Zobrazeno 1 - 10
of 80
pro vyhledávání: '"Carley Eoin P."'
Autor:
Zhang, Jinge, Reid, Hamish A. S., Carley, Eoin, Lamy, Laurent, Zucca, Pietro, Zhang, Peijin, Cecconi, Baptiste
Solar radio U-bursts are generated by electron beams traveling along closed magnetic loops in the solar corona. Low-frequency ($<$ 100 MHz) U-bursts serve as powerful diagnostic tools for studying large-sized coronal loops that extend into the middle
Externí odkaz:
http://arxiv.org/abs/2402.04822
Autor:
Carley Eoin P., Baldovin Carla, Benthem Pieter, Bisi Mario M., Fallows Richard A., Gallagher Peter T., Olberg Michael, Rothkaehl Hanna, Vermeulen Rene, Vilmer Nicole, Barnes David
Publikováno v:
Journal of Space Weather and Space Climate, Vol 10, p 7 (2020)
The low frequency array (LOFAR) is a phased array interferometer currently consisting of 13 international stations across Europe and 38 stations surrounding a central hub in the Netherlands. The instrument operates in the frequency range of ~10–240
Externí odkaz:
https://doaj.org/article/ce7a397249764b76af421f3451a36982
Publikováno v:
A&A 674, A218 (2023)
Solar flares are energetic events in the solar atmosphere that are often linked with solar radio bursts (SRBs). SRBs are observed at metric to decametric wavelengths and are classified into five spectral classes (Type I--V) based on their signature i
Externí odkaz:
http://arxiv.org/abs/2305.09327
Publikováno v:
A&A 670, A169 (2023)
Type II solar radio bursts are caused by magnetohydrodynamics (MHD) shocks driven by solar eruptive events such as Coronal Mass Ejections (CMEs). Often both fundamental and harmonic bands of type II bursts are split into sub-bands, generally believed
Externí odkaz:
http://arxiv.org/abs/2212.07698
Autor:
Dabrowski, Bartosz, Mikula, Katarzyna, Flisek, Pawel, Vocks, Christian, Zhang, PeiJin, Magdalenić, Jasmina, Warmuth, Alexander, Morosan, Diana E., Froń, Adam, Fallows, Richard A., Bisi, Mario M., Krankowski, Andrzej, Mann, Gottfried, Blaszkiewicz, Leszek, Carley, Eoin P., Gallagher, Peter T., Zucca, Pietro, Rudawy, Pawel, Hajduk, Marcin, Kotulak, Kacper, Sidorowicz, Tomasz
Publikováno v:
A&A 669, A52 (2023)
The Sun is the source of different types of radio bursts that are associated with solar flares, for example. Among the most frequently observed phenomena are type III solar bursts. Their radio images at low frequencies (below 100 MHz) are relatively
Externí odkaz:
http://arxiv.org/abs/2211.12756
Autor:
Rigney, Jeremy, Ramsay, Gavin, Carley, Eoin P., Doyle, J. Gerry, Gallagher, Peter T., Wang, Yuanming, Pritchard, Joshua, Murphy, Tara, Lenc, Emil, Kaplan, David L.
Solar radio emission at low frequencies (<1 GHz) can provide valuable information on processes driving flares and coronal mass ejections (CMEs). Radio emission has been detected from active M dwarf stars, suggestive of much higher levels of activity
Externí odkaz:
http://arxiv.org/abs/2207.00405
Autor:
Zhang, PeiJin, Zucca, Pietro, Kozarev, Kamen, Carley, Eoin, Wang, ChuanBing, Franzen, Thomas, Dabrowski, Bartosz, Krankowski, Andrzej, Magdalenic, Jasmina, Vocks, Christian
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:
http://arxiv.org/abs/2205.00065
Autor:
Badman, Samuel T., Carley, Eoin P., Cañizares, Luis Alberto, Dresing, Nina, Jian, Lan K., Lario, David, Gallagher, Peter T., Martínez-Oliveros, Juan C., Pulupa, Marc, Bale, Stuart D.
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:
http://arxiv.org/abs/2204.08497
Autor:
Louis, Corentin K., Jackman, Caitriona M., Griessmeier, Jean-Mathias, Wucknitz, Olaf, McKenna, David J., Murphy, Pearse, Gallagher, Peter T., Carley, Eoin, Fionnagáin, Dúalta Ó, Golden, Aaron, McCauley, Joe, Callanan, Paul, Redman, Matt, Vocks, Christian
Publikováno v:
RASTAI 1, 48-57 (2022)
The Low Frequency Array (LOFAR) is an international radio telescope array, consisting of 38 stations in the Netherlands and 14 international stations spread over Europe. Here we present an observation method to study the jovian decametric radio emiss
Externí odkaz:
http://arxiv.org/abs/2111.09599
Autor:
Carley, Eoin P., Cecconi, Baptiste, Reid, Hamish A., Briand, Carine, Raja, Sasikumar, Masson, Sophie, Dorovskyy, Vladimir V., Tiburzi, Caterina, Vilmer, Nicole, Zucca, Pietro, Zarka, Philippe, Tagger, Michel, Griessmeier, Jean-Mathias, Corbel, Stéphane, Theureau, Gilles, Loh, Alan, Girard, Julien
Eruptive activity in the solar corona can often lead to the propagation of shock waves. In the radio domain the primary signature of such shocks are type II radio bursts, observed in dynamic spectra as bands of emission slowly drifting towards lower
Externí odkaz:
http://arxiv.org/abs/2108.05587