Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Elena G. Kupriyanova"'
Autor:
Tatyana I Kaltman, Elena G Kupriyanova
The modulation of the intensity of microwave emission from a plasma slab caused by a standing linear kink fast magnetoacoustic wave is considered. The slab is stretched along a straight magnetic field, and can represent, for example, a current sheet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d71edb55332f876d9a78e456d3e2406e
Publikováno v:
Proceedings of The Multifaceted Universe: Theory and Observations - 2022 — PoS(MUTO2022).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cb95c7ebf819919b36b791cf7db5de39
https://doi.org/10.22323/1.425.0052
https://doi.org/10.22323/1.425.0052
Autor:
D. J. Pascoe, Ivan Zimovets, Dmitrii Y. Kolotkov, Gary Verth, Norbert Magyar, Ding Yuan, Abhishek K. Srivastava, Dong Li, Giuseppe Nisticò, Valery M. Nakariakov, Rajmal Jain, S. Vasheghani Farahani, Elena G. Kupriyanova, Sergey Anfinogentov, Patrick Antolin, J. Terradas
Publikováno v:
Space Science Reviews. 217
Kink oscillations of coronal loops, i.e., standing kink waves, is one of the most studied dynamic phenomena in the solar corona. The oscillations are excited by impulsive energy releases, such as low coronal eruptions. Typical periods of the oscillat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5409c72af62f62e8f741f425e5813fd8
https://doi.org/10.1007/s11214-021-00847-2
https://doi.org/10.1007/s11214-021-00847-2
Autor:
Q. M. Zhang, Il-Hyun Cho, Ivan Zimovets, Dong Li, James McLaughlin, Hui Tian, Abhishek K. Srivastava, Dmitrii Y. Kolotkov, Elena G. Kupriyanova, D. J. Pascoe, Alexey A. Kuznetsov, Fabio Reale, Ding Yuan, Andrew Inglis
The phenomenon of quasi-periodic pulsations (QPPs) in solar and stellar flares has been known for over 50 years and significant progress has been made in this research area. It has become clear that QPPs are not rare—they are found in many flares a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e86967793dda14457c5b5bc81ce812b5
http://hdl.handle.net/10447/521980
http://hdl.handle.net/10447/521980
Autor:
Sergey A. Anfinogentov, Patrick Antolin, Andrew R. Inglis, Dmitrii Kolotkov, Elena G. Kupriyanova, James A. McLaughlin, Giuseppe Nisticò, David J. Pascoe, S. Krishna Prasad, Ding Yuan
We review novel data analysis techniques developed or adapted for the field of coronal seismology. We focus on methods from the last ten years that were developed for extreme ultraviolet (EUV) imaging observations of the solar corona, as well as for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::afeb41e7c561c74141cc0bf19a6dccbf
Autor:
L. K. Kashapova, Abhishek K. Srivastava, Yong-Jae Moon, Partha Chowdhury, Elena G. Kupriyanova, Tom Van Doorsselaere
Publikováno v:
Monthly Notices of the Royal Astronomical Society
© 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. Two kinds of processes could occur during the flare decay phase: processes of energy release or processes of energy relaxation. Quasi-periodic pul
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b91f585bf748b2d341eb35acc873875
https://lirias.kuleuven.be/handle/123456789/647628
https://lirias.kuleuven.be/handle/123456789/647628
Publikováno v:
Solar Physics. 291:3143-3164
Quasi-periodic pulsations (or QPPs) are periodic intensity variations in the flare emission that occur across all wavelength bands. In this article, we review the observational and modelling achievements since the previous review on this topic by Nak
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1f8a7c4afb9862227e5e4a1f3c74033c
https://doi.org/10.1007/s11207-016-0977-z
https://doi.org/10.1007/s11207-016-0977-z
Publikováno v:
Astronomy & Astrophysics. 642:A195
Solar flares with a fan-spine magnetic topology can form circular ribbons. The previous study based on H\alpha line observations of the solar flares during March 05, 2014 by Xu et al. (2017) revealed uniform and continuous rotation of the magnetic fa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f6e53243c0ef1f0818f152e1e5242a8a
https://doi.org/10.1051/0004-6361/201833947
https://doi.org/10.1051/0004-6361/201833947
We studied a solar flare with pronounced quasi-periodic pulsations detected in the microwave, X-ray, and radio bands. We used the methods of correlation, Fourier, and wavelet analyses to examine the temporal fine structures and relationships between
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5bebb1824e41e831ff4c6aaa7977dfc2
http://arxiv.org/abs/1608.00129
http://arxiv.org/abs/1608.00129
Publikováno v:
Publications of the Astronomical Society of Japan. 65:S3
Quasi-periodic pulsations (QPP) of the microwave emission of a solar flare on 2002 July 3, observed with the Nobeyama Radioheliograph (Japan), were investigated with emphasise on the spatial structure of the emission source. It was shown that the tim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::371efd10465e8c693e99378272ef356a
https://doi.org/10.1093/pasj/65.sp1.s3
https://doi.org/10.1093/pasj/65.sp1.s3