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1.
Extensive work on the palaeomagnetism of the Deccan traps by several workers has revealed only one reversal (normal-reverse-normal)
of the geomagnetic field during the period of eruption of these flows. The scatter in the natural remanent magnetic directions
of different flows in a sequence of these traps is rather large and it persists even after magnetic cleaning. Generally this
large scatter of directions is attributed to the geomagnetic secular variation during formation of the traps. Recent studies
of the magnetic properties of the trap samples indicate that the presence of multidomain magnetite in a lava sequence differs
from locality to locality in the Deccan trap province and so the stability of their natural remanent magnetization. While
these features can be clearly perceived, an understanding of the same seems to be quite difficult. However, it appears that
part of the scatter in directions could be due to the alteration of the magnetic minerals in the Deccan traps and hence it
would not be proper to relate the entire scatter to the secular variation. 相似文献
2.
R. Pandiyan S. V. Subbarao T. Nagamani Chaitra Rao N. Hari Prasad Rao Harish Joglekar Naresh Kumar Surya Ratna Prakash Dumpa Anshu Chauhan B. P. Dakshayani 《Journal of Astrophysics and Astronomy》2017,38(2):35
On 28th September 2015, India launched its first astronomical space observatory AstroSat, successfully. AstroSat carried five astronomy payloads, namely, (i) Cadmium Zinc Telluride Imager (CZTI), (ii) Large Area X-ray Proportional Counter (LAXPC), (iii) Soft X-ray Telescope (SXT), (iv) Ultra Violet Imaging Telescope (UVIT) and (v) Scanning Sky Monitor (SSM) and therefore, has the capability to observe celestial objects in multi-wavelength. Four of the payloads are co-aligned along the positive roll axis of the spacecraft and the remaining one is placed along the positive yaw axis direction. All the payloads are sensitive to bright objects and specifically, require avoiding bright Sun within a safe zone of their bore axes in orbit. Further, there are other operational constraints both from spacecraft side and payloads side which are to be strictly enforced during operations. Even on-orbit spacecraft manoeuvres are constrained to about two of the axes in order to avoid bright Sun within this safe zone and a special constrained manoeuvre is exercised during manoeuvres. The planning and scheduling of the payloads during the Performance Verification (PV) phase was carried out in semi-autonomous/manual mode and a complete automation is exercised for normal phase/Guaranteed Time Observation (GuTO) operations. The process is found to be labour intensive and several operational software tools, encompassing spacecraft sub-systems, on-orbit, domain and environmental constraints, were built-in and interacted with the scheduling tool for appropriate decision-making and science scheduling. The procedural details of the complex scheduling of a multi-wavelength astronomy space observatory and their working in PV phase and in normal/GuTO phases are presented in this paper. 相似文献
3.
Subbarao Pichuka 《水文科学杂志》2017,62(3):467-482
An attempt is made to assess the future trend of spatio-temporal variation of precipitation over a medium-sized river basin. The Statistical Downscaling Model (SDSM, version 4.2) is used to downscale the outputs from two general circulation models (GCMs) for three future epochs: epoch-1 (2011–2040), epoch-2 (2041–2070) and epoch-3 (2071–2100). Considering the Upper Mahanadi Basin as a test bed, the study results indicate a “wetter” monsoon (June–September) and the annual increase in precipitation is 12% during epoch-3, which is consistent for both GCMs. Monthly analyses indicate that the precipitation totals are likely to increase and the magnitude of increase is greater during monsoon months than non-monsoon months. The number of month-wise daily extremes increases in most months in the year. However, the maximum percentage increase (with respect to baseline period, 1971–2000) in the number of extreme events is found in the non-monsoon months (specifically before and after the monsoon). 相似文献
4.
Deformation modulus of fly ash is one of the most important mechanical properties generally used in different design problems
and also as an input parameter to sophisticated numerical techniques employed to assess the response of different structures
resting on fly ash fill or embankment made of fly ash. Deformation modulus is usually expressed in terms of compressive strength.
This paper presents the deformation modulus of fly ash modified with lime alone or in combination with gypsum at different
strain levels. The values of deformation modulus obtained from both unconfined compression test and unconsolidated undrained
triaxial test results are presented herein. The specimens for unconfined compression test and for undrained triaxial tests
were cured up to 90 and 28 days, respectively. The effects of addition of lime (4–10%) and gypsum (0.5 and 1.0%) on the deformation
modulus of class F fly ash are highlighted. With addition of lime and gypsum, the class F fly ash achieved the deformation
modulus in the range of 190 MPa in UCS test and up to 300 MPa in triaxial test specimens tested under all round pressure of
0.4 MPa. Based on the present test results empirical relationships are developed to estimate deformation modulus of modified
fly ash from unconfined compressive strength and relationships between initial tangent modulus and secant modulus at different
strain levels are also developed. 相似文献
5.
V. Bhalerao D. Bhattacharya A. Vibhute P. Pawar A. R. Rao M. K. Hingar Rakesh Khanna A. P. K. Kutty J. P. Malkar M. H. Patil Y. K. Arora S. Sinha P. Priya Essy Samuel S. Sreekumar P. Vinod N. P. S. Mithun S. V. Vadawale N. Vagshette K. H. Navalgund K. S. Sarma R. Pandiyan S. Seetha K. Subbarao 《Journal of Astrophysics and Astronomy》2017,38(2):31
The Cadmium Zinc Telluride Imager (CZTI) is a high energy, wide-field imaging instrument on AstroSat. CZTI’s namesake Cadmium Zinc Telluride detectors cover an energy range from 20 keV to \(>200\) keV, with 11% energy resolution at 60 keV. The coded aperture mask attains an angular resolution of 17\(^\prime \) over a 4.6\(^\circ \) \(\times \) 4.6\(^\circ \) (FWHM) field-of-view. CZTI functions as an open detector above 100 keV, continuously sensitive to GRBs and other transients in about 30% of the sky. The pixellated detectors are sensitive to polarization above \(\sim \)100 keV, with exciting possibilities for polarization studies of transients and bright persistent sources. In this paper, we provide details of the complete CZTI instrument, detectors, coded aperture mask, mechanical and electronic configuration, as well as data and products. 相似文献
6.
7.
K. V. Subbarao 《Contributions to Mineralogy and Petrology》1972,37(2):111-120
Strontium isotopic differences between the basalts from the East Pacific and the Chile Rises (0.7026–0.7035, average 0.7028) and abyssal hills (0.7025–0.7037, average 0.7033) suggest that these are produced from different source materials. A progressive increase of K/Rb with decrease in Sr87/Sr86 ratio is interpreted in terms of relative depletion of dispersed elements in the source materials.Institute of Marine Sciences Contribution No. 163. 相似文献
8.
Kanchan?PandeEmail author S.?K.?Pattanayak K.?V.?Subbarao P.?Navaneethakrishnan T.?R.?Venkatesan 《Journal of Earth System Science》2004,113(4):755-758
We report here a40Ar-39Ar age of 66.0 ± 0.9 Ma (2σ) for a reversely magnetised tholeiitic lava flow from the Bhimashankar Formation (Fm.), Giravali Ghat, western Deccan province,
India. This age is consistent with the view that the 1.8–2 km thick bottom part of the exposed basalt flow sequence in the
Western Ghats was extruded very close to 67.4 Ma. 相似文献
9.
S. C. Patel S. Ravi S. S. Thakur T. K. Rao K. V. Subbarao 《Mineralogy and Petrology》2006,88(1-2):363-380
Summary Mineralogical characteristics of eclogite xenoliths from three kimberlite pipes (KL2, P2 and P10) of the Proterozoic Wajrakarur
kimberlite field of southern India have been studied. In a rare sample of enstatite eclogite from the KL2 pipe garnet contains
microscopic triangular arrays of needles or blebs of omphacite, enstatite and rutile consistent with an origin by exsolution
parallel to the isometric form {111}. Discrete omphacite grains in the sample contain exsolved needles or blebs of enstatite
and garnet. Kyanite eclogites are abundant in the KL2 pipe which occasionally show a secondary ring of pure celsian around
kyanite grains. Omphacite Na2O contents in the eclogites of the KL2 and P2 pipes are typically between 3 and 6 wt%, and garnet has widely variable composition
with end member ranges of Prp22-81Grs0-47Alm10-30Sps0-1Adr0-5Uv0-3. Eclogites of the P10 pipe comprise chromian omphacite
and garnet. Phase relations in the ACF projection exhibit systematic increase of the Ca-Tschermak’s component in omphacite
from enstatite eclogite through biminerallic eclogite to kyanite eclogite. Garnet-clinopyroxene Fe–Mg geothermometry yields
temperatures mostly in the range of 900–1100 °C. A formerly supersilicic nature of garnet in enstatite eclogite as inferred
from exsolution mineralogy indicates minimum peak pressure of 5 GPa. 相似文献
10.
Y. Nagaraja Rao Y. V. Subbarao K. S. Sundara Sarma R. L. Karale K. K. Narula Naveen Kalra 《Journal of the Indian Society of Remote Sensing》1987,15(1):41-47
Maize crop was sown at weekly intervals on six dates in a randomized replicated trial under nonlimiting moisture conditions. The different dates of sowing represent different growth stages in the same given environment. Spectral data were collected using a portable radiometer at different wavelengths, ranging form visible to infrared on two different dates. The spectral reflectance data in the red and infrared region were analysed for their sensitivity to leaf area index and leaf dry biomass. During active crop growth period significant correlations existed between leaf area index and ratio of infrared to red as well as the normalized differences. Similar relationships were also observed between dry biomass and spectral data. However, these relationships were found to be valid upto the crop growth stage when the leaf area index has reached its maximum, corresponding to flowering. Beyond this stage, the spectral reflectances were found to be not related to LAI. The relsults suggest the possibility of obtaining crop phenological information from the spectral response data. 相似文献