The Early Evolution of Solar Flaring Plasma Loops
Plasma loops are the elementary structures of solar flaring active regions and dominate the whole process of flaring eruptions. Standard flare models explain evolution and eruption after magnetic reconnection around the hot cusp-structure above the top of plasma loops very well; however, the early e...
Main Author: | Baolin Tan |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2021-10-01
|
Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/7/10/378 |
Similar Items
-
Understanding the Duration of Solar and Stellar Flares at Various Wavelengths
by: Jeffrey W. Reep, et al.
Published: (2023-01-01) -
The Transition Region of Solar Flare Loops
by: Costis Gontikakis, et al.
Published: (2023-01-01) -
Diagnostics of Flare Loop Parameters in Shrinkage and Ascent Stages Using Radio, X-ray, and UV Emission
by: Valery Zaitsev, et al.
Published: (2023-05-01) -
A Statistical Analysis of Magnetic Field Changes in the Photosphere during Solar Flares Using High-cadence Vector Magnetograms and Their Association with Flare Ribbons
by: Rahul Yadav, et al.
Published: (2023-01-01) -
Solar flares/
by: 243833 Svestka, Zdenek
Published: (1976)