correct_counts#
- hydrometlib.cosmos.correct_counts(cts_mod, factor_inten, factor_pa, factor_q)[source]#
Calculate corrected neutron counts using correction factors [counts h-1]
\[C_{corr} = C \cdot f_{inten} \cdot f_p \cdot f_Q\]Bogena et al. (2022): https://doi.org/10.5194/essd-14-1125-2022: “Variations of the incoming cosmic-ray intensity can have many causes, from galactic and solar disturbances to atmospheric and meteorological influences. Most of these anomalies are expected to change proportionally in every domain of the neutron energy spectrum and thus can be addressed by applying a set of correction factors.”
- Parameters:
cts_mod (
Expr) – Neutron counts to be corrected [counts h-1]factor_inten (
Expr) – Correction factor to neutron intensity counts [unitless]factor_pa (
Expr) – Atmospheric pressure correction factor to neutron counts [unitless]factor_q (
Expr) – Absolute humidity correction factor to neutron counts [unitless]
- Return type:
Expr- Returns:
Expression or Series of corrected mod counts [counts h-1].