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dc.contributor.authorBostanci, Z. Funda
dc.contributor.authorAl Erdogan, Nurol
dc.date.accessioned2021-03-06T07:53:48Z
dc.date.available2021-03-06T07:53:48Z
dc.identifier.citationBostanci Z. F. , Al Erdogan N., "Temporal evolution of mottles in H alpha", Coimbra Solar Physics Meeting on the Physics of Chromospheric Plasmas, Coimbra, Portekiz, 9 - 13 Ekim 2006, cilt.368, ss.123-124
dc.identifier.otherav_de61d252-5558-478a-a622-f80ffabb516d
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/146520
dc.description.abstractIn April 2002, Ha observations of the solar chromosphere with high spatial and spectral resolution were obtained with the Gottingen Fabry Perot Spectrometer mounted in the Vacuum Tower Telescope (VTT) at the Observatorio del Teide. In this work, we analyze a short time sequence of a quiet region with chains of mottles. Some physical parameters of dark mottles are determined by using Beckers' cloud model which takes the source function, the Doppler width, and the velocity to be constant within the cloud along the line of sight. Here, we present the results of our study.
dc.language.isoeng
dc.subjectMühendislik, Bilişim ve Teknoloji (ENG)
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectMühendislik ve Teknoloji
dc.subjectALETLER & GÖSTERİM
dc.subjectMühendislik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleTemporal evolution of mottles in H alpha
dc.typeBildiri
dc.contributor.department, ,
dc.identifier.volume368
dc.contributor.firstauthorID133051


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