Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Luis Preisser"'
Autor:
Arturo Tinoco-Arenas, Primož Kajdič, Luis Preisser, Xóchitl Blanco-Cano, Domenico Trotta, David Burgess
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
We perform 2D local hybrid simulations of collisionless shocks in order to study the properties of simulated magnetosheath jets as a function of shock properties, namely their Alfvénic Mach number (MA) and geometry (angle between the upstream magnet
Externí odkaz:
https://doaj.org/article/3bfc44d4cf114757a4a2327089718dbe
Autor:
Luis Preisser, Ferdinand Plaschke, Florian Koller, Manuela Temmer, Owen Roberts, Zoltan Vörös
Large scale solar wind (SW) structures called Coronal Mass Ejections (CMEs) and Stream Interaction Regions (SIRs) propagate through the interplanetary medium, where they might impact Earth and cause jet-like disturbances in the magnetosheath. Such je
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9faab734962b8c5d3cd6e422fbf6ea2b
https://doi.org/10.5194/egusphere-egu23-9495
https://doi.org/10.5194/egusphere-egu23-9495
Autor:
Florian Koller, Ferdinand Plaschke, Luis Preisser, Manuela Temmer, Owen Roberts, Zoltan Vörös
Large-scale solar wind (SW) structures like coronal mass ejections (CMEs) and stream interaction regions (SIRs) significantly alter the plasma within the Earth’s magnetosheath and change the foreshock region. Thus, they modulate the number and the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ea87d0d5063103d9dd16882a5e81cfc6
https://doi.org/10.5194/egusphere-egu23-10625
https://doi.org/10.5194/egusphere-egu23-10625
Autor:
Domenico Trotta, Francesco Pecora, Adriana Settino, Denise Perrone, David Burgess, David Lario, Heli Hietala, Timothy Horbury, Rami Vainio, Luis Preisser, William Matthaeus, Oreste Pezzi, Sergio Servidio, Francesco Valentini
The interaction between shock and turbulence is an important pathway to energy conversion and particle acceleration in a large variety of astrophysical systems. Novel insights of such an interaction will be presented.Using a combination of in-situ ob
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::57de7990e63804b0fc04e96ea4863d84
https://doi.org/10.5194/egusphere-egu23-8810
https://doi.org/10.5194/egusphere-egu23-8810
Autor:
Florian Koller, Ferdinand Plaschke, Manuela Temmer, Luis Preisser, Owen W. Roberts, Zoltan Vörös
Publikováno v:
Journal of Geophysical Research: Space Physics. 128
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e372cdfd19b4df04b8102aab768c2408
https://doi.org/10.1029/2023ja031339
https://doi.org/10.1029/2023ja031339
Localized enhancements in dynamic pressure observed in the Earth’s magnetosheath (EMS) have been studied since 20 years ago. These structures known as jets can propagate through the EMS transporting mass, momentum and energy being able to reach and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::da65c1a3679dfb9aec59bff3214c8554
https://doi.org/10.5194/egusphere-egu22-11999
https://doi.org/10.5194/egusphere-egu22-11999
Autor:
Xochitl Blanco-Cano, Primoz Kajdic, Diana Rojas-Castillo, Luis Preisser, Lan Jian, Christopher Russell, Janet Luhmann
Interplanetary (IP) shocks can be driven in the solar wind by fast coronal mass ejections and by the interaction of fast solar wind with slow streams of plasma. These shocks can be preceded by extended wave and suprathermal ion foreshocks. We use STE
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::28056f8d48701ae8ab547539c69f71f6
https://doi.org/10.5194/egusphere-egu22-6088
https://doi.org/10.5194/egusphere-egu22-6088
Magnetosheath jets are dynamic pressure enhancements frequently observed in the Earth’s magnetosheath. They are significant coupling elements between the solar wind and the magnetosphere of the Earth and they can be geoeffective. Jets travel anti-s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e68d7f7571554ee1a942c88e248e3f8e
https://doi.org/10.5194/egusphere-egu22-6521
https://doi.org/10.5194/egusphere-egu22-6521
Autor:
Florian Koller, Manuela Temmer, Luis Preisser, Ferdinand Plaschke, Paul Geyer, Lan K Jian, Owen Wyn Roberts, Heli Hietala, Adrian T. LaMoury
Magnetosheath jets constitute a significant coupling effect between the solar wind (SW) and the magnetosphere of the Earth. In order to investigate the effects and forecasting of these jets, we present the first-ever statistical study of the jet prod
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3a84cee96178465a0235d08ca48982cd
https://doi.org/10.1002/essoar.10508761.1
https://doi.org/10.1002/essoar.10508761.1