Zobrazeno 1 - 10
of 93
pro vyhledávání: '"É. Buchlin"'
Autor:
É. Buchlin
Publikováno v:
Nonlinear Processes in Geophysics, Vol 14, Iss 5, Pp 649-654 (2007)
As the dissipation mechanisms considered for the heating of the solar corona would be sufficiently efficient only in the presence of small scales, turbulence is thought to be a key player in the coronal heating processes: it allows indeed to transfer
Externí odkaz:
https://doaj.org/article/0e7420a7489e4881aaa0d24deb6524e6
Autor:
Z. F. Li, X. Cheng, M. D. Ding, L. P. Chitta, H. Peter, D. Berghmans, P. J. Smith, F. Auchère, S. Parenti, K. Barczynski, L. Harra, U. Schühle, É. Buchlin, C. Verbeeck, R. Aznar Cuadrado, A. N. Zhukov, D. M. Long, L. Teriaca, L. Rodriguez
Publikováno v:
Astronomy & Astrophysics, 673
Mini-filament eruptions are one of the most common small-scale transients in the solar atmosphere. However, their eruption mechanisms are still not understood thoroughly. Here, with a combination of 174 A images of high spatio-temporal resolution tak
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b42d89a02088dc3213047269f0c9602e
Autor:
N. Alipour, H. Safari, C. Verbeeck, D. Berghmans, F. Auchère, L. P. Chitta, P. Antolin, K. Barczynski, É. Buchlin, R. Aznar Cuadrado, L. Dolla, M. K. Georgoulis, S. Gissot, L. Harra, A. C. Katsiyannis, D. M. Long, S. Mandal, S. Parenti, O. Podladchikova, E. Petrova, É. Soubrié, U. Schühle, C. Schwanitz, L. Teriaca, M. J. West, A. N. Zhukov
Publikováno v:
Astronomy and Astrophysics
Context. Accurate detections of frequent small-scale extreme ultraviolet (EUV) brightenings are essential to the investigation of the physical processes heating the corona. Aims. We detected small-scale brightenings, termed campfires, using their mor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::55394cd59f5d8ee36103f7d034afffc1
https://nrl.northumbria.ac.uk/id/eprint/49741/1/aa43257-22.pdf
https://nrl.northumbria.ac.uk/id/eprint/49741/1/aa43257-22.pdf
Akademický článek
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Autor:
Ziwen Huang, L. Teriaca, R. Aznar Cuadrado, L. P. Chitta, S. Mandal, H. Peter, U. Schühle, S. K. Solanki, F. Auchère, D. Berghmans, É. Buchlin, M. Carlsson, A. Fludra, T. Fredvik, A. Giunta, T. Grundy, D. Hassler, S. Parenti, F. Plaschke
Publikováno v:
Astronomy & Astrophysics. 673:A82
The smallest extreme-ultraviolet (EUV) brightening events that were detected so far, called campfires, have recently been uncovered by the High Resolution EUV telescope (HRIEUV), which is part of the Extreme Ultraviolet Imager (EUI) on board Solar Or
Autor:
L. P. Chitta, H. Peter, S. Parenti, D. Berghmans, F. Auchère, S. K. Solanki, R. Aznar Cuadrado, U. Schühle, L. Teriaca, S. Mandal, K. Barczynski, É. Buchlin, L. Harra, E. Kraaikamp, D. M. Long, L. Rodriguez, C. Schwanitz, P. J. Smith, C. Verbeeck, A. N. Zhukov, W. Liu, M. C. M. Cheung
Publikováno v:
Astronomy & Astrophysics, 667
Relaxation of braided coronal magnetic fields through reconnection is thought to be a source of energy to heat plasma in active region coronal loops. However, observations of active region coronal heating associated with an untangling of magnetic bra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b99927465cedb7a5af0bffbb56739f51
Publikováno v:
Astronomy & Astrophysics. 670:A66
Context. Due to its physical nature, the solar corona exhibits large spatial variations of intensity that make it difficult to simultaneously visualize the features present at all levels and scales. Many general-purpose and specialized filters have b
Akademický článek
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Autor:
D. Berghmans, F. Auchère, D. M. Long, E. Soubrié, M. Mierla, A. N. Zhukov, U. Schühle, P. Antolin, L. Harra, S. Parenti, O. Podladchikova, R. Aznar Cuadrado, É. Buchlin, L. Dolla, C. Verbeeck, S. Gissot, L. Teriaca, M. Haberreiter, A. C. Katsiyannis, L. Rodriguez, E. Kraaikamp, P.J. Smith, K. Stegen, P. Rochus, J. P. Halain, L. Jacques, W. T. Thompson, B. Inhester
The goal of this paper is to study the smallest brightening events observed in the EUV quiet Sun. We use commissioning data taken by the EUI instrument onboard the recently launched Solar Orbiter mission. On 2020 May 30, EUI was situated at 0.556AU f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::124cb243229279337af02f451d783bf6
Autor:
A. N. Zhukov, M. Mierla, F. Auchère, S. Gissot, L. Rodriguez, E. Soubrié, W. T. Thompson, B. Inhester, B. Nicula, P. Antolin, S. Parenti, É. Buchlin, K. Barczynski, C. Verbeeck, E. Kraaikamp, P. J. Smith, K. Stegen, L. Dolla, L. Harra, D. M. Long, U. Schühle, O. Podladchikova, R. Aznar Cuadrado, L. Teriaca, M. Haberreiter, A. C. Katsiyannis, P. Rochus, J.-P. Halain, L. Jacques, D. Berghmans
Publikováno v:
Astronomy & Astrophysics. 656:A35
Context. The three-dimensional fine structure of the solar atmosphere is still not fully understood as most of the available observations are taken from a single vantage point. Aims. The goal of the paper is to study the three-dimensional distributio