Zobrazeno 1 - 10
of 186
pro vyhledávání: '"Kajdic, P."'
Autor:
Dimmock, Andrew P., Gedalin, Michael, Lalti, Ahmad, Trotta, Domenico, Khotyaintsev, Yuri V., Graham, Daniel B., Johlander, Andreas, Vainio, Rami, Blanco-Cano, Xochitl, Kajdič, Primoz, Owen, Christopher J., Wimmer-Schweingruber, Robert F.
Solar Orbiter, a mission developed by the European Space Agency, explores in situ plasma across the inner heliosphere while providing remote-sensing observations of the Sun. Our study examines particle observations for the 30 October 2021 shock. The
Externí odkaz:
http://arxiv.org/abs/2310.09050
Autor:
Trotta, Domenico, Pezzi, Oreste, Burgess, David, Preisser, Luis, Blanco-Cano, Xochitl, Kajdic, Primoz, Hietala, Heli, Horbury, Timothy S., Vainio, Rami, Dresing, Nina, Retino', Alessandro, Marcucci, Maria Federica, Sorriso-Valvo, Luca, Servidio, Sergio, Valentini, Francesco
The complex interaction between shocks and plasma turbulence is extremely important to address crucial features of energy conversion in a broad range of astrophysical systems. We study the interaction between a supercritical, perpendicular shock and
Externí odkaz:
http://arxiv.org/abs/2305.15168
Autor:
Madanian, H., Omidi, N., Sibeck, D. G., Andersson, L., Ramstad, R., Xu, S., Gruesbeck, J. R., Schwartz, S. J., Frahm, R. A., Brain, D. A., Kajdic, P., Eparvier, F. G., Mitchell, D. L., Curry, S. M.
Publikováno v:
Geophysical Research Letters Volume 50, Issue8 28 April 2023 e2022GL101734
We characterize the nature of magnetic structures in the foreshock region of Mars associated with discontinuities in the solar wind. The structures form at the upstream edge of moving foreshocks caused by slow rotations in the interplanetary magnetic
Externí odkaz:
http://arxiv.org/abs/2301.11452
Autor:
Dimmock, A. P., Yordanova, E., Graham, D. B., Khotyaintsev, Yu. V., Blanco-Cano, X., Kajdič, P., Karlsson, T., Fedorov, A., Owen, C. J., Werner, E. A. L. E., Johlander, A.
Mirror modes are ubiquitous in space plasma and grow from pressure anisotropy. Together with other instabilities, they play a fundamental role in constraining the free energy contained in the plasma. This study focuses on mirror modes observed in the
Externí odkaz:
http://arxiv.org/abs/2210.04734
Autor:
Kajdic, Primoz, Pfau-Kempf, Yann, Turc, Lucile, Dimmock, Andrew P, Palmroth, Minna, Takahashi, Kazue, Kilpua, Eemilia, Soucek, Jan, Takahashi, Naoko, Preisser, Luis, Blanco-Cano, Xochitl, Trotta, Domenico, Burgess, David
Publikováno v:
Journal of Geophysical Research: Space Physics, 126, e2021JA029283
We study the interaction of upstream ultra-low frequency (ULF) waves with collisionless shocks by analyzing the outputs of eleven 2D local hybrid simulation runs. Our simulated shocks have Alfv\'enic Mach numbers between 4.29-7.42 and their $\theta_{
Externí odkaz:
http://arxiv.org/abs/2201.10558
Autor:
Kajdic, Primoz, Sanchez-Cano, Beatriz, Neves-Ribeiro, Laura, Witasse, Olivier, Bernal, Giovanni C., Rojas-Castillo, Diana, Nilsson, Hans, Fedorov, Andrei
We study the interaction of three solar wind structures, two stream interaction regions and one interplanetary coronal mass ejection, with Mars' plasma environment during 20-27 November 2007. This period corresponds to the solar minimum between the s
Externí odkaz:
http://arxiv.org/abs/2107.00585
Magnetosheath jets are currently an important topic in the field of magnetosheath physics. It is thought that 97~\% of the jets are produced by the shock rippling at quasi-parallel shocks. Recently, large statistical studies of magnetosheath jets hav
Externí odkaz:
http://arxiv.org/abs/2106.15747
Akademický článek
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Publikováno v:
The ApJ Letters, Volume 874, Number 2, 2019
We present the first observational evidence of the irregular surface of interplanetary (IP) shocks by using multi-spacecraft observations of the Cluster mission. In total we discuss observations of four IP shocks that exhibit moderate Alfv\'enic Mach
Externí odkaz:
http://arxiv.org/abs/1903.11653
Akademický článek
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