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Hello could you please how to model an infrared lamp (with reflector) for simulating radiant spécular optical rays with reflections.
![IMG_2427](https://github.com/user-attachments/assets/bc51b021-…
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This issue follows on from issue cf-convention/vocabularies#158, in which a range of standard names were proposed for inclusion in the CF convention for diagnostics from a diagnostic call to a model's…
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Currently, the radiative loss function is specified as a power-law according to Eq. 3 of Klimchuk et al. Instead of just hardcoding this, we should allow the user to specify a different loss function …
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Requests:
- Radiate-button (turns on when all workflow steps are green)
- Export protocol feature after radiation
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I would like to ask if someone can give me some advice or if the author can make some small edits to the extension code:
- random value of presets prompt (embellish, style, negative)
- dynamic promp…
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Hello, I'm unsure if its a misuse or a bug, but in the following example, when I update the logged message in the actor, it still print the initial one. Is it because the actor is started before radia…
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CHIANTI version 9 introudced the `.auto` and `.rrllvl`such that the processes of autoionization and dielectronic recombination from the lower and upper stages, respectively, could be included the leve…
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Currently, the clear-sky TOA SW upwelling radiative fluxes have a global mean bias of ~10 W m^-2. Here are the plots of biases in ~5-yr mean TOA SW upwelling radiative fluxes. The clear-sky SW fluxes …
szy21 updated
2 months ago
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Currently, PROTEUS only supports volatile outgassing, but at higher temperatures we should expect significant amounts of rock vapour to be produced. Integrating these into the radiative transfer would…
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At relatively low temperatures, the emissivity can go negative. Since different element and charge states stop radiating at different temperatures (e.g. Ar+17 has little to no radiation below 100eV, b…