Results 11 to 20 of about 7,959 (209)

On the Kinetic Energy Input of Magnetosheath Jets Into the Magnetosheath

Geophysical Research Letters
Magnetosheath jets, plasma structures with enhanced dynamic pressure, are frequently observed in the terrestrial magnetosheath. However, their mass, momentum, and energy content are still unknown. We utilize Amitis, a 3D hybrid‐kinetic plasma simulation,
Eva Krämer, Shahab Fatemi, Maria Hamrin, Herbert Gunell, Gabriella Semrén   +4 more
doaj   +3 more sources

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   +3 more sources

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

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

Plasma and Magnetic Field Turbulence in the Earth’s Magnetosheath at Ion Scales

Frontiers in Astronomy and Space Sciences, 2021
Crossing the Earth’s bow shock is known to crucially affect solar wind plasma including changes in turbulent cascade. The present review summarizes results of more than 15 years of experimental exploration into magnetosheath turbulence.
Liudmila Rakhmanova, Maria Riazantseva, Georgy Zastenker   +2 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

Large-scale solar wind flow around Saturn's nonaxisymmetric magnetosphere [PDF]

, 2017
The interaction between the solar wind and a magnetosphere is fundamental to the dynamics of a planetary system. Here, we address fundamental questions on the large-scale magnetosheath flow around Saturn using a 3D magnetohydrodynamic (MHD) simulation ...
Achilleos, N., Gurnett, D. A., Jia, X., Kurth, W. S., Sergis, N., Sulaiman, A. H.   +5 more
core   +3 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