Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Peter Gömöry"'
Autor:
Jenny M. Rodríguez-Gómez, Christoph Kuckein, Sergio J. González Manrique, Jonas Saqri, Astrid Veronig, Peter Gömöry, Tatiana Podladchikova
Publikováno v:
The Astrophysical Journal, Vol 964, Iss 1, p 27 (2024)
A joint campaign of several spaceborne and ground-based observatories, such as the GREGOR solar telescope, the Extreme-ultraviolet Imaging Spectrometer (EIS), and the Interface Region Imaging Spectrograph (Hinode Observing Plan 381, 2019 October 11
Externí odkaz:
https://doaj.org/article/acb13948b32b47c4a62be59dd743e9bf
Autor:
S. J. González Manrique, Christoph Kuckein, H. Balthasar, Peter Gömöry, Jan Rybak, S. Yuan, Z. Xu, P. Schwartz
Publikováno v:
Proceedings of the International Astronomical Union. 15:58-61
We present the first images of a coordinated campaign to follow active region NOAA 12709 on 2018 May 13 as part of a joint effort between three observatories (China-Europe). The active region was close to disk center and enclosed a small pore, a tigh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::49767dab598f64498fabe2ee1d619c4d
https://doi.org/10.1017/s1743921320000101
https://doi.org/10.1017/s1743921320000101
Autor:
Peter Gömöry, Meetu Verma, Sergio Javier González Manrique, Christoph Kuckein, Carsten Denker, Stefan J. Hofmeister, Ioannis Kontogiannis, Judith Palacios Hernández, Dominik Utz, Andrea Diercke, Kilian Krikova, Horst Balthasar, Jose Iván Campos Rozo
Publikováno v:
Proceedings of the International Astronomical Union. 15:38-41
The Sun is our dynamic host star due to its magnetic fields causing plentiful of activity in its atmosphere. From high energetic flares and coronal mass ejections (CMEs) to lower energetic phenomena such as jets and fibrils. Thus, it is of crucial im
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::71af470583a113774192b51335253a44
https://doi.org/10.1017/s174392131900989x
https://doi.org/10.1017/s174392131900989x
Autor:
Hana Mészárosová, Peter Gömöry
We study the physical properties and behavior of the solar atmosphere during the GOES X1.6 solar flare on 2014 September 10. The steady plasma flows and the fast sausage MHD waves were analysed with the wavelet separation method. The magnetically cou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a20525c325e2fbd6738a2f6f0c146729
http://arxiv.org/abs/2010.01527
http://arxiv.org/abs/2010.01527
Autor:
Peter Gömöry, Yang Su, Julia K. Thalmann, Astrid M. Veronig, Bhuwan Joshi, Aaron Hernandez-Perez
We report a detailed study of the pre-eruption activities that led to the occurrence of an M9.0 flare/CME event on 2012 October 20 in NOAA AR 11598. This includes the study of the preceding confined C2.4 flare that occurred on the same AR ~25 minutes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64d05ffb744a8c1011a4c41ef531d422
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2019, 883 (1), pp.96. ⟨10.3847/1538-4357/ab3926⟩
The Astrophysical Journal, American Astronomical Society, 2019, 883 (1), pp.96. ⟨10.3847/1538-4357/ab3926⟩
We analyze the imaging observations of an M-class eruptive flare of 2015 November, 4. The pre-eruptive H alpha filament was modelled by the non-linear force free field model, which showed that it consisted of two helical systems. Tether-cutting recon
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::639ca96835a00dae0d9605d364cfd732
Autor:
T. Waldmann, Reza Rezaei, Thomas Berkefeld, J. Kavka, Klaus G. Strassmeier, Harald Nicklas, Axel Hofmann, D. Orozco Suárez, M. Collados Vera, R. Vasková, W. Schmidt, Michael Sigwarth, Peter Gömöry, Carsten Denker, Andreas Lagg, Alex Feller, Michal Sobotka, O. von der Lühe, S. J. González Manrique, Christoph Kuckein, P. Schwartz, Sami K. Solanki, Rolf Schlichenmaier, A. Pastor Yabar, A. Kučera, D. Soltau, H. Balthasar, Dirk Schmidt, Reiner Volkmer, J. Staude
Publikováno v:
Astronomische Nachrichten. 337:1050-1056
Arch filament systems occur in active sunspot groups, where a fibril structure connects areas of opposite magnetic polarity, in contrast to active region filaments that follow the polarity inversion line. We used the GREGOR Infrared Spectrograph (GRI
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::947e71ab4d5f08493d3d7fd86498867d
https://doi.org/10.1002/asna.201612432
https://doi.org/10.1002/asna.201612432
Autor:
Peter Gömöry, Julia K. Thalmann, Ewan C. Dickson, Yang Su, Astrid Veronig, Aaron Hernandez-Perez
We analyze a confined multiple-ribbon M2.1 flare (SOL2015-01-29T11:42) that originated from a fan-spine coronal magnetic field configuration, within active region NOAA 12268. The observed ribbons form in two steps. First, two primary ribbons form at
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7a18c79aad66af42dc40092bf7a7ccd7
http://arxiv.org/abs/1708.08612
http://arxiv.org/abs/1708.08612
Publikováno v:
Astronomische Nachrichten. 335:161-167
Spectropolarimetric observations of a sunspot were carried out with the Tenerife Infrared Polarimeter at Observatorio del Teide, Tenerife, Spain. Maps of the physical parameters were obtained from an inversion of the Stokes profiles observed in the i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7ef81d26eeec396404f9b619c8faf410
https://doi.org/10.1002/asna.201312017
https://doi.org/10.1002/asna.201312017
We analyzed high-cadence sit-and-stare observations acquired with the Hinode/EIS spectrometer and HXR measurements acquired with RHESSI during an M-class flare. During the flare impulsive phase, we observe no significant flows in the cooler Fe XIII l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd3837c16ba708623ba70a03b2028a43