Eclipse Observations of the Fe XI 789.2 nm Line

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216305%3A26210%2F10%3APU85227" target="_blank" >RIV/00216305:26210/10:PU85227 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Eclipse Observations of the Fe XI 789.2 nm Line

Original language description

The first image of the corona in Fe XI 789.2 nm was taken during the total solar eclipse of 29 March 2006. It revealed a number of surprises, primarily an emission extending out to at least 3 Rs and localized regions of enhanced Fe XI ion density relative to electrons. Subsequent observations of this spectral line were successfully made during the eclipses of 2008 and 2009. These Fe XI observations will be presented, together with simultaneous eclipse observations of the more widely observed Fe X 637.4,Fe XIII 1074.7 and Fe XIV 530.3 nm lines. Particular emphasis will be placed on the new insights gained by this suite of measurements into the thermodynamic properties of the inner corona.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

<a href="/en/project/GA205%2F09%2F1469" target="_blank" >GA205/09/1469: Study of solar coronal structures and their dynamics</a><br>

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year

2010

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Bulletin of the American Astronomical Society

ISSN

0002-7537

e-ISSN

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Volume of the periodical

2010 (43)

Issue of the periodical within the volume

1

Country of publishing house

US - UNITED STATES

Number of pages

1

Pages from-to

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UT code for WoS article

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EID of the result in the Scopus database

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