About: Space–time segmentation method for study of the vertical structure and evolution of solar supergranulation from data provided by local helioseismology     Goto   Sponge   NotDistinct   Permalink

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  • Most of the papers about supergranulation deal with its surface properties. Local helioseismology provides an opportunity to look below the surface and see the vertical structure of this convective feature. We present a concept of a (3 + 1)-D segmentation algorithm capable of recognising individual supergranules in a sequence of helioseismic 3-D flow maps. As an example, we applied this method to the state-of-the-art data and derived descriptive statistical properties of segmented supergranules – typical size of 20–30 Mm, characteristic lifetime of 18.7 h, and estimated depth of 15–20 Mm. We present preliminary results obtained on the topic of the three-dimensional structure and evolution of supergranulation. The method has great potential in analysing the better data expected from the helioseismic inversions, which are being developed.
  • Most of the papers about supergranulation deal with its surface properties. Local helioseismology provides an opportunity to look below the surface and see the vertical structure of this convective feature. We present a concept of a (3 + 1)-D segmentation algorithm capable of recognising individual supergranules in a sequence of helioseismic 3-D flow maps. As an example, we applied this method to the state-of-the-art data and derived descriptive statistical properties of segmented supergranules – typical size of 20–30 Mm, characteristic lifetime of 18.7 h, and estimated depth of 15–20 Mm. We present preliminary results obtained on the topic of the three-dimensional structure and evolution of supergranulation. The method has great potential in analysing the better data expected from the helioseismic inversions, which are being developed. (en)
Title
  • Space–time segmentation method for study of the vertical structure and evolution of solar supergranulation from data provided by local helioseismology
  • Space–time segmentation method for study of the vertical structure and evolution of solar supergranulation from data provided by local helioseismology (en)
skos:prefLabel
  • Space–time segmentation method for study of the vertical structure and evolution of solar supergranulation from data provided by local helioseismology
  • Space–time segmentation method for study of the vertical structure and evolution of solar supergranulation from data provided by local helioseismology (en)
skos:notation
  • RIV/67985815:_____/11:00355104!RIV13-AV0-67985815
http://linked.open...avai/predkladatel
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(IAA300030808), Z(AV0Z10030501), Z(MSM0021620860)
http://linked.open...iv/cisloPeriodika
  • 1
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
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http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 231150
http://linked.open...ai/riv/idVysledku
  • RIV/67985815:_____/11:00355104
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • Sun; photosphere; helioseismology (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • NL - Nizozemsko
http://linked.open...ontrolniKodProRIV
  • [12B050C07205]
http://linked.open...i/riv/nazevZdroje
  • New Astronomy
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  • 16
http://linked.open...iv/tvurceVysledku
  • Klvaňa, Miroslav
  • Švanda, Michal
  • Žlebčík, R.
http://linked.open...ain/vavai/riv/wos
  • 000282116700001
http://linked.open...n/vavai/riv/zamer
issn
  • 1384-1076
number of pages
http://bibframe.org/vocab/doi
  • 10.1016/j.newast.2010.06.002
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