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dc.contributor.authorHirzberger, Johann
dc.contributor.authorAl, Nurol
dc.contributor.authorKneer, Franz
dc.date.accessioned2021-03-04T11:01:44Z
dc.date.available2021-03-04T11:01:44Z
dc.date.issued2003
dc.identifier.citationAl N., Hirzberger J., Kneer F., "Two-dimensional speckle spectroscopy of H alpha features", ASTRONOMISCHE NACHRICHTEN, cilt.324, sa.4, ss.364-365, 2003
dc.identifier.issn0004-6337
dc.identifier.otherav_70402d75-9405-4897-a2b9-9c0025c7533e
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/77385
dc.identifier.urihttps://doi.org/10.1002/asna.200310129
dc.description.abstractIn May 2002, the solar chromosphere was observed with a two-dimensional spectrometer which is mounted in the German Vacuum Tower Telescope (VTT) at the Observatorio del Teide/Tenerife. The aim of this observation was to investigate the fine structure of the solar chromosphere seen in Halpha..We took narrow-band filtergrams (Deltalambda approximate to 72 mAngstrom) by scanning through this line. broad-band images taken strictly simultaneously with the narrow-band filtergrams were restored by speckle methods. The instantaneous optical transfer function from this restoration procedure was used for the reconstruction of the narrow-band images. Some results of this high spatial resolution observation are presented below.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectFizik
dc.subjectTemel Bilimler
dc.titleTwo-dimensional speckle spectroscopy of H alpha features
dc.typeMakale
dc.relation.journalASTRONOMISCHE NACHRICHTEN
dc.contributor.department, ,
dc.identifier.volume324
dc.identifier.issue4
dc.identifier.startpage364
dc.identifier.endpage365
dc.contributor.firstauthorID62458


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