Zobrazeno 1 - 10
of 137
pro vyhledávání: '"A G, Emslie"'
Autor:
E. P. Kontar, S. Yu, A. A. Kuznetsov, A. G. Emslie, B. Alcock, N. L. S. Jeffrey, V. N. Melnik, N. H. Bian, P. Subramanian
Publikováno v:
Nature Communications, Vol 8, Iss 1, Pp 1-9 (2017)
Radio observations of the solar atmosphere provide a unique view on the non-thermal processes in the outer atmosphere. Here the authors use LOFAR observations to demonstrate that the observed radio burst characteristics are dominated by propagation e
Externí odkaz:
https://doaj.org/article/897c741ce92044c28801e3193f1ee1d2
Autor:
E. P. Kontar, S. Yu, A. A. Kuznetsov, A. G. Emslie, B. Alcock, N. L. S. Jeffrey, V. N. Melnik, N. H. Bian, P. Subramanian
Publikováno v:
Nature Communications, Vol 9, Iss 1, Pp 1-1 (2018)
The original version of this article contained errors in Refs 15, 27, 32, 33 and 43, which were incorrectly given with the wrong journal name “Solid Phys.” rather than the correct “Sol. Phys.”. This has now been corrected in the PDF and HTML
Externí odkaz:
https://doaj.org/article/2032030996fb4d918cba4bb1b1e7e040
Autor:
Harlan E. Spence, Lennard A. Fisk, Alexa Halford, Paul Cassak, Susan K. Avery, Daniel N. Baker, A. G. Emslie
Publikováno v:
Journal of Geophysical Research: Space Physics. 122:4430-4435
Space physics is the study of Earth's home in space. Elements of space physics include how the Sun works from its interior to its atmosphere, the environment between the Sun and planets out to the interstellar medium, and the physics of the magnetic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f5a2a440059920aa60129bc70e4b7e4c
https://doi.org/10.1002/2017ja024219
https://doi.org/10.1002/2017ja024219
Electromagnetic wave scattering off density inhomogeneities in the solar corona is an important process which determines both the apparent source size and the time profile of radio bursts observed at 1 AU. Here we model the scattering process using a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb3301e05555082812480a030a6a995b
http://arxiv.org/abs/1902.00239
http://arxiv.org/abs/1902.00239
Autor:
Nicolas Bian, Prasad Subramanian, Sijie Yu, B. Alcock, A. G. Emslie, Eduard P. Kontar, Valentin Melnik, Natasha L. S. Jeffrey, Alexey A. Kuznetsov
Publikováno v:
Nature Communications
Nature Communications, Vol 9, Iss 1, Pp 1-1 (2018)
Nature Communications, Vol 9, Iss 1, Pp 1-1 (2018)
Solar radio observations provide a unique diagnostic of the outer solar atmosphere. However, the inhomogeneous turbulent corona strongly affects the propagation of the emitted radio waves, so decoupling the intrinsic properties of the emitting source
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::043d4824717af803abcc4d071d0d8197
http://europepmc.org/articles/PMC5765264
http://europepmc.org/articles/PMC5765264
Autor:
E P, Kontar, J E, Perez, L K, Harra, A A, Kuznetsov, A G, Emslie, N L S, Jeffrey, N H, Bian, B R, Dennis
Publikováno v:
Physical review letters. 118(15)
The energy released in solar flares derives from a reconfiguration of magnetic fields to a lower energy state, and is manifested in several forms, including bulk kinetic energy of the coronal mass ejection, acceleration of electrons and ions, and enh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::df6eaa47df7ccb4f494619963518f236
https://pubmed.ncbi.nlm.nih.gov/28452537
https://pubmed.ncbi.nlm.nih.gov/28452537
Autor:
Valentina Zharkova, K. Arzner, Arnold O. Benz, Eduard P. Kontar, Loukas Vlahos, Nicole Vilmer, Vahé Petrosian, G. Mann, Lyndsay Fletcher, Marco Onofri, C. Dauphin, A. G. Emslie, Philippa Browning, R. Turkmani
Publikováno v:
Space Science Reviews
Space Science Reviews, 2011, 159, pp.357-420. ⟨10.1007/s11214-011-9803-y⟩
Space Science Reviews, 2011, 159, pp.357-420. ⟨10.1007/s11214-011-9803-y⟩
We review basic theoretical concepts in particle acceleration, with particular emphasis on processes likely to occur in regions of magnetic reconnection. Several new developments are discussed, including detailed studies of reconnection in three-dime
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c70f5c368a349b48a9fa84994d3b9fb
https://doi.org/10.1007/s11214-011-9803-y
https://doi.org/10.1007/s11214-011-9803-y
Extending previous studies of nonthermal electron transport in solar flares which include the effects of collisional energy diffusion and thermalization of fast electrons, we present an analytic method to infer more accurate estimates of the accelera
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a0bba9a8b1ddae81462a45d9b204841a
https://nrl.northumbria.ac.uk/id/eprint/40606/1/Kontar_2015_ApJ_809_35.pdf
https://nrl.northumbria.ac.uk/id/eprint/40606/1/Kontar_2015_ApJ_809_35.pdf
Publikováno v:
Advances in Space Research. 34:462-466
Although designed primarily as a hard X-ray imager and spectrometer, the Ramaty High Energy Solar Spectroscopic Imager (RHESSI) is also capable of measuring the polarization of hard X-rays (20–100 keV) from solar flares. This capability arises from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e48dddcc6c171ad157a85cc0417dae76
https://doi.org/10.1016/j.asr.2004.02.007
https://doi.org/10.1016/j.asr.2004.02.007
Publikováno v:
Solar Physics. 210:125-142
Polarization measurements of hard X-rays from solar flares can provide a direct handle on the extent to which the accelerated electrons are beamed, which, in turn, has important implications for particle acceleration models. Past efforts to measured
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::954436272262a58c0529f694da707b33
https://doi.org/10.1023/a:1022413708738
https://doi.org/10.1023/a:1022413708738