Results 71 to 80 of about 15,246 (211)

Speeds and arrival times of solar transients approximated by self-similar expanding circular fronts

, 2012
The NASA STEREO mission opened up the possibility to forecast the arrival times, speeds and directions of solar transients from outside the Sun-Earth line.
A. Thernisien, A.P. Rouillard, A.P. Rouillard, B. Vršnak, B. Vršnak, B.E. Wood, C. Möstl, C. Möstl, C. Möstl, C. Möstl, C.A. de Koning, C.J. Davis, C.J. Davis, C.J. Eyles, C.J. Eyles, E.K.J. Kilpua, G. Siscoe, I.G. Richardson, I.G. Richardson, J. A. Davies, J.A. Davies, J.P. Byrne, L. Rodriguez, M. Mierla, M. Temmer, M.L. Kaiser, N. Gopalswamy, N. Gopalswamy, N. Lugaz, N. Lugaz, N. Lugaz, N. Lugaz, N.P. Savani, N.P. Savani, N.P. Savani, N.R. Sheeley, R. Schwenn, R.K. Burton, S. Yashiro, S.A. Maloney, S.J. Tappin, S.W. Kahler, T.A. Howard, Y. Liu, Y. Liu, Y. Liu   +45 more
core   +1 more source

Coronal Mass Ejections and Solar Polarity Reversal

The Astrophysical Journal, 2003
We report on a close relationship between the solar polarity reversal and the cessation of high-latitude coronal mass ejections (CMEs). This result holds good for individual poles of the Sun for cycles 21 and 23, for which CME data are available. The high-latitude CMEs provide a natural explanation for the disappearance of the polar crown filaments ...
N. Gopalswamy, A. Lara, S. Yashiro, R. A. Howard   +3 more
openaire   +1 more source

Numerical simulations of homologous coronal mass ejections in the solar wind [PDF]

Astronomy & Astrophysics, 2009
Context. Coronal mass ejections (CMEs) are enormous expulsions of magnetic flux and plasma from the solar corona. Most scientists agree that a coronal mass ejection is the sudden release of magnetic free energy stored in a strongly stressed field. However, the exact reason for this sudden release is still highly debated. Aims.
Soenen, Alexander, Zuccarello, Francesco, Jacobs, Carla, Poedts, Stefaan, Keppens, Rony, van der Holst, Bart   +5 more
openaire   +1 more source

Solar Wind‐Magnetosphere‐Ionosphere Coupling During the October 2024 Storms

Journal of Geophysical Research: Space Physics, Volume 131, Issue 5, May 2026.
Abstract Two geomagnetic storms occurred in October 2024 (Oct 6‐9 and 10–12), driven by the impact of a series of interplanetary coronal mass ejections on the magnetosphere. The first was a moderate storm, with peak Sym‐H near −150 nT, whereas the second was intense, Sym‐H reaching −340 nT.
S. E. Milan, M. K. Mooney, G. E. Bower, R. M. Hodnett, U. V. Amerstorfer, C. Möstl, A. Samsonov, B. J. Anderson, J. Gjerloev, S. K. Vines   +9 more
wiley   +1 more source

A Deep Learning Method for Automatic Coronal Mass Ejection Feature Identification

The Astrophysical Journal Supplement Series
Coronal mass ejections (CMEs), intense solar eruptive phenomena, are the primary drivers of extreme space weather storms on Earth. As space activities become increasingly frequent and infrastructure more reliant on space-based systems, the rapid and ...
P. Yang, H. S. Fu, J. B. Cao, F. Shen
doaj   +1 more source

Short term Variability of the Sun Earth System: An Overview of Progress Made during the CAWSES II Period [PDF]

, 2015
This paper presents an overview of results obtained during the CAWSES II period on the short term variability of the Sun and how it affects the near Earth space environment. CAWSES II was planned to examine the behavior of the solar terrestrial system as
Gopalswamy, Nat, Tsurutani, Bruce, Yan, Yihua   +2 more
core   +2 more sources

Evolution of Magnetospheric Boundary Layers Under the 10 May 2024 ICME Impact

Geophysical Research Letters, Volume 53, Issue 8, 28 April 2026.
Abstract On 10 May 2024, an interplanetary coronal mass ejection‐driven shock impacted the dayside magnetopause, compressing it to ∼5 RE. A northward interplanetary magnetic field suppressed dayside reconnection and allowed a clear investigation of the magnetosphere response.
Sheng Li, Gilbert Pi, Zdeněk Němeček, Jana Šafránková, Trevor W. Leonard, Yang‐Yi Sun   +5 more
wiley   +1 more source

Distorted Magnetic Flux Ropes within Interplanetary Coronal Mass Ejections

The Astrophysical Journal
Magnetic flux ropes (MFRs) at the center of interplanetary coronal mass ejections (ICMEs) are often characterized as simplistic cylindrical or toroidal tubes with field lines that twist around the cylinder or torus axis.
Andreas J. Weiss, Teresa Nieves-Chinchilla, Christian Möstl   +2 more
doaj   +1 more source

Lateral Confinement and the Remarkably Self-similar Nature of Coronal Pseudostreamer Mass Ejections

The Astrophysical Journal, 2023
Coronal mass ejections (CMEs) that originate from pseudostreamers, which separate coronal holes of the same magnetic polarity, are characterized by a narrow (∼5°–30°), fan-shaped appearance in white-light coronagraph images.
Y.-M. Wang, P. Hess
doaj   +1 more source

A Helicity-Based Method to Infer the CME Magnetic Field Magnitude in Sun and Geospace: Generalization and Extension to Sun-Like and M-Dwarf Stars and Implications for Exoplanet Habitability

, 2017
Patsourakos et al. (Astrophys. J. 817, 14, 2016) and Patsourakos and Georgoulis (Astron. Astrophys. 595, A121, 2016) introduced a method to infer the axial magnetic field in flux-rope coronal mass ejections (CMEs) in the solar corona and farther away in ...
A. Isavnin, A. Kumar, A. Nindos, A. Nindos, A. Nindos, A. Thernisien, A. Vourlidas, A.A. Vidotto, A.A. Vidotto, A.N. Aarnio, B. Gladman, B. Kliem, B. Vrsnak, B. Vršnak, B.E. Wood, B.J. Lynch, B.J. Lynch, B.J. Lynch, B.M. Jakosky, C. Cid, C. Garraffo, C. Karoff, C. Kay, C. Kay, C. Möstl, C.-C. Wu, C.H. Mandrini, C.J. Schrijver, C.R. DeVore, D. Cunha, D. Nogami, D.J. Armstrong, E. Bosman, E. Pariat, E.A. Jensen, E.R. Houdebine, E.R. Priest, E.W. Cliver, F. Selsis, G. Anglada-Escudé, G. Aulanier, G. Chintzoglou, G. Torres, G. Valori, G.A. Gary, H. Lammer, H. Maehara, I.G. Usoskin, J. Leconte, J. Scalo, J.-F. Donati, J.-M. Grießmeier, J.-M. Grießmeier, J.F. Kasting, J.J. Drake, J.R.A. Davenport, K. Hariharan, K. Moraitis, K. Shibata, K. Tziotziou, K. Tziotziou, L.K. Harra, L.M. Green, M. Leitner, M. Leitzinger, M. Leitzinger, M. Patzold, M. Semel, M. Vandas, M.A. Berger, M.A. Hidalgo, M.D. Andrews, M.D. Kazachenko, M.K. Georgoulis, M.K. Georgoulis, M.L. Khodachenko, M.L. Luoni, M.S. Nakwacki, N. Al-Haddad, N.P. Savani, P. Démoulin, P. Démoulin, P. Démoulin, P. MacNeice, P. Riley, Q. Hu, R. Kataoka, R. Osten, R.A. Osten, R.J. Forsyth, R.M. Winslow, R.P. Lepping, S. Chapman, S. Dasso, S. Lundquist, S. Mancuso, S. Patsourakos, S. Patsourakos, S. Régnier, S. Toriumi, S. Yashiro, S.D. Tun, S.E. Gibson, S.R. Kane, S.W. Good, T. Gold, T. Nieves-Chinchilla, T. Shibayama, T.A. Howard, T.G. Forbes, T.S. Bastian, V. Bothmer, V. Kunkel, V. See, V.S. Airapetian, W. Poomvises, X. Sun, Y. Guo, Y. Liu, Y. Wang   +119 more
core   +1 more source