Initial Study on Coronal Plasma Jet Formation
The sudden explosive events in the solar corona are thought to be best explained by ideal magnetohydrodynamic (MHD) instabilities and magnetic reconnection. One type of explosive event, the x-ray jet, has been observed to originate from ``anemone-type" active regions---dome-shaped magnetic stru...
Saved in:
| Main Author: | |
|---|---|
| Other Authors: | |
| Format: | Princeton University Senior Theses |
| Language: | English |
| Published: |
2020
|
| Online Access: | http://arks.princeton.edu/ark:/88435/dsp01gb19f885v |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|