Results 41 to 50 of about 89 (66)

Core-collapse supernovae as cosmic ray sources. [PDF]

Mon Not R Astron Soc, 2018
Marcowith A, Dwarkadas VV, Renaud M, Tatischeff V, Giacinti G.   +4 more
europepmc   +1 more source

Biological Anomalies around the 2009 L'Aquila Earthquake. [PDF]

Animals (Basel), 2013
Fidani C.
europepmc   +1 more source

Relativistic electron acceleration at the bow shock of Jupiter and beyond. [PDF]

Nature
Raptis S, Turner DL, Caprioli D, Szalay JR, Clark G, Haggerty CC.   +5 more
europepmc   +1 more source

Bow shock oscillations of Mars under weakly disturbed solar wind conditions. [PDF]

Nat Commun
Cheng L, Wang Y, Ma Y, Lillis R, Halekas J, Langlais B, Zhang T, Zhang A, Wang G, Xiao S, Zou Z, Chi Y, Hao X, Li Y, Pan Z, Liu K.   +15 more
europepmc   +1 more source

From Foreshock 30-Second Waves to Magnetospheric Pc3 Waves. [PDF]

Space Sci Rev
Turc L, Takahashi K, Kajdič P, Kilpua EKJ, Sarris T, Palmroth M, Soucek J, Pfau-Kempf Y, Dimmock A, Takahashi N.   +9 more
europepmc   +1 more source

Revealing an unexpectedly low electron injection threshold via reinforced shock acceleration. [PDF]

Nat Commun
Raptis S, Lalti A, Lindberg M, Turner DL, Caprioli D, Burch JL.   +5 more
europepmc   +1 more source

Jets Downstream of Collisionless Shocks: Recent Discoveries and Challenges. [PDF]

Space Sci Rev
Krämer E, Koller F, Suni J, LaMoury AT, Pöppelwerth A, Glebe G, Mohammed-Amin T, Raptis S, Vuorinen L, Weiss S, Xirogiannopoulou N, Archer M, Blanco-Cano X, Gunell H, Hietala H, Karlsson T, Plaschke F, Preisser L, Roberts O, Simon Wedlund C, Temmer M, Vörös Z.   +21 more
europepmc   +1 more source

Simulation Models for Exploring Magnetic Reconnection. [PDF]

Space Sci Rev
Shay M, Adhikari S, Beesho N, Birn J, Büchner J, Cassak P, Chen LJ, Chen Y, Cozzani G, Drake J, Guo F, Hesse M, Jain N, Pfau-Kempf Y, Lin Y, Liu YH, Oka M, Omelchenko Y, Palmroth M, Pezzi O, Reiff PH, Swisdak M, Toffoletto F, Toth G, Wolf RA.   +24 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Ion Acceleration by Foreshock Bubbles

Journal of Geophysical Research: Space Physics, 2021
AbstractForeshock bubbles (FBs) form as a result of the interaction between solar wind discontinuities and backstreaming ion beams in the foreshock. They are carried by the solar wind in the anti‐sunward direction and are associated with high energy ions.
N Omidi, S H Lee, D G Sibeck
exaly   +2 more sources

Formation and Topology of Foreshock Bubbles

Journal of Geophysical Research: Space Physics, 2020
AbstractWe use global and local hybrid (kinetic ions and fluid electrons) simulations to investigate the conditions under which foreshock bubbles (FBs) form and how their topology changes with solar wind conditions. FBs form as a result of the interaction between solar wind discontinuities and backstreaming ion beams in the foreshock.
N Omidi, S H Lee, D G Sibeck
exaly   +2 more sources