Results 91 to 100 of about 7,235 (203)

Transmission of foreshock waves through Earth's bow shock. [PDF]

Nat Phys, 2023
Turc L, Roberts OW, Verscharen D, Dimmock AP, Kajdič P, Palmroth M, Pfau-Kempf Y, Johlander A, Dubart M, Kilpua EKJ, Soucek J, Takahashi K, Takahashi N, Battarbee M, Ganse U.   +14 more
europepmc   +1 more source

bow shock breakout - uniform density

, 2019
bow shock breakout - uniform ...
Almog Yalinewich (4635409)
core   +1 more source

Bow Shock Ripples and Their Modulation of Whistler Wave Packets: MMS Observations

Geophysical Research Letters
The terrestrial bow shock is the boundary where supersonic solar wind slows down abruptly near the magnetopause. The shock front geometry could be modulated by surface waves to form rippled structures, which impact the acceleration process of the solar ...
Jing‐Huan Li, Xu‐Zhi Zhou, Shan Wang, Zhi‐Yang Liu, Qiu‐Gang Zong, Shu‐Tao Yao, Anton V. Artemyev, Yoshiharu Omura, Li Li, Chao Yue, Quan‐Qi Shi   +10 more
doaj   +1 more source

Experiment on Shock Wave Control of a Hypersonic Vehicle Standard Model Based on Plasma Synthetic Jet

气体物理
The novel active flow control technology based on plasma synthetic jet (PSJ) has great application potential in the field of shock wave control due to its advantages such as no gas source, strong control ability, and wide excitation frequency band.
Wei XIE, Guotun HU, Wei SHI, Yan ZHOU, Hongbo LU, Zhenbing LUO   +5 more
doaj   +1 more source

A Fast Bow Shock Location Predictor-Estimator From 2D and 3D Analytical Models: Application to Mars and the MAVEN Mission. [PDF]

J Geophys Res Space Phys, 2022
Simon Wedlund C, Volwerk M, Beth A, Mazelle C, Möstl C, Halekas J, Gruesbeck JR, Rojas-Castillo D.   +7 more
europepmc   +1 more source

Interaction of the Prominence Plasma within the Magnetic Cloud of an Interplanetary Coronal Mass Ejection with the Earth’s Bow Shock

The Astrophysical Journal
The magnetic cloud within an interplanetary coronal mass ejection (ICME) is characterized by high magnetic field intensities. In this study, we investigate the interaction of a magnetic cloud carrying a density structure with the Earth’s bow shock during
Hadi Madanian, Li-Jen Chen, Jonathan Ng, Michael J. Starkey, Stephen A. Fuselier, Naoki Bessho, Daniel J. Gershman, Terry Z. Liu   +7 more
doaj   +1 more source

The Drivers of the Martian Bow Shock Location: A Statistical Analysis of Mars Atmosphere and Volatile EvolutioN and Mars Express Observations. [PDF]

J Geophys Res Space Phys, 2022
Garnier P, Jacquey C, Gendre X, Génot V, Mazelle C, Fang X, Gruesbeck JR, Sánchez-Cano B, Halekas JS.   +8 more
europepmc   +1 more source

The structure of perpendicular bow shocks

Journal of Geophysical Research: Space Physics, 1982
A hybrid simulation model with kinetic ions, massless fluid electrons, and phenomenological resistivity is used to study the perpendicular configuration of the bow shocks of the earth and other planets. We investigate a wide range of parameters, including the upstream Mach number, electron and ion beta (ratios of thermal to magnetic pressure), and ...
M. M. Leroy, D. Winske, C. C. Goodrich, C. S. Wu, K. Papadopoulos   +4 more
openaire   +1 more source

SERENDIPITOUS DISCOVERY OF AN INFRARED BOW SHOCK NEAR PSR J1549-4848 WITH SPITZER

, 2013
We report on the discovery of an infrared cometary nebula around PSR J1549-4848 in our Spitzer survey of a few middle-aged radio pulsars. Following the discovery, multi-wavelength imaging and spectroscopic observations of the nebula were carried out.
Wang, Zhongxiang, Morrell, Nidia, Slane, Patrick, Kaplan, David L., Kaspi, Victoria M.   +4 more
core  

Pulsar bow-shock nebulae

, 2001
Pulsar bow-shock nebulae originate from the interaction of the ambient medium with the wind of a moving pulsar. The properties of these nebulae depend on both the physical conditions in the ambient medium and the characteristics of the pulsar wind, and ...
R. Bandiera, N. Bucciantini
core   +1 more source