Radiative loss function for coronal plasma
The influence of radiative core growth on coronal X ray emission from pre main sequence stars
... a radiative loss function Λ(T X ) and the volume emission measure, L X ≈ Λ(T X )EM ...piecewise function of the coronal temper- ature T X ...the coronal plasma and V the ...
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Effect of a radiation cooling and heating function on standing longitudinal oscillations in coronal loops
... cooling/heating function that accounts for radiation and unspecified heating of the coronal plasma can significantly affect longitudinal (slow magnetoacoustic) oscilla- tions of coronal ...
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The influence of the solar coronal radiation on coronal plasma structures, I: determination of the incident coronal radiation
... the radiative processes within coronal structures, it is necessary to determine the characteristics of the incident radiation from the corona incident on a point at an arbitrary height above the solar ...
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Radiative damping of standing acoustic waves in solar coronal loops
... A significantly stronger bulk flow would be required to transport ions across the temperature gradient before they could equili- brate with their surroundings, and drive the ionisation balance sufficiently far from ...
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Dynamical phenomena in stratified solar coronal plasma
... a plasma in hydrostatic equilibrium, would correspond to a plasma temperature of ...a plasma where the density scale-height is ...a plasma temperature of ...a function of the time ...
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Dynamics of plasma condensations in a gravitationally stratified coronal loop
... of coronal rain condensations are ob- served to fall directly towards the solar surface, the individual blobs are sometimes observed to longitudinally oscillate up and down before falling (Kohutova & Verwichte ...
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Excitation of vertical coronal loop oscillations by plasma condensations
... the coronal loop can be expected to readjust to some extent while the condensation region is being ...characteristic radiative cooling time scale with the typical oscillation ...The radiative cooling ...
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Gravitational Instability of a Two Component Rotating Viscous Plasma under the Effect of Arbitrary Radiative Heat-Loss Functions and Electron Inertia
... viscous plasma in the presence of magnetic field, electrical resistivity, the effect of arbitrary radiative heat-loss functions and finite electron inertia is ...
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Slingshot prominences : coronal structure, mass loss and spin down
... We present a new method of modelling the observational sig- natures of “slingshot prominences” - clouds of cool plasma trapped within the coronae of rapidly-rotating stars. We use maps of the surface magnetic ...
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Rare loss of function mutations in ANGPTL family members contribute to plasma triglyceride levels in humans
... multiple loss-of-function alleles in ANGPTL3 and ANGPTL5, together with those previously reported in ANGPTL4 (12), are associated with lower plasma levels of TG, suggesting a common role for these ...
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Collisional-Radiative Model for Spectroscopic Diagnostic of Optically Thick Helium Plasma
... Figures 2 (a) and 2 (b) show the line-of-sight inte- grated emission powers of the spectral lines of the sin- glet and triplet states obtained from signals of the abso- lutely calibrated optical system, respectively, at ...
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Comparison of Iron Plasma Atomic and Radiative Properties Computed with a Relativistic Collisional Radiative Average Atom Code versus Other Models
... collisional radiative balance with the new atomic model, allows now to compute plasmas in NLTE regime or coronal regime, widening considerably for all chemical elements the validity range of thermodynamic ...
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Beam effect on electromagnetic ion-cyclotron waves with general loss – cone distribution function in an anisotropic plasma-particle aspect analysis
... steep loss-cone distribution of the magnetosphere decreases the transverse resonant energy in the presence of EMIC ...steep loss-cone decreases the heating rate of the transversely accelerated ions through ...
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Nonlinear slow magnetoacoustic waves in coronal plasma structures
... β plasma and non-parallel propagation, the non-zero magnetic field fluctuations interact with the density and velocity pertur- bations and therefore affect the wave propagation speed as well as the wave ...
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Long wavelength torsional modes of solar coronal plasma structures
... cylindrical plasma structure with the use of the second order thin flux tube ...ious plasma structures in the corona of the Sun, e.g. coronal jets and plumes, as well as segments of coronal ...
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Cut off period for slow magnetoacoustic waves in coronal plasma structures
... Aims. We investigate the effects of obliqueness, magnetic field and non-uniformity of the medium on the evolution of long-wavelength slow magnetoacoustic waves guided by field-aligned plasma non-uniformities, also ...
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The role of the loss function in the probabilistic function approximation
... The copyright exception in section 29 of the Copyright, Designs and Patents Act 1988 allows the making of a single copy solely for the purpose of non-commercial research or private stu[r] ...
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Weight Loss and Plasma PLTP Activity
... PLTP has been reported to be elevated in obese individ- uals (8, 11–13) and in diabetic subjects (14–16) and has been associated with insulin resistance (14, 17, 18). How- ever, no perturbation studies have been carried ...
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Radiative decay of keV-mass sterile neutrino in magnetized electron plasma
... The radiative decay of sterile neutrinos with typical masses of 10 keV is in- vestigated in the presence of an external magnetic field and degenerate electron ...nonrelativistic plasma are ...magnetized ...
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High frequency Alfven waves in multi ion coronal plasma : observational implications
... the plasma due to waves or ...the plasma depends strongly on the assumptions and the modeling used in the reduction of the observations and on the correction for the instrumental effects [Kohl et ...
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