2023 - Research.com Earth Science in United States Leader Award
2019 - Arctowski Medal, U.S. National Academy of Sciences For her fundamental contributions to our understanding of the relationships between the sun and its planetary bodies, with a particular emphasis on the physics of collisionless shocks and the dynamics of the planetary magnetospheres of Earth, Jupiter, and Saturn." 2017,Mats Carlsson
2001 - Fellow of American Geophysical Union (AGU)
The scientist’s investigation covers issues in Magnetosphere, Geophysics, Solar wind, Computational physics and Atomic physics. Her study in Magnetosphere is interdisciplinary in nature, drawing from both Enceladus, Astrophysics and Saturn. The Geophysics study combines topics in areas such as Magnetopause, Magnetosheath, Convection, Ring current and Interplanetary magnetic field.
The concepts of her Solar wind study are interwoven with issues in Shock wave, Mechanics, Plasma sheet and Shock. She combines subjects such as Optics, Guiding center, Magnetohydrodynamics, Pitch angle and Magnetosphere particle motion with her study of Computational physics. She has included themes like Particle acceleration, Plasma, Electron temperature, Ion and Electron in her Atomic physics study.
Michelle F. Thomsen mostly deals with Magnetosphere, Geophysics, Plasma, Solar wind and Astrophysics. Michelle F. Thomsen interconnects Computational physics, Astronomy, Ionosphere and Saturn in the investigation of issues within Magnetosphere. Her research integrates issues of Magnetopause, Geosynchronous orbit, Plasmasphere, Ring current and Geomagnetic storm in her study of Geophysics.
Her Plasma study combines topics from a wide range of disciplines, such as Convection, Spacecraft, Atomic physics, Ion and Astrobiology. Michelle F. Thomsen focuses mostly in the field of Atomic physics, narrowing it down to topics relating to Electron and, in certain cases, Van Allen radiation belt. Her Solar wind study combines topics in areas such as Shock wave and Bow shock.
Her main research concerns Magnetosphere, Plasma, Saturn, Geophysics and Astrophysics. Her Magnetosphere research is multidisciplinary, incorporating elements of Astronomy and Solar wind. Her work carried out in the field of Plasma brings together such families of science as Ion, Computational physics, Electron and Atomic physics.
Her Saturn research incorporates themes from Line, Spectrometer, Charged particle and Flux. She works mostly in the field of Geophysics, limiting it down to topics relating to Field line and, in certain cases, Geomagnetic storm and Pitch angle. As a member of one scientific family, Michelle F. Thomsen mostly works in the field of Astrophysics, focusing on Plasmoid and, on occasion, Electron temperature.
Michelle F. Thomsen spends much of her time researching Magnetosphere, Geophysics, Plasma, Saturn and Magnetosphere of Saturn. Her Magnetosphere research integrates issues from Solar wind and Ionosphere. Her research in Geophysics intersects with topics in Magnetohydrodynamics, Current sheet, Astrophysics and Plasmasphere.
Her Astrophysics research is multidisciplinary, relying on both Magnetic field and Plasmoid. The various areas that Michelle F. Thomsen examines in her Plasma study include Computational physics, Torus, Atomic physics, Ion and Electron. Her biological study spans a wide range of topics, including Magnetosheath, Astronomy, Enceladus, Magnetosphere of Jupiter and Magnetic reconnection.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
Cassini plasma spectrometer investigation
D. T. Young;J. J. Berthelier;M. Blanc;J. L. Burch.
Space Science Reviews (2004)
The driving of the plasma sheet by the solar wind
Joseph E. Borovsky;Michelle F. Thomsen;Richard C. Elphic.
Journal of Geophysical Research (1998)
Electron velocity distributions near the Earth's bow shock
W. C. Feldman;R. C. Anderson;S. J. Bame;S. P. Gary.
Journal of Geophysical Research (1983)
Helium, Oxygen, Proton, and Electron (HOPE) Mass Spectrometer for the Radiation Belt Storm Probes Mission
H. O. Funsten;R. M. Skoug;A. A. Guthrie;E. A. MacDonald.
Space Science Reviews (2013)
Observations of reconnection of interplanetary and lobe magnetic field lines at the high‐latitude magnetopause
J. T. Gosling;M. F. Thomsen;S. J. Bame;R. C. Elphic.
Journal of Geophysical Research (1991)
Science Goals and Overview of the Radiation Belt Storm Probes (RBSP) Energetic Particle, Composition, and Thermal Plasma (ECT) Suite on NASA’s Van Allen Probes Mission
H. E. Spence;G. D. Reeves;D. N. Baker;J. B. Blake.
Space Science Reviews (2013)
Plasma flow reversals at the dayside magnetopause and the origin of asymmetric polar cap convection
J. T. Gosling;M. F. Thomsen;S. J. Bame;R. C. Elphic.
Journal of Geophysical Research (1990)
The Earth's plasma sheet as a laboratory for flow turbulence in high-β MHD
Joseph E. Borovsky;Richard C. Elphic;Herbert O. Funsten;Michelle F. Thomsen.
Journal of Plasma Physics (1997)
Dominant role of the asymmetric ring current in producing the stormtime Dst
M. W. Liemohn;J. U. Kozyra;M. F. Thomsen;J. L. Roeder.
Journal of Geophysical Research (2001)
Composition and dynamics of plasma in Saturn's magnetosphere.
D. T. Young;Jean-Jacques Berthelier;M. Blanc;J. L. Burch.
Science (2005)
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