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Dr. Antiochos is an internationally recognized authority on space and plasma physics. His research is distinguished by the development of innovative models to explain major observational problems, and combines both basic theory and state-of-the-art numerical simulation. Dr. Antiochos has made many fundamental advances to our understanding of the Sun and Heliosphere. Some of his best-known contributions include the following:
· his work on coronal loop dynamics, chromospheric evaporation and the cool loop model for the transition region.
· the thermal nonequilibrium theory for the formation of coronal condensations, which is widely believed to be the definitive explanation for how cool filaments/prominence mass forms in the hot corona
· the 3D sheared arcade model for the topology of prominence magnetic fields
· the breakout model for the initiation of coronal mass ejections/solar flares
· the resistive-kink and breakout models for coronal jets
· the S-Web theory for the sources of the slow solar wind
· the theory of “helicity condensation”, which explains three long-standing observational puzzles of the corona-heliosphere system: (1) the smoothness of coronal loops, (b) the magnetic shear in prominences/filaments, and (c) the variability of the slow solar wind.
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Bulletin of the AAS (2023)
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Advances in Space Research (2023)
arXiv (Cornell University) (2023)
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arxiv(2023)
ASTROPHYSICAL JOURNAL LETTERSno. 1 (2023): L15-L15
J. Qiu, M. Alaoui,S. K. Antiochos,J. T. Dahlin,M. Swisdak,J. F. Drake, A. Robison,C. R. DeVore, V. M. Uritsky
ASTROPHYSICAL JOURNALno. 1 (2023): 34-34
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