solar radio nuggets in September 2021

Eduard Kontar eduard.kontar at glasgow.ac.uk
Wed Oct 6 14:50:53 MDT 2021


Properties of High-Frequency Type II Radio Bursts and Their Relation to the Associated Coronal Mass Ejections
by A.C. Umuhire et al.*
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3067  <https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3067>

The active region source of a type III radio storm observed by Parker Solar Probe during encounter 2
by L. Harra et al*
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3058  <https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3058>

Langmuir wave motion observed in the most intense radio sources in the sky
by H. Reid and E. Kontar
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3028  <https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3028>


  --
CESRA Highlights of Solar Radio Physics, aka CESRA Nuggets,
are short communications written in language accessible to a non-expert
in the specific area and designed to keep solar and heliophysics communities informed and
up-to-date about current research. The highlights can be followed, discussed, commented
and shared viahttp://www.facebook.com/solarcesra/  <http://www.facebook.com/solarcesra/>  
andhttp://twitter.com/CESRA_community  <http://twitter.com/CESRA_community>  

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