THE ORIGIN OF TYPE I SPICULE OSCILLATIONS-Reference-Cited by-同舟云学术

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THE ORIGIN OF TYPE I SPICULE OSCILLATIONS

Published:2011-12-08 Issue:1 Volume:744 Page:L5
ISSN:2041-8205
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Jess D. B.,Pascoe D. J.,Christian D. J.,Mathioudakis M.,Keys P. H.,Keenan F. P.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference35 articles.

1. A Staggered Grid, Lagrangian–Eulerian Remap Code for 3-D MHD Simulations

2. TRACE observations of driven loop oscillations

3. Signatures of Alfvén waves in the polar coronal holes as seen by EIS/Hinode

4. The damping of slow MHD waves in solar coronal magnetic fields

5. Chromospheric Alfvénic Waves Strong Enough to Power the Solar Wind

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1. Sausage, kink, and fluting magnetohydrodynamic wave modes identified in solar magnetic pores by Solar Orbiter/PHI;Astronomy & Astrophysics;2024-07-30

2. Large-amplitude transverse MHD waves prevailing in the Hα chromosphere of a solar quiet region revealed by MiHI integrated field spectral observations;Astronomy & Astrophysics;2024-07

3. Unveiling the True Nature of Plasma Dynamics from the Reference Frame of a Superpenumbral Fibril;The Astrophysical Journal;2024-07-01

4. Can the Solar p-modes Contribute to the High-frequency Transverse Oscillations of Spicules?;The Astrophysical Journal;2024-01-01

5. Spectroscopic Detection of Alfvénic Waves in the Chromospheric Fibrils of a Solar-quiet Region;The Astrophysical Journal;2023-11-20

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