical scales. Dynamo theory concerns one of the few truly key questions of recent cosmic physics. There is increasing evidence for the magnetic character of most short-term activity phenomena in astrophysics. Obviously, the triangle "gravity, nuclear power, magnetism" dictates cosmic evolution over a very broad scale of magnitudes. A complicated interplay of rotation, magnetism and turbulence, that is hard to resolve, determines stellar and galactic activity for almost all the short and medium timescales. Behind these multiform phenomena, the cosmic dynamo works in various guise. . "I, all involving inductive and dissipative equilibria in rotating turbulent cosmic plasmas. The Sun, representing the cosmic dynamo par excellence, stands from the beginning at the centre of interest for those who followed the dynamo idea. Even the first models were able to present an explanation of the typical structural appearance of the solar magnetic field, i. e. a 22 year cycle, activity belts and their zonal migration, antisymmetry of t. he magnetic polarity. However, the solar dynamo still provides topics of further discussions, since confrontation with recent observational data raised and still raises new questions, non of which have yet found a plausible answer. These questions represent a challenge for the development of the basic theories: Understanding of turbulence, especially using methods of modern nonlinear physics. Numerical simulations are promising in the near future | ||
| 650 | 4 | |a Physics | |
| 650 | 4 | |a Astrophysics and Astroparticles | |
| 650 | 4 | |a Astronomy, Observations and Techniques | |
| 650 | 0 | 7 | |a Magnetfeld |0 (DE-588)4074450-4 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Galaxie |0 (DE-588)4057375-8 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Dynamotheorie |0 (DE-588)4135270-1 |2 gnd |9 rswk-swf |
| 655 | 7 | |8 1\p |0 (DE-588)1071861417 |a Konferenzschrift |y 1992 |z Potsdam |2 gnd-content | |
| 689 | 0 | 0 | |a Galaxie |0 (DE-588)4057375-8 |D s |
| 689 | 0 | 1 | |a Magnetfeld |0 (DE-588)4074450-4 |D s |
| 689 | 0 | 2 | |a Dynamotheorie |0 (DE-588)4135270-1 |D s |
| 689 | 0 | |8 2\p |5 DE-604 | |
| 700 | 1 | |a Krause, F. |4 edt | |
| 700 | 1 | |a Rädler, K.-H. |4 edt | |
| 700 | 1 | |a Rüdiger, G. |4 edt | |
| 830 | 0 | |a International Astronomical Union Symposia |p Union Astronomique Internationale |v 157 |w (DE-604)BV000000364 |9 157 | |
| 856 | 4 | 0 | |u https://doi.org/10.1007/978-94-011-0772-3 |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:BVB01-027851252 | ||
| 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 | |
Datensatz im Suchindex
| _version_ | 1804153083290189824 |
|---|---|
| any_adam_object | |
| author2 | Krause, F. Rädler, K.-H Rüdiger, G. |
| author2_role | edt edt edt |
| author2_variant | f k fk k h r khr g r gr |
| author_facet | Krause, F. Rädler, K.-H Rüdiger, G. |
| building | Verbundindex |
| bvnumber | BV042415759 |
| classification_tum | PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)905375161 (DE-599)BVBBV042415759 |
| 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 | 10.1007/978-94-011-0772-3 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>03988nmm a2200565zcb4500</leader><controlfield tag="001">BV042415759</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">20171019 </controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">150316s1993 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789401107723</subfield><subfield code="c">Online</subfield><subfield code="9">978-94-011-0772-3</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9780792325475</subfield><subfield code="c">Print</subfield><subfield code="9">978-0-7923-2547-5</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-94-011-0772-3</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)905375161</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV042415759</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="245" ind1="1" ind2="0"><subfield code="a">The Cosmic Dynamo</subfield><subfield code="b">Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992</subfield><subfield code="c">edited by F. Krause, K.-H. Rädler, G. Rüdiger</subfield></datafield><datafield tag="246" ind1="1" ind2="3"><subfield code="a">Proceedings of the 157th Symposium of the International Astronomical Union held in Potsdam, Germany, September 7--11, 1992</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Dordrecht</subfield><subfield code="b">Springer Netherlands</subfield><subfield code="c">1993</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (XXXII, 499 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="1" ind2=" "><subfield code="a">International Astronomical Union Symposia / Union Astronomique Internationale</subfield><subfield code="v">157</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">This IAU-symposium was the first which was entirely dedicated to dynamo processes, which are fundamental on all cosmical scales. Dynamo theory concerns one of the few truly key questions of recent cosmic physics. There is increasing evidence for the magnetic character of most short-term activity phenomena in astrophysics. Obviously, the triangle "gravity, nuclear power, magnetism" dictates cosmic evolution over a very broad scale of magnitudes. A complicated interplay of rotation, magnetism and turbulence, that is hard to resolve, determines stellar and galactic activity for almost all the short and medium timescales. Behind these multiform phenomena, the cosmic dynamo works in various guise. . "I, all involving inductive and dissipative equilibria in rotating turbulent cosmic plasmas. The Sun, representing the cosmic dynamo par excellence, stands from the beginning at the centre of interest for those who followed the dynamo idea. Even the first models were able to present an explanation of the typical structural appearance of the solar magnetic field, i. e. a 22 year cycle, activity belts and their zonal migration, antisymmetry of t. he magnetic polarity. However, the solar dynamo still provides topics of further discussions, since confrontation with recent observational data raised and still raises new questions, non of which have yet found a plausible answer. These questions represent a challenge for the development of the basic theories: Understanding of turbulence, especially using methods of modern nonlinear physics. Numerical simulations are promising in the near future</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">Magnetfeld</subfield><subfield code="0">(DE-588)4074450-4</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Galaxie</subfield><subfield code="0">(DE-588)4057375-8</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Dynamotheorie</subfield><subfield code="0">(DE-588)4135270-1</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="y">1992</subfield><subfield code="z">Potsdam</subfield><subfield code="2">gnd-content</subfield></datafield><datafield tag="689" ind1="0" ind2="0"><subfield code="a">Galaxie</subfield><subfield code="0">(DE-588)4057375-8</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2="1"><subfield code="a">Magnetfeld</subfield><subfield code="0">(DE-588)4074450-4</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2="2"><subfield code="a">Dynamotheorie</subfield><subfield code="0">(DE-588)4135270-1</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="700" ind1="1" ind2=" "><subfield code="a">Krause, F.</subfield><subfield code="4">edt</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rädler, K.-H.</subfield><subfield code="4">edt</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rüdiger, G.</subfield><subfield code="4">edt</subfield></datafield><datafield tag="830" ind1=" " ind2="0"><subfield code="a">International Astronomical Union Symposia </subfield><subfield code="p">Union Astronomique Internationale</subfield><subfield code="v">157</subfield><subfield code="w">(DE-604)BV000000364</subfield><subfield code="9">157</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-94-011-0772-3</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:BVB01-027851252</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></record></collection> |
| genre | 1\p (DE-588)1071861417 Konferenzschrift 1992 Potsdam gnd-content |
| genre_facet | Konferenzschrift 1992 Potsdam |
| id | DE-604.BV042415759 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:58Z |
| institution | BVB |
| isbn | 9789401107723 9780792325475 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027851252 |
| oclc_num | 905375161 |
| open_access_boolean | |
| owner | DE-91 DE-BY-TUM DE-83 |
| owner_facet | DE-91 DE-BY-TUM DE-83 |
| physical | 1 Online-Ressource (XXXII, 499 p) |
| psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
| publishDate | 1993 |
| publishDateSearch | 1993 |
| publishDateSort | 1993 |
| publisher | Springer Netherlands |
| record_format | marc |
| series | International Astronomical Union Symposia Union Astronomique Internationale |
| series2 | International Astronomical Union Symposia / Union Astronomique Internationale |
| spelling | The Cosmic Dynamo Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992 edited by F. Krause, K.-H. Rädler, G. Rüdiger Proceedings of the 157th Symposium of the International Astronomical Union held in Potsdam, Germany, September 7--11, 1992 Dordrecht Springer Netherlands 1993 1 Online-Ressource (XXXII, 499 p) txt rdacontent c rdamedia cr rdacarrier International Astronomical Union Symposia / Union Astronomique Internationale 157 This IAU-symposium was the first which was entirely dedicated to dynamo processes, which are fundamental on all cosmical scales. Dynamo theory concerns one of the few truly key questions of recent cosmic physics. There is increasing evidence for the magnetic character of most short-term activity phenomena in astrophysics. Obviously, the triangle "gravity, nuclear power, magnetism" dictates cosmic evolution over a very broad scale of magnitudes. A complicated interplay of rotation, magnetism and turbulence, that is hard to resolve, determines stellar and galactic activity for almost all the short and medium timescales. Behind these multiform phenomena, the cosmic dynamo works in various guise. . "I, all involving inductive and dissipative equilibria in rotating turbulent cosmic plasmas. The Sun, representing the cosmic dynamo par excellence, stands from the beginning at the centre of interest for those who followed the dynamo idea. Even the first models were able to present an explanation of the typical structural appearance of the solar magnetic field, i. e. a 22 year cycle, activity belts and their zonal migration, antisymmetry of t. he magnetic polarity. However, the solar dynamo still provides topics of further discussions, since confrontation with recent observational data raised and still raises new questions, non of which have yet found a plausible answer. These questions represent a challenge for the development of the basic theories: Understanding of turbulence, especially using methods of modern nonlinear physics. Numerical simulations are promising in the near future Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Magnetfeld (DE-588)4074450-4 gnd rswk-swf Galaxie (DE-588)4057375-8 gnd rswk-swf Dynamotheorie (DE-588)4135270-1 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift 1992 Potsdam gnd-content Galaxie (DE-588)4057375-8 s Magnetfeld (DE-588)4074450-4 s Dynamotheorie (DE-588)4135270-1 s 2\p DE-604 Krause, F. edt Rädler, K.-H. edt Rüdiger, G. edt International Astronomical Union Symposia Union Astronomique Internationale 157 (DE-604)BV000000364 157 https://doi.org/10.1007/978-94-011-0772-3 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 |
| spellingShingle | The Cosmic Dynamo Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992 International Astronomical Union Symposia Union Astronomique Internationale Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Magnetfeld (DE-588)4074450-4 gnd Galaxie (DE-588)4057375-8 gnd Dynamotheorie (DE-588)4135270-1 gnd |
| subject_GND | (DE-588)4074450-4 (DE-588)4057375-8 (DE-588)4135270-1 (DE-588)1071861417 |
| title | The Cosmic Dynamo Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992 |
| title_alt | Proceedings of the 157th Symposium of the International Astronomical Union held in Potsdam, Germany, September 7--11, 1992 |
| title_auth | The Cosmic Dynamo Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992 |
| title_exact_search | The Cosmic Dynamo Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992 |
| title_full | The Cosmic Dynamo Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992 edited by F. Krause, K.-H. Rädler, G. Rüdiger |
| title_fullStr | The Cosmic Dynamo Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992 edited by F. Krause, K.-H. Rädler, G. Rüdiger |
| title_full_unstemmed | The Cosmic Dynamo Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992 edited by F. Krause, K.-H. Rädler, G. Rüdiger |
| title_short | The Cosmic Dynamo |
| title_sort | the cosmic dynamo proceedings of the 157th symposium of the international astronomical union held in potsdam germany september 7 11 1992 |
| title_sub | Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7–11, 1992 |
| topic | Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Magnetfeld (DE-588)4074450-4 gnd Galaxie (DE-588)4057375-8 gnd Dynamotheorie (DE-588)4135270-1 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Magnetfeld Galaxie Dynamotheorie Konferenzschrift 1992 Potsdam |
| url | https://doi.org/10.1007/978-94-011-0772-3 |
| volume_link | (DE-604)BV000000364 |
| work_keys_str_mv | AT krausef thecosmicdynamoproceedingsofthe157thsymposiumoftheinternationalastronomicalunionheldinpotsdamgermanyseptember7111992 AT radlerkh thecosmicdynamoproceedingsofthe157thsymposiumoftheinternationalastronomicalunionheldinpotsdamgermanyseptember7111992 AT rudigerg thecosmicdynamoproceedingsofthe157thsymposiumoftheinternationalastronomicalunionheldinpotsdamgermanyseptember7111992 AT krausef proceedingsofthe157thsymposiumoftheinternationalastronomicalunionheldinpotsdamgermanyseptember7111992 AT radlerkh proceedingsofthe157thsymposiumoftheinternationalastronomicalunionheldinpotsdamgermanyseptember7111992 AT rudigerg proceedingsofthe157thsymposiumoftheinternationalastronomicalunionheldinpotsdamgermanyseptember7111992 |