Results 1 to 10 of about 916,158 (245)

Electron Energy Partition across Interplanetary Shocks. I. Methodology and Data Product. [PDF]

open access: yesAstrophys J Suppl Ser, 2019
Analyses of 15,314 electron velocity distribution functions (VDFs) within ±2 hr of 52 interplanetary (IP) shocks observed by the Wind spacecraft near 1 au are introduced.
Wilson LB   +12 more
europepmc   +3 more sources

Turbulence Upstream and Downstream of Interplanetary Shocks

open access: yesFrontiers in Physics, 2021
The paper reviews the interaction of collisionless interplanetary (IP) shocks with the turbulent solar wind. The coexistence of shocks and turbulence plays an important role in understanding the acceleration of particles via Fermi acceleration mechanisms,
A. Pitňa   +4 more
doaj   +2 more sources

Ion‐Acoustic Waves Associated With Interplanetary Shocks

open access: yesGeophysical Research Letters
Ion‐acoustic waves (IAWs) commonly occur near interplanetary (IP) shocks. These waves are important because of their potential role in the dissipation required for collisionless shocks to exist.
J. J. Boldú   +12 more
doaj   +6 more sources

Interplanetary circumstances of quasi‐perpendicular interplanetary shocks in 1996–2005 [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 2010
The angle (θBn) between the normal to an interplanetary shock front and the upstream magnetic field direction, though often thought of as a property “of the shock,” is also determined by the configuration of the magnetic field immediately upstream of the shock. We investigate the interplanetary circumstances of 105 near‐Earth quasi‐perpendicular shocks
I. G. Richardson, H. V. Cane
openaire   +2 more sources

ARTEMIS Observations of Plasma Waves in Laminar and Perturbed Interplanetary Shocks [PDF]

open access: yesAstrophysical Journal, 2020
The “Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon's Interaction with the Sun” mission provides a unique opportunity to study the structure of interplanetary shocks and the associated generation of plasma waves with frequencies ...
L. Davis   +5 more
semanticscholar   +1 more source

Interplanetary shock data base

open access: yesFrontiers in Astronomy and Space Sciences, 2023
In this manuscript, I provide an updated interplanetary shock data base I published in previous works. This list has now 603 events. I also present and describe the data and methodologies used to compile this list. The main contribution of this work is to provide an updated end accurate interplanetary shock data base for future space physics and space ...
Denny M. Oliveira, Denny M. Oliveira
openaire   +3 more sources

In Situ Observation of Electron Acceleration by a Double Layer in the Bow Shock

open access: yesThe Astrophysical Journal, 2023
The importance of the electric potential along the field direction in the acceleration of electrons in the quasi-perpendicular bow shock has been proposed.
C. M. Wang   +6 more
doaj   +1 more source

Variation of the Interplanetary Shocks in the Inner Heliosphere

open access: yes, 2021
Observations of the solar wind plasma and interplanetary magnetic field in the ecliptic plane by the Voyager 1 and 2 spacecraft are utilized to study the variation of the interplanetary shocks (with magnetosonic Mach number >1) encountered in the inner ...
R. Hajra
semanticscholar   +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

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

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