Closed jwreep closed 6 months ago
Good point. I copied the power-law radiative loss function straight from HYDRAD which also includes this comment: https://github.com/rice-solar-physics/HYDRAD/blob/0fa1f9949540e6b9379548c72a030621fdee381d/Radiation_Model/source/radiation.cpp#L712 so I would pass that question on to @sjbradshaw.
My assumption was that the continuum is included in that power-law approximation everywhere but that it dominates at $\log{T}>7.63$. Here's a plot that shows a comparison between the RK loss (the one used here) and the radiative losses from CHIANTI that include the continuum contribution:
Naively, it appears that the component > 7.63 is specifically constructed to mimic the dominant continuum component at those high temperatures.
The power-law radiation function in HYDRAD includes the free-free (continuum) emission at the highest temperatures (> log T = 7.63). So, this will also be what is used in EBTEL++.
[FYI: The HYDRAD radiation code also includes a separate function to calculate just the free-free emission, which is added to the line emission calculated ion-by-ion for (e.g.) non-equilibrium radiation, in the appropriate temperature range.]
Hope this helps.
Cheers,
Steve
From: Will Barnes @.> Sent: Tuesday, December 19, 2023 8:28 PM To: rice-solar-physics/ebtelPlusPlus @.> Cc: sjbradshaw @.>; Mention @.> Subject: Re: [rice-solar-physics/ebtelPlusPlus] Free-free emission in radiative losses? (Issue #83)
Good point. I copied the power-law radiative loss function straight from HYDRAD which also includes this comment: https://github.com/rice-solar-physics/HYDRAD/blob/0fa1f9949540e6b9379548c72a030621fdee381d/Radiation_Model/source/radiation.cpp#L712 https://urldefense.com/v3/__https:/github.com/rice-solar-physics/HYDRAD/blob/0fa1f9949540e6b9379548c72a030621fdee381d/Radiation_Model/source/radiation.cpp*L712__;Iw!!BuQPrrmRaQ!jaC70dJJYEChJWaEy99PTlACBmZ0wjTBHY3-zQi0vUX4GmCdeD12VNajGDjFZF0wFSJPu68m_tdYjNN12GHXQ77BOALhnfKGwiE$ so I would pass that question on to @sjbradshaw https://urldefense.com/v3/__https:/github.com/sjbradshaw__;!!BuQPrrmRaQ!jaC70dJJYEChJWaEy99PTlACBmZ0wjTBHY3-zQi0vUX4GmCdeD12VNajGDjFZF0wFSJPu68m_tdYjNN12GHXQ77BOALh_QfL-zA$ .
My assumption was that the continuum is included in that power-law approximation everywhere but that it dominates at $\log{T}>7.63$. Here's a plot that shows a comparison between the RK loss (the one used here) and the radiative losses from CHIANTI that include the continuum contribution:
Naively, it appears that the component > 7.63 is specifically constructed to mimic the dominant continuum component at those high temperatures.
— Reply to this email directly, view it on GitHub https://urldefense.com/v3/__https:/github.com/rice-solar-physics/ebtelPlusPlus/issues/83*issuecomment-1863754774__;Iw!!BuQPrrmRaQ!jaC70dJJYEChJWaEy99PTlACBmZ0wjTBHY3-zQi0vUX4GmCdeD12VNajGDjFZF0wFSJPu68m_tdYjNN12GHXQ77BOALh3me8p1I$ , or unsubscribe https://urldefense.com/v3/__https:/github.com/notifications/unsubscribe-auth/ACC6C7SHIS5VNPIIC4BR7T3YKJEKNAVCNFSM6AAAAABA36MGP6VHI2DSMVQWIX3LMV43OSLTON2WKQ3PNVWWK3TUHMYTQNRTG42TINZXGQ__;!!BuQPrrmRaQ!jaC70dJJYEChJWaEy99PTlACBmZ0wjTBHY3-zQi0vUX4GmCdeD12VNajGDjFZF0wFSJPu68m_tdYjNN12GHXQ77BOALh873bQWI$ . You are receiving this because you were mentioned. https://github.com/notifications/beacon/ACC6C7TXBPR44OBND2RXJHLYKJEKNA5CNFSM6AAAAABA36MGP6WGG33NNVSW45C7OR4XAZNMJFZXG5LFINXW23LFNZ2KUY3PNVWWK3TUL5UWJTTPC2SBM.gif Message ID: @. @.> >
Does that mean HYDRAD neglects free-free for lower temperatures when using power law losses?
The power-law losses are just a fit to a (presumably) fairly detailed calculation of radiative losses. So, if those original calculations included free-free at lower temperatures then the power-law losses will too; if not, then no.
From: Jeffrey Reep @.> Sent: Wednesday, December 20, 2023 6:47 PM To: rice-solar-physics/ebtelPlusPlus @.> Cc: sjbradshaw @.>; Mention @.> Subject: Re: [rice-solar-physics/ebtelPlusPlus] Free-free emission in radiative losses? (Issue #83)
Does that mean HYDRAD neglects free-free for lower temperatures when using power law losses?
— Reply to this email directly, view it on GitHub https://urldefense.com/v3/__https:/github.com/rice-solar-physics/ebtelPlusPlus/issues/83*issuecomment-1865323924__;Iw!!BuQPrrmRaQ!jO6ag6GSOKDytTtgt_RfvXSVC2Hu487-df8wVqT3kUpMeEaCxsF-shV-duwbO9o3fI0PRt1mo3q4QSQLMW0V-iPfHZS7YHxq0wo$ , or unsubscribe https://urldefense.com/v3/__https:/github.com/notifications/unsubscribe-auth/ACC6C7WROC3NETILPHW2SETYKOBGRAVCNFSM6AAAAABA36MGP6VHI2DSMVQWIX3LMV43OSLTON2WKQ3PNVWWK3TUHMYTQNRVGMZDGOJSGQ__;!!BuQPrrmRaQ!jO6ag6GSOKDytTtgt_RfvXSVC2Hu487-df8wVqT3kUpMeEaCxsF-shV-duwbO9o3fI0PRt1mo3q4QSQLMW0V-iPfHZS7c3TVh78$ . You are receiving this because you were mentioned. https://github.com/notifications/beacon/ACC6C7WQECRSMXSM3GF7DZLYKOBGRA5CNFSM6AAAAABA36MGP6WGG33NNVSW45C7OR4XAZNMJFZXG5LFINXW23LFNZ2KUY3PNVWWK3TUL5UWJTTPF2KZI.gif Message ID: @. @.> >
I'm going to close this because at the very least, I think this is out of scope for ebtel++. Feel free to reopen if you think there are still questions that need to be answered.
The code has this comment:
Is f-f radiation not included at lower temperatures in the power law fit? If so, why? It should be non-negligible down to much lower temperatures.