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A correlation Study of Coronal EUV Brightenings and Radio Emission Observed by Parker Solar Probe

2019
The dynamic nature of our host star is clearly observable in the solar corona. Different structures are visible in it (coronal loops, streamers, coronal holes), which have a direct relationship with changes that the Sun is experiencing in its interior and photosphere.
Martinez Oliveros, J. C.   +10 more
openaire   +1 more source

Auroral emissions and inner magnetospheric dynamics during Earth's response to the 28th October 2021 Coronal Mass Ejection, Planetary, Solar and Heliospheric Radio Emissions IX

2023
Waters, J.   +14 more
openaire   +1 more source

Erratum: Study of solar brightness profiles in the 18-26 GHz frequency range with INAF radio telescopes: II. Evidence of coronal emission (Astronomy and Astrophysics (2024) 684 (A123) DOI: 10.1051/0004-6361/202348770)

An error occurred during the production process. Some units have been mistakenly changed in the text: each “mm” (millimeter) unit should read “Mm” (megameter).
M. Marongiu   +44 more
openaire   +1 more source

Metric Type II Solar Radio Emission associated with Coronal Mass Ejections: Some New Insights

Proceedings of the 6th URSI Regional Conference on Radio Science – RCRS 2024
Susanta Kumar Bisoi   +2 more
openaire   +1 more source

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