Zobrazeno 1 - 10
of 35
pro vyhledávání: '"Aaron Reid"'
Autor:
Aysegul Ors, Alex Daniel Chitsazan, Aaron Reid Doe, Ryan M Mulqueen, Cigdem Ak, Yahong Wen, Syber Haverlack, Mithila Handu, Spandana Naldiga, Joshua C Saldivar, Hisham Mohammed
Publikováno v:
Nucleic Acids Research. 50:11492-11508
Breast cancers are known to be driven by the transcription factor estrogen receptor and its ligand estrogen. While the receptor's cis-binding elements are known to vary between tumors, heterogeneity of hormone signaling at a single-cell level is unkn
Autor:
Mats Carlsson, Lyndsay Fletcher, Joel Allred, Petr Heinzel, Jana Kašparová, Adam Kowalski, Mihalis Mathioudakis, Aaron Reid, Paulo J. A. Simões
Context: Solar flares are the result of the sudden release of magnetic energy in the corona. Much of this energy goes into accelerating charged particles to high velocity. These particles travel along the magnetic field and the energy is dissipated w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eb4860f57ff5da0968daf9fbeb44a8b6
Akademický článek
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Flare Induced Sunquake Signatures in the Ultraviolet as Observed by the Atmospheric Imaging Assembly
Autor:
Mihalis Mathioudakis, Sean Quinn, David B. Jess, Christopher J. Nelson, Ryan O. Milligan, Aaron Reid
Publikováno v:
Mathioudakis, M, Jess, D, Nelson, C, Reid, A, Milligan, R & Quinn, S 2021, ' Flare Induced Sunquake Signatures in the Ultraviolet as Observed by the Atmospheric Imaging Assembly ', The Astrophysical Journal, vol. 920, 25 . https://doi.org/10.3847/1538-4357/ac0139
Sunquakes (SQs) have been routinely observed in the solar photosphere, but it is only recently that signatures of these events have been detected in the chromosphere. We investigate whether signatures of SQs are common in Ultraviolet (UV) continua, w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6640aac4ae56db3603ded5db70580f73
https://pure.qub.ac.uk/en/publications/3deb0558-13a8-4b83-921f-27564bf19269
https://pure.qub.ac.uk/en/publications/3deb0558-13a8-4b83-921f-27564bf19269
Publikováno v:
Monson, A J, Mathioudakis, M, Reid, A, Milligan, R & Kuridze, D 2021, ' Flare Induced Photospheric Velocity Diagnostics ', The Astrophysical Journal, vol. 915, no. 1, 16 . https://doi.org/10.3847/1538-4357/abfda8
We present radiative hydrodynamic simulations of solar flares generated by the RADYN and RH codes to study the perturbations induced in photospheric Fe I lines by electron beam heating. We investigate how variations in the beam parameters result in d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6f399d0908cdbb3aaa3be45a01205525
https://pure.qub.ac.uk/en/publications/658f9664-b373-42f6-9aa9-496ba4c51f41
https://pure.qub.ac.uk/en/publications/658f9664-b373-42f6-9aa9-496ba4c51f41
Autor:
Rebecca L. Hewitt, Marco Stangalini, David B. Jess, Mihalis Mathioudakis, Aaron Reid, Peter H. Keys, Shahin Jafarzadeh, Sergiy Shelyag, Vasco Manuel de Jorge Henriques, D. Del Moro
Publikováno v:
Keys, P, Reid, A, Mathioudakis, M, Shelyag, S, de Jorge Henriques, V M, Hewitt, R, Del Moro, D, Jafarzadeh, S, Jess, D & Stangalini, M 2020, ' High-resolution spectropolarimetric observations of the temporal evolution of magnetic fields in photospheric bright points ', Astronomy and Astrophysics, vol. 633, A60 . https://doi.org/10.1051/0004-6361/201936545
Astronomy & Astrophysics
Astronomy & Astrophysics
Context. Magnetic bright points (MBPs) are dynamic, small-scale magnetic elements often found with field strengths of the order of a kilogauss within intergranular lanes in the photosphere. Aims. Here we study the evolution of various physical proper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d45e7c973a06870ff6d8b5ebcee8ceb1
https://pure.qub.ac.uk/en/publications/highresolution-spectropolarimetric-observations-of-the-temporal-evolution-of-magnetic-fields-in-photospheric-bright-points(4c20812d-cb42-4020-b711-d0bdc11fec36).html
https://pure.qub.ac.uk/en/publications/highresolution-spectropolarimetric-observations-of-the-temporal-evolution-of-magnetic-fields-in-photospheric-bright-points(4c20812d-cb42-4020-b711-d0bdc11fec36).html
Publikováno v:
Shetye, J, Shelyag, S, Reid, A L, Scullion, E, Doyle, J G & Arber, T D 2018, ' Signatures of quiet Sun reconnection events in Ca II, Hα, and Fe I ', Monthly Notices of the Royal Astronomical Society, vol. 479, no. 3, pp. 3274–3287 . https://doi.org/10.1093/mnras/sty1548
We use observations of quiet Sun (QS) regions in the Hα 6563 Å, Ca II 8542 Å, and Fe I 6302 Å lines. We observe brightenings in the wings of the Hα and Ca II combined with observations of the interacting magnetic concentrations observed in the S
Autor:
Scott E. Nielsen, Clayton T. Lamb, Michael F. Proctor, Stan Boutin, Laura Smit, Bruce N. McLellan, Garth Mowat, Aaron Reid
Publikováno v:
Journal of Applied Ecology. 55:1406-1417
Autor:
Peter H. Keys, C. Quintero Noda, Aaron Reid, Mihalis Mathioudakis, R. J. Campbell, Sergiy Shelyag
Publikováno v:
Campbell, R J, Shelyag, S, Quintero Noda, C, Mathioudakis, M, Keys, P & Reid, A 2021, ' Constraining the magnetic vector in the quiet solar photosphere and the impact of instrumental degradation ', Astronomy and Astrophysics . https://doi.org/10.1051/0004-6361/202141421
With the advent of next generation high resolution telescopes, our understanding of how the magnetic field is organized in the internetwork (IN) photosphere is likely to advance.We aim to evaluate the extent to which we can retrieve information about
Autor:
R. J. Campbell, Michail Mathioudakis, Manuel Collados, Chris J. Nelson, David Kuridze, Aaron Reid, A. Asensio Ramos, P. H. Keys
Publikováno v:
Astronomy & Astrophysics. 652:C2
We correct a typographical error in the original paper. Figures 10, 12, 14, 15, and 16 contain a table in the top right panel with four columns and four rows of values. The line of sight velocity, vLOS, values for scheme 1 inversions (in the fourth r