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This is a summary of some of my thoughts about saving files, mostly to help organize my thoughts on paper.
I am not considering any changes to kete for this at the moment, merely "thinking out loud…
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See if scaling from 525 km for optical Cherenkov properties, Cherenkov spectrum, Cherenkov light density, Cherenkov angles (this should be fine, but will check)
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Hello,
I am trying to run your QBOX and other repos as this is very interesting but there seems to be missing the custom CUBE_REPORT import:
```
import CUBE_REPORT # Import the custom report m…
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Hi team, the new version appears to have problems when taking reducers with the Landsat 8 data.
Sharing a code snippet here:
```
#Acquire optical data using hf.dataset
optical = hf.Landsat8(tonl…
mn5hk updated
8 months ago
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When defining the emission spectrum (or re-emission in the case of WLS materials) as a function of the wavelength, Ratpac uses the spectrum defined in the RATDB file, but it converts the wavelength to…
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P. Polimeno, A. Magazzu, M. A. Iati, R. Saija, L. Folco, D. Bronte Ciriza, M. G. Donato, A. Foti, P. G. Gucciardi, A. Saidi, C. Cecchi-Pestellini, A. Jimenez Escobar, E. Ammannito, G. Sindoni, I. Bert…
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The optical filter profiles should be stored in this object, thus featuring many of the Spectrum's properties and qualities (#7 ). The spectral call should also feature generator functions to expand a…
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Hello,
I have a question on how to properly model aerosols in RRTM_LW. I am trying to model scattering and absorption of aerosol in the first two layers of my model atmosphere. I am using the DISOR…
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Pro: Future proof, not mistakes, guaranteed to be unique definition.
Con: Validation warnings on reading GDML, doesn't solve kryptonite materials.
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Can we reproduce the offsets seen in rapidly vs slowly rotating stars in the optical, based on their Kepler spot properties?
Requires Issue #2 to be built first