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Observation and Modeling of Solar Jets View all abstracts by submitter

Yuandeng Shen   Submitted: 2021-01-14 02:21

The solar atmosphere is full of complicated transients manifesting the reconfiguration of solar magnetic field and plasma. Solar jets represent collimated, beam-like plasma ejections; they are ubiquitous in the solar atmosphere and important for the understanding of solar activities at different scales, magnetic reconnection process, particle acceleration, coronal heating, solar wind acceleration, as well as other related phenomena. Recent high spatiotemporal resolution, wide-temperature coverage, spectroscopic, and stereoscopic observations taken by ground-based and space-borne solar telescopes have revealed many valuable new clues to restrict the development of theoretical models. This review aims at providing the reader with the main observational characteristics of solar jets, physical interpretations and models, as well as unsolved outstanding questions in future studies.

Authors: Yuandeng Shen
Projects: SDO-AIA

Publication Status: accepted for publication in Proceedings of the Royal Society A
Last Modified: 2021-01-14 13:38
Go to main E-Print page  The non-Fourier image reconstruction method for the STIX instrument  Challenges and Advances in Modeling of the Solar Atmosphere: A White Paper of Findings and Recommendations  Edit Entry  Download Preprint  Delete Entry 

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