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Shocks and shells in hot star winds
Astrophysics and Space Science, 1995Radiation-driven winds of hot, massive stars show variability in UV and optical line profiles on time scales of hours to days. Shock heating of wind material is indicated by the observed X-ray emission. We present time-dependent hydrodynamical models of these winds, where flow structures originate from a strong instability of the radiative driving ...
A. Feldmeier +5 more
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Winding factor analysis of star-delta windings
2017 IEEE Transportation Electrification Conference and Expo (ITEC), 2017Windings utilizing the star-delta (Y-D) topology are known to offer an improved MMF spectrum as the main winding factor is increased while parasitic spatial harmonics are decreased or even cancelled. Although several windings were proposed in the past, winding factors were mostly calculated individually depending on the specific winding under ...
Boris Dotz, Dieter Gerling
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Effects of rotation on hot star winds
Astrophysics and Space Science, 1994We discuss the structure of a radiatively-driven wind from a rapidly rotating hot star. When the rotation rate is large, there is a region at low latitudes near the stellar surface where the force of gravity is larger than the radiation pressure. Within this region, the streamlines “fall” toward the equator, and if the rotation rate is large enough ...
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Global climatology of synoptically‐forced downslope winds
International Journal of Climatology, 2021John T Abatzoglou +2 more
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Variations of Thermospheric Winds Observed by a Fabry–Perot Interferometer at Mohe, China
Journal of Geophysical Research: Space Physics, 2021Libo Liu, Cong Huang, Craig Unick
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Tropical Cyclone Winds from WindSat, AMSR2, and SMAP: Comparison with the HWRF Model
Remote Sensing, 2021Thomas Meissner +2 more
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Origin of Jupiter’s cloud-level zonal winds remains a puzzle even after Juno
Proceedings of the National Academy of Sciences of the United States of America, 2018Gerald Schubert +2 more
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