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solar radiation term in heat budget #5

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mrke opened this issue Dec 11, 2023 · 5 comments
Open

solar radiation term in heat budget #5

mrke opened this issue Dec 11, 2023 · 5 comments

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@mrke
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mrke commented Dec 11, 2023

Rsol <- 2*PPFD/UMOLPERJ # W m-2

Hi Remko,
I was comparing the predictions of leaf temperature from FindTleaf with other approaches and found that FindTleaf predicted way too high. I think it is because you multiply the incoming solar by two at the line referenced above. I think instead, because only one side gets the full blast, and the other side should get what is reflected from whatever surface is below.
All the best,
Mike

@mrke
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mrke commented Dec 11, 2023

sorry I missed a bit - should have said 'I think instead, you should either just multiply by 1 or be explicit about reflected solar hitting the underside ...'

@RemkoDuursma
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RemkoDuursma commented Dec 11, 2023 via email

@RemkoDuursma
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RemkoDuursma commented Dec 11, 2023 via email

@mrke
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mrke commented Dec 17, 2023

Actually, I take it back - I think the x2 might be because you are assuming 0.5 of the global solar is PAR and so multiplying the PPFD by two

@s-kganz
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s-kganz commented Feb 9, 2024

Hi,

I'm also finding that FindTLeaf returns too high of temperatures. The supplemental of this paper reports the same thing, especially when leaf size is large. I think the issue is coming from the treatment of longwave radiation:

# Longwave radiation
# (positive flux is heat loss from leaf)
Rlongup <- Emissivity*Boltz*Tk(Tleaf)^4
# Rnet
Rsol <- 2*PPFD/UMOLPERJ # W m-2
Rnet <- LeafAbs*Rsol - Rlongup # full
# Isothermal net radiation (Leuning et al. 1995, Appendix)
ea <- esat(Tair) - 1000*VPD
ema <- 0.642*(ea/Tk(Tair))^(1/7)
Rnetiso <- LeafAbs*Rsol - (1 - ema)*Boltz*Tk(Tair)^4 # isothermal net radiation

My understanding about longwave radiation is that:

  1. Both sides of the leaf are radiating energy
  2. Longwave radiation is emitted by air in all directions, so both sides of the leaf receive the incoming flux

This would translate to multiplying both Rlongup and (1 - ema)*Boltz*Tk(Tair)^4 by 2 in the above snippet. I've been working on some energy balance models that are formulated similarly, and I find that this results in more reasonable (i.e. cooler) temperatures. I don't have permission to share data from that project, but if this is of interest I could find something in the literature to compare on.

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