Results 11 to 20 of about 3,171 (217)

Acceleration of an interplanetary shock through the magnetosheath: a global hybrid simulation

open access: yesFrontiers in Astronomy and Space Sciences
According to most observations and simulations, interplanetary shocks slow down when they propagate through the magnetosheath. In this article, we present results from a self-consistent global hybrid PIC simulation of an interplanetary shock which, by ...
C. Moissard   +4 more
doaj   +2 more sources

Drift acceleration at interplanetary shocks [PDF]

open access: yesThe Astrophysical Journal Supplement Series, 1994
AbstractScatter-free acceleration of energetic particles by quasi-perpendicular interplanetary shocks is investigated. A brief review is given on the predictions of the gradient drift acceleration model concerning the energy, time, and angular dependence of the particle flux caused by a single shock encounter interaction.
G. Erdös, A. Balogh
openaire   +1 more source

Particle Acceleration at Interplanetary Shocks [PDF]

open access: yesSpace Science Reviews, 2007
This paper briefly reviews proton acceleration at interplanetary shocks. This is key to describing the acceleration of heavy ions at interplanetary shocks because wave excitation—and hence particle scattering—at oblique shocks is controlled by the protons and not the heavy ions.
Zank, G. P.   +2 more
openaire   +2 more sources

CLASSIFICATION OF THE INTERPLANETARY SHOCKS BY SHOCK DRIVERS [PDF]

open access: yesJournal of The Korean Astronomical Society, 2002
From the data of solar wind observation by ACE spacecraft orbiting the Earth-Sun Lagrangian point, we selected 48 forward interplanetary shocks(IPSs) occurred in 2000, maximum solar activity period. Examining the profiles of solar wind parameters, the IPSs are classified by their shock drivers.
SU YEON OH   +3 more
openaire   +1 more source

Interaction between an interplanetary shock and the geomagnetic frontiers: Hybrid PIC simulations

open access: yes, 2021
International audienceIn the hybrid PIC code LatHyS - which is used to simulate the interaction between the solar wind and planetary magnetic environments - we injected a fast magnetic cloud which self consistently leads to the formation of an ...
Savoini, Philippe   +3 more
core   +5 more sources

Interaction of a strong interplanetary shock with the termination shock [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 1999
The 1991 global merged interaction region (GMIR) shock is a strong forward shock observed from Voyager 2 on day 146 of 1991 at 34.6 AU. As the GMIR shock propagated out‐ward in the distant heliosphere, it eventually encounters the termination shock. We study the interaction of the GMIR shock with the termination shock taking into account the influence ...
J. Y. Lu, Y. C. Whang, L. F. Burlaga
openaire   +1 more source

Cassini encounters with hot flow anomaly-like phenomena at Saturn's bow shock [PDF]

open access: yes, 2008
The first observations of the kronian equivalent of hot flow anomalies (HFAs) are presented. Using magnetic field and plasma data we discuss two events that were observed upstream of Saturn's bow shock during the first two orbits of the Cassini ...
Bertucci, Cesar   +21 more
core   +1 more source

Unusual enhancement of ~ 30 MeV proton flux in an ICME sheath region

open access: yesEarth, Planets and Space, 2021
In gradual Solar Energetic Particle (SEP) events, shock waves driven by coronal mass ejections (CMEs) play a major role in accelerating particles, and the energetic particle flux enhances substantially when the shock front passes by the observer.
Mitsuo Oka   +5 more
doaj   +1 more source

Statistical study on interplanetary drivers behind intense geomagnetic storms and substorms

open access: yesEarth and Planetary Physics, 2019
Geomagnetic storms and substorms play a central role in both the daily life of mankind and in academic space physics. The profiles of storms, especially their initial phase morphology and the intensity of their substorms under different interplanetary ...
Tian Tian   +5 more
doaj   +1 more source

Sources of interplanetary shocks [PDF]

open access: yesAdvances in Space Research, 1995
Abstract The sources of interplanetary shocks are reviewed from the standpoint of today's knowledge. Recent progress from both new and accumulated observations and models indicates that contributions from the two major sources of the shocks: CMEs and stream interactions, have distinctive radial, latitudinal and temporal dependencies.
openaire   +1 more source

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