Results 141 to 150 of about 652 (191)

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

Acceleration of protons by interplanetary shocks [PDF]

Journal of Geophysical Research, 1971
Short duration proton energy increases observation by Explorer 34, considering interpretation as acceleration associated interplanetary ...
K W Ogilvie
exaly   +2 more sources

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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

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
exaly   +2 more sources

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
exaly   +2 more sources

Interaction of interplanetary shocks with the bow shock

Planetary and Space Science, 2007
Abstract Fast forward interplanetary (IP) shocks have been identified as a source of large geomagnetic disturbances. However, the shocks can evolve in the solar wind, they are modified by interaction with the bow shock and during their propagation through the magnetosheath.
J. Šafránková, Z. Němeček, L. Přech, A.A. Samsonov, A. Koval, K. Andréeová   +5 more
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Coronal mass ejections and interplanetary shocks

Journal of Geophysical Research: Space Physics, 1985
A comparison between Solwind observations of coronal mass ejections (CME's) and Helios 1 observations of interplanetary shocks during 1979–1982 indicates that 72% of the shocks were associated with large, low‐latitude mass ejections on the nearby limb.
Sheeley Jr., N., Howard, R., Koomen, M., Michels, D., Schwenn, R., Mühlhäuser, K., Rosenbauer, H.   +6 more
openaire   +2 more sources