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**Is your feature request related to a problem? Please describe.**
We should implement Coen's new mass transfer stability prescription into COMPAS.
**Describe the solution you'd like**
This cons…
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### Routes
```routes
/springer/journal/:journal
```
### Full routes
```fullroutes
https://rsshub.app/springer/journal/40820
https://rsshub.app/springer/journal/41114
```
### Relat…
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### 路由地址
```routes
/acs/journal/:id
```
### 完整路由地址
```fullroutes
acs/journal/accacs
acs/journal/jacsat
```
### 相关文档
https://docs.rsshub.app/zh/routes/journal#american-chemistry…
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This issue adresses the integration of the high order approach from the AixLib into the model structure of this library.
A model with all necessary ports and inputs should be added in order to int…
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EDIT: [Scroll down to here](https://github.com/isofit/isofit/issues/188#issuecomment-733902032) to see the actual issue.
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I was trying to do some basic runs using the the sRTMnet but ran int…
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This issue is motivated by an email correspondence and related E3SM issue https://github.com/E3SM-Project/E3SM/issues/4073. Please see the E3SM issue for detailed history of the debug.
My understan…
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As Tiago Pereira said:
> stellar atmosphere models are often tabulated on a depth scale, which means that the top of the atmosphere (surface in photospheric models) is the first element in the array. …
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**Submitting author:** @simonrp84 (Simon Proud)
**Repository:** https://github.com/simonrp84/PyCoxMunk
**Branch with paper.md** (empty if default branch): paper
**Version:** v1.1.0
**Editor:** @pdebuy…
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Example: https://mila.quebec/en/publications/
It would be nice to reuse the same code as in the Mila website. Not sure if that's 'easily' possible via RTD
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A historical preamble: this code _started_ as a telluric modeling code and has morphed into a stellar modeling code. But the infrastructure exists to do line-by-line radiative transfer of the Earth's…
gully updated
2 years ago