Hi everyone !!
I am a total noob in CANTERA, so my questions might be totally stupid... However, I could not find any topic on this matter, and would really appreciate some help !
I am currently using a Python interface.
Here we go : I was using CHEMKIN II to model a sort of "extinction" residence time with the PSR option, by restarting calculations with a smaller and smaller residence time.
Also, I had a good enough grasp onto the equations (for mass fractions & temperature) that solver used to come up with solutions.
I am currently failing in both areas with CANTERA in that :
- I cannot find a way to model that kind of, I guess would be a Reactor
for which I could control the residence time & the pressure, and not worry so much about neither the mass
flow rate nor the rho
- I cannot for the life of me understand what kind of equations CANTERA is solving when launching a Reactor calculation.
My questions are, then :
- Has anyone ever tried to capture that type of "extinction" values with CANTERA ? And if so, how did you do it ?? What type of classes did you use, how did you specify the inlet temp and the
tau !
- Is CANTERA solving the same equations for mass frac & temp when using the ReactorNet option as CHEMKIN - PSR did ? Does he perform an equil as a first guess ? Is he taking the T provided
at the beginning of a simulation to be the inlet temperature then ? And does he uses that temperature for each "time step" (sim = ReactorNet(blabla); sim.advance(t) ) ?
(redirection towards a comprehensive manual, and not
http://cantera.github.io/dev-docs/sphinx/html/index.html would be totaly acceptable :) )
I guess the inlet temperature and residence time really bug me in that I don't know if CANTERA makes use of them somewhere... Maybe Reactor is more similar to SENKIN ?
I find it really weird though that such an extinction procedure would be impossible to perform with Cantera, as it is a test broadly used in the literature today !
Anyway, help will be greatly appreciated, and thank you for reading !!
AF