The Coronal Imprints of Eruptive Prominences and CMEs as Revealed by the Total Solar Eclipse Observations of 11 July 2010

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216305%3A26210%2F11%3APU102620" target="_blank" >RIV/00216305:26210/11:PU102620 - isvavai.cz</a>

Výsledek na webu

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DOI - Digital Object Identifier

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Jazyk výsledku

angličtina

Název v původním jazyce

The Coronal Imprints of Eruptive Prominences and CMEs as Revealed by the Total Solar Eclipse Observations of 11 July 2010

Popis výsledku v původním jazyce

Total solar eclipses continue to provide unique opportunities for observing the corona, due primarily to the exceptional diagnostic capabilities offered by emission from forbidden lines. Such observations span the heliocentric distance range of 1 - 3 solar radii, providing information that is currently inaccessible to any space-borne or ground-based observatory. Taking advantage of such an opportunity, the most ambitious multi-wavelength observations to date were made simultaneously in broadband white light, H alpha 656.3 nm, Fe IX 435.9 nm, Fe X 637.4 nm, Fe XI 789.2 nm, Fe XIII 1074.7 nm, Fe XIV 530.3 nm and Ni XV 670.2 nm, during the total solar eclipse of 11 July 2010 from Tatakoto, an atoll in French Polynesia. A number of curious coronal structures, namely ripples, streaks and a structure in the shape of a hook, were detected in the images. The ripples were most prominent in emission from spectral lines associated with temperatures around 106 K. The most prominent streak was asso

Název v anglickém jazyce

The Coronal Imprints of Eruptive Prominences and CMEs as Revealed by the Total Solar Eclipse Observations of 11 July 2010

Popis výsledku anglicky

Total solar eclipses continue to provide unique opportunities for observing the corona, due primarily to the exceptional diagnostic capabilities offered by emission from forbidden lines. Such observations span the heliocentric distance range of 1 - 3 solar radii, providing information that is currently inaccessible to any space-borne or ground-based observatory. Taking advantage of such an opportunity, the most ambitious multi-wavelength observations to date were made simultaneously in broadband white light, H alpha 656.3 nm, Fe IX 435.9 nm, Fe X 637.4 nm, Fe XI 789.2 nm, Fe XIII 1074.7 nm, Fe XIV 530.3 nm and Ni XV 670.2 nm, during the total solar eclipse of 11 July 2010 from Tatakoto, an atoll in French Polynesia. A number of curious coronal structures, namely ripples, streaks and a structure in the shape of a hook, were detected in the images. The ripples were most prominent in emission from spectral lines associated with temperatures around 106 K. The most prominent streak was asso

Druh

J_x - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)

CEP obor

BL - Fyzika plasmatu a výboje v plynech

OECD FORD obor

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Projekt

<a href="/cs/project/GA205%2F09%2F1469" target="_blank" >GA205/09/1469: Studium slunečních koronálních struktur a jejich dynamiky</a><br>

Návaznosti

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

Rok uplatnění

2011

Kód důvěrnosti údajů

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

Název periodika

Bulletin of the American Astronomical Society

ISSN

0002-7537

e-ISSN

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Svazek periodika

2011 (43)

Číslo periodika v rámci svazku

1

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

5

Strana od-do

1-5

Kód UT WoS článku

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EID výsledku v databázi Scopus

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