Zobrazeno 1 - 10
of 193
pro vyhledávání: '"Milic I"'
When interpreting spectropolarimetric observations of the solar atmosphere, wavelength variations of the emergent intensity and polarization translate into information on the depth stratification of physical parameters. We aim to quantify how the inf
Externí odkaz:
http://arxiv.org/abs/2409.13677
Autor:
Santos, J. M. da Silva, Molnar, M., Milić, I., Rempel, M., Reardon, K., Rodríguez, J. de la Cruz
Accurately assessing the balance between acoustic wave energy fluxes and radiative losses is critical for understanding how the solar chromosphere is thermally regulated. We investigate the energy balance in the chromosphere by comparing deposited ac
Externí odkaz:
http://arxiv.org/abs/2408.15908
One-dimensional, semi-empirical models of the solar atmosphere are widely employed in numerous contexts within solar physics, ranging from the determination of element abundances and atomic parameters to studies of the solar irradiance and from Stoke
Externí odkaz:
http://arxiv.org/abs/2404.07067
Chromospheric umbral oscillations produce periodic brightenings in the core of some spectral lines, known as umbral flashes. They are also accompanied by fluctuations in velocity, temperature, and, according to several recent works, magnetic field. I
Externí odkaz:
http://arxiv.org/abs/2107.02160
In this work, we discuss the application of convolutional neural networks (CNNs) as a tool to advantageously initialize Stokes profile inversions. To demonstrate the usefulness of CNNs, we concentrate in this paper on the inversion of LTE Stokes prof
Externí odkaz:
http://arxiv.org/abs/2103.09651
Oscillations in sunspot umbrae exhibit remarkable differences between the photosphere and chromosphere. We evaluate two competing scenarios proposed for explaining those observations: a chromospheric resonant cavity and waves traveling from the photo
Externí odkaz:
http://arxiv.org/abs/2008.10623
Akademický článek
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Publikováno v:
A&A 586, A87 (2016)
One of the necessary parameters needed for the interpretation of the light curves of transiting exoplanets or eclipsing binaries, as well as interferometric measurements of a star or microlensing events is how the intensity and polarization of a ligh
Externí odkaz:
http://arxiv.org/abs/1511.07213
Autor:
Ademowo, O.S., Dias, H.K.I., Milic, I., Devitt, A., Moran, R., Mulcahy, R., Howard, A.N., Nolan, J.M., Griffiths, H.R.
Publikováno v:
In Free Radical Biology and Medicine July 2017 108:77-85
Akademický článek
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