Results 151 to 160 of about 252,334 (205)

Mars's induced magnetosphere can degenerate. [PDF]

Nature
Zhang Q, Barabash S, Holmstrom M, Wang XD, Futaana Y, Fowler CM, Ramstad R, Nilsson H.   +7 more
europepmc   +1 more source

Magnetosheath jets at Jupiter and across the solar system. [PDF]

Nat Commun
Zhou Y, Raptis S, Wang S, Shen C, Ren N, Ma L.   +5 more
europepmc   +1 more source

Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]

Living Rev Sol Phys
Veronig AM, Dissauer K, Kliem B, Downs C, Hudson HS, Jin M, Osten R, Podladchikova T, Prasad A, Qiu J, Thompson B, Tian H, Vourlidas A.   +12 more
europepmc   +1 more source

The Solar Wind Electron (SWE) Instrument for the Interstellar Mapping and Acceleration Probe Mission. [PDF]

Space Sci Rev
Skoug RM, Schultz TB, Venhaus DM, Amaya CE, Choedon T, Christian ER, Crosier RD, De Los Santos A, Fernandes PA, Ford JJ, Gkioulidou M, Hanley JJ, Harvey DS, Hoeper PJ, Kubeczka PW, Liu Y, Martinez JP, McComas DJ, Mohr HD, Nunez C, Pacheco TR, Pope SE, Rodriguez H, Sandoval BF, Schiferl CM, Schwadron NA, Spalsbury LC, Seitz DN, Smith RM, Steinberg JT, Storms SA, Toczynski W, Tyler YD, Vigil VJ.   +33 more
europepmc   +1 more source

Forecasting solar energetic particles using multi-source data from solar flares, CMEs, and radio bursts with machine learning approaches. [PDF]

Sci Rep
Ali MA, Abdelkawy AGA, Shaltout AMK, Beheary MM.   +3 more
europepmc   +1 more source

Multiscale Perspectives on Solid-Phase Astrochemistry: Laboratory, Computation, and Open Questions. [PDF]

Space Sci Rev
Dickers MD, Mifsud DV, Mason NJ, Fantuzzi F.   +3 more
europepmc   +1 more source

SMILE Modeling Working Group: Modeling and Analysis of X-ray and Ultraviolet Images of Solar Wind - Earth Interactions. [PDF]

Space Sci Rev
Connor HK, Sun T, Samsonov A, Liang J, Read A, Li D, Cucho-Padin G, Jung J, Bickner B, Philippe Escoubet C, Forsyth C, Sembay S, Sibeck D, Spanswick E, Sydorenko D, Wang C.   +15 more
europepmc   +1 more source

Interplanetary Circumstances of Quasi-Perpendicular Interplanetary Shocks in 1996–2005 [PDF]

Journal of Geophysical Research: Space Physics, 2010
The angle (θBn) between the normal to an interplanetary shock front and the upstream magnetic field direction, though often thought of as a property “of the shock,” is also determined by the configuration of the magnetic field immediately upstream of the shock. We investigate the interplanetary circumstances of 105 near‐Earth quasi‐perpendicular shocks
Ian Richardson, H V Cane
exaly   +3 more sources

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Observations of Interplanetary Shocks: Recent Progress

Space Science Reviews, 1983
Interplanetary shock observations since the prior Solar Terrestrial Physics Symposium in 1978 are reviewed. Since the interval coincides with the recent solar maximum, emphasis is placed on shocks associated with transient solar phenomena, including coronal transients and eruptive prominences as well as flares.
E J Smith, E J Smith
exaly   +2 more sources

Interplanetary shocks and foreshocks

2023
The 28th IUGG General Assembly (IUGG2023) (Berlin 2023)
Blanco-Cano, X., Trota, D., Hietala, H., Kajdic, P., Rojas-Castillo, D., Dimmock, A., Horbury, T., Vainio, R., Jian, L.   +8 more
openaire   +2 more sources