Results 171 to 180 of about 934,352 (223)

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

Solar Wind Magnetosphere Ionosphere Link Explorer (SMILE): Science and Mission Overview. [PDF]

Space Sci Rev
Wang C, Branduardi-Raymont G, Escoubet CP, Forsyth C.   +3 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

STEREO interplanetary shocks and foreshocks

AIP Conference Proceedings, 2013
We use STEREO data to study shocks driven by stream interactions and the waves associated with them. During the years of the extended solar minimum 2007-2010, stream interaction shocks have Mach numbers between 1.1-3.8 and θBn ∼20-86°. We find a variety of waves, including whistlers and low frequency fluctuations.
X. Blanco‐Cano, P. Kajdič, E. Aguilar-Rodriguez, C. Russell, L. Jian, J. Luhmann   +5 more
semanticscholar   +2 more sources

Zooming in on interplanetary shocks

Physics Today, 2020

semanticscholar   +2 more sources

A theoretical perspective on particle acceleration by interplanetary shocks and the Solar Energetic Particle problem

Physics Reports, 2015
Gary P Zank, Olga Verkhoglyadova, Gang Li   +2 more
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

Langmuir waves upstream of interplanetary shocks: Dependence on shock and plasma parameters

Journal of Geophysical Research, 2010
Marc Pulupa, S D Bale, Justin Kasper
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
openaire   +1 more source