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Correlation between solar radiation and total syspended particulate matter in Santiago, Chile-Preliminary results
(1995)
This is a first-approach study tending to correlate solar radiation and temperature with total particulate matter in Santiago, Chile, a city heavily polluted by this contaminant. Experimental data for monthly average total ...
3D radiative transfer of intrinsically polarized dust emission based on aligned aspherical grains
(Oxford University Pres, 2017)
(Sub-)millimetre observations of the polarized emission of aligned aspherical dust grains enable us to study the magnetic fields within protoplanetary disc. However, the interpretation of these observations is complex. One ...
Variations in UV radiation in Chile
(1995)
The first observation of UV global radiation in Chile with a portable multichannel radiometer are reported. Four UV wavelengths are included: 305, 320, 340 and 380 nm. Observation latitudes spanning from 18° to 53 °S allow ...
Magnetic fields in protoplanetary discs: from MHD simulations to ALMA observations
(Oxford University Press, 2017-01)
Magnetic fields significantly influence the evolution of protoplanetary discs and the formation of planets, following the predictions of numerous magnetohydrodynamic (MHD) simulations. However, these predictions are yet ...
Prostate cancer survivors with symptoms of radiation cystitis have elevated fibrotic and vascular proteins in urine
(Public Library Science, 2020)
Radiation for pelvic cancers can result in severe bladder damage and radiation cystitis (RC), which is characterized by chronic inflammation, fibrosis, and vascular damage. RC development is poorly understood because bladder ...
Benchmarking the calculation of stochastic heating and emissivity of dust grains in the context of radiative transfer simulations
(EDP Sciences, 2015)
Context. Thermal emission by stochastically heated dust grains (SHGs) plays an important role in the radiative transfer (RT) problem
for a dusty medium. It is therefore essential to verify that RT codes properly calculate ...
Explosion of red supergiant stars: influence of the atmospheric structure on shock breakout and early time supernova radiation
(EDP Sciences, 2017)
Early-time observations of Type II supernovae (SNe) 2013cu and 2013fs have revealed an interaction of ejecta with material near the star surface. Unlike Type IIn SN 2010jl, which interacts with a dense wind for similar to ...
Processes in auroral oval and outer electron radiation belt
(Springer, 2018)
We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is ...
Processes in auroral oval and outer electron radiation belt
(Springer Berlin Heidelberg, 2018)
© 2018, The Author(s). We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of ...
Investigation of Charged Particles Radiation Moving in a Homogeneous Dispersive Medium
(Materials & Energy Research Center-Merc, 2017)
In this work, we use Drude-Lorents model description to study the radiation of a charged particles moving in a homogeneous dispersive medium. A suitable quantized electromagnetic field for such medium is utilized to obtain ...