Аннотация:A set of ten diamonds from different sources representing the main types of physical classification (IaA, IaAB, IaB and IIa) has been first explored by FTIR spectroscopy and SIMS calibrated by hydrogen ion implantation. The concentrations of hydrogen in the studied diamonds measured by SIMS range between 9.98 and 47.6 at.ppm or from 1.76 × 1018 to 8.40 × 1018 at./cm3. The 3107 cm-1 absorption line has been detected by FTIR spectroscopy (resolution near 1 cm-1) in five studied diamonds (IaB and IaAB). The 3107 cm-1 IR absorption lines due to H defects in these diamonds have been successfully described by the Lorentzian shape and their parameters have been evaluated. Based on the linear regression equation relating intensities of the 3107 cm-1 IR absorption lines in the four studied diamonds with H defect concentrations in them, the H defect IR absorption at 3107 cm-1 in diamond has been quantified. The absorption calibration constant for the 3107 cm-1 absorption line in diamond is 386 ± 64 ppb cm2. The corresponding cross-section per one H defect σ3107 (cm2) = (9.34 ± 1.25)×10-18/Γ (cm-1), Γ is the full width at half maximum of the 3107 absorption line. Based on a widely accepted interpretation that the H defect resulting in the 3107 cm-1 IR absorption peak in diamonds is actually the N3VH defect, the values of the obtained calibration constant and cross-section have been assigned to the N3VH defect in diamond. The equations relating concentration of the N3VH defect ([N3VH]) with the 3107 cm-1 IR absorption line integrated intensity (I3107) and intensity (α3107) are as follows: [N3VH] (ppb) = (386 ± 64) I3107 (cm-2);[N3VH] (ppm) = (0.607 ± 0.080) α 3107 (cm-1)Γ (cm-1).The presence of hydrogen impurities that do not contribute to the IR absorption at the 3107cm-1 peak were detected in all studied diamonds.