Alfvén Pulse driven Cool Spicule-like Jets in the Sun's Atmosphere | Balveer Singh
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08.06.2023
Co-author
A.K. Srivastava
Affiliation
Department of Physics, Indian Institute of Technology (BHU), India
Main category
Natural Sciences (Astrophysics and Astrononmy)
Caption
The complex magnetic structuring and highly dynamical nature of the solar atmosphere allow triggering of various cool spicule-like thin jets (T<105 K). These cool jets are basically collimated plasma ejecta that rise and fall quasi-periodically along the magnetic field lines in the Sun’s atmosphere. Several multiwavelength observations have been captured from space and ground based observatories revealing the evolution of these small scale cool jets and associated plasma processes (e.g., waves and oscillations, instabilities etc). Their physics can be understood extensively by performing numerical simulations. We numerically model such plasma jets in 2.5 D regime using the theory of Magnetohydrodynamics (MHD). Read more at https://espos.stream/2023/06/08/Singh/ .
Further information
Further reading
Link to the European Solar Physics Online Seminars (ESPOS) webpage: https://espos.stream/2023/06/08/Singh/
Language
English
DOI
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