Five times the solar disk in a long row from left to right with main colors orange, light green, blue, green-red sprinkles, blue-to-red gradient, respresenting exemplary PMI data products after on-board analysis from left to right: continuum intensity, magnetic field strength, magnetic field inclination, magnetic field azimuth and line-of-sight velocity.

Publications of M. Švanda

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Journal Article (4)

1.
Journal Article
Roudier, T.; Rieutord, M.; Malherbe, J. M.; Renon, N.; Berger, T.; Frank, Z.; Prat, V.; Gizon, L.; Švanda, M.: Quasi full-disk maps of solar horizontal velocities using SDO/HMI data. Astronomy and Astrophysics 540, A88 (2012)
MPG.PuRe
DOI
2.
Journal Article
Švanda, M.; Gizon, L.; Hanasoge, S. M.; Ustyugov, S. D.: Validated helioseismic inversions for 3D vector flows. Astronomy and Astrophysics 530, A148 (2011)
MPG.PuRe
DOI
3.
Journal Article
Žlebčík, R.; Švanda, M.; Klvana, M.: Space-time segmentation method for study of the vertical structure and evolution of solar supergranulation from data provided by local helioseismology. New Astron. 16 (1), pp. 1 - 5 (2011)
MPG.PuRe
DOI
4.
Journal Article
Švanda, M.; Klvana, M.; Sobotka, M.: Large-scale horizontal flows in the solar photosphere V: Possible evidence for the disconnection of bipolar sunspot groups from their magnetic roots. Astronomy and Astrophysics 506, pp. 875 - 884 (2009)
MPG.PuRe
DOI

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