Parameters of quiescent prominences derived from magnetic field measurements

Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower.

Gespeichert in:

Autor*in:	Anzer, Ulrich [verfasserIn]

Format:	Artikel
Sprache:	Englisch

Erschienen:	1995

Schlagwörter:	Magnetic Field Field Vector Field Measurement Vector Measurement Magnetic Field Vector

Anmerkung:	© Kluwer Academic Publishers 1995

Übergeordnetes Werk:	Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 161(1995), 1 vom: Okt., Seite 49-55
Übergeordnetes Werk:	volume:161 ; year:1995 ; number:1 ; month:10 ; pages:49-55

Links:	Volltext

DOI / URN:	10.1007/BF00732083

Katalog-ID:	OLC2033578623

Internformat


LEADER	01000caa a22002652 4500
001	OLC2033578623
003	DE-627
005	20230504045605.0
007	tu
008	200819s1995 xx \|\|\|\|\| 00\| \|\|eng c
024	7		\|a 10.1007/BF00732083 \|2 doi
035			\|a (DE-627)OLC2033578623
035			\|a (DE-He213)BF00732083-p
040			\|a DE-627 \|b ger \|c DE-627 \|e rakwb
041			\|a eng
082	0	4	\|a 530 \|q VZ
084			\|a 16,12 \|2 ssgn
100	1		\|a Anzer, Ulrich \|e verfasserin \|4 aut
245	1	0	\|a Parameters of quiescent prominences derived from magnetic field measurements
264		1	\|c 1995
336			\|a Text \|b txt \|2 rdacontent
337			\|a ohne Hilfsmittel zu benutzen \|b n \|2 rdamedia
338			\|a Band \|b nc \|2 rdacarrier
500			\|a © Kluwer Academic Publishers 1995
520			\|a Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower.
650		4	\|a Magnetic Field
650		4	\|a Field Vector
650		4	\|a Field Measurement
650		4	\|a Vector Measurement
650		4	\|a Magnetic Field Vector
773	0	8	\|i Enthalten in \|t Solar physics \|d Kluwer Academic Publishers, 1967 \|g 161(1995), 1 vom: Okt., Seite 49-55 \|w (DE-627)129856010 \|w (DE-600)281593-X \|w (DE-576)015160033 \|x 0038-0938 \|7 nnns
773	1	8	\|g volume:161 \|g year:1995 \|g number:1 \|g month:10 \|g pages:49-55
856	4	1	\|u https://doi.org/10.1007/BF00732083 \|z lizenzpflichtig \|3 Volltext
912			\|a GBV_USEFLAG_A
912			\|a SYSFLAG_A
912			\|a GBV_OLC
912			\|a SSG-OLC-PHY
912			\|a SSG-OLC-AST
912			\|a SSG-OPC-AST
912			\|a GBV_ILN_11
912			\|a GBV_ILN_22
912			\|a GBV_ILN_40
912			\|a GBV_ILN_47
912			\|a GBV_ILN_70
912			\|a GBV_ILN_2002
912			\|a GBV_ILN_2279
912			\|a GBV_ILN_2286
912			\|a GBV_ILN_4012
912			\|a GBV_ILN_4306
951			\|a AR
952			\|d 161 \|j 1995 \|e 1 \|c 10 \|h 49-55

Indexfelder

author_variant	u a ua
matchkey_str	article:00380938:1995----::aaeesfuecnpoiecseiefomgei
hierarchy_sort_str	1995
publishDate	1995
allfields	10.1007/BF00732083 doi (DE-627)OLC2033578623 (DE-He213)BF00732083-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Anzer, Ulrich verfasserin aut Parameters of quiescent prominences derived from magnetic field measurements 1995 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1995 Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower. Magnetic Field Field Vector Field Measurement Vector Measurement Magnetic Field Vector Enthalten in Solar physics Kluwer Academic Publishers, 1967 161(1995), 1 vom: Okt., Seite 49-55 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:161 year:1995 number:1 month:10 pages:49-55 https://doi.org/10.1007/BF00732083 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 161 1995 1 10 49-55
spelling	10.1007/BF00732083 doi (DE-627)OLC2033578623 (DE-He213)BF00732083-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Anzer, Ulrich verfasserin aut Parameters of quiescent prominences derived from magnetic field measurements 1995 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1995 Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower. Magnetic Field Field Vector Field Measurement Vector Measurement Magnetic Field Vector Enthalten in Solar physics Kluwer Academic Publishers, 1967 161(1995), 1 vom: Okt., Seite 49-55 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:161 year:1995 number:1 month:10 pages:49-55 https://doi.org/10.1007/BF00732083 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 161 1995 1 10 49-55
allfields_unstemmed	10.1007/BF00732083 doi (DE-627)OLC2033578623 (DE-He213)BF00732083-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Anzer, Ulrich verfasserin aut Parameters of quiescent prominences derived from magnetic field measurements 1995 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1995 Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower. Magnetic Field Field Vector Field Measurement Vector Measurement Magnetic Field Vector Enthalten in Solar physics Kluwer Academic Publishers, 1967 161(1995), 1 vom: Okt., Seite 49-55 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:161 year:1995 number:1 month:10 pages:49-55 https://doi.org/10.1007/BF00732083 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 161 1995 1 10 49-55
allfieldsGer	10.1007/BF00732083 doi (DE-627)OLC2033578623 (DE-He213)BF00732083-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Anzer, Ulrich verfasserin aut Parameters of quiescent prominences derived from magnetic field measurements 1995 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1995 Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower. Magnetic Field Field Vector Field Measurement Vector Measurement Magnetic Field Vector Enthalten in Solar physics Kluwer Academic Publishers, 1967 161(1995), 1 vom: Okt., Seite 49-55 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:161 year:1995 number:1 month:10 pages:49-55 https://doi.org/10.1007/BF00732083 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 161 1995 1 10 49-55
allfieldsSound	10.1007/BF00732083 doi (DE-627)OLC2033578623 (DE-He213)BF00732083-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Anzer, Ulrich verfasserin aut Parameters of quiescent prominences derived from magnetic field measurements 1995 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1995 Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower. Magnetic Field Field Vector Field Measurement Vector Measurement Magnetic Field Vector Enthalten in Solar physics Kluwer Academic Publishers, 1967 161(1995), 1 vom: Okt., Seite 49-55 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:161 year:1995 number:1 month:10 pages:49-55 https://doi.org/10.1007/BF00732083 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 161 1995 1 10 49-55
language	English
source	Enthalten in Solar physics 161(1995), 1 vom: Okt., Seite 49-55 volume:161 year:1995 number:1 month:10 pages:49-55
sourceStr	Enthalten in Solar physics 161(1995), 1 vom: Okt., Seite 49-55 volume:161 year:1995 number:1 month:10 pages:49-55
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Magnetic Field Field Vector Field Measurement Vector Measurement Magnetic Field Vector
dewey-raw	530
isfreeaccess_bool	false
container_title	Solar physics
authorswithroles_txt_mv	Anzer, Ulrich @@aut@@
publishDateDaySort_date	1995-10-01T00:00:00Z
hierarchy_top_id	129856010
dewey-sort	3530
id	OLC2033578623
language_de	englisch
fullrecord	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2033578623</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504045605.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s1995 xx \|\|\|\|\| 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/BF00732083</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2033578623</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)BF00732083-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Anzer, Ulrich</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Parameters of quiescent prominences derived from magnetic field measurements</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1995</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Kluwer Academic Publishers 1995</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Magnetic Field</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Field Vector</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Field Measurement</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Vector Measurement</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Magnetic Field Vector</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Solar physics</subfield><subfield code="d">Kluwer Academic Publishers, 1967</subfield><subfield code="g">161(1995), 1 vom: Okt., Seite 49-55</subfield><subfield code="w">(DE-627)129856010</subfield><subfield code="w">(DE-600)281593-X</subfield><subfield code="w">(DE-576)015160033</subfield><subfield code="x">0038-0938</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:161</subfield><subfield code="g">year:1995</subfield><subfield code="g">number:1</subfield><subfield code="g">month:10</subfield><subfield code="g">pages:49-55</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF00732083</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2002</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2286</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">161</subfield><subfield code="j">1995</subfield><subfield code="e">1</subfield><subfield code="c">10</subfield><subfield code="h">49-55</subfield></datafield></record></collection>
author	Anzer, Ulrich
spellingShingle	Anzer, Ulrich ddc 530 ssgn 16,12 misc Magnetic Field misc Field Vector misc Field Measurement misc Vector Measurement misc Magnetic Field Vector Parameters of quiescent prominences derived from magnetic field measurements
authorStr	Anzer, Ulrich
ppnlink_with_tag_str_mv	@@773@@(DE-627)129856010
format	Article
dewey-ones	530 - Physics
delete_txt_mv	keep
author_role	aut
collection	OLC
remote_str	false
illustrated	Not Illustrated
issn	0038-0938
topic_title	530 VZ 16,12 ssgn Parameters of quiescent prominences derived from magnetic field measurements Magnetic Field Field Vector Field Measurement Vector Measurement Magnetic Field Vector
topic	ddc 530 ssgn 16,12 misc Magnetic Field misc Field Vector misc Field Measurement misc Vector Measurement misc Magnetic Field Vector
topic_unstemmed	ddc 530 ssgn 16,12 misc Magnetic Field misc Field Vector misc Field Measurement misc Vector Measurement misc Magnetic Field Vector
topic_browse	ddc 530 ssgn 16,12 misc Magnetic Field misc Field Vector misc Field Measurement misc Vector Measurement misc Magnetic Field Vector
format_facet	Aufsätze Gedruckte Aufsätze
format_main_str_mv	Text Zeitschrift/Artikel
carriertype_str_mv	nc
hierarchy_parent_title	Solar physics
hierarchy_parent_id	129856010
dewey-tens	530 - Physics
hierarchy_top_title	Solar physics
isfreeaccess_txt	false
familylinks_str_mv	(DE-627)129856010 (DE-600)281593-X (DE-576)015160033
title	Parameters of quiescent prominences derived from magnetic field measurements
ctrlnum	(DE-627)OLC2033578623 (DE-He213)BF00732083-p
title_full	Parameters of quiescent prominences derived from magnetic field measurements
author_sort	Anzer, Ulrich
journal	Solar physics
journalStr	Solar physics
lang_code	eng
isOA_bool	false
dewey-hundreds	500 - Science
recordtype	marc
publishDateSort	1995
contenttype_str_mv	txt
container_start_page	49
author_browse	Anzer, Ulrich
container_volume	161
class	530 VZ 16,12 ssgn
format_se	Aufsätze
author-letter	Anzer, Ulrich
doi_str_mv	10.1007/BF00732083
dewey-full	530
title_sort	parameters of quiescent prominences derived from magnetic field measurements
title_auth	Parameters of quiescent prominences derived from magnetic field measurements
abstract	Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower. © Kluwer Academic Publishers 1995
abstractGer	Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower. © Kluwer Academic Publishers 1995
abstract_unstemmed	Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower. © Kluwer Academic Publishers 1995
collection_details	GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306
container_issue	1
title_short	Parameters of quiescent prominences derived from magnetic field measurements
url	https://doi.org/10.1007/BF00732083
remote_bool	false
ppnlink	129856010
mediatype_str_mv	n
isOA_txt	false
hochschulschrift_bool	false
doi_str	10.1007/BF00732083
up_date	2024-07-03T17:32:47.748Z
_version_	1803580046309326850
fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2033578623</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504045605.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s1995 xx \|\|\|\|\| 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/BF00732083</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2033578623</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)BF00732083-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Anzer, Ulrich</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Parameters of quiescent prominences derived from magnetic field measurements</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1995</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Kluwer Academic Publishers 1995</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Based upon the new magnetic field vector measurements of Bommieret al. (1994) we construct prominence models which are in magnetohydrostatic equilibrium. We compare these new models with earlier ones and find that they are on average more massive and also considerably narrower.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Magnetic Field</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Field Vector</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Field Measurement</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Vector Measurement</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Magnetic Field Vector</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Solar physics</subfield><subfield code="d">Kluwer Academic Publishers, 1967</subfield><subfield code="g">161(1995), 1 vom: Okt., Seite 49-55</subfield><subfield code="w">(DE-627)129856010</subfield><subfield code="w">(DE-600)281593-X</subfield><subfield code="w">(DE-576)015160033</subfield><subfield code="x">0038-0938</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:161</subfield><subfield code="g">year:1995</subfield><subfield code="g">number:1</subfield><subfield code="g">month:10</subfield><subfield code="g">pages:49-55</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF00732083</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2002</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2286</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">161</subfield><subfield code="j">1995</subfield><subfield code="e">1</subfield><subfield code="c">10</subfield><subfield code="h">49-55</subfield></datafield></record></collection>
score	7.399638

Nicht das Richtige dabei?

Schreiben Sie uns!

Parameters of quiescent prominences derived from magnetic field measurements

Nicht das Richtige dabei?

Zugang & Verfügbarkeit

Vorhandene Bände

Nicht das Richtige dabei?