params

Reference Species Parallel Thermal-to-Magnetic Pressure Ratio. 8 pi n_ref T_ref,par/B^2

Wavenumber perpendicular to B0, normalized to reference gyroradius. k_perp rho_ref = k_perp w_perp,ref/Omega_ref

Wavenumber parallel to B0, normalized to reference gyroradius. k_perp rho_ref = k_perp w_t,ref,perp/Omega_ref

Parallel reference thermal velocity normalized to the speed of light. v_t,ref,par/c

Number of species/components to be included in calculation.

Number of parameter scans.

Selection for the type of dispersion calculation to be undertaken. -1: Calculate disp(om) at a single (omega, gamma) 0: Calculate Roots for input plasma parameters. 1: Calculate Roots for input plasma parameters or Reads in root value and then scan over plasma parameters, with range and type specified in .in file. 2: Calculate Roots for input plasma parameters or Reads in root value and then scan over two-dimensional plasma parameters space, with range and type specified in .in file. 3: deprecated 4: Make multiple maps of complex frequency space. 5: Find roots for parameters along a prescribed path Path is set by solar wind models, with values calculated and output by helper function (in development, the radial scan function.).

Input specified nroots to follow.

Determines method for selecting initial solutions. T-> Use map routine to determine solutions in defined regions of complex frequency space. Map parameters determined by &maps list in .in file. F-> Read nroot_max initial guesses for complex frequency solutions. Guesses determined by &guess_N lists in .in file.

Toggle on low-n susceptibility suplementary calculation.

Flag to use Revised low_n for LD/TTD separation. This modifies the Collisionless Power Absorption Calculation! IF TRUE THEN low_n MUST BE TRUE TOO! (GGH: 1/18/23)

Enables or suppressed output to screen.

Data Subdirectory where output is stored.

Common name string for output files.