Research Updates
In the present study, seven-year-long observations of rain microphysical properties are presented using a ground-based disdrometer located at Braemore; a site on the windward slope of the Western Ghats (WG) over the Indian Peninsula. The annual cycle of rainfall shows a bimodal distribution with a primary peak during summer monsoon and secondary peak during pre-monsoon. Pre-monsoon rain events are less in number but are with high intensity and characterize large raindrops and low number concentration. During summer monsoon, short and less intense rain events with small drops are noticed. Post-monsoon rain is having a long duration less intense events with lower concentration of large raindrops compared to the summer monsoon. In the seasonal variation of mean diameter (Dm) and raindrop concentration (NT ) with Rain Intensity (RI), winter and pre-monsoon rains exhibit higher values of Dm and lower values of NT compared to the summer and post-monsoon seasons for all the RI ranges. The mean features of the rain microphysical parameters are also supported by the case studies of rain events. RI, Dmand N T are categorized into different range bins for all the seasons to identify their variation and relative rainfall contribution to the total seasonal rainfall. Heavy drizzle/Light rain has maximum rain duration, and the relative contribution to the rainfall is high from heavy rain type. Winter and pre-monsoon rains are mostly contributed from the larger raindrops (>Dm 3), and during summer and post-monsoons it is from Dm 2 onwards. The distribution of occurrence frequency of NT and rainfall are similar during all four seasons. NT 2 recorded rainfall percentage nearly the same as NT 1 in summer monsoon and this also supports large number of raindrops in this season. In RI-Duration analysis, all seasons showed similar distribution, and 90% of total duration is contributed from RI with less than 20 mm h-1.
Bibliographic Info: Sreekanth, T. S., Hamza Varikoden, Mohan Kumar, G., Resmi, E. A. [2019]. Microphysical features of rain and rain events during different seasons over a tropical mountain location using an Optical Disdrometer. Scientific Reports, Vol. 9 (1), Art. 19083. https://doi.org/10.1038/s41598-019-55583-z
A methodology was invented to detect the unknown API gravity of oils/oils in HCFIs/oil condensates using fluid inclusion techniques coupled with microscope-based fluorescence emission spectroscopy. The API gravity (American Petroleum Institute’s gravity) is a commercial value indicator of petroleum (HCFIs). A diode laser emitting at 405 nm was used for the study. We have derived an arithmetic equation y = y0 (x0−x)t ± 1 for determining the unknown API gravity based on fluorescence emission ratio at F620/F560. With the use of a laser as an excitation source it is possible to specifically target the fluorophores that have absorption at this wavelength within the HCFIs. The precise determination of API gravity of oils in HCFIs at the time of drilling itself leads to the estimation of the quality of oils in a basin that gives an impetus for further exploration activities in petroleum industry. In general, 40% of the exploratory wells may end up as a dry well and the patented invention can help to determine the quality of minute quantities of oil detected by means of fluid inclusion studies and determination of API gravity values using a non-destructive micro-spectrometric technique could lead to further exploration in adjoining areas areas of such dry & abandoned wells...
Patentee Info: Dr. V. Nandakumar, Dr. J. L. Jayanthi
National Centre for Earth Science Studies
Patent No. 315456 dated 03/07/2019
The challenge with Raman spectral studies on natural hydrocarbon-bearing fluid inclusions (HCFIs) is the common presence of fluorescence emission from minerals and aromatic compounds in HCFIs leading to the masking of Raman signals. Selection of optimum excitation wavelength is another challenge. To overcome these hurdles, special wafer preparation techniques, along with the use of fluorescence quenchers, were employed in our study to obtain Raman signals from natural HCFIs. The present study is a demonstration of how best the Raman signals from natural hydrocarbon-bearing fluid inclusions could be detected using an excitation wavelength of 785 nm with suitable optical parameters and with special wafer preparation techniques to negate the background fluorescence. Using the laser Raman technique we were able to detect peaks corresponding to cyclohexane, benzene and bromobenzene, carbon monoxide, nitrogen, ethylene, sulphur oxide, carbonyl sulphide, hydrogen sulphide in liquid form along with the presence of a broad peak of liquid water, peaks of calcium carbonate and calcium sulphate. The chemical constituents in natural HCFIs from the same basin identified using laser Raman spectrometric methods with a 785 nm laser excitation agrees well with the GC-MS results of oil in the same basin, which again supports the utility of the laser Raman technique with 785 nm laser for the chemical constituents identification in natural HCFIs. The present study elucidates the potential of Raman spectroscopic methods using a 785 nm laser excitation for detecting the chemical constituents of HCFIs..
Bibliographic Info: JL Jayanthi, V. Nandakumar and S. S. Anoop [2017]. Feasibility of a 785 nm diode laser in Raman spectroscopy for characterizing hydrocarbon-bearing fluid inclusions in Mumbai Offshore Basin, India. Petroleum Geoscience, 23 (3), 2017, 369-375. doi: https://doi.org/10.1144/petgeo2016-071
The charnockite suites of rocks possess greater significance in addressing the processes operating at lower continental crust and, thereby, provide ample evidence to decipher the petro-tectonic evolution of the Earth’s crust. The new research findings of Ravindra Kumar and Sreejith, published in ‘Lithos’ provide a comprehensive understanding on the lower crustal processes leading to protolith diversification on the genesis of different charnockite suites of southern India. The study distinguishes three different suites of charnockites, viz., tonalitic, granitic, and augen suites based on their petrological and geochemical attributes. Further, the study envisages four-stage magmatic crustal evolution model for the Kerala Khondalite Belt (KKB), spanning from Meso- to Neoarchaean up to Mesoproterozoic. The authors propose that the onset of juvenile magmatism in the KKB was initiated by the formation of Meso- to Neoarchaean basaltic crust in an oceanic lithosphere, which underwent melting due to basaltic underplating leading to the formation of TTGs. Subsequent intra-crustal melting during a stage of arc accretion initiated differentiation of the TTG crust into tonalitic and granitic magmas during Palaeoproterozoic. The fourth stage of crustal evolution is correlated with the Mesoproterozoic emplacement of megacrystic K-feldspar granites. This novel research contribution offers an insight into the long ignored aspect of origin and evolution of orthopyroxene-bearing, felsic ortho-granulites (charnockite) of KKB and their geodynamic setting. The study also establishes fairly–well correlation between the magmatic episodes of KKB and prominent crustal growth events recorded globally. The full-article can be read online at “Lithos” journal website hosted by SciVerse ScienceDirect.
Bibliographic Info: Ravindra Kumar, G.R. and Sreejith, C., 2016. Petrology and geochemistry of charnockites (felsic ortho-granulites) from the Kerala Khondalite Belt, Southern India: Evidence for intra-crustal melting, magmatic differentiation and episodic crustal growth. Lithos, vol. 262, pp. 334-354. doi: 10.1016/j.lithos.2016.07.009
In-situ zircon U-Pb isotopic ages obtained on a garnet + cordierite bearing leucosome in migmatitic paragneiss at Kanjampara in the Trivandrum Block, demonstrate zircon crystallisation from melt at 1.92 ± 0.04 Ga. The unique trace element chemistry of the zircon, including high U/Yb, low Th/U, and flat MREE-HREE patterns with pronounced negative Eu anomalies, coupled with the presence of inclusions of sillimanite, apatite, quartz, feldspar and rare biotite in the zircon, confirms its formation as a result of anatexis associated with a high-T metamorphism at 1.92 Ga. This conclusion is supported by the local preservation of Palaeoproterozoic chemical age domains (820-860ºC. The strongly REE-P zoned garnet present in the Kanjampara leucosome, which is demonstrated to not be in HREE or Eu equilibrium with the 1.92 Ga zircon, formed as a result of anatexis and melt interaction during this Neoproterozoic-Cambrian tectonothermal event. Th-U-Pb chemical age data indicates that monazite was either formed or extensively recrystallized at during this anatexis at 565 ± 6 Ma, undergoing further modification to form high-Th cuspate rims at 517 ± 15 Ma. The age of the final monazite chemical modification is equivalent to the lower intercept age of 528 ± 18 Ma for extensive Pb-loss from the highly discordant but otherwise well-preserved Palaeoproterozoic (1.92 Ga) zircon. The growth or recrystallisation of monazite at ca. 565 Ma and its further modification at ca. 520 Ma indicates that the high-T metamorphism in the Pan-African was long-lived, with a duration of at least 45 Myr. The new age-event results from Kanjampara confirm that at least some of the metasedimentary paragneisses in the Trivandrum Block are polymetamorphic, initially metamorphosed in the Palaeoproterozoic in an event older than the 1.89-1.85 Ga granitic orthogneisses recognised from the region.