The Relation between Solar Spicules and Magnetohydrodynamic Shocks
Spicules are thin, elongated, jet-like features seen in observations of the solar atmosphere, at the interface between the solar photosphere and the corona. These features exhibit highly complex dynamics and are a necessary connecting link between the cooler, denser solar chromosphere and the extrem...
Saved in:
| Main Authors: | Sankalp Srivastava, Piyali Chatterjee, Sahel Dey, Robertus Erdélyi |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ade9b4 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
3D Magnetohydrodynamic Wave Propagation and Energy Transport in a Simulated Solar Vortex
by: Samuel J. Skirvin, et al.
Published: (2025-01-01) -
Dissipation of Magnetohydrodynamic Waves in the Solar Stratified Flux Tubes
by: Zahra Fazel
Published: (2023-12-01) -
ALMA Observations of Solar Spicules in a Polar Coronal Hole
by: T. S. Bastian, et al.
Published: (2025-01-01) -
Temporal Evolution of a Network Jet’s Physical Properties Inferred from FISS/GST and IRIS Observations
by: Eun-Kyung Lim, et al.
Published: (2025-01-01) -
Propagating Bright Knots in the Chromospheric Fibrils
by: Shaoxuan Tong, et al.
Published: (2025-01-01)