We estimated intrinsic attenuation Q 1 i , scattering attenuation Q 1 s , site amplification Z, and source energy S from inversion of three-component coda envelopes of the 1999 Chamoli earthquake of India for central frequencies 1.5, 3, 6, 12, and 24 Hz. The multiple isotropic scattering of S waves was numerically simulated by using a Monte Carlo method based on the radiative transfer theory. Isotropic sources and acoustic scattering in a full space were assumed. Adapting a grid search for scattering coefficient g and least-squares inversion for intrinsic attenuation parameter b, and source energy S, we inverted the observed envelopes of ten aftershocks (M L ≥ 3:5) in 1-24 Hz.Our results reveal that both Q 1 s and Q 1 i are weakly frequency dependent with the power-law forms of 0:006 0:004f 0:890:33 and 0:003 0:0005f 0:840:08 , respectively. High scattering loss can be interpreted to be due to the presence of large lateral velocity heterogeneities in the crust. The total attenuation Q 1 decreases with frequency, taking the power-law form of 0:009 0:003f 0:870:19 . The mean free path ranges from 30 to 300 km, with an average value of 100 km, and the intrinsic attenuation parameter b ranges from 0.01 to 0:05 sec 1 , with an average value of 0:03 sec 1 . Our estimates of source energy are in good agreement with the values obtained assuming an ω 2 -source model. Site effects estimated using the fixed values of S k , b, and g exhibit less scatter, ranging from 0.73 to 2.54 with no significant frequency dependence consistent with the rock sites.