Results 31 to 40 of about 2,630,706 (301)
The Solar Wind in Time II: 3D stellar wind structure and radio emission [PDF]
International audienceIn this work, we simulate the evolution of the solar wind along its main-sequence lifetime andcompute its thermal radio emission. To study the evolution of the solar wind, we use a sample ofsolar mass stars at different ages.
Morin, J. +23 more
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On solar protons and polar cap absorption: Constraints on an empirical relationship [PDF]
International audienceA large database of Solar Proton Events (SPE) from the period 1995 to 2001 is used to investigate the relationship between proton flux at geostationary orbit and Cosmic Noise Absorption (CNA) in the auroral zone. The effect of solar
A. Senior +9 more
core +2 more sources
Observations of Solar Type III radio bursts by Cassini/RPWS experiment [PDF]
In this study, we report on the occurrence of solar Type III radio bursts recorded by radio and plasma wave experiment (RPWS) experiment onboard Cassini spacecraft.
M. Y. Boudjada +4 more
doaj +1 more source
On the character and distribution of lower-frequency radio emissions at Saturn and their relationship to substorm-like events [PDF]
With the arrival of the Cassini spacecraft at Saturn in July 2004, there have been quasi-continuous observations of Saturn kilometric radiation (SKR) emissions.
L. Lamy +24 more
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The quiet Sun, i.e., in its nonflaring state or nonflaring regions, emits thermal radiation from radio to ultraviolet. The quiet Sun also produces nonthermal radiation observed in gamma rays due to interactions of Galactic cosmic rays (GCRs) with the ...
Elena Orlando +2 more
doaj +1 more source
Many particles are accelerated during solar flares. To understand the acceleration and propagation processes of electrons, we require the pitch-angle distributions of the particles.
Keitarou Matsumoto +2 more
doaj +1 more source
Complex Type II Solar Radio Event on 4 July 2022
Publisher Copyright: © 2022 J. Kallunki et al., published by Sciendo.On 4 July 2022, a complex low-frequency solar radio burst was observed in Metsähovi Radio Observatory of Aalto University.
Kallunki, J.
core +1 more source
Ichon Solar Radio Spectrogaphic System and Development of its Operation Software [PDF]
A solar radio spectrograph for monitoring solar radio emission was installed at Ichon branch of Radio Research Laboratory in 1995. The spectrograph consists of three different antennas to sweep a wide band of frequencies in the range of 30MHz-2500MHz. We
K. S. Cho, G. H. Lee, K.-S. Kim
doaj
Understanding electron acceleration associated with magnetic energy release at subsecond scales presents major challenges in solar physics. Solar radio spikes observed as subsecond, narrow-bandwidth bursts with Δ f / f ∼ 10 ^−3 –10 ^−2 are indicative of ...
Daniel L. Clarkson +5 more
doaj +1 more source
Structure of the Solar Atmosphere: A Radio Perspective
Solar radio emission has been providing information about the Sun for over half a century. In order to fully exploit this information, one needs to have a broader view of the solar atmosphere, which cannot be provided by radio observations alone.
Costas E. Alissandrakis
doaj +1 more source

