10 results match your criteria: "Institute of Geophysics and extraterrestrial Physics[Affiliation]"
Space Sci Rev
December 2024
Space Research Institute, Austrian Academy of Sciences, Schmiedlstraße 6, Graz, 8042 Austria.
Plasma flows with enhanced dynamic pressure, known as magnetosheath jets, are often found downstream of collisionless shocks. As they propagate through the magnetosheath, they interact with the surrounding plasma, shaping its properties, and potentially becoming geoeffective upon reaching the magnetopause. In recent years (since 2016), new research has produced vital results that have significantly enhanced our understanding on many aspects of jets.
View Article and Find Full Text PDFJ Eng Math
December 2023
Space Research Institute, Austrian Academy of Sciences, Schmiedlstraße 6, 8042 Graz, Austria.
Gas flow through layers of porous materials plays a crucial role in technical applications, geology, petrochemistry, and space sciences (e.g., fuel cells, catalysis, shale gas production, and outgassing of volatiles from comets).
View Article and Find Full Text PDFPhys Rev E
March 2023
Technische Universität Braunschweig, Institute of Geophysics and extraterrestrial Physics, Mendelssohnstr. 3, 38106 Braunschweig, Germany.
We analyzed the translational and rotational Brownian motion of aggregates of micrometer-sized silica spheres under microgravity conditions and in rarefied gas. The experimental data was collected in the form of high-speed recordings using a long-distance microscope as part of the ICAPS (Interactions in Cosmic and Atmospheric Particle Systems) experiment on board of the sounding rocket flight Texus-56. Our data analysis shows that the translational Brownian motion can be used to determine the mass and translational response time of each individual dust aggregate.
View Article and Find Full Text PDFShocks are one of nature's most powerful particle accelerators and have been connected to relativistic electron acceleration and cosmic rays. Upstream shock observations include wave generation, wave-particle interactions and magnetic compressive structures, while at the shock and downstream, particle acceleration, magnetic reconnection and plasma jets can be observed. Here, using Magnetospheric Multiscale (MMS) we show in-situ evidence of high-speed downstream flows (jets) generated at the Earth's bow shock as a direct consequence of shock reformation.
View Article and Find Full Text PDFSensors (Basel)
December 2021
Institute of Geosystems and Bioindication, TU Braunschweig, 38106 Braunschweig, Germany.
Lakes are integrators of past climate and ecological change. This information is stored in the sediment record at the lake bottom, and to make it available for paleoclimate research, potential target sites with undisturbed and continuous sediment sequences need to be identified. Different geophysical methods are suitable to identify, explore, and characterize sediment layers prior to sediment core recovery.
View Article and Find Full Text PDFSensors (Basel)
October 2021
Research Unit Geophysics, Department of Geodesy and Geoinformation, Technische Universität Wien, 1040 Vienna, Austria.
Water-borne transient electromagnetic (TEM) soundings provide the means necessary to investigate the geometry and electrical properties of rocks and sediments below continental water bodies, such as rivers and lakes. Most water-borne TEM systems deploy separated magnetic transmitter and receiver loop antennas-typically in a central or offset configuration. These systems mostly require separated floating devices with rigid structures for both loop antennas.
View Article and Find Full Text PDFGeophys Res Lett
August 2015
School of Physics and Astronomy University of Minnesota, Twin Cities Minneapolis Minnesota USA.
Substorms generally inject tens to hundreds of keV electrons, but intense substorm electric fields have been shown to inject MeV electrons as well. An intriguing question is whether such MeVelectron injections can populate the outer radiation belt. Here we present observations of a substorm injection of MeV electrons into the inner magnetosphere.
View Article and Find Full Text PDFScience
May 2009
Institute of Geophysics and Extraterrestrial Physics, Technical University of Braunschweig, Braunschweig, and Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany.
Phys Rev Lett
November 2006
Institute of Geophysics and Extraterrestrial Physics, Mendelssohnstrasse 3, D-38106 Braunschweig, Germany.
Wave-number spectra of magnetic field fluctuations are directly determined in the terrestrial foreshock region (upstream of a quasiparallel collisionless shock wave) using four-point Cluster spacecraft measurements. The spectral curve is characterized by three ranges reminiscent of turbulence: energy injection, inertial, and dissipation range. The spectral index for the inertial range spectrum is close to Kolmogorov's slope, -5/3.
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