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fab13
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Hello,
In physical radiative processes, I am studying the solution of the following equation :
##S=(1-\epsilon) J + \epsilon B##
with :
1) S the source function
2) J the mean intensity ( ##J=\dfrac{1}{2}\int_{-1}^{1} I_{\nu}\text{d}\tau_{\nu}##)
3) B the Boltzmann distribution
4) ##\epsilon## a coefficient
5) Below ##\tau_{\nu}## is optical depth
With Milne-Eddington approximation, we get : ##J=3K## (with K the seond moment of RTE (Radiation Transfer Equation)).
Moreover, we have : ##\dfrac{\text{d}K}{\text{d}\tau_{\nu}}=H\quad(1)## and ##\dfrac{\text{d}H}{\text{d}\tau_{\nu}}=J-S\quad(2)##
Taking these two equations (1), (2) and ##J=3K##, one has the following solution for J :
##J = J(\tau_{\nu}) = B - \dfrac{B}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}##
which implies :
##J = B \bigg[1-\dfrac{1}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg]##
So : ##S=(1-\epsilon) J + \epsilon B = J - \epsilon J + \epsilon B = B \bigg[1-\dfrac{1}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg] - \epsilon B \bigg[1-\dfrac{1}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg] + \epsilon B ##
##S= B \bigg[1-\dfrac{1}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}} + \dfrac{\epsilon}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg]##
##S=B\bigg[1-\dfrac{(1-\epsilon)}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg]##
##S=B\bigg(1-(1-\sqrt{\epsilon})\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg)\quad(3)##
As a conclusion, It is asked to do a graphical representation of normalized source function S/B and to comment about non-LTE "law" that ##S \approx \sqrt{\epsilon} B## ?
I would like to know what graphical representation is expected for normalized function S/B and what can I comment about the equation I got ##(1)## and the "non-LTE" law that says : ##S \approx \sqrt{\epsilon} B## ??
I mean, I would like to correctly and physically interpret the result in (3) and do the link between "LTE" and "non-LTE" cases.
Could I say that :
1) If ##\tau_{\nu}## is small (at the surface), then I find the non-LTE case :
##S/B=\sqrt{\epsilon}\quad(4)##
2) If ##\tau_{\nu}## is large (i.e, large depth), then I find the Boltzmann case :
##S/B=1\quad(5)##
?
Any help is welcome
Thanks in advance
In physical radiative processes, I am studying the solution of the following equation :
##S=(1-\epsilon) J + \epsilon B##
with :
1) S the source function
2) J the mean intensity ( ##J=\dfrac{1}{2}\int_{-1}^{1} I_{\nu}\text{d}\tau_{\nu}##)
3) B the Boltzmann distribution
4) ##\epsilon## a coefficient
5) Below ##\tau_{\nu}## is optical depth
With Milne-Eddington approximation, we get : ##J=3K## (with K the seond moment of RTE (Radiation Transfer Equation)).
Moreover, we have : ##\dfrac{\text{d}K}{\text{d}\tau_{\nu}}=H\quad(1)## and ##\dfrac{\text{d}H}{\text{d}\tau_{\nu}}=J-S\quad(2)##
Taking these two equations (1), (2) and ##J=3K##, one has the following solution for J :
##J = J(\tau_{\nu}) = B - \dfrac{B}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}##
which implies :
##J = B \bigg[1-\dfrac{1}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg]##
So : ##S=(1-\epsilon) J + \epsilon B = J - \epsilon J + \epsilon B = B \bigg[1-\dfrac{1}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg] - \epsilon B \bigg[1-\dfrac{1}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg] + \epsilon B ##
##S= B \bigg[1-\dfrac{1}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}} + \dfrac{\epsilon}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg]##
##S=B\bigg[1-\dfrac{(1-\epsilon)}{1+\sqrt{\epsilon}}\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg]##
##S=B\bigg(1-(1-\sqrt{\epsilon})\,e^{-\sqrt{3\epsilon} \tau_{\nu}}\bigg)\quad(3)##
As a conclusion, It is asked to do a graphical representation of normalized source function S/B and to comment about non-LTE "law" that ##S \approx \sqrt{\epsilon} B## ?
I would like to know what graphical representation is expected for normalized function S/B and what can I comment about the equation I got ##(1)## and the "non-LTE" law that says : ##S \approx \sqrt{\epsilon} B## ??
I mean, I would like to correctly and physically interpret the result in (3) and do the link between "LTE" and "non-LTE" cases.
Could I say that :
1) If ##\tau_{\nu}## is small (at the surface), then I find the non-LTE case :
##S/B=\sqrt{\epsilon}\quad(4)##
2) If ##\tau_{\nu}## is large (i.e, large depth), then I find the Boltzmann case :
##S/B=1\quad(5)##
?
Any help is welcome
Thanks in advance
Last edited: