2022-07-05 07:09
We present a short overview on the results from the first association analysis between in situ observed solar energetic electrons at 1 AU using the ACE/EPAM instrument (Samwel and Miteva, 20… Read More
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Solar Radio Astronomy Blog
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The Highlights of Solar Radio Physics (science nuggets) are short communications written in the language accessible to a non-expert in the specific area. The nugget is a brief description of a new and interesting scientific result, not as detailed as a scientific article, but rather written in a more discursive ‘news & views’ style.
2022-06-21 07:09
A solar radio burst (SRB) is the intense solar radio emission often related to a solar flare and one of the possibly extreme space weather events which may affect Earth’s ionosphere an… Read More
Subarcsecond Imaging Of A Solar Active Region filament With ALMA And IRIS By Da Silva Santos Et Al.*
2022-06-07 07:09
Filaments (or prominences) are “clouds” of cool (4 K) material suspended in the solar corona by up to tens of megameters above the photosphere, and they can be broadly divided in… Read More
2022-05-24 08:09
We investigate angular broadening of radio wave scattering by density irregularities in the outer heliosphere and the very local interstellar medium (VLISM), incorporating an inner scale, la… Read More
2022-05-03 07:09
Langmuir-Slow extraordinary mode (L-SE) waves have been routinely observed in the Solar wind and in Earth’s electron foreshock since the early age of the space exploration. They are in… Read More
2022-04-19 07:09
The plasma density and magnetic field in the upper solar corona and inner heliosphere are not sufficient to produce detectable bremsstrahlung hard X-ray or gyrosynchrotron microwave emission… Read More
2022-04-05 08:09
Solar radio bursts of Type III were currently observed since decades in the interplanetary space (Reid and Ratcliffe, 2014). They result from a series of successive processes arising in sola… Read More
2022-03-15 08:09
While it is widely accepted that the type II radio bursts observed in the interplanetary medium are due to the coronal mass ejections (CMEs), the energetic disturbance responsible for the sh… Read More
Spectral Analysis Of Solar Radio Type III Bursts From 20 KHz To 410 MHz By K. Sasikumar Raja Et Al.*
2022-03-01 08:09
Solar type III radio bursts are produced by electron beams that are propagating along open magnetic field lines in the corona and interplanetary medium (IPM). Type III bursts drift from high… Read More
Harvest Of Scientific Results By Solar Orbiter Radio And Plasma Waves Instrument By Milan Maksimovic
2022-02-15 08:09
For a mission that has just entered its primary science phase, Solar Orbiter has already produced many remarkable results. Released on December 14, 2021, a special issue of Astronomy and Ast… Read More
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