Results 111 to 120 of about 3,171 (217)

Large-Amplitude Electrostatic Waves Observed at a Supercritical Interplanetary Shock

, 2010
We present the first observations at an interplanetary shock of large-amplitude (> 100 mV/m pk-pk) solitary waves and large-amplitude (approx.30 mV/m pk-pk) waves exhibiting characteristics consistent with electron Bernstein waves.
Kersten, K., Kellogg, P. J., Wilson, L. B., III, Wilber, M., Kasper, J. C., Goetz, K., Cattell, C. A., Szabo, A.   +7 more
core  

Dynamic acceleration of energetic protons by an interplanetary collisionless shock

Context. Interplanetary collisionless shocks are known to be capable of accelerating charged particles up to hundreds of MeV. However, the underlying acceleration mechanisms are still under debate. Aims.
R. F. Wimmer-Schweingruber, Z. Xu, J. Rodríguez-Pacheco, L. Berger, G. C. Ho, W. Wang, L. Wang, A. Kollhoff, D. Pacheco, L. Yang, V. Heidrich-Meisner   +10 more
core   +1 more source

Parker Solar Probe Observations of Turbulence and Waves between a Current Sheet and an Interplanetary Coronal Mass Ejection–Driven Shock

The Astrophysical Journal
We report on unusual magnetic wave activity seen in a region between the crossing of a current sheet and an interplanetary shock by the Parker Solar Probe (PSP).
Juan Zhang, Joe Giacalone, Xiaohang Chen, Lan K. Jian, Kristopher G. Klein   +4 more
doaj   +1 more source

Atypical Particle Heating at a Supercritical Interplanetary Shock

, 2010
We present the first observations at an interplanetary shock of large amplitude (> 100 mV/m pk-pk) solitary waves and large amplitude (approx.30 mV/m pk-pk) waves exhibiting characteristics consistent with electron Bernstein waves.
Wilson, Lynn B., III
core   +1 more source

Identification of Coronal Mass Ejection–Driven Shocks Based on Numerical Simulation and Deep Learning

The Astrophysical Journal
Coronal mass ejections (CMEs) are eruptions originating from the solar corona, usually carrying a large amount of fast-flowing plasma into interplanetary space, accompanied by an enhanced magnetic field.
Jing’en Li, Fang Shen, Yi Yang, Mengxuan Ma, Liping Yang   +4 more
doaj   +1 more source

MHD waves in the pre-front region of the interplanetary shock on May 10, 2024

Solar-Terrestrial Physics
The article reports on the study of the dynamics of the IMF turbulent component from the quiet period on May 7, 2024 to the arrival of an interplanetary shock wave in the second half of May 10, 2024.
Starodubtsev Sergei
doaj   +1 more source

Post-shock spikes: A new feature of proton and alpha enhancements associated with an interplanetary shock wave

, 1974
Abrupt and prolonged enhancements in the intensities of 100 to approximately 2000 keV nucleon protons and alpha particles observed in interplanetary space are interpreted as particle populations confined between an interplanetary shock front and a ...
Fan, C. Y., Gloeckler, G., Hovestadt, D., Ipavich, F. M.   +3 more
core   +1 more source

Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]

Space Sci Rev
Szalay JR, Provornikova E, Ayari E, Bzowski M, Christian ER, Funsten HO, Galli A, Gkioulidou M, Horányi M, Livi S, McComas DJ, Möbius E, Ogasawara K, Rahmanifard F, Rankin JS, Reisenfeld DB, Schwadron NA, Sternovsky Z, Swaczyna P, Turner D, Zank GP, Zirnstein EJ.   +21 more
europepmc   +1 more source

Increases in the low energy cosmic ray intensity at the front of propagating interplanetary shock waves

, 1970
Increases in low energy cosmic ray intensity at front of propagating interplanetary shock ...
Fisk, L. A.
core   +1 more source

Multiwavelength Multipoint Observations of the October 28, 2021 Type III Radio Burst. [PDF]

Sol Phys
Martinez Oliveros JC, Krupar V, Ervin T, Krucker S, Pulupa M, Badman ST, Buitrago Casas JC, Mondal S, Bale SD.   +8 more
europepmc   +1 more source