Using Flare-Induced Modulation of Three- and Five-Minute Oscillations for Studying Wave Propagation in the Solar Atmosphere
- 16 December 2021
- journal article
- research article
- Published by Springer Science and Business Media LLC in Solar Physics
- Vol. 296 (12), 1-8
- https://doi.org/10.1007/s11207-021-01910-5
Abstract
No abstract availableOther Versions
Funding Information
- Российский Фонд Фундаментальных Исследований (20-32-70076)
- Siberian Branch, Russian Academy of Sciences (II.16.3.2)
This publication has 36 references indexed in Scilit:
- Measuring the apparent phase speed of propagating EUV disturbancesAstronomy & Astrophysics, 2012
- ACCELERATING WAVES IN POLAR CORONAL HOLES AS SEEN BY EIS AND SUMERThe Astrophysical Journal, 2010
- WAVE PROPAGATION AND SHOCK FORMATION IN DIFFERENT MAGNETIC STRUCTURESThe Astrophysical Journal, 2009
- Impulsive Phase Flare Energy Transport by Large‐Scale Alfvén Waves and the Electron Acceleration ProblemThe Astrophysical Journal, 2008
- Channeling 5 Minute Photospheric Oscillations into the Solar Outer Atmosphere through Small-Scale Vertical Magnetic Flux TubesThe Astrophysical Journal, 2008
- Variations of microwave emission from solar active regionsAstronomy Letters, 2004
- Photoelectric observations of chromospheric sunspot oscillations. II - Propagation characteristicsThe Astrophysical Journal, 1984
- Motions in solar magnetic tubesSolar Physics, 1978
- Some properties of velocity fields in the solar photosphereSolar Physics, 1974
- Observational Study of Macroscopic Inhomogeneities in the Solar Atmosphere.VI. Photospheric Oscillations and Chromospheric Structure.The Astrophysical Journal, 1965