Solar Flares and Collisions between Current-Carrying Loops: Types and Mechanisms of Solar Flares and Coronal Loop Heating
In this volume we compare modem observations of solar flares with results from recent theoretical research and simulation studies on current-carrying loops and their interaction. These topics have undergone rapid developments in the course of recent years. Observational results by X-ray monitoring a...
Gespeichert in:
| Weitere Verfasser: | , |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1996
|
| Schlagworte: | |
| Online-Zugang: | BTU01 Volltext |
| Zusammenfassung: | In this volume we compare modem observations of solar flares with results from recent theoretical research and simulation studies on current-carrying loops and their interaction. These topics have undergone rapid developments in the course of recent years. Observational results by X-ray monitoring and imaging spacecraft in the seventies and by dedicated imaging instrumentation in the satellites Solar Max imum Mission and Hinotori, launched 1980 and 1981, have shown the importance of X-ray imaging for understanding the ignition processes of solar flares. Such observations, in tum, stimulated theoretical studies, centered around the flux-tube concept. The classical idea that flares originate by interaction of current-carrying loops was developed and proved to be promising. Concepts on reconnection and coalescence of flux tubes were developed, and their consequences studied. The Yohkoh spacecraft, launched 1991, showed the overwhelming importance of coro nal flux tubes and their many possible ways of interaction. Subsequent and parallel theoretical studies and simulations, differentiating between the topology of interact ing fluxtubes, demonstrated that the mutual positioning and the way of interaction are important for the subsequent processes of energy release in flares and the many associated phenomena such as the expUlsion of jets and the emission of X -ray and microwave radiation. The new developments now enable researchers to understand and classify flares in a physically significant way. Various processes of accelera tion are active in and after flares on greatly varying timescales; these can now be distinguished and explained |
| Beschreibung: | 1 Online-Ressource (VI, 192 p) |
| ISBN: | 9789400903319 |
| DOI: | 10.1007/978-94-009-0331-9 |
Internformat
MARC
| LEADER | 00000nmm a2200000zc 4500 | ||
|---|---|---|---|
| 001 | BV045178820 | ||
| 003 | DE-604 | ||
| 005 | 20210530 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 180911s1996 |||| o||u| ||||||eng d | ||
| 020 | |a 9789400903319 |9 978-94-009-0331-9 | ||
| 024 | 7 | |a 10.1007/978-94-009-0331-9 |2 doi | |
| 035 | |a (ZDB-2-EES)978-94-009-0331-9 | ||
| 035 | |a (OCoLC)1053800409 | ||
| 035 | |a (DE-599)BVBBV045178820 | ||
| 040 | |a DE-604 |b ger |e aacr | ||
| 041 | 0 | |a eng | |
| 049 | |a DE-634 | ||
| 082 | 0 | |a 523.4 |2 23 | |
| 245 | 1 | 0 | |a Solar Flares and Collisions between Current-Carrying Loops |b Types and Mechanisms of Solar Flares and Coronal Loop Heating |c edited by Jun-Ichi Sakai, Cornelis De Jager |
| 264 | 1 | |a Dordrecht |b Springer Netherlands |c 1996 | |
| 300 | |a 1 Online-Ressource (VI, 192 p) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 520 | |a In this volume we compare modem observations of solar flares with results from recent theoretical research and simulation studies on current-carrying loops and their interaction. These topics have undergone rapid developments in the course of recent years. Observational results by X-ray monitoring and imaging spacecraft in the seventies and by dedicated imaging instrumentation in the satellites Solar Max imum Mission and Hinotori, launched 1980 and 1981, have shown the importance of X-ray imaging for understanding the ignition processes of solar flares. Such observations, in tum, stimulated theoretical studies, centered around the flux-tube concept. The classical idea that flares originate by interaction of current-carrying loops was developed and proved to be promising. Concepts on reconnection and coalescence of flux tubes were developed, and their consequences studied. The Yohkoh spacecraft, launched 1991, showed the overwhelming importance of coro nal flux tubes and their many possible ways of interaction. Subsequent and parallel theoretical studies and simulations, differentiating between the topology of interact ing fluxtubes, demonstrated that the mutual positioning and the way of interaction are important for the subsequent processes of energy release in flares and the many associated phenomena such as the expUlsion of jets and the emission of X -ray and microwave radiation. The new developments now enable researchers to understand and classify flares in a physically significant way. Various processes of accelera tion are active in and after flares on greatly varying timescales; these can now be distinguished and explained | ||
| 650 | 4 | |a Earth Sciences | |
| 650 | 4 | |a Planetology | |
| 650 | 4 | |a Astrophysics and Astroparticles | |
| 650 | 4 | |a Nuclear Physics, Heavy Ions, Hadrons | |
| 650 | 4 | |a Earth sciences | |
| 650 | 4 | |a Planetology | |
| 650 | 4 | |a Astrophysics | |
| 650 | 4 | |a Nuclear physics | |
| 650 | 4 | |a Heavy ions | |
| 650 | 4 | |a Hadrons | |
| 700 | 1 | |a Sakai, Jun-Ichi |d 1936- |0 (DE-588)172550394 |4 edt | |
| 700 | 1 | |a Jager, Cornelis de |d 1921-2021 |0 (DE-588)127810188 |4 edt | |
| 776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe |z 9789401066358 |
| 856 | 4 | 0 | |u https://doi.org/10.1007/978-94-009-0331-9 |x Verlag |z URL des Erstveröffentlichers |3 Volltext |
| 912 | |a ZDB-2-EES | ||
| 940 | 1 | |q ZDB-2-EES_Archiv | |
| 999 | |a oai:aleph.bib-bvb.de:BVB01-030568050 | ||
| 966 | e | |u https://doi.org/10.1007/978-94-009-0331-9 |l BTU01 |p ZDB-2-EES |q ZDB-2-EES_Archiv |x Verlag |3 Volltext | |
Datensatz im Suchindex
| _version_ | 1804178869619523584 |
|---|---|
| any_adam_object | |
| author2 | Sakai, Jun-Ichi 1936- Jager, Cornelis de 1921-2021 |
| author2_role | edt edt |
| author2_variant | j i s jis c d j cd cdj |
| author_GND | (DE-588)172550394 (DE-588)127810188 |
| author_facet | Sakai, Jun-Ichi 1936- Jager, Cornelis de 1921-2021 |
| building | Verbundindex |
| bvnumber | BV045178820 |
| collection | ZDB-2-EES |
| ctrlnum | (ZDB-2-EES)978-94-009-0331-9 (OCoLC)1053800409 (DE-599)BVBBV045178820 |
| dewey-full | 523.4 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.4 |
| dewey-search | 523.4 |
| dewey-sort | 3523.4 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-009-0331-9 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>03405nmm a2200493zc 4500</leader><controlfield tag="001">BV045178820</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">20210530 </controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">180911s1996 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789400903319</subfield><subfield code="9">978-94-009-0331-9</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-94-009-0331-9</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ZDB-2-EES)978-94-009-0331-9</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1053800409</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV045178820</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-634</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">523.4</subfield><subfield code="2">23</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Solar Flares and Collisions between Current-Carrying Loops</subfield><subfield code="b">Types and Mechanisms of Solar Flares and Coronal Loop Heating</subfield><subfield code="c">edited by Jun-Ichi Sakai, Cornelis De Jager</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Dordrecht</subfield><subfield code="b">Springer Netherlands</subfield><subfield code="c">1996</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (VI, 192 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="520" ind1=" " ind2=" "><subfield code="a">In this volume we compare modem observations of solar flares with results from recent theoretical research and simulation studies on current-carrying loops and their interaction. These topics have undergone rapid developments in the course of recent years. Observational results by X-ray monitoring and imaging spacecraft in the seventies and by dedicated imaging instrumentation in the satellites Solar Max imum Mission and Hinotori, launched 1980 and 1981, have shown the importance of X-ray imaging for understanding the ignition processes of solar flares. Such observations, in tum, stimulated theoretical studies, centered around the flux-tube concept. The classical idea that flares originate by interaction of current-carrying loops was developed and proved to be promising. Concepts on reconnection and coalescence of flux tubes were developed, and their consequences studied. The Yohkoh spacecraft, launched 1991, showed the overwhelming importance of coro nal flux tubes and their many possible ways of interaction. Subsequent and parallel theoretical studies and simulations, differentiating between the topology of interact ing fluxtubes, demonstrated that the mutual positioning and the way of interaction are important for the subsequent processes of energy release in flares and the many associated phenomena such as the expUlsion of jets and the emission of X -ray and microwave radiation. The new developments now enable researchers to understand and classify flares in a physically significant way. Various processes of accelera tion are active in and after flares on greatly varying timescales; these can now be distinguished and explained</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Earth Sciences</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Planetology</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">Nuclear Physics, Heavy Ions, Hadrons</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Earth sciences</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Planetology</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Astrophysics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Nuclear physics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Heavy ions</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Hadrons</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sakai, Jun-Ichi</subfield><subfield code="d">1936-</subfield><subfield code="0">(DE-588)172550394</subfield><subfield code="4">edt</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Jager, Cornelis de</subfield><subfield code="d">1921-2021</subfield><subfield code="0">(DE-588)127810188</subfield><subfield code="4">edt</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druck-Ausgabe</subfield><subfield code="z">9789401066358</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-94-009-0331-9</subfield><subfield code="x">Verlag</subfield><subfield code="z">URL des Erstveröffentlichers</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-2-EES</subfield></datafield><datafield tag="940" ind1="1" ind2=" "><subfield code="q">ZDB-2-EES_Archiv</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-030568050</subfield></datafield><datafield tag="966" ind1="e" ind2=" "><subfield code="u">https://doi.org/10.1007/978-94-009-0331-9</subfield><subfield code="l">BTU01</subfield><subfield code="p">ZDB-2-EES</subfield><subfield code="q">ZDB-2-EES_Archiv</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield></record></collection> |
| id | DE-604.BV045178820 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T08:10:50Z |
| institution | BVB |
| isbn | 9789400903319 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-030568050 |
| oclc_num | 1053800409 |
| open_access_boolean | |
| owner | DE-634 |
| owner_facet | DE-634 |
| physical | 1 Online-Ressource (VI, 192 p) |
| psigel | ZDB-2-EES ZDB-2-EES_Archiv ZDB-2-EES ZDB-2-EES_Archiv |
| publishDate | 1996 |
| publishDateSearch | 1996 |
| publishDateSort | 1996 |
| publisher | Springer Netherlands |
| record_format | marc |
| spelling | Solar Flares and Collisions between Current-Carrying Loops Types and Mechanisms of Solar Flares and Coronal Loop Heating edited by Jun-Ichi Sakai, Cornelis De Jager Dordrecht Springer Netherlands 1996 1 Online-Ressource (VI, 192 p) txt rdacontent c rdamedia cr rdacarrier In this volume we compare modem observations of solar flares with results from recent theoretical research and simulation studies on current-carrying loops and their interaction. These topics have undergone rapid developments in the course of recent years. Observational results by X-ray monitoring and imaging spacecraft in the seventies and by dedicated imaging instrumentation in the satellites Solar Max imum Mission and Hinotori, launched 1980 and 1981, have shown the importance of X-ray imaging for understanding the ignition processes of solar flares. Such observations, in tum, stimulated theoretical studies, centered around the flux-tube concept. The classical idea that flares originate by interaction of current-carrying loops was developed and proved to be promising. Concepts on reconnection and coalescence of flux tubes were developed, and their consequences studied. The Yohkoh spacecraft, launched 1991, showed the overwhelming importance of coro nal flux tubes and their many possible ways of interaction. Subsequent and parallel theoretical studies and simulations, differentiating between the topology of interact ing fluxtubes, demonstrated that the mutual positioning and the way of interaction are important for the subsequent processes of energy release in flares and the many associated phenomena such as the expUlsion of jets and the emission of X -ray and microwave radiation. The new developments now enable researchers to understand and classify flares in a physically significant way. Various processes of accelera tion are active in and after flares on greatly varying timescales; these can now be distinguished and explained Earth Sciences Planetology Astrophysics and Astroparticles Nuclear Physics, Heavy Ions, Hadrons Earth sciences Astrophysics Nuclear physics Heavy ions Hadrons Sakai, Jun-Ichi 1936- (DE-588)172550394 edt Jager, Cornelis de 1921-2021 (DE-588)127810188 edt Erscheint auch als Druck-Ausgabe 9789401066358 https://doi.org/10.1007/978-94-009-0331-9 Verlag URL des Erstveröffentlichers Volltext |
| spellingShingle | Solar Flares and Collisions between Current-Carrying Loops Types and Mechanisms of Solar Flares and Coronal Loop Heating Earth Sciences Planetology Astrophysics and Astroparticles Nuclear Physics, Heavy Ions, Hadrons Earth sciences Astrophysics Nuclear physics Heavy ions Hadrons |
| title | Solar Flares and Collisions between Current-Carrying Loops Types and Mechanisms of Solar Flares and Coronal Loop Heating |
| title_auth | Solar Flares and Collisions between Current-Carrying Loops Types and Mechanisms of Solar Flares and Coronal Loop Heating |
| title_exact_search | Solar Flares and Collisions between Current-Carrying Loops Types and Mechanisms of Solar Flares and Coronal Loop Heating |
| title_full | Solar Flares and Collisions between Current-Carrying Loops Types and Mechanisms of Solar Flares and Coronal Loop Heating edited by Jun-Ichi Sakai, Cornelis De Jager |
| title_fullStr | Solar Flares and Collisions between Current-Carrying Loops Types and Mechanisms of Solar Flares and Coronal Loop Heating edited by Jun-Ichi Sakai, Cornelis De Jager |
| title_full_unstemmed | Solar Flares and Collisions between Current-Carrying Loops Types and Mechanisms of Solar Flares and Coronal Loop Heating edited by Jun-Ichi Sakai, Cornelis De Jager |
| title_short | Solar Flares and Collisions between Current-Carrying Loops |
| title_sort | solar flares and collisions between current carrying loops types and mechanisms of solar flares and coronal loop heating |
| title_sub | Types and Mechanisms of Solar Flares and Coronal Loop Heating |
| topic | Earth Sciences Planetology Astrophysics and Astroparticles Nuclear Physics, Heavy Ions, Hadrons Earth sciences Astrophysics Nuclear physics Heavy ions Hadrons |
| topic_facet | Earth Sciences Planetology Astrophysics and Astroparticles Nuclear Physics, Heavy Ions, Hadrons Earth sciences Astrophysics Nuclear physics Heavy ions Hadrons |
| url | https://doi.org/10.1007/978-94-009-0331-9 |
| work_keys_str_mv | AT sakaijunichi solarflaresandcollisionsbetweencurrentcarryingloopstypesandmechanismsofsolarflaresandcoronalloopheating AT jagercornelisde solarflaresandcollisionsbetweencurrentcarryingloopstypesandmechanismsofsolarflaresandcoronalloopheating |