Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Eoin Carley"'
Autor:
Jinge Zhang, Hamish A. S. Reid, Eoin Carley, Laurent Lamy, Pietro Zucca, Peijin Zhang, Baptiste Cecconi
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 2, p 107 (2024)
Solar radio U-bursts are generated by electron beams traveling along closed magnetic loops in the solar corona. Low-frequency (
Externí odkaz:
https://doaj.org/article/a57a920cc9a54ea79de9db805a9c4501
Publikováno v:
Computer Science, Vol 15, Iss 3, p 271 (2014)
The Sun is responsible for the eruption of billions of tons of plasma andthe generation of near light-speed particles that propagate throughout the solarsystem and beyond. If directed towards Earth, these events can be damaging toour tecnological inf
Externí odkaz:
https://doaj.org/article/182f734cac66429b9f75cd517f8f7346
Publikováno v:
Solar Physics. 298
Solar flares are one of the most extreme space weather events in our solar system. The impulsive solar radio emission associated with a solar flare is known as a solar radio burst (SRB). They are generally studied in dynamic spectra and are classifie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f9dd8aab7972fe53614a873e4015fb6
https://doi.org/10.1007/s11207-022-02099-x
https://doi.org/10.1007/s11207-022-02099-x
NenuFAR is the tied-array radio instrument recently deployed in France. It is the low-frequency extension of LOFAR. It covers frequencies between 10 and 85 MHz. Its large collecting surface (53000m2 at 25MHz) makes it very sensitive. Spectral and tem
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2b198ac79b0dfe7c237d88ddd942cdeb
https://doi.org/10.5194/egusphere-egu22-2920
https://doi.org/10.5194/egusphere-egu22-2920
Autor:
Samuel T. Badman, Eoin Carley, Luis Alberto Cañizares, Nina Dresing, Lan K. Jian, David Lario, Peter T. Gallagher, Juan C. Martínez Oliveros, Marc Pulupa, Stuart D. Bale
Type III radio bursts are the result of plasma emission from mildly relativistic electron beams propagating from the low solar corona into the heliosphere where they can eventually be detected in situ if they align with the location of a heliospheric
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::58006d12cfe372ff915cca9550fd3c60
Autor:
PeiJin Zhang, Pietro Zucca, Kamen Kozarev, Eoin Carley, ChuanBing Wang, Thomas Franzen, Bartosz Dabrowski, Andrzej Krankowski, Jasmina Magdalenic, Christian Vocks
Publikováno v:
The Astrophysical Journal. 932:17
Radio emission of the quiet Sun is considered to be due to thermal bremsstrahlung emission of the hot solar atmosphere. The properties of the quiet Sun in the microwave band have been well studied, and they can be well described by the spectrum of br
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::050daa08ce6c15865aebe1d08486cbf2
https://doi.org/10.3847/1538-4357/ac6b37
https://doi.org/10.3847/1538-4357/ac6b37
Autor:
Eoin Carley
Solar flares are often associated with high-intensity radio emission known as `solar radio bursts' (SRBs). SRBs are generally observed in dynamic spectra and have five major spectral classes, labelled type I to type V depending on their shape and ext
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::57234b364551beab542c5891d2d3b396
https://doi.org/10.5194/egusphere-egu2020-5109
https://doi.org/10.5194/egusphere-egu2020-5109
The Sun regularly produces large-scale eruptive events, such as coronal mass ejections (CMEs) that can drive shock waves through the solar corona. Such shocks can result in electron acceleration and subsequent radio emission in the form of a type II
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::225bb24794dcdd2fad8c63c59e0a97aa
https://doi.org/10.5194/egusphere-egu2020-11425
https://doi.org/10.5194/egusphere-egu2020-11425