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  • For the first time the set of two lines Ha and Call H was used to construct semi-empirical models of EBs. Our analysis shows that EBs can be described by a %22hot spot%22 model, with the temperature and/or density increase through a few hundred km atmospheric structure. We confirmed that EBs are located close to the temperature minimum or in the lower chromosphere. Two spectral features (lines in our case), observed simultaneously, significantly strengthen the constraints on a realistic model.
  • For the first time the set of two lines Ha and Call H was used to construct semi-empirical models of EBs. Our analysis shows that EBs can be described by a %22hot spot%22 model, with the temperature and/or density increase through a few hundred km atmospheric structure. We confirmed that EBs are located close to the temperature minimum or in the lower chromosphere. Two spectral features (lines in our case), observed simultaneously, significantly strengthen the constraints on a realistic model. (en)
Title
  • Observations and NLTE modeling of Ellerman bombs
  • Observations and NLTE modeling of Ellerman bombs (en)
skos:prefLabel
  • Observations and NLTE modeling of Ellerman bombs
  • Observations and NLTE modeling of Ellerman bombs (en)
skos:notation
  • RIV/67985815:_____/14:00433755!RIV15-GA0-67985815
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  • I, P(GAP209/11/2463)
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  • July
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  • 33741
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  • RIV/67985815:_____/14:00433755
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  • Sun: chromosphere; line: profiles; imaging spectroscopy (en)
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  • FR - Francouzská republika
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  • [14B6088B21F7]
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  • Astronomy & Astrophysics
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  • 567
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  • Heinzel, Petr
  • Berlicki, Arkadiusz
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  • 000341185300053
issn
  • 0004-6361
number of pages
http://bibframe.org/vocab/doi
  • 10.1051/0004-6361/201323244
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