A high speed near infrared photometer for lunar occultation studies     

Ashok  N. M.  Chandrasekhar  T.  Ragland  Sam  Bhatt  H. C. 《Experimental Astronomy》1994,4(3-4):177-188

A recently developed near infrared high speed photometer intended for lunar oc-cultation studies is described. The primary scientific objective is to reach milli arc second levels of angular resolution so that circumstellar structure of the occulted sources can be resolved. Near infrared sky brightness close to the lunar limb is also studied. Angular diameter derived from the observed occultation of IRC +20169 is presented and system performance discussed.  相似文献   

Optical interferometric observations of a transient event of 1986 March 13 in the coma of Comet Halley     

C. Debi Prasad  T. Chandrasekhar  J. N. Desai  N. M. Ashok  Vinod Krishan 《Journal of Astrophysics and Astronomy》1989,10(1):1-20

During the recent apparition of Comet Halley in 1985-86 a transient ionic event in the form of a blob of H₂ O⁺ emission was recorded in thecoma at ～ 0^h UT on 1986 March 13. Observations were carried out using a special IHW filter for H₂ O⁺ emission at 7000 å/175 å, a 35 cm telescope, a Fabry-Perot interferometer and an image intensifier camera from Gurushikhar, Mt Abu. (24?39’N,72? 47’E). A Fabry-Perot inter-ferogram in Ha taken a few minutes later at the same location reveals strong hydrogen emission (Hα) associated with the blob. The velocity field in the blob is structured with relative velocities upto ～ 35km s^?1. The event is interpreted as arising due to the sector boundary crossing of the interplanetary magnetic field by the comet  相似文献   

Near-infrared observations of the peculiar binary system epsilon Aurigae     

H. C. Bhatt  T. Chandrasekhar  N. M. Ashok  J. N. Desai 《Astrophysics and Space Science》1984,104(2):293-296

Near-infrared photometric and low-resolution spectroscopic observations of Aurigae at two phases during the current eclipse are presented. The eclipse depths are found to be wavelength-independent in the infrared right up to 2.5 m. There is no infrared excess at wavelengths shorter than 2.5 m. The light absorbing particles in the eclipsing body must be larger than 10 m in size.  相似文献   

Geothermal energy potential of Tulsishyam thermal springs of Gujarat,India     

Hemant Kumar Singh  Aswathi Thankappan  Poonam Mohite  Satish Kumar Sinha  Dornadula Chandrasekharam  Trupti Chandrasekhar 《Arabian Journal of Geosciences》2018,11(6):137

Tulsishyam thermal springs are located in the Saurashtra region of Gujarat, India with discharge temperatures varying from 39 to 42 °C. The pH of these thermal springs varies from 7.1 to 7.4, indicating neutral character. Though these thermal springs propagate through the near surface layer of Deccan basalt, detailed geochemical analysis of the thermal waters using Piper diagram suggests that the water is interacting with the granitic basement rock. Silica and cation geothermometry estimates have reservoir temperature in the range of 138 to 207 °C categorizing it into a low to moderate enthalpy geothermal system. Furthermore, the area has high heat flow values of 53–90 mW/m² because of shallow Moho depth. The prevailing conditions suggest that the geothermal energy can potentially be exploited through an enhanced geothermal system (EGS). The study also indicates different mineral phases that may precipitate out of water during exploitation of geothermal energy and it should be taken into account while designing an EGS for the area.  相似文献   

Wind gradients at meteor heights over mid-latitude stations     

P. C. S. Devara  G. Chandrasekhar  M. I. Ahmed 《Journal of Earth System Science》1986,95(3):427-434

The gradients of amplitude and phase of diurnal and semidiurnal components of zonal and meridional winds in the height intervals of 80–90 km and 90–100 km are studied using the meteor wind radar data collected at Atlanta (34°N, 84°W) during the period August 1974–March 1978. The results are compared with those at Adelaide (35°S, 139°E). It is found that the gradients vary in an opposite manner between the two height intervals.  相似文献   

Infrared Observations of Comet Hale–Bopp (C/1995 O1) from Gurushikhar Observatory     

Chandrasekhar  T.  Ashok  N. M.  Tej  Anandamayee  Mondal  Soumen  Watson  P. V. 《Earth, Moon, and Planets》1998,81(2):111-121

During the recent apparition of comet Hale—Bopp (1995 O1) near infrared photometric observations were carried out in the J, H, K filter bands and also in the 3.0—3.4 μm region at the 1.2 m telescope at Gurushikkar, India. The effective temperature of the comet was substantially higher than the equilibrium blackbody temperature. A mean superheat value of 1.83 was derived in the post-perihelion phase which implies that a large fraction of the grain population are made up of small and hot grains with radii <0.5 μm. High albedo values of ∼0.4 were also derived in the scattering angle range 135° to 160° which could explain the unusual brightness of comet Hale—Bopp. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

印度遥感展望     

Chan.  MG 陈虹 《测绘通报》1998,(1):41-43

本文主要论述印度１９９５年底以来遥感卫星发射和应用的情况,提出了到２００５年的连续性十年规划和任务为完成任务而采取的战略措施,同时,对未来的卫星功能及人类需求进行了全面分析和展望,并分析由此而带来的对应用领域的拓展。  相似文献   

The excitation mechanism of [Fe XIV] 5303 å line in the inner regions of solar corona     

K. P .Raju  J. N. Desai  T. Chandrasekhar  N. M. Ashok 《Journal of Astrophysics and Astronomy》1991,12(4):311-317

The line intensity of the green coronal line and the continuum intensity are derived from the filter and white light photographs of the solar corona obtained during the 1980 total solar eclipse. Ratio of the line to continuum intensity is plotted against the radial distancer(=R/R₀,R ₀ is the solar radius), in various position angles. A simple model assuming an electron density dependence of the line and continuum intensities suggests a dominant collisional mechanism for the excitation of the line in the innermost regions (～ 1.4R ₀). The measured line to continuum ratio tends to a constant value at different radial distances in different position angles. The constancy of the measured line to continuum ratio indicates significant radiative excitation beyond 1.4 R₀, in some of the position angles.  相似文献   

Dust structure around the Wolf–Rayet star WR104 from lunar occultation observations at 2.2 μm     

Soumen Mondal  T. Chandrasekhar 《Monthly notices of the Royal Astronomical Society》2002,334(1):143-148

A rare opportunity of observing a lunar occultation of a Wolf–Rayet star (WR104) in the near-infrared K band (2.2 μm) was utilized to probe the thick dust envelope surrounding the star at a high one-dimensional angular resolution (∼2 mas). Analysis of the occultation light curve shows a dust structure departing significantly from the uniform disc profile. Our results are in good agreement with recent aperture-masking interferometry carried out at the Keck I telescope, which shows a pinwheel structure around WR104. We report additional fine structures in the dust envelope.  相似文献   

Doppler shift measurements on the green coronal line—evidence for largescale macroscopic mass motion     

J. N. Desai  T. Chandrasekhar  P. D. Angreji 《Journal of Astrophysics and Astronomy》1982,3(1):69-77

Fabry-Perot interferometric observations on the green coronal line (λ 5303 å) carried out during the total solar eclipse of 1980 February 16 have yielded relative Doppler shift velocities with an accuracy of ± 7 km s^-1. The values show a peak in the 30–50 km s^-1 range indicating largescale macroscopic mass motion in the solar maximum corona.  相似文献