Results 171 to 180 of about 13,868 (214)

A Novel Determination of the Foreshock ULF Boundary: Statistical Approach. [PDF]

J Geophys Res Space Phys
Salohub A, Šafránková J, Němeček Z, Pi G.   +3 more
europepmc   +1 more source

Space Physiology and Technology: Adaptations, Countermeasures, and Opportunities for Wearable Systems. [PDF]

Cyborg Bionic Syst
Khan SUE, Varghese RJ, Kassanos P, Farina D, Burdet E.   +4 more
europepmc   +1 more source

Nonmagnetic framboid and associated iron nanoparticles with a space-weathered feature from asteroid Ryugu. [PDF]

Nat Commun
Kimura Y, Kato T, Anada S, Yoshida R, Yamamoto K, Tanigaki T, Akashi T, Kasai H, Kurosawa K, Nakamura T, Noguchi T, Sato M, Matsumoto T, Morita T, Kikuiri M, Amano K, Kagawa E, Yada T, Nishimura M, Nakato A, Miyazaki A, Yogata K, Abe M, Okada T, Usui T, Yoshikawa M, Saiki T, Tanaka S, Terui F, Nakazawa S, Yurimoto H, Okazaki R, Yabuta H, Naraoka H, Sakamoto K, Watanabe SI, Tsuda Y, Tachibana S.   +37 more
europepmc   +1 more source

A Comparative Analysis of Performance Simulation for PUI Detectors Based on Traditional Probability Model and the Vasyliunas and Siscoe Model. [PDF]

Sensors (Basel)
Cao Y, Zhang Y, Peng X, Xue C, Su B.
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

Energetic neutral atom imaging reveals nearly 11-year cycle of the ring current of Saturn. [PDF]

Nat Commun
Li Y, Yue C, Sun Y, Jia X, Zong Q, Zhou X.   +5 more
europepmc   +1 more source

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Modeling Particle Acceleration at Interplanetary Shocks

AIP Conference Proceedings, 2008
A brief review of particle acceleration at inner heliospheric interplanetary and coronal mass ejection (CME)‐driven shocks is presented. The discussion is presented in terms of a specific event that was modeled using the Particle Acceleration and Transport in the Heliosphere model (hereafter PATH) code.
G P Zank, Olga P Verkhoglyadova, Qiang Hu   +2 more
exaly   +2 more sources

Particle acceleration by propagating interplanetary shocks

AIP Conference Proceedings, 1979
The process of charged particle acceleration in interplanetary shocks has been simulated for typical parameters. Since space probe observations of charged particle fluxes are the principle means of inferring the action of an acceleration mechanism, the simulation was designed to follow particles backwards in time from a given observing point, usually 1
R B Decker
exaly   +2 more sources

Observations of Particle Acceleration at Interplanetary Shocks

AIP Conference Proceedings, 2009
Collisionless shocks accelerate charged particles throughout heliosphere, from low in the solar corona to the outer edge of the supersonic solar wind. Particles can gain energy while interacting with shocks in different ways, depending on conditions at the shock and on particle species and energy.
George C Ho, D Lario, R B Decker
exaly   +2 more sources

A theoretical perspective on particle acceleration by interplanetary shocks and the Solar Energetic Particle problem

Physics Reports, 2015
Abstract Understanding the physics of Solar Energetic Particle (SEP) events is of importance to the general question of particle energization throughout the cosmos as well as playing a role in the technologically critical impact of space weather on society.
Olga P Verkhoglyadova, G P Zank, Gang Li   +2 more
exaly   +2 more sources