Horizontal Velocities in Solar Filament Channel

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00398902" target="_blank" >RIV/67985815:_____/13:00398902 - 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

Horizontal Velocities in Solar Filament Channel

Original language description

Chromosphere fibrils oriented along the neutral line in close vicinity of solar filaments create typical characteristics of the filament channel. From systematic Doppler velocities measurements made at Kanzelhöhe Solar Observatory with the Magneto OpticFilter (MOF) we derived the horizontal velocity fields. Horizontal velocities were determined in areas strongly connected with filament channels and also outside these regions. Close along the filament axis in the direction of the polarity inversion linea strong shear of the mean horizontal velocities was detected.

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/IAA300030808" target="_blank" >IAA300030808: Interaction of moving plasma with magnetic fields in the solar photosphere</a><br>

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year

2013

Confidentiality

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

Name of the periodical

Central European Astrophysical Bulletin

ISSN

1845-8319

e-ISSN

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Volume of the periodical

37

Issue of the periodical within the volume

2

Country of publishing house

HR - CROATIA

Number of pages

6

Pages from-to

495-500

UT code for WoS article

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EID of the result in the Scopus database

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