Zobrazeno 1 - 10
of 17
pro vyhledávání: '"David I. Pontin"'
Autor:
Valentin Aslanyan, Roger B. Scott, Chloe P. Wilkins, Karen A. Meyer, David I. Pontin, Anthony R. Yeates
Publikováno v:
The Astrophysical Journal, Vol 971, Iss 2, p 137 (2024)
We present a new code for the tracing of magnetic field lines and calculation of related quantities such as the squashing factor in the solar corona. The Universal Fieldline Tracer ( UFiT ) is an open-source package that can currently take inputs dir
Externí odkaz:
https://doaj.org/article/f776db2a5372472498ab33ebf940028e
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 2, p 80 (2024)
In this paper, we introduce a new method for exact decomposition of propagating, nonlinear magnetohydrodynamic (MHD) disturbances into their component eigenenergies associated with the familiar slow, Alfvén, and fast wave eigenmodes, and the entropy
Externí odkaz:
https://doaj.org/article/4531fc0e9ab2430fb054512c287f3c3d
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 2, p 139 (2024)
In the present paper, using MPI-AMRVAC , we perform a 2.5D numerical magnetohydrodynamic simulation of the dynamics and associated thermodynamical evolution of an initially force-free Harris current sheet subjected to an external velocity perturbatio
Externí odkaz:
https://doaj.org/article/553369416eb94409b0814ac7b36231eb
Autor:
Hardi Peter, Lakshmi Pradeep Chitta, Feng Chen, David I. Pontin, Amy R. Winebarger, Leon Golub, Sabrina L. Savage, Laurel A. Rachmeler, Ken Kobayashi, David H. Brooks, Jonathan W. Cirtain, Bart De Pontieu, David E. McKenzie, Richard J. Morton, Paola Testa, Sanjiv K. Tiwari, Robert W. Walsh, Harry P. Warren
The outer atmosphere of the Sun is composed of plasma heated to temperatures well in excess of the visible surface. We investigate short cool and warm (
Accepted for publication in the Astrophysical Journal, 24 pages, 18 figures
Accepted for publication in the Astrophysical Journal, 24 pages, 18 figures
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e5e542037fe0439fb65797caee7fe811
http://hdl.handle.net/10852/97372
http://hdl.handle.net/10852/97372
Publikováno v:
Physics of Plasmas. 30:022901
Three-dimensional (3D) magnetic nulls are preferential sites for triggering solar coronal transients. Although these nulls are abundant in the solar atmosphere, their generation is yet to be thoroughly explored. This paper explores the mechanism of n
Publikováno v:
The astrophysical journal, 2021, Vol.923(2), pp.163 [Peer Reviewed Journal]
Magnetic reconnection is widely accepted to be a major contributor to nonthermal particle acceleration in the solar atmosphere. In this paper we investigate particle acceleration during the impulsive phase of a coronal jet, which involves bursty reco
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::213bcb979ac43b45fc41d21afa372447
https://doi.org/10.3847/1538-4357/ac2e6d
https://doi.org/10.3847/1538-4357/ac2e6d
Publikováno v:
Astrophysical Journal; 9/10/2019, Vol. 882 Issue 2, p1-1, 1p
Publikováno v:
Astrophysical Journal; 12/10/2018, Vol. 869 Issue 1, p1-1, 1p
Publikováno v:
Astrophysical Journal; 3/1/2018, Vol. 855 Issue 1, p1-1, 1p
Publikováno v:
Astrophysical Journal; 10/20/2017, Vol. 848 Issue 2, p1-1, 1p