Institution
Vikram Sarabhai Space Centre
Facility•Thiruvananthapuram, India•
About: Vikram Sarabhai Space Centre is a facility organization based out in Thiruvananthapuram, India. It is known for research contribution in the topics: Aerosol & Ultimate tensile strength. The organization has 2092 authors who have published 3058 publications receiving 47975 citations. The organization is also known as: VSSC.
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TL;DR: In this paper, the authors investigated the postbuckling behavior of shear deformable laminated composite plates by employing a four-node rectangular C(sup 1) continuous finite element.
Abstract: Thermal buckling and postbuckling behavior of shear deformable laminated composite plates is investigated by employing a four-node rectangular C(sup 1) continuous finite element. The investigation reveals that the postbuckling path may not remain stable throughout. It is shown that secondary instabilities coupled with changes in the spatial deformation do take place from the postbuckling path. 15 refs.
53 citations
TL;DR: In this paper, the authors present the results of a spectral study of the soft X-ray emission from low-latitude (disk) regions of Jupiter, obtained during two observing campaigns with XMM-Newton in April and November 2003.
53 citations
TL;DR: This study clearly demonstrates the applicability of Taguchi method to capture the essential Monte-Carlo simulation results in the stage separation process.
53 citations
TL;DR: In this article, an empirical model of the energy spectra for hydrogen NEs backscattered from the lunar surface based on Chandrayaan-1 Energetic Neutral Atom (CENA) observations is presented.
Abstract: [1] We present an empirical model of the energy spectra for hydrogen energetic neutral atoms (ENA) backscattered from the lunar surface based on Chandrayaan-1 Energetic Neutral Atom (CENA) observations The observed energy spectra of the backscattered ENAs are well reproduced by Maxwell-Boltzmann distribution functions The backscatter fraction is constant and independent of any solar wind parameters and the impinging solar wind angle The calculated backscatter fraction is 019, and the 25% and 75% percentiles are 016 and 021 The empirical parameters of the Maxwell-Boltzman distribution derived from the CENA imager have no correlations with the upstream solar wind parameters, except for a good correlation between the solar wind velocity and the temperature of the backscattered ENAs These results suggest that the reflected ENAs have experienced several collisions during the interaction with the loose lunar grains, and are then released into space The mathematical model of the energy spectra of the backscattered ENAs is expressed by a function of the solar wind flux and velocity, which can be used for future investigations of regolith-solar wind interaction
53 citations
TL;DR: In this paper, two closed-form solutions for boundary layer equations of the title problem were found, and discussions were made to trace among them the physically realistic solution, which was shown to be the best solution.
Abstract: Two closed-form solutions were found for the boundary layer equations of the title problem. Discussions are made to trace among them the physically realistic solution.
52 citations
Authors
Showing all 2111 results
| Name | H-index | Papers | Citations |
|---|---|---|---|
| M. Santosh | 103 | 1344 | 49846 |
| Sabu Thomas | 102 | 1554 | 51366 |
| S. Suresh Babu | 70 | 498 | 17113 |
| K. Krishna Moorthy | 54 | 263 | 9749 |
| Sathianeson Satheesh | 53 | 172 | 11099 |
| M. Y. Hussaini | 49 | 207 | 16794 |
| J.R. Banerjee | 44 | 146 | 5620 |
| C. P. Reghunadhan Nair | 37 | 181 | 4825 |
| K. N. Ninan | 36 | 159 | 4156 |
| Anil Bhardwaj | 35 | 230 | 4527 |
| Ivatury S. Raju | 33 | 121 | 6626 |
| Venkata Sai Kiran Chakravadhanula | 32 | 102 | 3011 |
| P.K. Sinha | 32 | 118 | 2918 |
| J.-P. St.-Maurice | 31 | 113 | 3446 |
| Subramaniam Gopalakrishnan | 28 | 123 | 2951 |