2008 - Fellow of American Physical Society (APS) Citation In recognition of his farreaching scientific contributions to solar astrophysics, among them several compelling models explaining a variety of phenomena originating in the interactions between magnetic fields and plasmas, and his service to the international solar and space physics communities
2005 - Fellow of American Geophysical Union (AGU)
Spiro K. Antiochos mainly investigates Astrophysics, Coronal mass ejection, Magnetohydrodynamics, Solar flare and Corona. Spiro K. Antiochos interconnects Coronal loop, Photosphere, Astronomy, Chromosphere and Magnetic reconnection in the investigation of issues within Astrophysics. His work in the fields of Coronal mass ejection, such as Magnetic cloud, overlaps with other areas such as Breakout and Magnetic energy.
The concepts of his Magnetohydrodynamics study are interwoven with issues in Field line and Polar. Solar flare and Flare are commonly linked in his work. His Corona research includes themes of Heliospheric current sheet, Interplanetary spaceflight and Nanoflares.
Astrophysics, Magnetic reconnection, Mechanics, Coronal mass ejection and Coronal loop are his primary areas of study. His Astrophysics research incorporates themes from Coronal hole, Magnetohydrodynamics and Nanoflares. His research in Magnetic reconnection intersects with topics in Jet and Current sheet.
His Mechanics study also includes
Spiro K. Antiochos focuses on Astrophysics, Coronal mass ejection, Magnetic reconnection, Coronal hole and Protein filament. His study on Corona, Solar flare and Flare is often connected to Breakout as part of broader study in Astrophysics. His Corona research is multidisciplinary, relying on both Nanoflares, Coronal loop, Magnetic helicity, Photosphere and Solar wind.
His Solar wind research is multidisciplinary, incorporating elements of Solar prominence, Magnetohydrodynamics, Meteorology and Solar dynamics observatory. His Coronal mass ejection study integrates concerns from other disciplines, such as Field line, Space weather and Magnetic flux. The various areas that he examines in his Coronal hole study include Heliosphere and Helmet streamer.
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A Model for Solar Coronal Mass Ejections
S. K. Antiochos;C. R. DeVore;J. A. Klimchuk.
The Astrophysical Journal (1999)
The magnetic topology of solar eruptions
Spiro K. Antiochos.
The Astrophysical Journal (1998)
CME Theory and Models
T. G. Forbes;J. A. Linker;J. Chen;C. Cid.
Space Science Reviews (2006)
A MODEL FOR SOLAR POLAR JETS
E. Pariat;E. Pariat;E. Pariat;S. K. Antiochos;C. R. DeVore.
The Astrophysical Journal (2009)
The Dynamic Formation of Prominence Condensations
Spiro K. Antiochos;Peter J. MacNeice;Daniel S. Spicer;James.
arXiv: Astrophysics (1998)
The Topology and Evolution of the Bastille Day Flare
G. Aulanier;E. E. DeLuca;S. K. Antiochos;R. A. McMullen.
The Astrophysical Journal (2000)
Are Magnetic Dips Necessary for Prominence Formation
J. T. Karpen;S. K. Antiochos;M. Hohensee;J. A. Klimchuk.
The Astrophysical Journal (2001)
Force-free magnetic fields - The magneto-frictional method
W. H. Yang;P. A. Sturrock;S. K. Antiochos.
The Astrophysical Journal (1986)
Homologous Confined Filament Eruptions via Magnetic Breakout
C. Richard DeVore;Spiro K. Antiochos;Spiro K. Antiochos.
The Astrophysical Journal (2008)
Numerical modeling of quasi-static coronal loops. I - Uniform energy input
J. F. Vesecky;S. K. Antiochos;J. H. Underwood.
The Astrophysical Journal (1979)
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