Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Daniel L. Clarkson"'
Autor:
Francesco Azzollini, A. Gordon Emslie, Daniel L. Clarkson, Nicolina Chrysaphi, Eduard P. Kontar
Publikováno v:
The Astrophysical Journal, Vol 968, Iss 2, p 72 (2024)
Radio signals propagating via the solar corona and solar wind are significantly affected by compressive waves, impacting the properties of solar bursts as well as sources viewed through the turbulent solar atmosphere. While static fluctuations scatte
Externí odkaz:
https://doaj.org/article/9100aca7096c44a2a3dcc75eefa8069d
Autor:
Eduard P. Kontar, A. Gordon Emslie, Daniel L. Clarkson, Xingyao Chen, Nicolina Chrysaphi, Francesco Azzollini, Natasha L. S. Jeffrey, Mykola Gordovskyy
Publikováno v:
The Astrophysical Journal, Vol 956, Iss 2, p 112 (2023)
Solar radio bursts are strongly affected by radio-wave scattering on density inhomogeneities, changing their observed time characteristics, sizes, and positions. The same turbulence causes angular broadening and scintillation of galactic and extragal
Externí odkaz:
https://doaj.org/article/a889556a2a57456fb956950067ea7522
Autor:
Daniel L. Clarkson, Eduard P. Kontar, Nicole Vilmer, Mykola Gordovskyy, Xingyao Chen, Nicolina Chrysaphi
Publikováno v:
The Astrophysical Journal, Vol 946, Iss 1, p 33 (2023)
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 i
Externí odkaz:
https://doaj.org/article/7a227a2fa3fa49d28ec405fb0f4d23ff
Decametric radio emission provides a unique insight into the physics of solar and heliospheric plasmas. Along with dynamic spectra, the spatial characteristics of the emission sources observed in solar radio bursts yield important information about t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b6b0c897d21c8968cfd4a96d7d3f2644
https://doi.org/10.5194/egusphere-egu21-15852
https://doi.org/10.5194/egusphere-egu21-15852
Autor:
Mykola Gordovskyy, Eduard P. Kontar, Daniel L. Clarkson, Nicolina Chrysaphi, Philippa K. Browning
Publikováno v:
The Astrophysical Journal. 925:140
Metric and decametric radio-emissions from the Sun are the only direct source of information about the dynamics of non-thermal electrons in the upper corona. In addition, the combination of spectral and imaging (sizes, shapes, and positions) observat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5ba1abfa2e22f3287d0ed617451c6ad6
https://doi.org/10.3847/1538-4357/ac3bb7
https://doi.org/10.3847/1538-4357/ac3bb7