cosmicsense.core.corrfact_baro¶
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cosmicsense.core.corrfact_baro(p, p_0, L)¶ Compute correction factor for barometric effects.
The equation was suggested by Zreda et al. (2012). For default values of the mass attenuation length for high-energy neutrons
L, refer to Fig. 1 in Andreasen et al. (2017).- Parameters
p (float or array of floats) – Barometric pressure at the probe (mbar)
p_0 (float) – Reference value for barometric pressure (mbar)
L (float) – Mass attenuation length for high-energy neutrons
- Returns
output – Correction factor for barometric effects (dimensionless)
- Return type
float or array of floats