OP Computations of radiative accelerations 
MassFractions 
Metal Fractional Composition (default = solar) 

Note: metal abundances are renormalised to the value of Z which has been set  it is necessary to specify only the relative abundance for each metal. 



Output options 
Please choose ONE of the following output options: 
An intermediate file containing radiative acceleration data for a selected element and a range of its abundance multiplier (χ) to be used locally for interpolation with the code accfit.tar.gz 

log_{10}(χ) range 


Selected element 
Initial 
Interval 
No. points 









Radiative accelerations, RMOs, and diffusion coefficients for a selected element, a range of its abundance multiplier (χ) and a stellar model (T_{eff} and depth profile {log_{10}(T) , log_{10}(ρ), r/R*}). 

log_{10}(χ) range 


Selected element 
Initial 
Interval 
No. points 

T_{eff} 







Please introduce local file with depth profile 



