optically thin
A Simple Optical Model Well Explains Plasmonic Nanoparticle Enhanced Spectral Photocurrent in Optically Thin Solar Cells
... for optically thin GaAs solar cells with Ag and Al nanoparticles of various dimensions, demonstrating the validity of our modeling ...enhanced thin-film solar cells to provide design princi- ples for ...
10
Slip flow of an optically thin radiating non-Gray couple stress fluid past a stretching sheet
... an optically thin limit, the fluid does not absorb its own emitted radiation, it means that there is no self- absorption, but the fluid does absorb radiation emitted by the ...called optically thick ...
10
A method for improved SCIAMACHY CO 2retrieval in the presence of optically thin clouds
... cally thin cirrus clouds because on the one hand it is not pos- sible to get enough information from below an optically thick cloud and on the other hand the foregoing cloud screening fil- ters already the ...
24
Spectral energy distributions of passive T Tauri and Herbig Ae disks: grain mineralogy, parameter dependences and comparison with ISO-LWS observations
... We improve upon the radiative, hydrostatic equilibrium models of passive circumstellar disks con- structed by Chiang & Goldreich. New features include (1) an account for a range of particle sizes, (2) employment of ...
13
Radiation effects on unsteady MHD free convection with Hall current near an infinite vertical porous plate
... the optically thin limit along an infinite vertical porous plate are investigated in the presence of strong transverse magnetic field imposed perpendicu- larly to the plate, taking Hall currents into ...
7
Preliminary verification for application of a support vector machine-based cloud detection method to GOSAT-2 CAI-2
... feasible. Accordingly, it is difficult to discriminate between ice or snow and clouds. The difference or similarity between CLAUDIA1–CAI and CLAUDIA3–CAI was attributed to this source of error. In Thailand, CLAUDIA3–CAI ...
16
Heat transfer in an unsteady MHD flow through an infinite annulus with radiation
... On account of the axial symmetry and the annulus being infinite in the z-direction, the temperature field is independent of θ and z. In (), the rate of radiative heat flux in the optically thin limit for a ...
17
The abundance and thermal history of water ice in the disk surrounding HD 142527 from the DIGIT Herschel Key Program
... of optically thin emission from the spec- tral region with the ice ...an optically thin warm surface layer and make a linear least-squares fit to a part of their spectrum assuming a single ...
11
Excited states of molecular helium and oxygen
... The conditions used produced 10% yield of metastable states in 0.1 Torr partial pressure of oxygen with 2 watts of microwave energy.. is the most optically thin and thus least in error..[r] ...
195
Use of spectral cloud emissivities and their related uncertainties to infer ice cloud boundaries: methodology and assessment using CALIPSO cloud products
... particularly optically thin ice clouds known as cirrus, the plane-parallel assumption breaks down because cirrus tends to be optically thin but geometrically thick, which is different with ...
16
Swift observations of the cooling accretion disk of XTE J1817−330
... simple optically thick geometrically thin accretion disk with multiple blackbody components, as described in “diskbb” (Mitsuda et ...hot optically thin Comptonizing corona (Titarchuk ...
12
Herschel Planetary Nebula Survey (HerPlaNS): hydrogen recombination laser lines in Mz 3
... of optically thin ionized gas, as would be typical for nebular gas in PNe; (ii) the compact core of Mz 3 is responsible for a large fraction of the Herschel HRLs emission; (iii) the line intensity ratios ...
13
Grid-free simulation of radiative transport in a participating medium
... an optically-thin computational ring has been presented in section ...an optically-thick ring was proposed in the previous ...an optically-thin ring using a scaling of the spherical ...
13
Fragmentation and disk formation in high-mass star formation: The ALMA view of G351.77-0.54 at 0.06′′ resolution
... Assuming optically thin dust emission at 200 K (see more details below), our 3σ detection limit of 21 mJy beam −1 corresponds to mass and column density sensi- tivities of ...
13
Unlocking the secrets of the midplane gas and dust distribution in the young hybrid disc HD 141569
... for optically thin emission, considerably lower than that of thermal continuum emission in this regime and so its e ff ect may be seen in the spectral ...
6
Enrichment of the Hot Intracluster Medium: Observations
... Specifically, the hot ( ∼ 10 6 –10 8 K), optically thin plasma (or intra- cluster medium, ICM 1 ) pervading galaxy clusters, groups, and giant elliptical galaxies is rich in chemical ele[r] ...
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0e8d288eb0ab73a1786db01a00c97f2257d36a34.pdf
... The comparison SWS sample was chosen from spectra classi fi ed as carbon stars by Kraemer et al. ( 2002 ) . Their classi fi cation scheme assigns spectra to groups based on the overall shape of the spectrum, with naked ...
19
Chemically Reacting Unsteady Magnetohydrodynamic Oscillatory Slip Flow of a Micropolar Fluid in a Planer Channel with Varying Concentration
... generating, optically thin and chemically reacting oscillatory fluid flow in a planer channel filled with porous medium in the presence of thermal radiation with temperature and concentration ...
8
Radial structure in the TW Hya circumstellar disk
... The TW Hya disk has been spatially resolved at many wavelengths. Wilner et al. (2000, 2003), Qi et al. (2004), and Isella et al. (2009) resolved the outer disk in the millimeter regime and found range of 70–140 AU for ...
10
Aspects of the MHD stability of coronal and laboratory plasmas
... of the optically thin radiative energy loss on temperature, and is generally accepted to be important for the formation of prominences - in an equilibrium that includes magnetic field li[r] ...
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