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Description
  • Na echelle spektrografu na dalekohledu VTT na Sacramento Peak Observatory byla získána optická spektra chromosféry s vysokým rozlišením v několika spektrálních čarách (H?, H?, CII H a CII 8542 ?) společně s filtrogramy snímků ze štěrbiny. Spektra čar H? a H??byla?kalibrována a korigována na vplyv rozptýleného světla ve spektrografu. Filtrogramy snímků ze štěrbiny jsou použity k identifikaci tmavých chromosférických struktur. Z různých částí těchto struktur jsou získány profily čar H??a?H?? Z těchto profilů jsou pomocí tzv. „cloud modelu“ určeny parametry plazmatu jako např. rychlost ve směru zorného paprsku, zdrojová funkce, optická hroubka, dopplerovská šířka, atd. Výsledky získané ze spekter čar H??a?H??jsou navzájem porovnány. (cs)
  • High resolution optical spectra of the solar chromosphere in several spectra lines (H?, H?, CII H and CII 8542 ?) were recorded simultaneously with the echelle spectrograph of the VTT at Scramento Peak Observatory together with slit-jaw filtergrams. H?, H? line spectra were calibrated and corrected for scattered light. The slit-jaw filtergrams are used for identification of the dark mottles, while H?, H? line profiles in different parts of these structures are obtained from the spectra. Several parameters (e.g. line-of-sight velocity, source function, optical thickness, Doppler width) are derived from these profiles using cloud model. Then these results obtained from H? and H??spectra?are compared.
  • High resolution optical spectra of the solar chromosphere in several spectra lines (H?, H?, CII H and CII 8542 ?) were recorded simultaneously with the echelle spectrograph of the VTT at Scramento Peak Observatory together with slit-jaw filtergrams. H?, H? line spectra were calibrated and corrected for scattered light. The slit-jaw filtergrams are used for identification of the dark mottles, while H?, H? line profiles in different parts of these structures are obtained from the spectra. Several parameters (e.g. line-of-sight velocity, source function, optical thickness, Doppler width) are derived from these profiles using cloud model. Then these results obtained from H? and H??spectra?are compared. (en)
Title
  • Physical Parameters of Dark Mottles Derived from High Resolution Optical Spectra
  • Fyzikální parametry tmavých chromosférických struktur určené z optického spektra s vysokým rozlišením (cs)
  • Physical Parameters of Dark Mottles Derived from High Resolution Optical Spectra (en)
skos:prefLabel
  • Physical Parameters of Dark Mottles Derived from High Resolution Optical Spectra
  • Fyzikální parametry tmavých chromosférických struktur určené z optického spektra s vysokým rozlišením (cs)
  • Physical Parameters of Dark Mottles Derived from High Resolution Optical Spectra (en)
skos:notation
  • RIV/67985815:_____/05:00031821!RIV06-AV0-67985815
http://linked.open.../vavai/riv/strany
  • ;;;
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(IAA3003203), Z(AV0Z10030501)
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
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  • 536002
http://linked.open...ai/riv/idVysledku
  • RIV/67985815:_____/05:00031821
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • chromosphere; fine structure (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [ED5E78B4C23A]
http://linked.open...v/mistoKonaniAkce
  • Leuven
http://linked.open...i/riv/mistoVydani
  • Nizozemí
http://linked.open...i/riv/nazevZdroje
  • The Dynamic Sun: Challenges for Theory and Observations. Proceedings of the 11th European Solar Physics Meeting
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...iv/tvurceVysledku
  • Heinzel, Petr
  • Kotrč, Pavel
  • Schwartz, Pavol
  • Tsiropoula, G.
  • Tziotziou, K.
http://linked.open...vavai/riv/typAkce
http://linked.open.../riv/zahajeniAkce
http://linked.open...n/vavai/riv/zamer
number of pages
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  • ESA Publications Division
https://schema.org/isbn
  • 92-9092-911-1
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