Results 141 to 150 of about 1,158 (191)

Relation between magnetopause position and reconnection rate under quasi-steady solar wind dynamic pressure. [PDF]

Earth Planets Space
Kim H, Connor HK, Zou Y, Park J, Nakamura R, McWilliams K.   +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

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

Evaluation of the <i>Salmonella</i> type 3 secretion system (T3SS) as part of a protein production platform for space biology applications. [PDF]

Front Bioeng Biotechnol
Kang MK, Bevington J, Tullman-Ercek D.
europepmc   +1 more source

First direct observations of atmospheric sputtering at Mars. [PDF]

Sci Adv
Curry SM, Hara T, Luhmann JG, Leblanc F, Jolitz R, Mitchell D, Modolo R, Brain DA, Espley J, Benna M, Halekas J.   +10 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

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

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

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

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
openaire   +1 more source

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