Annales Geophysicae
Annales Geophysicae
ANGEO
Articles | Volume 37, issue 5
Articles | Volume 37, issue 5
https://doi.org/10.5194/angeo-37-891-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
Special issue:
https://doi.org/10.5194/angeo-37-891-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
Articles | Volume 37, issue 5
Regular paper
 | 
24 Sep 2019
Regular paper |  | 24 Sep 2019

On modelling the kinematics and evolutionary properties of pressure-pulse-driven impulsive solar jets

Balveer Singh, Kushagra Sharma, and Abhishek K. Srivastava

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Latest update: 10 Dec 2024
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Short summary
Solar jets driven by heat or pressure pulses at their footpoints in the photosphere transfer energy and mass in to the corona. These jets energize the coronal part of the atmosphere with collimated plasma, similar to the fluid filled in a pipe. Understanding the physical drivers of such jets is of great significance to study the plasma in confined magnetic fields. The modelled jets in our paper allow for the study of the evolution of chromospheric plasma and support many existing observations.
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Special issue
Solar magnetism from interior to corona and beyond