Zobrazeno 1 - 10
of 384
pro vyhledávání: '"Riedl, A. M."'
Autor:
Pelouze, Gabriel, Van Doorsselaere, Tom, Karampelas, Konstantinos, Riedl, Julia M., Duckenfield, Timothy
Publikováno v:
A&A 672, A105 (2023)
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:
http://arxiv.org/abs/2301.03100
Autor:
Sieyra, M. V., Prasad, S. Krishna, Stenborg, G., Khomenko, E., Van Doorsselaere, T., Costa, A., Esquivel, A., Riedl, J. M.
Publikováno v:
A&A 667, A21 (2022)
Recurrent, arc-shaped intensity disturbances were detected by EUV channels in an active region. The fronts were observed to propagate along a coronal loop bundle rooted in a small area within a sunspot umbra. Previous works have linked these intensit
Externí odkaz:
http://arxiv.org/abs/2208.10857
Autor:
Riedl, Julia M., Van Doorsselaere, Tom, Reale, Fabio, Goossens, Marcel, Petralia, Antonino, Pagano, Paolo
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:
http://arxiv.org/abs/2109.02971
Autor:
Riedl, Julia M., Gilchrist-Millar, Caitlin A., Van Doorsselaere, Tom, Jess, David B., Grant, Samuel D. T.
Publikováno v:
A&A 648, A77 (2021)
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:
http://arxiv.org/abs/2102.12420
Autor:
Gilchrist-Millar, Caitlin A., Jess, David B., Grant, Samuel D. T., Keys, Peter H., Beck, Christian, Jafarzadeh, Shahin, Riedl, Julia M., Van Doorsselaere, Tom, Cobo, Basilio Ruiz
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:
http://arxiv.org/abs/2007.11594
Publikováno v:
A&A 625, A144 (2019)
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:
http://arxiv.org/abs/1905.01865
Akademický článek
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Akademický článek
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Autor:
Maisel, Franziska 1, Smolle, Maria A. 2, 3, Mollnar, Stefanie 1, Riedl, Jakob M. 1, Barth, Dominik A. 1, Seles, Maximilian 4, Terbuch, Angelika 1, Rossmann, Christopher H. 1, Eisner, Florian 1, Mannweiler, Sebastian 5, Hutterer, Georg 4, Zigeuner, Richard 4, Pummer, Karl 4, Smolle-Jüttner, Freyja-Maria 6, Lindenmann, Jörg 6, Stotz, Michael 1, Gerger, Armin 1, 3, Jost, Philipp J. 1, 7, Bauernhofer, Thomas 1, Pichler, Martin 1, 8, Posch, Florian 9, ⁎
Publikováno v:
In Clinical Genitourinary Cancer August 2022 20(4):344-353
Autor:
Riedl, Jakob M. a, Posch, Florian a, Horvath, Lena b, Gantschnigg, Antonia c, Renneberg, Felix d, Schwarzenbacher, Esther a, Moik, Florian e, Barth, Dominik A. a, Rossmann, Christopher H. a, Stotz, Michael a, Schaberl-Moser, Renate a, Pichler, Martin a, Stöger, Herbert a, Greil, Richard d, Djanani, Angela f, Schlick, Konstantin d, Gerger, Armin g, ∗
Publikováno v:
In European Journal of Cancer July 2021 151:3-13