Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Julia M. Riedl"'
Autor:
Gabriel Pelouze, Tom Van Doorsselaere, Konstantinos Karampelas, Julia M. Riedl, Timothy Duckenfield
Context. Transverse oscillations are ubiquitously observed in the solar corona, both in coronal loops and open magnetic flux tubes. Numerical simulations suggest that their dissipation could heat coronal loops, counterbalancing radiative losses. Thes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da2258483472b88e5a19275629921926
http://arxiv.org/abs/2301.03100
http://arxiv.org/abs/2301.03100
Autor:
S. D. T. Grant, Caitlin A. Gilchrist-Millar, Julia M. Riedl, T. Van Doorsselaere, David B. Jess
Publikováno v:
Riedl, J M, Gilchrist-Millar, C A, Van Doorsselaere, T, Jess, D B & Grant, S D T 2021, ' Finding the mechanism of wave energy flux damping in solar pores using numerical simulations ', Astronomy & Astrophysics, vol. 648, A77 . https://doi.org/10.1051/0004-6361/202040163
Context. Solar magnetic pores are, due to their concentrated magnetic fields, suitable guides for magnetoacoustic waves. Recent observations have shown that propagating energy flux in pores is subject to strong damping with height; however, the reaso
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68adb1e69522dc75d52404ffa8990d65
https://pure.qub.ac.uk/en/publications/finding-the-mechanism-of-wave-energy-flux-damping-in-solar-pores-using-numerical-simulations(8fa0709f-66ff-4658-9906-9b18ccd49c05).html
https://pure.qub.ac.uk/en/publications/finding-the-mechanism-of-wave-energy-flux-damping-in-solar-pores-using-numerical-simulations(8fa0709f-66ff-4658-9906-9b18ccd49c05).html
Autor:
Caitlin A. Gilchrist-Millar, Julia M. Riedl, David B. Jess, S. D. T. Grant, Shahin Jafarzadeh, Christian Beck, Peter H. Keys, Tom Van Doorsselaere, Basilio Ruiz Cobo
Publikováno v:
Philos Trans A Math Phys Eng Sci
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
Gilchrist-Millar, C, Jess, D B, Grant, S D T, Keys, P H, Beck, C, Jafarzadeh, S, Riedl, J M, Van Doorsselaere, T & Ruiz Cobo, B 2020, ' Magnetoacoustic Wave Energy Dissipation in the Atmosphere of Solar Pores ', Philosophical Transactions of the Royal Society of London A: Mathematical, Physical and Engineering Sciences, vol. 379, no. 2190 . https://doi.org/10.1098/rsta.2020.0172
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
Gilchrist-Millar, C, Jess, D B, Grant, S D T, Keys, P H, Beck, C, Jafarzadeh, S, Riedl, J M, Van Doorsselaere, T & Ruiz Cobo, B 2020, ' Magnetoacoustic Wave Energy Dissipation in the Atmosphere of Solar Pores ', Philosophical Transactions of the Royal Society of London A: Mathematical, Physical and Engineering Sciences, vol. 379, no. 2190 . https://doi.org/10.1098/rsta.2020.0172
The suitability of solar pores as magnetic wave guides has been a key topic of discussion in recent years. Here we present observational evidence of propagating magnetohydrodynamic wave activity in a group of five photospheric solar pores. Employing
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::70ce8ccbdd6ba6caa4092ee87044c52f
https://pubmed.ncbi.nlm.nih.gov/33342383
https://pubmed.ncbi.nlm.nih.gov/33342383
Publikováno v:
Astronomy & Astrophysics
Context. Waves are ubiquitous in the solar corona and there are indications that they are excited by photospheric p-modes. However, it is unclear how p-modes in coronal loops are converted to sausage modes and transverse (kink) modes, which are obser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e1ae42276b993f8495a372487a46de93
https://lirias.kuleuven.be/handle/123456789/637197
https://lirias.kuleuven.be/handle/123456789/637197
Autor:
Paolo Pagano, Julia M. Riedl, A. Petralia, Marcel Goossens, Fabio Reale, Tom Van Doorsselaere
Publikováno v:
The Astrophysical Journal. 922(2):225
Acoustic waves excited in the photosphere and below might play an integral part in the heating of the solar chromosphere and corona. However, it is yet not fully clear how much of the initially acoustic wave flux reaches the corona and in what form.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5dd5eb6111a3a5345cacb7ef6987e0fa