Yes, correct. The physical solution is stored at the solution points and 
extrapolated to the flux points.

Cheers

Peter

Dr Peter Vincent MSci ARCS DIC PhD
Senior Lecturer and EPSRC Early Career Fellow
Department of Aeronautics
Imperial College London
South Kensington
London
SW7 2AZ
UK

web: 
www.imperial.ac.uk/aeronautics/research/vincentlab<http://www.imperial.ac.uk/aeronautics/research/vincentlab>
twitter: @Vincent_Lab<https://twitter.com/Vincent_Lab>





On 27 Oct 2014, at 09:15, Antonio Garcia-Uceda 
<[email protected]<mailto:[email protected]>> wrote:

Dear Freddie,

Thank you very much for the reference. As I see the only time you utilise the 
Determinant of the Jacobian is when updating the solution in time. In the 
extrapolation to Face Flux points it does not intervene, right?

Best regards,
Antonio

On Monday, October 27, 2014 11:47:51 AM UTC+1, Freddie Witherden wrote:
On 27/10/14 09:13, Antonio Garcia-Uceda wrote:
> Dear All,
>
> My name is Antonio Garcia-Uceda, and I'm working on Flux Reconstruction.
> I have the following question:
>
> In pyFR, when we extrapolate the solution from Solution Points in Cells
> to Flux Points on Faces, Is this carried out over primitive variables
> (rho, u, v, w, p) or conserved variables (rho, rhou, rhov, rhow, rhoE)?
> In the second case, Are this variables also multiplied by the
> Determinant of the Jacobian computed at the solution point, i.e. bar
> state is indicated in FR literature (Jrho, Jrhou, Jrhov, Jrhow, JrhoE)?

PyFR works exclusively in terms of conservative variables.  Details on
the transformations can be found in our paper

  http://www.sciencedirect.com/science/article/pii/S0010465514002549

specifically equations 6, 12, 10, and 11.

Regards, Freddie.

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