Results 171 to 180 of about 1,718 (220)

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

Detection of visible-wavelength aurora on Mars. [PDF]

Sci Adv
Knutsen EW, McConnochie TH, Lemmon M, Donaldson C, Francis R, Legett C, Viet SB, Soret L, Toledo D, Apéstigue V, Witasse O, Montmessin F, Jolitz R, Schneider NM, Tamppari L, Cousin A, Wiens RC, Maurice S, Bell JF, Forni O, Lasue J, Pilleri P, Bertrand T, Patel P, Schröder S, Curry S, Lee CO, Rahmati A.   +27 more
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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

Geoeffectiveness of interplanetary shocks controlled by impact angles: A review [PDF]

Advances in Space Research, 2018
The high variability of the Sun’s magnetic field is responsible for the generation of perturbations that propagate throughout the heliosphere. Such disturbances often drive interplanetary shocks in front of their leading regions.
Denny M Oliveira, A A Samsonov
exaly   +2 more sources

Statistical Analysis of Interplanetary Shocks from Mercury to Jupiter

Solar Physics, 2023
International audienceAbstract In situ observations of interplanetary (IP) coronal mass ejections (ICMEs) and IP shocks are important to study as they are the main components of solar activity.
M Janvier, TERESA Nieves-Chinchilla, P Demoulin   +2 more
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
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Waves upstream of interplanetary shocks

2023
Interplanetary (IP) shocks can be driven in the solar wind by fast coronal mass ejections and by the interaction of fast solar wind with slow streams of plasma. These shocks can be preceded by extended waves and suprathermal ion foreshocks. Shocks characteristics as well as the level of wave activity near them change as they propagate through the ...
Xochitl Blanco-Cano, Domenico Trotta, Heli Hietala, Primoz Kajdic, Diana Rojas-Castillo, Andrew Dimmock, Tim Horbury, Rami Vainio, Lan Jian   +8 more
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Interplanetary shock collisions: Forward with reverse shocks

Astrophysics and Space Science, 1986
When one interplanetary shock overtakes another, the structure that results depends upon the nature of the interacting shocks. We examine, numerically, the results of collisions of forward with reverse shocks, in two dimensions, and show that the results depend primarily upon shock strength.
Z. K. Smith, M. Dryer, S. M. Han
openaire   +1 more source