The First Low-frequency Radio Observations of the Solar Corona on ≈200 km Long Interferometer Baseline
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8213/aaaf64/pdf
Reference56 articles.
1. Observations of 384 Radio Sources at a Frequency of 158 Mc/s with a Long Baseline Interferometer
2. Low-frequency solar radiophysics with LOFAR and FASR
3. Coronal Magnetic Energy Releases
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1. Polarization Observations of a Split-band Type II Radio Burst from the Solar Corona;The Astrophysical Journal;2022-11-01
2. Circular Polarization Observations of Type II Solar Radio Bursts and the Coronal Magnetic Field;The Astrophysical Journal;2022-06-01
3. Exploring the Circular Polarisation of Low–Frequency Solar Radio Bursts with LOFAR;Solar Physics;2022-04
4. Radio, X-Ray, and Extreme-ultraviolet Observations of Weak Energy Releases in the “Quiet” Sun;The Astrophysical Journal Letters;2021-08-31
5. New Results on the Direct Observations of Thermal Radio Emission from a Solar Coronal Mass Ejection;Geophysical Research Letters;2021-04-21
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