Zobrazeno 1 - 10
of 3 543
pro vyhledávání: '"impulsive events"'
Autor:
Mondal, Biswajit, Klimchuk, James A, Vadawale, Santosh V., Sarkar, Aveek, Del Zanna, Giulio, Athiray, P. S., Mithun, N. P. S., Mason, Helen E., Bhardwaj, A.
Small-scale impulsive events, known as nanoflares, are thought to be one of the prime candidates that can keep the solar corona hot at its multi-million Kelvin temperature. Individual nanoflares are difficult to detect with the current generation ins
Externí odkaz:
http://arxiv.org/abs/2301.02519
Autor:
Nhalil, Nived Vilangot, Nelson, Chris J., Mathioudakis, Mihalis, Doyle, J. Gerry, Ramsay, Gavin
Numerous studies have analysed inferred power-law distributions between frequency and energy of impulsive events in the outer solar atmosphere in an attempt to understand the predominant energy supply mechanism in the corona. Here, we apply a burst d
Externí odkaz:
http://arxiv.org/abs/2009.03123
Publikováno v:
Phys. Rev. D 102, 123021 (2020)
The Murchison Widefield Array (MWA) recorded \cite{Mondal-2020} impulsive radio events in the quiet solar corona at frequencies 98, 120, 132, and 160 MHz. We propose that these radio events are the direct manifestation of dark matter annihilation eve
Externí odkaz:
http://arxiv.org/abs/2009.00004
Autor:
Gil, Agnieszka1,2 (AUTHOR) gila@uph.edu.pl, Berendt-Marchel, Monika3 (AUTHOR), Modzelewska, Renata1 (AUTHOR), Siluszyk, Agnieszka1 (AUTHOR), Siluszyk, Marek1,4 (AUTHOR), Wawrzaszek, Anna2 (AUTHOR), Wawrzynczak, Anna3,5 (AUTHOR)
Publikováno v:
Solar Physics. Feb2023, Vol. 298 Issue 2, p1-21. 21p.
This paper investigates the conditions for producing rapid variations of solar ener- getic particle (SEP) intensity commonly known as dropouts. In particular, we use numerical model simulations based on solving the focused transport equation in the 3
Externí odkaz:
http://arxiv.org/abs/1403.6544
Autor:
Biswajit Mondal, James A Klimchuk, Santosh V. Vadawale, Aveek Sarkar, Giulio Del Zanna, P. S. Athiray, N. P. S. Mithun, Helen E. Mason, Anil Bhardwaj
Publikováno v:
The Astrophysical Journal, Vol 945, Iss 1, p 37 (2023)
Small-scale impulsive events, known as nanoflares, are thought to be one of the prime candidates that can keep the solar corona hot at its multimillion-Kelvin temperature. Individual nanoflares are difficult to detect with the current generation of i
Externí odkaz:
https://doaj.org/article/527132ea13e0407084dc55cf2827cf6d
Publikováno v:
In Journal of Fluids and Structures February 2016 61:60-75
Autor:
de Felice, F.
Publikováno v:
Nuovo Cim.B122:481-488,2007
Continued gravitational collapse gives rise to curvature singularities. If a curvature singularity is globally naked then the space-time may be causally future ill-behaved admitting closed time-like or null curves which extend to asymptotic distances
Externí odkaz:
http://arxiv.org/abs/0710.0983
Publikováno v:
Astrophys.J. 661: L207-L210, 2007
Spectroscopic observations of a solar limb flare recorded by SUMER on SOHO reveal, for the first time, hot fast magnetic reconnection outflows in the corona. As the reconnection site rises across the SUMER spectrometer slit, significant blue- and red
Externí odkaz:
http://arxiv.org/abs/0709.2329
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