Zobrazeno 1 - 10
of 32
pro vyhledávání: '"Ineke De Moortel"'
Autor:
Thomas Howson, Ineke De Moortel
Publikováno v:
Physics, Vol 5, Iss 1, Pp 140-160 (2023)
Recent studies have identified the potential for coronal wave heating to balance radiative losses in a transversely oscillating low-density loop undergoing resonant absorption, phase mixing and the Kelvin–Helmholtz instability. This result relied o
Externí odkaz:
https://doaj.org/article/52da834a61334dd580b506eed9ddbdb1
Autor:
Ineke de Moortel, Jonathan Eastwood, John Bridges, Maerk Burchell, Yvonne Elseworth, Suzie Imber, Ashley King, Richard Morton
Publikováno v:
Astronomy & Geophysics. 64:3.34-3.38
A new Roadmap for Solar System Research in the UK has been published, and the Solar System Advisory Panel report on the processes involved in updating the previous iteration
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ab2f32dc496758ff076cc5a69416d36d
https://doi.org/10.1093/astrogeo/atad023
https://doi.org/10.1093/astrogeo/atad023
Funding: D.J.P. and T.V.D. were supported by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (grant agreement No. 724326) and the C1 grant TRACEspace of Internal Funds KU Leuven. The researc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2435bd4bbea819f9377916e077667417
https://hdl.handle.net/10023/25225
https://hdl.handle.net/10023/25225
Autor:
Nicholeen M. Viall, Fabio Reale, S. Parenti, Ineke De Moortel, James A. Klimchuk, Cooper Downs
Publikováno v:
Solar Physics and Solar Wind
The solar corona, the outer atmosphere of the Sun, is heated to millions of Kelvin. This is several orders of magnitude hotter than the photosphere, the optical surface of the Sun, below, and a mystery that has baffled scientists for centuries. The a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e76c03404f3659e3ad2d8b7527eefbb
http://hdl.handle.net/10447/522115
http://hdl.handle.net/10447/522115
Autor:
Leon Ofman, Mingzhe Guo, Abhishek K. Srivastava, Tom Van Doorsselaere, Soheil Vasheghani Farahani, Ineke De Moortel, D. J. Pascoe, Norbert Magyar, Dmitrii Y. Kolotkov, Hui Tian, Iñigo Arregui, Patrick Antolin
Publikováno v:
Space Science Reviews
The heating of the solar chromosphere and corona to the observed high temperatures, imply the presence of ongoing heating that balances the strong radiative and thermal conduction losses expected in the solar atmosphere. It has been theorized for dec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7260de57822f8b4f52b7067d5fa690b6
http://arxiv.org/abs/2012.01371
http://arxiv.org/abs/2012.01371
Publikováno v:
Astronomy & Astrophysics
Aims. We investigate the formation of small scales and the dissipation of MHD wave energy through non-linear interactions of counter-propagating, phase-mixed Alfvenic waves in a complex magnetic field. Methods. We conducted fully 3-D, non-ideal MHD s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0773f8ffdeef055cc3d7843c0760d35d
http://arxiv.org/abs/2003.05226
http://arxiv.org/abs/2003.05226
Publikováno v:
Astronomy & Geophysics
Publons
Publons
Ineke De Moortel, Isobel Falconer and Robert Stack explore the achievements and influence of Hannes Alfvén, in particular his seminal Monthly Notices paper of 1947 on the heating of the solar corona.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dba06cd323d186ef33ea166558436ea4
Publikováno v:
Astronomy & Astrophysics. 656:A112
Context. The magnetic Kelvin-Helmholtz instability (KHI) has been proposed as a means of generating magnetohy- drodynamic turbulence and encouraging wave energy dissipation in the solar corona, particularly within transversely oscillating loops. Aims
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1fb7b29625d28b81abe299165982005e
https://doi.org/10.1051/0004-6361/202141620
https://doi.org/10.1051/0004-6361/202141620
Autor:
Tom Van Doorsselaere, Ineke De Moortel, Mingzhe Guo, Bo Li, Patrick Antolin, Konstantinos Karampelas
Publikováno v:
The Astrophysical Journal
Funding: This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No.724326 and No.647214) (IDM). P.A. acknowledges funding from his STFC E
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c4b3732a6f1cd4d24c2bc9976f54f44e
The role of type II spicules in the corona has been a much debated topic in recent years. This paper aims to shed light on the impact of type II spicules in the corona using novel 2.5D radiative MHD simulations including ion-neutral interaction effec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::daa2a7a5e4f8b540444dd52f62fde6f1