Coronal Magnetometry (Record no. 64354)

MARC details
000 -LEADER
fixed length control field 02417naaaa2200361uu 4500
001 - CONTROL NUMBER
control field https://directory.doabooks.org/handle/20.500.12854/44090
005 - DATE AND TIME OF LATEST TRANSACTION
control field 20220220041138.0
020 ## - INTERNATIONAL STANDARD BOOK NUMBER
International Standard Book Number 978-2-88945-220-0
020 ## - INTERNATIONAL STANDARD BOOK NUMBER
International Standard Book Number 9782889452200
024 7# - OTHER STANDARD IDENTIFIER
Standard number or code 10.3389/978-2-88945-220-0
Terms of availability doi
041 0# - LANGUAGE CODE
Language code of text/sound track or separate title English
042 ## - AUTHENTICATION CODE
Authentication code dc
100 1# - MAIN ENTRY--PERSONAL NAME
Personal name Laurel A. Rachmeler
Relationship auth
245 10 - TITLE STATEMENT
Title Coronal Magnetometry
260 ## - PUBLICATION, DISTRIBUTION, ETC.
Name of publisher, distributor, etc. Frontiers Media SA
Date of publication, distribution, etc. 2017
300 ## - PHYSICAL DESCRIPTION
Extent 1 electronic resource (172 p.)
506 0# - RESTRICTIONS ON ACCESS NOTE
Terms governing access Open Access
Source of term star
Standardized terminology for access restriction Unrestricted online access
520 ## - SUMMARY, ETC.
Summary, etc. Magnetism defines the complex and dynamic solar corona. It determines the magnetic loop structure that dominates images of the corona, and stores the energy necessary to drive coronal eruptive phenomena and flare explosions. At great heights the corona transitions into the ever-outflowing solar wind, whose speed and three-dimensional morphology are controlled by the global coronal magnetic field. Coronal magnetism is thus at the heart of any understanding of the nature of the corona, and essential for predictive capability of how the Sun affects the Earth. Coronal magnetometry is a subject that requires a concerted effort to draw together the different strands of research happening around the world. Each method provides some information about the field, but none of them can be used to determine the full 3D field structure in the full volume of the corona. Thus, we need to combine them to understand the full picture. The purpose of this Frontiers Research Topic on Coronal Magnetometry is to provide a forum for comparing and coordinating these research methods, and for discussing future opportunities.
540 ## - TERMS GOVERNING USE AND REPRODUCTION NOTE
Terms governing use and reproduction Creative Commons
Use and reproduction rights https://creativecommons.org/licenses/by/4.0/
Source of term cc
-- https://creativecommons.org/licenses/by/4.0/
546 ## - LANGUAGE NOTE
Language note English
653 ## - INDEX TERM--UNCONTROLLED
Uncontrolled term solar corona
653 ## - INDEX TERM--UNCONTROLLED
Uncontrolled term Solar Activity
653 ## - INDEX TERM--UNCONTROLLED
Uncontrolled term magnetohydrodynamics
653 ## - INDEX TERM--UNCONTROLLED
Uncontrolled term solar flares
653 ## - INDEX TERM--UNCONTROLLED
Uncontrolled term Coronal mass ejections
653 ## - INDEX TERM--UNCONTROLLED
Uncontrolled term Magnetic Fields
653 ## - INDEX TERM--UNCONTROLLED
Uncontrolled term spectropolarimetry
653 ## - INDEX TERM--UNCONTROLLED
Uncontrolled term Sun
700 1# - ADDED ENTRY--PERSONAL NAME
Personal name Sarah E. Gibson
Relationship auth
700 1# - ADDED ENTRY--PERSONAL NAME
Personal name Stephen M. White
Relationship auth
856 40 - ELECTRONIC LOCATION AND ACCESS
Host name www.oapen.org
Uniform Resource Identifier <a href="http://journal.frontiersin.org/researchtopic/3547/coronal-magnetometry">http://journal.frontiersin.org/researchtopic/3547/coronal-magnetometry</a>
Access status 0
Public note DOAB: download the publication
856 40 - ELECTRONIC LOCATION AND ACCESS
Host name www.oapen.org
Uniform Resource Identifier <a href="https://directory.doabooks.org/handle/20.500.12854/44090">https://directory.doabooks.org/handle/20.500.12854/44090</a>
Access status 0
Public note DOAB: description of the publication

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