Fig. 3From: Methane genesis within olivine-hosted fluid inclusions in dolomitic marble of the Hida Belt, JapanRepresentative Raman spectra of olivine-hosted fluid inclusions in dolomitic marble from the Hida Belt. a, b Raman spectra of the olivine-hosted fluid inclusions. c–e Raman spectra of olivine-hosted fluid inclusion (c), lizardite in olivine rim (d), and host olivine (e) in low wavenumber spectral range (110–750 cm−1). f, g Raman spectra of olivine-hosted fluid inclusion in high wavenumber spectral range (2800–3800 cm−1). h, i Raman spectra of lizardite (h) and olivine-hosted fluid inclusion (i) in O–H stretching region (3600–3750 cm−1)Back to article page