Results 11 to 20 of about 887 (157)

Sunward flows in the magnetosheath associated with the magnetic pressure gradient and magnetosheath expansion

Frontiers in Astronomy and Space Sciences
A density structure within the magnetic cloud of an interplanetary coronal mass ejection impacted Earth and caused significant perturbations in plasma boundaries.
H. Madanian, H. Madanian, Y. Pfau-Kempf, R. Rice, R. Rice, T. Liu, T. Karlsson, S. Raptis, D. Turner, J. Beedle   +9 more
doaj   +4 more sources

Magnetosheath jets at Mars. [PDF]

Sci Adv, 2023
Plasma entities, known as magnetosheath jets, with higher dynamic pressure than the surrounding plasma, are often seen at Earth. They generate waves and contribute to energy transfer in the magnetosheath. Affecting the magnetopause, they cause surface waves and transfer energy into the magnetosphere, causing throat auroras and magnetic signatures ...
Gunell H, Hamrin M, Nesbit-Östman S, Krämer E, Nilsson H.   +4 more
europepmc   +4 more sources

Magnetopause stand-off distance in dependence on the magnetosheath and solar wind parameters [PDF]

Annales Geophysicae, 1998
A model of the magnetosheath structure proposed in a recent paper from the authors is extended to estimate the magnetopause stand-off distance from solar wind data.
M. I. Pudovkin, B. P. Besser, S. A. Zaitseva   +2 more
doaj   +1 more source

Magnetosheath-cusp interface [PDF]

Annales Geophysicae, 2004
Abstract. We advance the achievements of Interball-1 and other contemporary missions in exploration of the magnetosheath-cusp interface. Extensive discussion of published results is accompanied by presentation of new data from a case study and a comparison of those data within the broader context of three-year magnetopause (MP) crossings by Interball-1.
S. Savin, L. Zelenyi, S. Romanov, I. Sandahl, J. Pickett, E. Amata, L. Avanov, J. Blecki, E. Budnik, J. Büchner, C. Cattell, G. Consolini, J. Fedder, S. Fuselier, H. Kawano, S. Klimov, V. Korepanov, D. Lagoutte, F. Marcucci, M. Mogilevsky, Z. Nemecek, B. Nikutowski, M. Nozdrachev, M. Parrot, J. L. Rauch, V. Romanov, T. Romantsova, C. T. Russell, J. Safrankova, J. A. Sauvaud, A. Skalsky, V. Smirnov, K. Stasiewicz, K. Stasiewicz, J. G. Trotignon, YU. Yermolaev   +35 more
openaire   +6 more sources

Asymmetries in the Earth's dayside magnetosheath: results from global hybrid-Vlasov simulations [PDF]

Annales Geophysicae, 2020
Bounded by the bow shock and the magnetopause, the magnetosheath forms the interface between solar wind and magnetospheric plasmas and regulates solar wind–magnetosphere coupling.
L. Turc, V. Tarvus, A. P. Dimmock, M. Battarbee, U. Ganse, A. Johlander, M. Grandin, Y. Pfau-Kempf, M. Dubart, M. Palmroth, M. Palmroth   +10 more
doaj   +1 more source

Relaxation of the turbulent magnetosheath

Monthly Notices of the Royal Astronomical Society, 2023
ABSTRACTIn turbulence, non-linear terms drive energy transfer from large-scale eddies into small scales through the so-called energy cascade. Turbulence often relaxes toward states that minimize energy; typically these states are considered globally.
F Pecora, Y Yang, A Chasapis, S Servidio, M E Cuesta, S Roy, R Chhiber, R Bandyopadhyay, D J Gershman, B L Giles, J L Burch, W H Matthaeus   +11 more
openaire   +2 more sources

Scalar-potential mapping of the steady-state magnetosheath model [PDF]

Annales Geophysicae
The steady-state magnetosheath model has various applications for studying the plasma and magnetic field profile around the planetary magnetospheres.
Y. Narita, D. Schmid, S. Toepfer
doaj   +1 more source

South-north asymmetry of proton density distribution in the Martian magnetosheath

Earth and Planetary Physics, 2020
We perform a statistical analysis of data from the Mars Atmosphere and Volatile Evolution (MAVEN) project on the global distribution of protons in the Martian magnetosheath.
Jing Wang, XiaoJun Xu, Jiang Yu, YuDong Ye   +3 more
doaj   +1 more source

Characteristics of > 290 keV magnetosheath ions [PDF]

Annales Geophysicae, 1999
We performed a statistical analysis of 290-500 keV ion data obtained by IMP-8 during the years 1982-1988 within the earth's magnetosheath and analysed in detail some time periods withdistinct ion bursts.
I. Karanikola, G. C. Anagnostopoulos, G. C. Anagnostopoulos, A. Rigas   +3 more
doaj   +1 more source

Large-Scale Solar Wind Phenomena Affecting the Turbulent Cascade Evolution behind the Quasi-Perpendicular Bow Shock

Universe, 2022
The Earth’s magnetosphere is permanently influenced by the solar wind. When supersonic and superalfvenic plasma flow interacts with the magnetosphere, the magnetosheath region is formed, which is filled with shocked turbulent plasma.
Liudmila S. Rakhmanova, Maria O. Riazantseva, Georgy N. Zastenker, Yuri I. Yermolaev   +3 more
doaj   +1 more source