Zobrazeno 1 - 10
of 301
pro vyhledávání: '"Brigitte, Schmieder"'
Publikováno v:
The Astrophysical Journal, Vol 973, Iss 1, p 33 (2024)
With the aid of high-resolution spatial and temporal observations from the Goode Solar Telescope, we present an investigation of the emergence, coalescence, and submergence of a moving magnetic feature (MMF) in the region surrounding a magnetic pore
Externí odkaz:
https://doaj.org/article/c2a166368bac40b384282958bc453461
Autor:
Réka M. Winslow, Camilla Scolini, Lan K. Jian, Teresa Nieves-Chinchilla, Manuela Temmer, Fernando Carcaboso, Brigitte Schmieder, Stefaan Poedts, Benjamin J. Lynch, Brian E. Wood, Erika Palmerio, Noé Lugaz, Charles J. Farrugia, Christina O. Lee, Emma E. Davies, Florian Regnault, Tarik M. Salman, Tibor Török, Nada Al-Haddad, Angelos Vourlidas, Ward B. Manchester, Meng Jin, Benoit Lavraud, Antoinette B. Galvin
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
This perspective paper brings to light the need for comprehensive studies on the evolution of interplanetary coronal mass ejection (ICME) complexity during propagation. To date, few studies of ICME complexity exist. Here, we define ICME complexity an
Externí odkaz:
https://doaj.org/article/40f90fe46fc04559838ba41b0357ef6f
Publikováno v:
Reviews of Modern Plasma Physics; 8/10/2024, Vol. 8 Issue 1, p1-33, 33p
Autor:
Brigitte Schmieder
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
Solar jets are observed as collimated plasma beams over a large range of temperatures and wavelengths. They have been observed in H α and optical lines for more than 50 years and called surges. The term “jet” comes from X-ray observations after
Externí odkaz:
https://doaj.org/article/684d77c72a154fb08a402576c0f988b3
Publikováno v:
The Astrophysical Journal, Vol 955, Iss 1, p 50 (2023)
The propagation of interplanetary coronal mass ejections (ICMEs) in the heliosphere is influenced by many physical phenomena, related to the internal structure of the ICME and its interaction with the ambient solar wind and magnetic field. As the sol
Externí odkaz:
https://doaj.org/article/295e1de54a494505ab6ff1cdc2d4704f
Publikováno v:
The Astrophysical Journal, Vol 949, Iss 1, p 2 (2023)
Coronal jets are eruptions identified by a collimated, sometimes twisted spire. They are small-scale energetic events compared with flares. Using multiwavelength observations from the Solar Dynamics Observatory/Atmospheric Imaging Assembly and a magn
Externí odkaz:
https://doaj.org/article/f009e0e892cd466ebf07d79d0f9b4d66
Autor:
Stanislav Gunár, Nicolas Labrosse, Manuel Luna, Brigitte Schmieder, Petr Heinzel, Therese A. Kucera, Peter J. Levens, Arturo López Ariste, Duncan H. Mackay, Maciej Zapiór
Publikováno v:
Space Science Reviews. 219
The term ‘tornado’ has been used in recent years to describe several solar phenomena, from large-scale eruptive prominences to small-scale photospheric vortices. It has also been applied to the generally stable quiescent prominences, sparking a r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a2faa917e14e5f864421899afdcc8dcc
https://doi.org/10.1007/s11214-023-00976-w
https://doi.org/10.1007/s11214-023-00976-w
Magnetic flux ropes are bundles of twisted magnetic field lines produced by the internal flowing electric currents, which are regarded as one of the basic and pivot structures in solar and space physics. Statistics showed that about 90% of the erupti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c98b0e84c8af89a433fd8016d169212f
https://doi.org/10.5194/egusphere-egu23-4394
https://doi.org/10.5194/egusphere-egu23-4394
Coronal Mass Ejections (CMEs) are the main drivers of interplanetary shocks and space weather disturbances. Strong CMEs directed towards Earth can have a severe impact on our planet and their timely prediction can enable us to mitigate (part of) the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f80498dfa793fd83f650b34179305722
https://doi.org/10.5194/egusphere-egu23-3579
https://doi.org/10.5194/egusphere-egu23-3579
Large-amplitude oscillations (LAOs) are often detected in filaments. Using multiwavelength observations, their origin can be traced back to the interaction with eruptions and jets. We present two different case studies as observational evidence in su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9767a264caec820f028ba2b104e9d1fb