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of 102
pro vyhledávání: '"Zdeněk Švestka"'
Autor:
Zdeněk Švestka
Publikováno v:
Solar Physics. 267:235-250
I recount my career in solar physics beginning at Ondřejov Observatory in 1948 and ending with my ∼30 year stay at the Laboratory of Space Research in Utrecht.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f1c9c7475478e2690c14cf3f6aea0c16
https://doi.org/10.1007/s11207-010-9675-4
https://doi.org/10.1007/s11207-010-9675-4
Autor:
Zdeněk Švestka
Publikováno v:
Solar Physics. 246:393-397
Attention is drawn to the fact that the term “post-flare loops” is incorrect and should be avoided, because the loops are parts of the flare itself. Two other names for these loop systems are suggested.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a9083a714480d54a6b51ccc6fddcf7a6
https://doi.org/10.1007/s11207-007-9088-1
https://doi.org/10.1007/s11207-007-9088-1
Autor:
F. Farnik, Zdeněk Švestka
Publikováno v:
Solar Physics. 229:305-312
Outflow of slow solar wind from solar active regions has been reported in recent years by many different authors. Therefore, in this paper we have studied synoptic maps of the solar wind density (SWD) based on interplanetary scintillation (IPS) data
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4787d5408be6daf49983973e2022308b
https://doi.org/10.1007/s11207-005-6881-6
https://doi.org/10.1007/s11207-005-6881-6
Autor:
Zdeněk Švestka, František Fárník
Publikováno v:
Solar Physics. 206:143-154
We present examples of X-ray jets, observed by the Soft X-ray Telescope on board Yohkoh, which followed trajectories of transequatorial interconnecting loops (TILs). All these TILs were preexisting, seen some time before, but were mostly invisible at
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8482e1a992fc6d4f7d59a29f80a1f409
https://doi.org/10.1023/a:1014963812437
https://doi.org/10.1023/a:1014963812437
Publikováno v:
Solar Physics. 202:81-98
We discuss footpoints of loops seen by Yohkoh in soft X-rays that connect active regions across the equator (transequatorial interconnecting loops – TILs). While most TILs are rooted in moderately strong fields at peripheries of active regions, the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0ede8cbe5132e76c3de7ce191101d4c1
https://doi.org/10.1023/a:1011812000475
https://doi.org/10.1023/a:1011812000475
Autor:
Zdeněk Švestka
Publikováno v:
Space Science Reviews. 95:135-146
Most coronal mass ejections (CMEs) start as coronal storms which are caused by an opening of channels of closed field lines along the zero line of the longitudinal magnetic field. This can happen along any zero line on the Sun where the configuration
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::634fa8ff342b1c1ed6143c25b69ef846
https://doi.org/10.1023/a:1005225208925
https://doi.org/10.1023/a:1005225208925
Autor:
Zdenek Svestka, P. Simon
This Catalog originated as a common enterprise of solar physicists and space scientists under the auspices of the Second Working Group of the Inter-Union Commission of Solar Terrestrial Physics (IUCSTP). It is a pleasure to acknowledge the support we
Autor:
Zdenek Svestka
This book is the first part of the originally planned publication by Z. Svestka and L. D. de Feiter'Solar High Energy Photon and Particle Emission'. The second part, with the original title, was to be published by de Feiter in about one year from now
Autor:
Zdenek Svestka, John W. Harvey
Most papers in this book were presented at the SOHO-9 Workshop'Helioseismic Diagnostics of Solar Convection and Activity', held on 12-15 July 1999 at Stanford University, California, U.S.A. Some papers which were not presented at the work shop have