About: Inferring the structure of the solar Corona and inner heliosphere during the maunder minimum using global thermodynamic magnetohydrodynamic simulations

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About: Inferring the structure of the solar Corona and inner heliosphere during the maunder minimum using global thermodynamic magnetohydrodynamic simulations Goto Sponge Distinct Permalink

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scientific article published in the Astrophysical Journal

Attributes	Values
rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) наукова стаття, опублікована в березні 2015 (uk) im März 2015 veröffentlichter wissenschaftlicher Artikel (de) article publié dans la revue scientifique Astrophysical Journal (fr) scientific article published in the Astrophysical Journal (en)
publication date	wds:Q58246261-38D95135-DE09-4479-9AD8-7D2B655D71CC
publication date	2015-03-31 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q58246261-8D8CB890-439E-439E-B719-DAB69BCE458C
language of work or name	English
author name string	wds:Q58246261-3AE6BF3A-4403-4B88-A7B4-F4FA8A2F62E7 wds:Q58246261-625ECD93-CEFC-4708-9423-C9219F646779 wds:Q58246261-A6DF1485-F787-4C3F-A592-4178AF3F783E wds:Q58246261-B61084EB-833E-41BF-8E17-3FD2BFCE4CE1 wds:Q58246261-BEA500C4-15C3-421A-BEE9-79DD5B008371 wds:Q58246261-C32D29AE-99E4-4EB7-9D9C-251ED0F0606E wds:Q58246261-D206FEAD-DC45-486B-B74D-7D20CD8B5619 wds:Q58246261-ED83756D-3A8B-4A82-8FA1-FEAD10F89E1B
author name string	Jürg Beer S. Koutchmy Ken McCracken Jon A. Linker Andre Balogh Ed Cliver Marc DeRosa Matt Owens
rdfs:label	INFERRING THE STRUCTURE OF THE SOLAR CORONA AND INNER HELIOSPHERE DURING THE MAUNDER MINIMUM USING GLOBAL THERMODYNAMIC MAGNETOHYDRODYNAMIC SIMULATIONS (nl) Inferring the structure of the solar Corona and inner heliosphere during the maunder minimum using global thermodynamic magnetohydrodynamic simulations (en)
skos:prefLabel	INFERRING THE STRUCTURE OF THE SOLAR CORONA AND INNER HELIOSPHERE DURING THE MAUNDER MINIMUM USING GLOBAL THERMODYNAMIC MAGNETOHYDRODYNAMIC SIMULATIONS (nl) Inferring the structure of the solar Corona and inner heliosphere during the maunder minimum using global thermodynamic magnetohydrodynamic simulations (en)
name	INFERRING THE STRUCTURE OF THE SOLAR CORONA AND INNER HELIOSPHERE DURING THE MAUNDER MINIMUM USING GLOBAL THERMODYNAMIC MAGNETOHYDRODYNAMIC SIMULATIONS (nl) Inferring the structure of the solar Corona and inner heliosphere during the maunder minimum using global thermodynamic magnetohydrodynamic simulations (en)
author	wds:Q58246261-1F01F8CD-55CE-4EFD-BF41-F8917E5113DE wds:Q58246261-2B404EB5-363E-4D30-95BB-6AE4D3FC3D12 wds:Q58246261-2EA190F4-3737-4B58-8861-6FA12BF52832 wds:Q58246261-9279490C-DAF2-4F12-B947-3D7143666752 wds:Q58246261-BB4A0BCD-9234-4117-ABC6-E32FEB61F991 wds:Q58246261-da6243da-4622-1141-492f-606462ff82d1
author	Nancy Crooker Paul Charbonneau Ilya G. Usoskin Mike Lockwood Pete Riley Roberto Lionello
title	wds:Q58246261-F33768B3-228D-4BF0-AF58-D1A1E33D1096
title	Inferring the structure of the solar Corona and inner heliosphere during the maunder minimum using global thermodynamic magnetohydrodynamic simulations (en)
page(s)	wds:Q58246261-20908CAB-A6A7-4BFA-892C-0A9DBCE58E2B
page(s)	105
instance of	wds:Q58246261-C9BC5121-3B2B-409C-8DF8-AF59261674D0
instance of	scholarly article
published in	wds:Q58246261-229BB3AF-B5C2-4F55-B71F-BAE7BFD7268E
full work available at URL	wds:Q58246261-2682A470-AEB8-4B6E-A62B-A6FB876AF990
published in	The Astrophysical Journal
full work available at URL	https://iopscience.iop.org/article/10.1088/0004-637X/802/2/105/pdf
issue	wds:Q58246261-C3F049C3-933B-48B0-8CD2-19B19A2085E0
volume	wds:Q58246261-6F0D85D7-3602-4AB2-BDED-ABAB64AC2618
issue	2
volume	802
DOI	wds:Q58246261-41BFADDE-68D1-4BE1-A6BA-1F8E8BD89EB3
DOI	http://dx.doi.org/10.1088/0004-637X/802/2/105
DOI	10.1088/0004-637X/802/2/105
ADS bibcode	wds:Q58246261-1CFD30C2-D4E7-45CA-B7CB-ADA986BB3575
ADS bibcode	2015ApJ...802..105R
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q58246261
is cites work of	Global solar wind variations over the last four centuries. The Maunder minimum (1645–1715) was indeed a grand minimum: A reassessment of multiple datasets Near-Earth heliospheric magnetic field intensity since 1750: 2. Cosmogenic radionuclide reconstructions Minimal Magnetic States of the Sun and the Solar Wind: Implications for the Origin of the Slow Solar Wind The State of the Solar Wind, Magnetosphere, and Ionosphere During the Maunder Minimum
is cites work of	wds:Q60050039-7499F7E1-870F-4F82-973E-42710674691D wds:Q37615186-B84B9B6D-1259-4422-A7A1-A6AFAC2871C5 wds:Q56068919-A43E0763-DB4B-456B-8709-E3ABC419CD7C wds:Q58318203-44238854-000F-4096-805F-C6659331DB4A wds:Q58246205-D26EAD28-8450-49AB-85C8-A08E44B48B07

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