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Fritz M. Neubauer

Researcher at University of Cologne

Publications -  273
Citations -  17002

Fritz M. Neubauer is an academic researcher from University of Cologne. The author has contributed to research in topics: Solar wind & Magnetosphere. The author has an hindex of 65, co-authored 273 publications receiving 16023 citations. Previous affiliations of Fritz M. Neubauer include Goddard Space Flight Center & Braunschweig University of Technology.

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The WIND magnetic field investigation

TL;DR: The magnetic field experiment on WIND will provide data for studies of a broad range of scales of structures and fluctuation characteristics of the interplanetary magnetic field throughout the mission, and, where appropriate, relate them to the statics and dynamics of the magnetosphere.
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Solar wind protons: Three-dimensional velocity distributions and derived plasma parameters measured between 0.3 and 1 AU

TL;DR: In this paper, it was found that a strong anisotropy in the core of proton distributions, with a temperature that is larger perpendicular rather than parallel to the magnetic field, is a persistent feature of high-speed streams, becoming most pronounced in the perihelion, or about 0.3 AU.
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In situ measurements of the physical characteristics of Titan's environment

TL;DR: The temperature and density profiles, as determined by the Huygens Atmospheric Structure Instrument (HASI), from an altitude of 1,400 km down to the surface were higher than expected and the extent of atmospheric electricity was also hitherto unknown.
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The Cassini Magnetic Field Investigation

TL;DR: The dual technique magnetometer system onboard the Cassini orbiter is described in this paper, which consists of vector helium and fluxgate magnetometers with the capability to operate the helium device in a scalar mode.
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Nonlinear standing Alfvén wave current system at Io: Theory

TL;DR: In this article, a nonlinear analytical model of the Alfven current tubes continuing the currents through Io (or rather its ionosphere) generated by the unipolar inductor effect due to Io's motion relative to the magnetospheric plasma was presented.