Study of Waveguides and Resonant Cavities over Sunspot Volumes Using Multichannel Solar Dynamics Observatory Observations
For the first time, we have determined the spatial distribution of magnetic waveguides and resonant cavities at different heights of sunspot atmosphere. We analyzed the time series of EUV/UV images observed by the Solar Dynamics Observatory in the different temperature channels. We have decomposed t...
Saved in:
| Main Authors: | Robert Sych, Yihua Yan |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adda48 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Nonlinearity of 3 minute Slow Magnetoacoustic Waves in the Sunspot Umbral Atmosphere
by: Y. Sanjay, et al.
Published: (2025-01-01) -
Bright Dots and Coronal Plume Formation in Sunspot Penumbra
by: Ayla Weitz, et al.
Published: (2025-01-01) -
Hemispheric Asymmetry of Relative Sunspot Numbers during Solar Cycles 17–25
by: Wenhua Wang, et al.
Published: (2025-01-01) -
Statistical Comparison between Pores and Sunspots during the Time Interval 2010–2023
by: Yang Peng, et al.
Published: (2024-01-01) -
Superstrong Magnetic Fields in Sunspot Bipolar Light Bridges
by: J. S. Castellanos Durán, et al.
Published: (2025-01-01)