Morphometric and rheological study of lunar domes of Marius Hills volcanic complex region using Chandrayaan-1 and recent datasets

Marius Hills volcanic complex is one of the most important regions on the lunar surface having an abundant number of volcanic features like domes and cones. Systematic mapping of 106 domes/cones in the Marius Hills region was carried out in this study using high-resolution orthoimage and digital elevation models of Chandrayaan-1 and Kaguya missions. Various morphometric parameters like diameter, height, volume, flank slope, circularity index and form factor are derived for all the mapped domes. The rheological parameters, such as viscosity and eruption rate are estimated for isolated domes and cones superimposed over low domes. The morphometric and rheological properties of these domes are comparable to those located in the area near to Hortensius crater and other mare regions. Surface ages derived for a selected region in NW portion of the Marius Hills volcanic complex using crater size-frequency distribution technique yields ages of 2.98 and 1.91 Ga. It suggests that the domes in this region formed at about 2.98 Ga ago, and then, the younger mare basalts likely embayed this region about 1.98 Ga ago. Stratigraphic sequence of rilles, wrinkle ridge and domes shows that wrinkle ridges are the oldest, while the rilles are younger than the domes.     

Matched block bootstrap for resampling multiseason hydrologic time series

A nonparametric method for resampling multiseason hydrologic time series is presented. It is based on the idea of rank matching, for simulating univariate time series with strong and/or long‐range dependence. The rank matching rule suggests concatenating with higher likelihood those blocks that match at their ends. In the proposed method, termed ‘multiseason matched block bootstrap’, nonoverlapping within‐year blocks of hydrologic data (formed from the observed time series) are conditionally resampled using the rank matching rule. The effectiveness of the method in recovering various statistical attributes, including the dependence structure from finite samples generated from a known population, is demonstrated through a two‐level hypothetical Monte Carlo simulation experiment. The method offers enough flexibility to the modeller and is shown to be appropriate for modelling hydrologic data that display strong dependence, nonlinearity and/or multimodality in the time series depicting the hydrologic process. The method is shown to be more efficient than the nonparametric ‘k‐nearest neighbor bootstrap’ method in simulating the monthly streamflows that exhibit a complex dependence structure and bimodal marginal probability density. Even with short block sizes, this bootstrap method is able to predict the drought characteristics reasonably accurately. Copyright © 2005 John Wiley & Sons, Ltd.     

Identifying and linking source areas of flow and P transport in dairy‐grazed headwater catchments,North Island,New Zealand

We examined the applicability of the critical‐source area (CSA) concept to the dairy‐grazed 192‐ha Upper Toenepi catchment and its 8·7‐ha Kiwitahi sub‐catchment, New Zealand. We evaluated if phosphorus (P) transport from land into stream is dominated by saturation‐excess (SE) and infiltration‐excess (IE) runoff during stormflow and by sub‐surface (<1·5 m depth) flows during baseflow. We measured stream flow and shallow groundwater levels, collected monthly stream, tile drain (TDA) and groundwater samples, and flow‐proportional stream samples from the Kiwitahi sub‐catchment, and determined their dissolved reactive phosphorus (DRP) and total phosphorus (TP) concentrations. In the Kiwitahi sub‐catchment, during storm events, IE contributions were significant. Contributions from SE appeared significant in the Upper Toenepi catchment. However, in both catchments, sub‐surface contributions dominated stormflow and baseflow periods. Absence of water table at the surface and the water table gradient towards the stream indicated that P transport during events was not limited to surface runoff. The dynamics of the groundwater table and the occurrence of SE areas were influenced by proximity to the stream and hillslope positions. Baseflow accounted for 42% of the annual flow in the Kiwitahi sub‐catchment, and contributed 37 and 52% to the DRP and TP loads, respectively. The P transport during baseflow appeared equally important as P losses from CSAs during stormflow. The close resemblance in P levels between groundwater and stream samples during baseflow demonstrates the importance of shallow groundwater for stream flow. In the Upper Toenepi catchment, contributions from effluent ponds (EFFs) dominated P loads. Management strategies should focus on controlling P release from EFFs, and on decreasing Olsen P concentrations in soil to minimize leaching of P via sub‐surface flow to streams. Research is needed to quantify the role of sub‐surface flow as well as to expand management strategies to minimize P transfers during stormflow and baseflow conditions. Copyright © 2010 John Wiley & Sons, Ltd.     

Very high 18o enrichment in Archean cherts from South India: implications for Archean ocean temperature

Stable carbon and oxygen isotopic compositions of essentially unmetamorphosed Archean (> 2.6 Gyr old) cherts and carbonates of the Dharwar Sequence of southern India, from the northernmost part of the Dharwar-Shimoga supracrustal belt (Kalche and Nagargali), have been determined. The cherts from the Nagargali area, which preserve oolitic texture and cryptocrystalline silica, show highly enriched δ¹⁸O values ranging from 28 to 31.4%o relative to SMOW. Such values are the highest yet reported from Archean nondetrital sediments, but are similar to those of modern marine cherts. On the assumption of a seawater δ¹⁸O of 0%₀, calculation of temperature based on the maximum δ¹⁸O value of 31.4%₀ yields a value of 40°C. This is significantly less than 70–80°C reported for the Archean oceans based on cherts and chert-phosphate pairs. Diagenetically recrystallized microcrystalline chert-dolomite pairs of Kalche area exhibit a range of oxygen isotopic ratios similar to those reported for Archean cherts and carbonates from other parts of the world. The temperature of diagenesis is estimated to be about 68°C.     

Short note: Applications of third-order statistics for the automatic time picking of seismic events

We present a new automatic time-picking method based on third-order statistics, namely bicoherence correlation. Contrary to conventional methods, which are based on second-order statistics (i.e. cross-correlation or neural-network trainings), our method is less sensitive to coloured noise as well as the bandwidth of the signal. Bicoherence correlation can also be used for autotracking events in seismic data for an interpretation.     

The evolution of Indian summer monsoon in 1997 and 1983

Summary During most El-Ni?o events the Indian summer monsoon rainfall has been below normal. El-Ni?o that occurred during 1997 was one of the strongest in the 20th century, but did not have an adverse impact on the Indian summer monsoon rainfall in 1997. This is despite the fact that most parameters observed in May 1997 suggested that the Indian summer monsoon rainfall may be below normal. This intriguing feature of the 1997 Indian summer monsoon rainfall has been examined by studying the evolution of various parameters from May to August. The behavior of the 1997 monsoon is related to its evolution during June and July, with westward migration of cloudbands from West Pacific that increased convection over Bay of Bengal. We find that there exists a significant correlation between convective activity over Bay of Bengal and winds over the Arabian Sea with the latter lagging convection over Bay of Bengal by about three days. The convective activity over Bay of Bengal induces stronger winds over the Arabian Sea and this in turn enhances advection of moisture into the Indian landmass and leads to increased precipitable water and strength of the monsoon. Using a simple thermodynamic model we show that increased precipitable water during July leads to increased rainfall. A similar behavior has also been noticed during the 1983 monsoon, with precursors indicating a possible poor monsoon but subsequent events changed the course of the monsoon. Received May 21, 2001 Revised October 10, 2001     

The interstellar clouds of adams and blaauw revisited: An HI absorption study-II

In the preceding paper (Paper I), we presented HI absorption spectra towards radio sources very close to the lines of sight towards twenty five bright stars against which optical absorption spectra had been obtained earlier, In this paper we analyse the results and draw some conclusions. To summarize briefly, in most cases we found HI absorption at velocities corresponding to the optical absorption features provided one restricted oneself to velocities ≲10 kms-1. At higher velocities we did not detect any HI absorption down to an optical depth limit of 0.1 (except in four cases which we attribute to gas in systematic motion rather than clouds in random motion). After discussing various scenarios, we suggest that this trend should perhaps be understood in terms of the high velocity interstellar clouds being accelerated, heated and ablated by expanding supernova remnants.     

The interstellar clouds of adams and blaauw revisited: An HI absorption study-I

This investigation is aimed at clarifying the nature of the interstellar gas seen in absorption against bright O and B stars. Towards this end we have obtained for the first time HI absorption spectra towards radio sources very close to the lines of sight towards twenty five bright stars previously studied. In this paper we describe the selection criteria, the details regarding our observations, and finally present the absorption spectra. In the accompanying paper we analyse the results and draw conclusions.     

Structural evolution of the Peninsular Gneiss — an early Precambrian migmatitic complex from South India

The Peninsular Gneiss, which is considered by a number of workers to be the basement on which the supracrustal rocks of the Dharwar Group were deposited, is a composite gneiss formed by migmatization of pre-existing metasedimentary and meta-igneous rocks. These gneisses show the same style and sequence of superposed deformation as those in the enclaves of metamorphic rocks and in the linear Dharwar schist belts outside. The main migmatization is broadly coeval with the isoclinal first folding, which is followed by near-coaxial refolding and non-coaxial upright folding. Small inclusions of migmatized amphibolite and granodioritic to dioritic gneiss, with a fabric athwart to, and overprinted by, the earliest deformation affecting the Dharwar Group of rocks in a large part of the gneissic terrane, point to at least one deformation, a metamorphic event and one episode of migmatization antedating the isoclinal first folds in the rocks of the Dharwar Group. The Peninsular Gneiss in its present state, therefore, represents an extensively remobilized basement.

---

Zusammenfassung Der Peninsula-Gneis, der von einigen Bearbeitern als das Basement angesehen wird, auf dem die Gesteine der Dharwar-Gruppe abgelagert wurden, ist ein Migmatit aus Komponenten älterer metamorpher Sedimentgesteine und Magmatite. Abfolge der Deformation und Deformationsart dieser Gneise entspricht der Deformation des Dharwar Schiefergürtels. Die Hauptmigmatisierung verlief zeitgleich mit der isoklinalen ersten Faltung, die von einer zweiten fast coaxialen und einer dritten aufrecht coaxialen Faltung gefolgt wird. Es existieren Einschlüsse migmatisierten Amphibolits und granodioritischen bis dioritischen Gneises, deren Gefüge auf die älteste die Dharwar-Gruppe beeinflussenden Deformation zurückgeführt wird. Diese Beobachtungen sprechen für mindestens eine Deformation, eine Metamorphose und eine Migmatisierungsphase, die älter sind als die isoklinalen Falten der ersten Generation der Dharwar-Gruppe. Nach heutigen Erkenntnissen stellt also der Peninsular-Gneis ein intensiv durchbewegtes Basement dar.

---

Résumé La formation des «Peninsular Gneiss» est considérée par de nombreux auteurs comme le socle sur lequel se sont déposées les roches supracrustales du Groupe de Dharwar. Il s'agit de gneiss composites formés par migmatitisation de roches méta-sédimentaires et méta-ignées préexistantes. Ces gneiss présentent le même style de déformation et la même succession de déformations superposées que la ceinture des schistes de Dharwar. La migmatitisation est contemporaine d'un premier plissement isoclinal, qui a été suivi d'un deuxième plissement sensiblement coaxial et d'une troisième déformation en plis droits non coaxiaux. Il existe toutefois des inclusions d'amphibolites migmatitiques et de gneiss granodioritiques à dioritiques dont la structure, transverse à la déformation la plus ancienne du Groupe de Dharwar, est remaniée par celleci. Ces observations plaident en faveur de l'existence d'au moins une phase de déformation, de métamorphisme et de migmatitisation antérieure aux plis isoclinaux de première génération du Groupe de Dharwar. A la lumière des connaissances actuelles, les Peninsular Gneiss apparaissent ainsi comme un socle polycyclique intensément remanié.

---

, , Dharwar, . Dharwar. , , - - , - . , Dharwar. , , , , , Dharwar. , .