Results 111 to 120 of about 7,235 (203)

Airfoil leading edge blowing to control bow shock waves. [PDF]

Sci Rep, 2020
Lozano F, Paniagua G.
europepmc   +1 more source

Magnetic pumping model for energizing superthermal particles applied to observations of the Earth's bow shock. [PDF]

Nat Commun, 2020
Lichko E, Egedal J.
europepmc   +1 more source

X-ray tomography of a cometary bow shock

, 2005
The volume intensity of the cometary X-ray emission is enhanced behind the bow shock by a factor of up to three. This effect offers the opportunity to identify the bow shock by a tomographic method in X-ray images of comets.
Wegmann, R., Dennerl, K., R. Wegmann, K. Dennerl   +3 more
core   +1 more source

The Influence of the Stretch of Mini‐Magnetospheres Formed by Crustal Fields on the Martian Bow Shock Location

Geophysical Research Letters
Mars lacks an intrinsic dipolar magnetic field but possesses strong crustal magnetic fields scattered across its surface. There has been an ongoing debate about how these crustal fields influence the bow shock, the outermost plasma boundary of the ...
Mengdan Guo, Lihui Chai, Charles F. Bowers, Yingjuan Ma, Shaosui Xu   +4 more
doaj   +1 more source

Review of boundary model studies in the Venusian and Martian induced magnetosphere

地球与行星物理论评
Although Venus and Mars do not have a global magnetic field but have atmospheres and ionospheres. During their coupling with the solar wind, the induced magnetospheres are created, as well as the boundaries of the bow shock and the magnetic pileup ...
Jiaqi Zhang, Ming Wang, Haoyang Sui, Zijian Guan, Jinyu Li, Kehan Du, Jianyong Lü   +6 more
doaj   +1 more source

Magnetohydrodynamic Perspective on the Disappearance of Mercury’s Bow Shock by Helios Data Exploration

The Astrophysical Journal
In the magnetohydrodynamic (MHD) perspective, the planet’s bow shock would disappear when the fast-mode Mach number ( M _F ) of the solar wind is less than one.
S. H. Lai, Y.-H. Yang, W.-H. Ip
doaj   +1 more source

The bow shock and mach disk of HH 111V

, 1993
We present spatially resolved line profiles in Hα and [S II] λλ16716, 6731 across the working surface region in the Herbig-Haro object HH 111V. Data were acquired with the Rutgers/CTIO imaging Fabry-Perot interferometer on the CTIO 4 m telescope at ∼1″.3
Hartigan, P., Cecil, G., Morse, J.A., Raymond, J.C., Heathcote, S.   +4 more
core   +1 more source

Entropy Generation Across Earth's Bow Shock

, 2011
Earth's bow shock is a transition layer that causes an irreversible change in the state of plasma that is stationary in time. Theories predict entropy increases across the bow shock but entropy has never been directly measured.
Canu, Patrick, Reme, Henri, Wilber, Mark, Fazakerley, Andrew, Parks, George K., Fu, Suiyan, Lin, Naiguo, McCarthy, Michael, Cao, Jinbin, Lee E. s, Goldstein, Melvyn L., Dandouras, Iannis S.   +11 more
core  

Candidate bow shock stars: Spectral analysis and environment

International audienceAims. Infrared bow shocks are arc-shaped structures located ahead of a star and generally observed at mid-to far-IR wavelengths.
Bouret, J, C, Adami, C, Russeil, D, Zavagno, A   +3 more
core   +2 more sources

Relativistic electrons generated at Earth's quasi-parallel bow shock. [PDF]

Sci Adv, 2019
Liu TZ, Angelopoulos V, Lu S.
europepmc   +1 more source