Autor:	Xiaoma Gu, Jinping Dun, Shuhua Zhong
Rok vydání:	2000
Předmět:	Physics Physics::Instrumentation and Detectors business.industry Astronomy and Astrophysics Cloud computing Spectral line Computational physics Model method Space and Planetary Science Observatory Astrophysics::Solar and Stellar Astrophysics Effective method Spectral data business Remote sensing
Zdroj:	Astrophysics and Space Science. 274:473-479
ISSN:	0004-640X
Popis:	Multi-Cloud Model(MCM) is an effective method for dealing with asymmetric profiles of spectral line formed by active objects on the sun. A typical example is given for the application of the MCM method in this paper. The Hβ spectral data of a large post-flare loop (PFL) system which occurred on the solar western limb are obtained with MW-SSHG at the Yunnan Observatory and analysed based on the MCM method. The line-of-sight velocity fields observed in different times are derived and discussed.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::af5d962b6eed93f84236c96ca42deb3c https://doi.org/10.1023/a:1026574327395 Zobrazit plný text záznamu Full text from SpringerLink