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6 results for “clumpiness”
Land use and land cover scenarios for the Maurienne valley (French Alps) at 2085 horizon produced using CLUMPY model
<p>We built three contrasted future LULC scenarios from 2020 to 2085 with the CLUMPY model (Mazy and Longaretti, 2022). The CLUMPY model is an innovative model of land use and land cover change comprising a calibration-estimation module separate from a non-biased allocation module. It is calibrated by using time series of past LULC maps (Mazy and Longaretti, 2022). The model then calculates transition probabilities for each LULC class according to relevant spatial explanatory variables. Next, the model can produce maps of future LULC distributions according to information it learned during the calibration-estimation phase. This model has the benefits of being easy to use, proposing nonbiased allocation methods and producing scenarios of future LULC change either by adjusting manually the matrix of LULC transitions probabilities (used for the Conservation and Tourism scenarios) or by training the model on specific areas of the past time series (only used for the Conservation scenario).</p>
Land use and land cover scenarios for the Maurienne valley (French Alps) at 2085 horizon produced using CLUMPY model
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Unified Clumpy AGN Torus Model and X-ray spectrum
<p>In Buchner et al. (in prep) we develop a geometry for the X-ray obscurer of AGN. Its cloud population is consistent with existing CLUMPY (Nenkova+02) infrared models. However, we find that a inner torus ring component is required to fit local Compton-thick AGN.</p> <p>More information at <a href="https://github.com/JohannesBuchner/xars/blob/master/doc/uxclumpy.rst">https://github.com/JohannesBuchner/xars/blob/master/doc/uxclumpy.rst</a></p> <p>Our model has two geometry parameter:<br> 1) The opening of the torus, or the vertical extent of the clouds (sigma)<br> 2) The covering of the inner Compton-thick wall.<br> Further parameters are:<br> 3) Photon index and energy cut-off of the corona<br> 4) Column density in the line of sight (up to 10^26)<br> 5) Viewing angle.</p> <p>We release XSPEC table spectra here.</p>
Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era Halo
<p>This is a persistent version of the datasets and data table associated with Spilker et al. (2022), ApJL. I (Justin) recommend checking https://github.com/spt-smg/publicdata for any updates to the datasets contained here; this is just a tarball of the folder in that repository for this paper, commit 9e129f2.</p>
X-ray spectrum for CAT3D-WIND clumpy model
<p>In Buchner et al. (in prep) computations of a clumpy X-ray obscurer of AGN is computed. Here the same method is applied to some CAT3D-WIND models.</p> <p>See https://github.com/JohannesBuchner/xars for more information.</p>
Clumpy AGN outflows due to thermal instability
<p>Movies of models A, B, C, and D from Dannen et al. 2020.</p>
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