His primary scientific interests are in Coronal mass ejection, Solar wind, Heliosphere, Geophysics and Astrophysics. His research in Coronal mass ejection intersects with topics in Astronomy, Space weather, Magnetohydrodynamics and Interplanetary spaceflight. His work in Solar wind covers topics such as Meteorology which are related to areas like Space environment and Lagrangian point.
His Heliosphere research is multidisciplinary, incorporating elements of Flow, Deflection, Interplanetary space and Shock. His Geophysics study combines topics from a wide range of disciplines, such as Coronal hole, Solar physics, Latitude, Leading edge and Outflow. His work carried out in the field of Astrophysics brings together such families of science as Drag, Kinematics and Solar prominence.
His main research concerns Solar wind, Coronal mass ejection, Heliosphere, Geophysics and Space weather. Dusan Odstrcil has researched Solar wind in several fields, including Spacecraft, Magnetohydrodynamics and Meteorology. His Coronal mass ejection research integrates issues from Astronomy, Solar physics, Astrophysics, Corona and Interplanetary spaceflight.
His Heliosphere research incorporates themes from Geomagnetic storm, Satellite and Magnitude. His Geophysics research is multidisciplinary, incorporating perspectives in Coronal hole, Magnetosphere, Heliospheric current sheet and Outflow. His research integrates issues of Space environment and Solar energetic particles in his study of Space weather.
The scientist’s investigation covers issues in Solar wind, Coronal mass ejection, Space weather, Heliosphere and Astrophysics. His work deals with themes such as Impact ionization, Magnetohydrodynamics and Geophysics, which intersect with Solar wind. His study in Coronal mass ejection is interdisciplinary in nature, drawing from both Astronomy, Mars Exploration Program, Interplanetary spaceflight and Solar minimum.
He has included themes like Solar energetic particles, Solar physics and Interplanetary scintillation in his Space weather study. His biological study spans a wide range of topics, including Spacecraft and Solar maximum. His work on Event and Telescope as part of his general Astrophysics study is frequently connected to Proton and Population, thereby bridging the divide between different branches of science.
Dusan Odstrcil mainly focuses on Solar wind, Heliosphere, Coronal mass ejection, Astronomy and Mars Exploration Program. His studies deal with areas such as Spacecraft, Aerospace engineering and Astrophysics as well as Solar wind. His Heliosphere study integrates concerns from other disciplines, such as Solar maximum, Space weather, Heliospheric current sheet and Solar energetic particles.
His Space weather study is concerned with the larger field of Meteorology. The Coronal mass ejection study combines topics in areas such as Geophysics and Solar minimum. His Geophysics research is multidisciplinary, relying on both Coronal loop, Solar physics and Remote sensing.
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.
Modeling 3-D solar wind structure
D. Odstrcil.
Advances in Space Research (2003)
Numerical simulation of the 12 May 1997 interplanetary CME event
D. Odstrcil;P. Riley;X. P. Zhao.
Journal of Geophysical Research (2004)
Stream structure and coronal sources of the solar wind during the May 12th, 1997 CME
C.N. Arge;J.G. Luhmann;D. Odstrcil;C.J. Schrijver.
Journal of Atmospheric and Solar-Terrestrial Physics (2004)
Improved Method for Specifying Solar Wind Speed Near the Sun
Charles N. Arge;Dusan Odstrcil;Victor J. Pizzo;Leslie R. Mayer.
SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference (2003)
Three-dimensional propagation of coronal mass ejections (CMEs) in a structured solar wind flow: 2. CME launched adjacent to the streamer belt
D. Odstrčil;V. J. Pizzo.
Journal of Geophysical Research (1999)
Ensemble modeling of CMEs using the WSA-ENLIL+Cone model
M. L. Mays;A. Taktakishvili;A. A. Pulkkinen;P. J. MacNeice.
arXiv: Solar and Stellar Astrophysics (2015)
Characteristics of kinematics of a coronal mass ejection during the 2010 August 1 CME-CME interaction event
Manuela Temmer;Bojan Vrsnak;Tanja Rollett;Bianca Bein.
arXiv: Solar and Stellar Astrophysics (2012)
Propagation of the 12 May 1997 interplanetary coronal mass ejection in evolving solar wind structures
D. Odstrcil;D. Odstrcil;V. J. Pizzo;C. N. Arge.
Journal of Geophysical Research (2005)
Distortion of the interplanetary magnetic field by three‐dimensional propagation of coronal mass ejections in a structured solar wind
D. Odstrcil;V. J. Pizzo.
Journal of Geophysical Research (1999)
Ensemble Modeling of CMEs Using the WSA–ENLIL+Cone Model
M. L. Mays;M. L. Mays;A. Taktakishvili;A. Taktakishvili;A. Pulkkinen;P. J. MacNeice.
Solar Physics (2015)
If you think any of the details on this page are incorrect, let us know.
We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below:
University of California, Berkeley
Science Applications International Corporation (United States)
Lamont-Doherty Earth Observatory
University of Michigan–Ann Arbor
Goddard Space Flight Center
University of Colorado Boulder
Johns Hopkins University Applied Physics Laboratory
University of California, Berkeley
University of New Hampshire
University of Michigan–Ann Arbor
Hong Kong University of Science and Technology
Shandong University of Science and Technology
Peking University
Spanish National Research Council
Hunan Agricultural University
Rutherford Appleton Laboratory
King Abdullah University of Science and Technology
California Institute of Technology
Seoul National University
University of Sargodha
University of Michigan–Ann Arbor
Saint Mary's University
National Institute of Geophysics and Volcanology
Mayo Clinic
Johns Hopkins University School of Medicine
Oregon Health & Science University