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I am interested to study the effect of spectral response functions of different satellites on the calculated brightness temperature.
What I need is to provide a blackbody (in the easiest case) at …
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reported by: @CloudyLex
the linda.in sim reported by linda strubbe is very slowly converging the H line optical depths. it is an optically thin static sphere which has not been well tested - all we…
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PyRTM contains functional python wrappers for SMARTS and SBdart, and is capable of modelling spectra in clear-sky and cloudy conditions. This would be a great set of functionality to incorporate into …
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# Updates from last week
- FoRTE
- Meeting presentation and Git tutorial - done
- Some analysis of ED parameters
- Working PEcAn multi-node setup -- can submit more ED runs more efficientl…
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Can somebody explain the meaning of this error message, and possible ways to avoid it? It originates in solver.c, where the photon is supposed to choose the next edge to follow (or something like that…
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reported by: @CloudyLex
the sim grains_conserve.in was added to auto by gjf on 08 may 31 - this exposes this bug clearly and quickly. The sim is irradiated by an STE blackbody at 500K and sphere is…
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reported by: @CloudyLex
http://adsabs.harvard.edu/abs/2015A%26A...579A..72B
2015A&A...579A..72B
```
Title:
H2 formation on PAHs in photodissociation regions: a high-temperature pathway to molecu…
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I would like to simulate TOA total upwelling radiances in the visible/SWIR region. Having looked at the LBLRTM instructions, and online, I *think* what I have to do is run two TAPE5's, and I have cop…
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# Bug report
## Summary
When building a standard atmosphere ("atmosphere = ertsc.atmosphere.MolecularAtmosphere()") or when checking the database komodo ("eradiate data check komodo"), eradiate …
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### Name and Institution (Required)
Name: Bob Yantosca
Institution: Harvard + GCST
### Confirm you have reviewed the following documentation
- [x] [Contributing guidelines](https://geos-che…