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Solar radio emission and diagnostics of Solar coronal plasma

2008
Sunčeva atmosfera, protkana izranjajućim magnetskim poljima, dinamičan je plazmeni sustav u kojem dolazi od brojnih eruptivnih procesa. Najveće provale energije su Sunčevi bljeskovi i koronini izbačaji tijekom kojih se magnetska energija pretvara u toplinsku, dolazi do ubrzavanja snopova visokoenergetskih čestica, i stvaranja udarnih valova. Intenzitet
openaire  

Moving Solar Radio Bursts and Their Association With Coronal Mass Ejections

Astronomy and Astrophysics, 2021
Anshu Kumari   +2 more
exaly  

A Type II Solar Radio Burst Without a Coronal Mass Ejection

Astronomy and Astrophysics, 2023
Anshu Kumari, Rami Vainio, Emilia Kilpua
exaly  

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

Solar Flares and Coronal Mass Ejections

Annual Review of Astronomy and Astrophysics, 1992
Stephen W Kähler
exaly  

Spectral Characteristics of Large-Scale Radio Emission Areas in Coronal Holes

Geomagnetism and Aeronomy, 2013
I Yu Grigor'Eva, A A Kochanov
exaly  

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