Zobrazeno 1 - 10
of 81
pro vyhledávání: '"Tibor Torok"'
The physical mechanisms by which solar prominences (or filaments) form are still not well understood. The presently favored scenario invokes the evaporation of chromospheric plasma via localized heating at the footprints of a magnetic flux rope (MFR)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::83acc09d03941001a0ea9e89b8f0d293
https://doi.org/10.5194/egusphere-egu23-2300
https://doi.org/10.5194/egusphere-egu23-2300
The proposed COronal Solar Magnetism Observatory (COSMO) Large Coronagraph (LC) will provide unique observations to study coronal mass ejections (CMEs) with its ability to diagnose the magnetic field and plasma properties in the solar corona. Here we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5d7dadd6bb3513e3fa1ec828ff0f27c7
https://doi.org/10.21203/rs.3.rs-2801458/v1
https://doi.org/10.21203/rs.3.rs-2801458/v1
Autor:
Tibor Torok, Michal Ben-Nun, Cooper Downs, Viacheslav S. Titov, Ronald M. Caplan, Roberto Lionello
As suggested by Isenberg and Forbes (2007) and demonstrated numerically by Kliem et al. (2012), the Lorentz forces stemming from the interaction of the axial current in an erupting magnetic flux rope (MFR) with an ambient magnetic-field component tha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a1dd4330c29adf374b3026909a856b8b
https://doi.org/10.5194/egusphere-egu22-2040
https://doi.org/10.5194/egusphere-egu22-2040
The torus instability (TI) of current-carrying magnetic flux tubes is thought to drive many solar coronal mass ejections (CMEs). The background magnetic field provides the stabilizing force: if it decreases with height at a rate slower than a critica
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77af0b47e609b91eb5e41c3935bf057e
Autor:
Tibor Torok, Jon A. Linker, Roberto Lionello, Viacheslav S. Titov, Ronald M. Caplan, Cooper Downs
The so-called regularized Biot-Savart laws (RBSLs, Titov et al. 2018) provide an efficient and flexible method for modeling pre-eruptive magnetic configurations whose characteristics are constraine...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::666587e98e0a4f398ae54b3faadeac24
https://doi.org/10.1002/essoar.10505478.1
https://doi.org/10.1002/essoar.10505478.1
Autor:
Jie Zhang, P. Syntelis, Tibor Torok, Ronald L. Moore, Georgios Chintzoglou, Spiros Patsourakos, Guillaume Aulanier, Manolis K. Georgoulis, Stephanie L. Yardley, Alexander Nindos, Vasilis Archontis, James E. Leake, Spiro K. Antiochos, Lucie M. Green, Vasyl Yurchyshyn, Angelos Vourlidas, Bernhard Kliem, Xin Cheng
Publikováno v:
Space Science Reviews. 216
A clear understanding of the nature of the pre-eruptive magnetic field configurations of Coronal Mass Ejections (CMEs) is required for understanding and eventually predicting solar eruptions. Only two, but seemingly disparate, magnetic configurations
The physical conditions that determine the eruptive activity of solar active regions (ARs) are still not well understood. Various proxies for predicting eruptive activity have been suggested, with relatively limited success. Moreover, it is presently
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fd124e5c0fdc7d8dd26fa387e327acd9
https://doi.org/10.5194/egusphere-egu2020-1654
https://doi.org/10.5194/egusphere-egu2020-1654
Publikováno v:
The Astrophysical Journal Supplement Series. 255:9