Cosmic plasmas and electromagnetic phenomena:
During the past few decades, plasma science has witnessed a great growth in laboratory studies, in simulations, and in space. Plasma is the most common phase of ordinary matter in the universe. It is a state in which ionized matter (even as low as 1%) becomes highly electrically conductive. As such,...
Gespeichert in:
| Format: | Elektronisch E-Book |
|---|---|
| Sprache: | English |
| Veröffentlicht: |
Basel ; Beijing ; Wuhan ; Barcelona ; Belgrade
MDPI
[2019]
|
| Schlagworte: | |
| Online-Zugang: | Volltext https://mdpi.com/books/pdfview/book/1741 |
| Zusammenfassung: | During the past few decades, plasma science has witnessed a great growth in laboratory studies, in simulations, and in space. Plasma is the most common phase of ordinary matter in the universe. It is a state in which ionized matter (even as low as 1%) becomes highly electrically conductive. As such, long-range electric and magnetic fields dominate its behavior. Cosmic plasmas are mostly associated with stars, supernovae, pulsars and neutron stars, quasars and active galaxies at the vicinities of black holes (id est, their jets and accretion disks). Cosmic plasma phenomena can be studied with different methods, such as laboratory experiments, astrophysical observations, and theoretical/computational approaches (id est, MHD, particle-in-cell simulations, et cetera). They exhibit a multitude of complex magnetohydrodynamic behaviors, acceleration, radiation, turbulence, and various instability phenomena. This Special Issue addresses the growing need of the plasma science principles in astrophysics and presents our current understanding of the physics of astrophysical plasmas, their electromagnetic behaviors and properties (e.g., shocks, waves, turbulence, instabilities, collimation, acceleration and radiation), both microscopically and macroscopically. This Special Issue provides a series of state-of-the-art reviews from international experts in the field of cosmic plasmas and electromagnetic phenomena using theoretical approaches, astrophysical observations, laboratory experiments, and state-of-the-art simulation studies |
| Beschreibung: | This is a reprint of articles from the special issue published online in the open access journal Galaxies |
| Beschreibung: | 1 electronic resource (264 pages) |
| ISBN: | 9783039214662 |
Internformat
MARC
| LEADER | 00000nam a2200000 c 4500 | ||
|---|---|---|---|
| 001 | BV046749706 | ||
| 003 | DE-604 | ||
| 005 | 20200824 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 200604s2019 xx o|||| 00||| eng d | ||
| 020 | |a 9783039214662 |c PDF |9 9783039214662 | ||
| 024 | 7 | |a 10.3390/books978-3-03921-466-2 |2 doi | |
| 035 | |a (ZDB-94-OAB)DOAB42600 | ||
| 035 | |a (OCoLC)1164611981 | ||
| 035 | |a (DE-599)HBZHT020324049 | ||
| 040 | |a DE-604 |b ger | ||
| 041 | 0 | |a eng | |
| 049 | |a DE-12 |a DE-210 |a DE-521 |a DE-1102 |a DE-1046 |a DE-1028 |a DE-1050 |a DE-573 |a DE-M347 |a DE-92 |a DE-1051 |a DE-898 |a DE-859 |a DE-860 |a DE-1049 |a DE-861 |a DE-863 |a DE-862 |a DE-Re13 |a DE-Y3 |a DE-255 |a DE-Y7 |a DE-Y2 |a DE-70 |a DE-2174 |a DE-127 |a DE-22 |a DE-155 |a DE-91 |a DE-384 |a DE-473 |a DE-19 |a DE-355 |a DE-703 |a DE-20 |a DE-706 |a DE-824 |a DE-29 |a DE-739 | ||
| 245 | 1 | 0 | |a Cosmic plasmas and electromagnetic phenomena |c special issue editors Athina Meli, Yosuke Mizuno, José L. Gómez |
| 264 | 1 | |a Basel ; Beijing ; Wuhan ; Barcelona ; Belgrade |b MDPI |c [2019] | |
| 300 | |a 1 electronic resource (264 pages) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 500 | |a This is a reprint of articles from the special issue published online in the open access journal Galaxies | ||
| 520 | 3 | |a During the past few decades, plasma science has witnessed a great growth in laboratory studies, in simulations, and in space. Plasma is the most common phase of ordinary matter in the universe. It is a state in which ionized matter (even as low as 1%) becomes highly electrically conductive. As such, long-range electric and magnetic fields dominate its behavior. Cosmic plasmas are mostly associated with stars, supernovae, pulsars and neutron stars, quasars and active galaxies at the vicinities of black holes (id est, their jets and accretion disks). Cosmic plasma phenomena can be studied with different methods, such as laboratory experiments, astrophysical observations, and theoretical/computational approaches (id est, MHD, particle-in-cell simulations, et cetera). They exhibit a multitude of complex magnetohydrodynamic behaviors, acceleration, radiation, turbulence, and various instability phenomena. This Special Issue addresses the growing need of the plasma science principles in astrophysics and presents our current understanding of the physics of astrophysical plasmas, their electromagnetic behaviors and properties (e.g., shocks, waves, turbulence, instabilities, collimation, acceleration and radiation), both microscopically and macroscopically. This Special Issue provides a series of state-of-the-art reviews from international experts in the field of cosmic plasmas and electromagnetic phenomena using theoretical approaches, astrophysical observations, laboratory experiments, and state-of-the-art simulation studies | |
| 546 | |a eng | ||
| 650 | 0 | 7 | |a Astrophysik |0 (DE-588)4003326-0 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Plasma |0 (DE-588)4046249-3 |2 gnd |9 rswk-swf |
| 653 | 0 | |a Science (General) | |
| 653 | 0 | |a Physics | |
| 653 | 0 | |a Astronomy | |
| 689 | 0 | 0 | |a Astrophysik |0 (DE-588)4003326-0 |D s |
| 689 | 0 | 1 | |a Plasma |0 (DE-588)4046249-3 |D s |
| 689 | 0 | |5 DE-604 | |
| 700 | 1 | |a Meli, Athina |e Sonstige |4 oth | |
| 700 | 1 | |a Mizuno, Yosuke |e Sonstige |4 oth | |
| 700 | 1 | |a Gómez, Jose L. |e Sonstige |4 oth | |
| 776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe, Paperback |z 9783039214655 |
| 856 | 4 | 0 | |u https://www.doabooks.org/doab?func=fulltext&uiLanguage=en&rid=42600 |x Verlag |z kostenfrei |3 Volltext |
| 856 | 4 | |u https://mdpi.com/books/pdfview/book/1741 | |
| 912 | |a ZDB-94-OAB | ||
| 943 | 1 | |a oai:aleph.bib-bvb.de:BVB01-032159457 | |
Datensatz im Suchindex
| _version_ | 1822074954183606272 |
|---|---|
| adam_text | |
| adam_txt | |
| any_adam_object | |
| any_adam_object_boolean | |
| building | Verbundindex |
| bvnumber | BV046749706 |
| collection | ZDB-94-OAB |
| ctrlnum | (ZDB-94-OAB)DOAB42600 (OCoLC)1164611981 (DE-599)HBZHT020324049 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>00000nam a2200000 c 4500</leader><controlfield tag="001">BV046749706</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">20200824</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">200604s2019 xx o|||| 00||| eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9783039214662</subfield><subfield code="c">PDF</subfield><subfield code="9">9783039214662</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.3390/books978-3-03921-466-2</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ZDB-94-OAB)DOAB42600</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1164611981</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)HBZHT020324049</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-12</subfield><subfield code="a">DE-210</subfield><subfield code="a">DE-521</subfield><subfield code="a">DE-1102</subfield><subfield code="a">DE-1046</subfield><subfield code="a">DE-1028</subfield><subfield code="a">DE-1050</subfield><subfield code="a">DE-573</subfield><subfield code="a">DE-M347</subfield><subfield code="a">DE-92</subfield><subfield code="a">DE-1051</subfield><subfield code="a">DE-898</subfield><subfield code="a">DE-859</subfield><subfield code="a">DE-860</subfield><subfield code="a">DE-1049</subfield><subfield code="a">DE-861</subfield><subfield code="a">DE-863</subfield><subfield code="a">DE-862</subfield><subfield code="a">DE-Re13</subfield><subfield code="a">DE-Y3</subfield><subfield code="a">DE-255</subfield><subfield code="a">DE-Y7</subfield><subfield code="a">DE-Y2</subfield><subfield code="a">DE-70</subfield><subfield code="a">DE-2174</subfield><subfield code="a">DE-127</subfield><subfield code="a">DE-22</subfield><subfield code="a">DE-155</subfield><subfield code="a">DE-91</subfield><subfield code="a">DE-384</subfield><subfield code="a">DE-473</subfield><subfield code="a">DE-19</subfield><subfield code="a">DE-355</subfield><subfield code="a">DE-703</subfield><subfield code="a">DE-20</subfield><subfield code="a">DE-706</subfield><subfield code="a">DE-824</subfield><subfield code="a">DE-29</subfield><subfield code="a">DE-739</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Cosmic plasmas and electromagnetic phenomena</subfield><subfield code="c">special issue editors Athina Meli, Yosuke Mizuno, José L. Gómez</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Basel ; Beijing ; Wuhan ; Barcelona ; Belgrade</subfield><subfield code="b">MDPI</subfield><subfield code="c">[2019]</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 electronic resource (264 pages)</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="500" ind1=" " ind2=" "><subfield code="a">This is a reprint of articles from the special issue published online in the open access journal Galaxies</subfield></datafield><datafield tag="520" ind1="3" ind2=" "><subfield code="a">During the past few decades, plasma science has witnessed a great growth in laboratory studies, in simulations, and in space. Plasma is the most common phase of ordinary matter in the universe. It is a state in which ionized matter (even as low as 1%) becomes highly electrically conductive. As such, long-range electric and magnetic fields dominate its behavior. Cosmic plasmas are mostly associated with stars, supernovae, pulsars and neutron stars, quasars and active galaxies at the vicinities of black holes (id est, their jets and accretion disks). Cosmic plasma phenomena can be studied with different methods, such as laboratory experiments, astrophysical observations, and theoretical/computational approaches (id est, MHD, particle-in-cell simulations, et cetera). They exhibit a multitude of complex magnetohydrodynamic behaviors, acceleration, radiation, turbulence, and various instability phenomena. This Special Issue addresses the growing need of the plasma science principles in astrophysics and presents our current understanding of the physics of astrophysical plasmas, their electromagnetic behaviors and properties (e.g., shocks, waves, turbulence, instabilities, collimation, acceleration and radiation), both microscopically and macroscopically. This Special Issue provides a series of state-of-the-art reviews from international experts in the field of cosmic plasmas and electromagnetic phenomena using theoretical approaches, astrophysical observations, laboratory experiments, and state-of-the-art simulation studies</subfield></datafield><datafield tag="546" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Astrophysik</subfield><subfield code="0">(DE-588)4003326-0</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Plasma</subfield><subfield code="0">(DE-588)4046249-3</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Science (General)</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Physics</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Astronomy</subfield></datafield><datafield tag="689" ind1="0" ind2="0"><subfield code="a">Astrophysik</subfield><subfield code="0">(DE-588)4003326-0</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2="1"><subfield code="a">Plasma</subfield><subfield code="0">(DE-588)4046249-3</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2=" "><subfield code="5">DE-604</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Meli, Athina</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Mizuno, Yosuke</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Gómez, Jose L.</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druck-Ausgabe, Paperback</subfield><subfield code="z">9783039214655</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://www.doabooks.org/doab?func=fulltext&uiLanguage=en&rid=42600</subfield><subfield code="x">Verlag</subfield><subfield code="z">kostenfrei</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="856" ind1="4" ind2=" "><subfield code="u">https://mdpi.com/books/pdfview/book/1741</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-94-OAB</subfield></datafield><datafield tag="943" ind1="1" ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-032159457</subfield></datafield></record></collection> |
| id | DE-604.BV046749706 |
| illustrated | Not Illustrated |
| index_date | 2024-07-03T14:41:39Z |
| indexdate | 2025-01-23T21:01:26Z |
| institution | BVB |
| isbn | 9783039214662 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-032159457 |
| oclc_num | 1164611981 |
| open_access_boolean | 1 |
| owner | DE-12 DE-210 DE-521 DE-1102 DE-1046 DE-1028 DE-1050 DE-573 DE-M347 DE-92 DE-1051 DE-898 DE-BY-UBR DE-859 DE-860 DE-1049 DE-861 DE-863 DE-BY-FWS DE-862 DE-BY-FWS DE-Re13 DE-BY-UBR DE-Y3 DE-255 DE-Y7 DE-Y2 DE-70 DE-2174 DE-127 DE-22 DE-BY-UBG DE-155 DE-BY-UBR DE-91 DE-BY-TUM DE-384 DE-473 DE-BY-UBG DE-19 DE-BY-UBM DE-355 DE-BY-UBR DE-703 DE-20 DE-706 DE-824 DE-29 DE-739 |
| owner_facet | DE-12 DE-210 DE-521 DE-1102 DE-1046 DE-1028 DE-1050 DE-573 DE-M347 DE-92 DE-1051 DE-898 DE-BY-UBR DE-859 DE-860 DE-1049 DE-861 DE-863 DE-BY-FWS DE-862 DE-BY-FWS DE-Re13 DE-BY-UBR DE-Y3 DE-255 DE-Y7 DE-Y2 DE-70 DE-2174 DE-127 DE-22 DE-BY-UBG DE-155 DE-BY-UBR DE-91 DE-BY-TUM DE-384 DE-473 DE-BY-UBG DE-19 DE-BY-UBM DE-355 DE-BY-UBR DE-703 DE-20 DE-706 DE-824 DE-29 DE-739 |
| physical | 1 electronic resource (264 pages) |
| psigel | ZDB-94-OAB |
| publishDate | 2019 |
| publishDateSearch | 2019 |
| publishDateSort | 2019 |
| publisher | MDPI |
| record_format | marc |
| spelling | Cosmic plasmas and electromagnetic phenomena special issue editors Athina Meli, Yosuke Mizuno, José L. Gómez Basel ; Beijing ; Wuhan ; Barcelona ; Belgrade MDPI [2019] 1 electronic resource (264 pages) txt rdacontent c rdamedia cr rdacarrier This is a reprint of articles from the special issue published online in the open access journal Galaxies During the past few decades, plasma science has witnessed a great growth in laboratory studies, in simulations, and in space. Plasma is the most common phase of ordinary matter in the universe. It is a state in which ionized matter (even as low as 1%) becomes highly electrically conductive. As such, long-range electric and magnetic fields dominate its behavior. Cosmic plasmas are mostly associated with stars, supernovae, pulsars and neutron stars, quasars and active galaxies at the vicinities of black holes (id est, their jets and accretion disks). Cosmic plasma phenomena can be studied with different methods, such as laboratory experiments, astrophysical observations, and theoretical/computational approaches (id est, MHD, particle-in-cell simulations, et cetera). They exhibit a multitude of complex magnetohydrodynamic behaviors, acceleration, radiation, turbulence, and various instability phenomena. This Special Issue addresses the growing need of the plasma science principles in astrophysics and presents our current understanding of the physics of astrophysical plasmas, their electromagnetic behaviors and properties (e.g., shocks, waves, turbulence, instabilities, collimation, acceleration and radiation), both microscopically and macroscopically. This Special Issue provides a series of state-of-the-art reviews from international experts in the field of cosmic plasmas and electromagnetic phenomena using theoretical approaches, astrophysical observations, laboratory experiments, and state-of-the-art simulation studies eng Astrophysik (DE-588)4003326-0 gnd rswk-swf Plasma (DE-588)4046249-3 gnd rswk-swf Science (General) Physics Astronomy Astrophysik (DE-588)4003326-0 s Plasma (DE-588)4046249-3 s DE-604 Meli, Athina Sonstige oth Mizuno, Yosuke Sonstige oth Gómez, Jose L. Sonstige oth Erscheint auch als Druck-Ausgabe, Paperback 9783039214655 https://www.doabooks.org/doab?func=fulltext&uiLanguage=en&rid=42600 Verlag kostenfrei Volltext https://mdpi.com/books/pdfview/book/1741 |
| spellingShingle | Cosmic plasmas and electromagnetic phenomena Astrophysik (DE-588)4003326-0 gnd Plasma (DE-588)4046249-3 gnd |
| subject_GND | (DE-588)4003326-0 (DE-588)4046249-3 |
| title | Cosmic plasmas and electromagnetic phenomena |
| title_auth | Cosmic plasmas and electromagnetic phenomena |
| title_exact_search | Cosmic plasmas and electromagnetic phenomena |
| title_exact_search_txtP | Cosmic plasmas and electromagnetic phenomena |
| title_full | Cosmic plasmas and electromagnetic phenomena special issue editors Athina Meli, Yosuke Mizuno, José L. Gómez |
| title_fullStr | Cosmic plasmas and electromagnetic phenomena special issue editors Athina Meli, Yosuke Mizuno, José L. Gómez |
| title_full_unstemmed | Cosmic plasmas and electromagnetic phenomena special issue editors Athina Meli, Yosuke Mizuno, José L. Gómez |
| title_short | Cosmic plasmas and electromagnetic phenomena |
| title_sort | cosmic plasmas and electromagnetic phenomena |
| topic | Astrophysik (DE-588)4003326-0 gnd Plasma (DE-588)4046249-3 gnd |
| topic_facet | Astrophysik Plasma |
| url | https://www.doabooks.org/doab?func=fulltext&uiLanguage=en&rid=42600 https://mdpi.com/books/pdfview/book/1741 |
| work_keys_str_mv | AT meliathina cosmicplasmasandelectromagneticphenomena AT mizunoyosuke cosmicplasmasandelectromagneticphenomena AT gomezjosel cosmicplasmasandelectromagneticphenomena |