Zobrazeno 1 - 10
of 561
pro vyhledávání: '"S. K. Antiochos"'
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 2, p 168 (2024)
Coronal mass ejections (CMEs) from pseudostreamers represent a significant fraction of large-scale eruptions from the Sun. In some cases, these CMEs take a narrow jet-like form reminiscent of coronal jets; in others, they have a much broader fan-shap
Externí odkaz:
https://doaj.org/article/80e9809bd41f49d983e3b40ec847957e
Autor:
J. Qiu, M. Alaoui, S. K. Antiochos, J. T. Dahlin, M. Swisdak, J. F. Drake, A. Robison, C. R. DeVore, V. M. Uritsky
Publikováno v:
The Astrophysical Journal, Vol 955, Iss 1, p 34 (2023)
Using observations from the Solar Dynamics Observatory’s Atmosphere Imaging Assembly and the Ramaty High Energy Solar Spectroscopic Imager, we present novel measurements of the shear of post-reconnection flare loops (PRFLs) in SOL20141218T21:40 and
Externí odkaz:
https://doaj.org/article/56bd6bb042ab42948819a9c060be5bff
Publikováno v:
The Astrophysical Journal, 2022, Vol.929(2), pp.185 [Peer Reviewed Journal]
The slow solar wind is generally believed to result from the interaction of open and closed coronal magnetic flux at streamers and pseudostreamers. We use 3-dimensional magnetohydrodynamic simulations to determine the detailed structure and dynamics
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3583a05c4be5d33efbbae22ea1fa19ed
http://dro.dur.ac.uk/35948/1/35948.pdf
http://dro.dur.ac.uk/35948/1/35948.pdf
Publikováno v:
The Astrophysical Journal, 2022, Vol.931(2), pp.96 [Peer Reviewed Journal]
The boundaries of solar coronal holes are difficult to uniquely define observationally but are sites of interest in part because the slow solar wind appears to originate there. The aim of this article is to explore the dynamics of interchange magneti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::720241acdf798f11ee22094ba54c1da1
http://dro.dur.ac.uk/36100/
http://dro.dur.ac.uk/36100/
Autor:
D. A. N. Müller, S. K. Antiochos
Publikováno v:
Annales Geophysicae, Vol 26, Pp 2967-2974 (2008)
Bald patches are magnetic topologies in which the magnetic field is concave up over part of a photospheric polarity inversion line. A bald patch topology is believed to be the essential ingredient for filament channels and is often found in extrap
Externí odkaz:
https://doaj.org/article/a863b8950c1342b3b4e5a1c5f7ad113c
Autor:
Peter F. Wyper, C. R. DeVore, S. K. Antiochos, D. I. Pontin, Aleida K. Higginson, Roger Scott, Sophie Masson, Theo Pelegrin-Frachon
Publikováno v:
The Astrophysical Journal Letters, 2022, Vol.941(2), pp.L29 [Peer Reviewed Journal]
The solar wind is known to be highly structured in space and time. Observations from Parker Solar Probe have revealed an abundance of so-called magnetic switchbacks within the near-Sun solar wind. In this Letter, we use a high-resolution, adaptive-me
We analyze the structure and evolution of ribbons from the M7.3 SOL2014-04-18T13 flare using ultraviolet images from the Interface Region Imaging Spectrograph and the Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly (AIA), magnetic data
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::21c373fa2001d2aefaed4d9d4307cc0c
Publikováno v:
Space Sciences Series of ISSI ISBN: 9781493935468
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::faf0df1979ff024e17886fc59c29b005
https://doi.org/10.1007/978-1-4939-3547-5_8
https://doi.org/10.1007/978-1-4939-3547-5_8
Autor:
Zihao Yang1,2, Hui Tian2,3 huitian@pku.edu.cn, Tomczyk, Steven4,5, Xianyu Liu2,6, Gibson, Sarah1, Morton, Richard J.7, Downs, Cooper8
Publikováno v:
Science. 10/4/2024, Vol. 386 Issue 6717, p76-82. 7p. 5 Diagrams.
Publikováno v:
Magnetic Reconnection ISBN: 9781461430452
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6d32a5ac6bc47e31643a2cb95747d0d4
https://doi.org/10.1007/978-1-4614-3046-9_1
https://doi.org/10.1007/978-1-4614-3046-9_1