Closed mkovari closed 5 months ago
Definitions.
The table of energy confinement times now looks like this:
****************** Energy confinement times, and required H-factors : ***********************
scaling law confinement time (s) H-factor for
for H = 1 power balance
ITPA20 (H) 2.072 1.165
IPB98(y,2) (H) 2.454 0.984
ISS95 (stell) 1.441 1.675
ISS04 (stell) 2.502 0.965
DS03 (H) 3.803 0.635
NSTX (Spherical) (H) 5.437 0.444
NSTX-Petty08 Hybrid (H) 4.571 0.528
NSTX gyro-Bohm Buxton(H) 38.020 0.063
You can see that the ITPA20 confinement time is less than the IPB98(y,2) value.
With the large-tokamak scenario (rmajor
fixed, hfact
variable), the outcome when ITPA20 is selected is a little unexpected: hfact
hardly changes (and remains below the upper bound), but all the other variables change, including the plasma current, helium content and radiation power. The xenon content has doubled.
Now that we have an up-to-date confinement scaling, I suggest people use it.
* Switch for energy confinement time scaling law
isc = 50
A unit test can be derived from this check I did:
Discussed in https://github.com/ukaea/PROCESS/discussions/2889