Results 71 to 80 of about 2,940 (168)

Role of ULF Waves in Reforming the Martian Bow Shock

AGU Advances
Understanding the nature of planetary bow shocks is beneficial for advancing our knowledge of solar wind interactions with planets and fundamental plasma physics processes.
Chi Zhang, Chuanfei Dong, Terry Z. Liu, Christian Mazelle, Savvas Raptis, Hongyang Zhou, Jacob Fruchtman, Jasper Halekas, Jing‐Huan Li, Kathleen G. Hanley, Shannon M. Curry, David L. Mitchell, Xinmin Li   +12 more
doaj   +1 more source

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

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

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

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

Autogenous and efficient acceleration of energetic ions upstream of Earth's bow shock. [PDF]

Nature, 2018
Turner DL, Wilson LB, Liu TZ, Cohen IJ, Schwartz SJ, Osmane A, Fennell JF, Clemmons JH, Blake JB, Westlake J, Mauk BH, Jaynes AN, Leonard T, Baker DN, Strangeway RJ, Russell CT, Gershman DJ, Avanov L, Giles BL, Torbert RB, Broll J, Gomez RG, Fuselier SA, Burch JL.   +23 more
europepmc   +1 more source

Mach 10 Bow-Shock Unsteadiness Modeled by Linear Combination of Two Mechanisms. [PDF]

AIAA J, 2017
Balla RJ.
europepmc   +1 more source

CONSTRAINING RELATIVISTIC BOW SHOCK PROPERTIES IN ROTATION-POWERED MILLISECOND PULSAR BINARIES. [PDF]

Astrophys J, 2017
Wadiasingh Z, Harding AK, Venter C, Böttcher M, Baring MG.   +4 more
europepmc   +1 more source