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Institution

Cochin University of Science and Technology

EducationKochi, Kerala, India
About: Cochin University of Science and Technology is a education organization based out in Kochi, Kerala, India. It is known for research contribution in the topics: Thin film & Natural rubber. The organization has 5382 authors who have published 7690 publications receiving 103827 citations. The organization is also known as: CUSAT & Cochin University.


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Journal ArticleDOI
TL;DR: The strong cross-equatorial low level jet stream (LLJ) with its core around 850 hPa of the Asian summer monsoon (June-September) is found to have large intraseasonal variability.
Abstract: The strong cross-equatorial low level jet stream (LLJ) with its core around 850 hPa of the Asian summer monsoon (June–September) is found to have large intraseasonal variability. During the monsoon onset over Kerala, India, and during break monsoon periods, when the convective heating of the atmosphere is over the low latitudes of the Indian Ocean, the axis of the LLJ is oriented southeastward over the eastern Arabian Sea and it flows east between Sri Lanka and the equator and there is no LLJ through peninsular India. This affects the transport of moisture produced over the Indian Ocean to peninsular India and the Bay of Bengal. In contrast, during active monsoon periods when there is an east–west band of strong convective heating in the latitudes 10°–20°N from about longitude 70° to about 120°E, the LLJ axis passes from the central Arabian Sea eastward through peninsular India and it provides moisture for the increased convection in the Bay of Bengal and for the monsoon depressions forming there...

261 citations

Journal ArticleDOI
Yousef Abou El-Neaj1, Cristiano Alpigiani2, Sana Amairi-Pyka3, Henrique Araujo4, Antun Balaž5, Angelo Bassi6, Lars Bathe-Peters7, Baptiste Battelier8, Aleksandar Belić5, Elliot Bentine9, Jose Bernabeu10, Andrea Bertoldi8, Robert Bingham11, Robert Bingham12, Diego Blas13, Vasiliki Bolpasi14, Kai Bongs15, Sougato Bose16, Philippe Bouyer8, T. J. V. Bowcock17, William B. Bowden18, Oliver Buchmueller4, Clare Burrage19, Xavier Calmet20, Benjamin Canuel8, Laurentiu Ioan Caramete, Andrew Carroll17, Giancarlo Cella6, Vassilis Charmandaris14, S. Chattopadhyay21, S. Chattopadhyay22, Xuzong Chen23, Maria Luisa Chiofalo24, J. P. Coleman17, J. P. Cotter4, Y. Cui25, Andrei Derevianko26, Albert De Roeck27, Goran S. Djordjevic28, P. J. Dornan4, Michael Doser27, Ioannis Drougkakis14, Jacob Dunningham20, Ioana Dutan, Sajan Easo12, G. Elertas17, John Ellis13, John Ellis29, John Ellis27, Mai El Sawy30, Mai El Sawy31, Farida Fassi, D. Felea, Chen Hao Feng8, R. L. Flack16, Christopher J. Foot9, Ivette Fuentes19, Naceur Gaaloul32, A. Gauguet33, Remi Geiger34, Valerie Gibson35, Gian F. Giudice27, J. Goldwin15, O. A. Grachov36, Peter W. Graham37, Dario Grasso24, Maurits van der Grinten12, Mustafa Gündoğan3, Martin G. Haehnelt35, Tiffany Harte35, Aurélien Hees34, Richard Hobson18, Jason M. Hogan37, Bodil Holst38, Michael Holynski15, Mark A. Kasevich37, Bradley J. Kavanagh39, Wolf von Klitzing14, Tim Kovachy40, Benjamin Krikler41, Markus Krutzik3, Marek Lewicki42, Marek Lewicki13, Yu-Hung Lien16, Miaoyuan Liu23, Giuseppe Gaetano Luciano6, Alain Magnon43, Mohammed Mahmoud44, Sudhir Malik4, Christopher McCabe13, J. W. Mitchell21, Julia Pahl3, Debapriya Pal14, Saurabh Pandey14, Dimitris G. Papazoglou45, Mauro Paternostro46, Bjoern Penning47, Achim Peters3, Marco Prevedelli48, Vishnupriya Puthiya-Veettil49, J. J. Quenby4, Ernst M. Rasel32, Sean Ravenhall9, Jack Ringwood17, Albert Roura50, D. O. Sabulsky8, M. Sameed51, Ben Sauer4, Stefan A. Schäffer52, Stephan Schiller53, Vladimir Schkolnik3, Dennis Schlippert32, Christian Schubert32, Haifa Rejeb Sfar, Armin Shayeghi54, Ian Shipsey9, Carla Signorini24, Yeshpal Singh15, Marcelle Soares-Santos47, Fiodor Sorrentino6, T. J. Sumner4, Konstantinos Tassis14, S. Tentindo55, Guglielmo M. Tino56, Guglielmo M. Tino6, Jonathan N. Tinsley56, James Unwin57, Tristan Valenzuela12, Georgios Vasilakis14, Ville Vaskonen13, Ville Vaskonen29, Christian Vogt58, Alex Webber-Date17, André Wenzlawski59, Patrick Windpassinger59, Marian Woltmann58, Efe Yazgan60, Ming Sheng Zhan60, Xinhao Zou8, Jure Zupan61 
Harvard University1, University of Washington2, Humboldt University of Berlin3, Imperial College London4, University of Belgrade5, Istituto Nazionale di Fisica Nucleare6, Technical University of Berlin7, University of Bordeaux8, University of Oxford9, University of Valencia10, University of Strathclyde11, Rutherford Appleton Laboratory12, King's College London13, Foundation for Research & Technology – Hellas14, University of Birmingham15, University College London16, University of Liverpool17, National Physical Laboratory18, University of Nottingham19, University of Sussex20, Northern Illinois University21, Fermilab22, Peking University23, University of Pisa24, University of California, Riverside25, University of Nevada, Reno26, CERN27, University of Niš28, National Institute of Chemical Physics and Biophysics29, Beni-Suef University30, British University in Egypt31, Leibniz University of Hanover32, Paul Sabatier University33, University of Paris34, University of Cambridge35, Wayne State University36, Stanford University37, University of Bergen38, University of Amsterdam39, Northwestern University40, University of Bristol41, University of Warsaw42, University of Illinois at Urbana–Champaign43, Fayoum University44, University of Crete45, Queen's University Belfast46, Brandeis University47, University of Bologna48, Cochin University of Science and Technology49, German Aerospace Center50, University of Manchester51, University of Copenhagen52, University of Düsseldorf53, University of Vienna54, Florida State University55, University of Florence56, University of Illinois at Chicago57, University of Bremen58, University of Mainz59, Chinese Academy of Sciences60, University of Cincinnati61
TL;DR: The Atomic Experiment for Dark Matter and Gravity Exploration (AEDGE) as mentioned in this paper is a space experiment using cold atoms to search for ultra-light dark matter, and to detect gravitational waves in the frequency range between the most sensitive ranges of LISA and the terrestrial LIGO/Virgo/KAGRA/INDIGO experiments.
Abstract: We propose in this White Paper a concept for a space experiment using cold atoms to search for ultra-light dark matter, and to detect gravitational waves in the frequency range between the most sensitive ranges of LISA and the terrestrial LIGO/Virgo/KAGRA/INDIGO experiments. This interdisciplinary experiment, called Atomic Experiment for Dark Matter and Gravity Exploration (AEDGE), will also complement other planned searches for dark matter, and exploit synergies with other gravitational wave detectors. We give examples of the extended range of sensitivity to ultra-light dark matter offered by AEDGE, and how its gravitational-wave measurements could explore the assembly of super-massive black holes, first-order phase transitions in the early universe and cosmic strings. AEDGE will be based upon technologies now being developed for terrestrial experiments using cold atoms, and will benefit from the space experience obtained with, e.g., LISA and cold atom experiments in microgravity.

259 citations

Journal ArticleDOI
TL;DR: In this paper, the influence of aggregate content on the engineering properties of geopolymer concrete has been investigated and it has been concluded that a geopolymers concrete with proper proportioning of total aggregate content and ratio of fine aggregate to total aggregate, along with the optimum values of other parameters, can have better engineering properties than the corresponding properties of ordinary cement concrete.

259 citations

Journal ArticleDOI
TL;DR: In this paper, the authors present results from sun/sky radiometer measurements of aerosol optical characteristics carried out in New Delhi during March-June, 2006, as part of the Indian Space Research Organization's Integrated Campaign for Aerosol Radiation Budget.
Abstract: [1] We present results from sun/sky radiometer measurements of aerosol optical characteristics carried out in New Delhi during March–June, 2006, as part of the Indian Space Research Organization's Integrated Campaign for Aerosol Radiation Budget. For the first time at this site, derived are parameters such as aerosol optical depth (AOD), single scattering albedo (SSA), asymmetry parameter, Angstrom exponent, and real and imaginary refractive indices in five spectral channels. During the campaign, a consistent increase in aerosol loading from March to June with monthly average AOD values at 0.5μm of 0.55, 0.75, 1.22 and 1.18, respectively, was observed. Angstrom exponent gradually decreases from 1.28 (March) to 0.47 (June), indicating an increased abundance of coarse particles due to dust storms that transport desert dust from the Thar desert and adjoining regions. SSA at 0.5 μm is found to be in the range of 0.84 to 0.74 from March to June, indicating an increasing contribution from the mixture of anthropogenic and desert dust absorbing aerosols. Optical properties derived during the campaign are used in a radiative-transfer model to estimate aerosol radiative forcing at the surface and at the top-of-the atmosphere. A consistent increase in surface cooling is evident, ranging from −39 W m−2 (March) to −99 W m−2 (June) and an increase in heating of the atmosphere from 27 W m−2 (March) to 123 W m−2 (June). Heating rates in the lower atmosphere (up to 5 km) are 0.6, 1.3, 2.1, and 2.5K/d from March, April, May, and June 2006, respectively. Higher aerosol induced heating in the premonsoon period has been shown to have an impact on the regional monsoon climate.

250 citations

Journal ArticleDOI
P. Adamson1, C. Ader1, M. P. Andrews1, N. Anfimov2  +255 moreInstitutions (38)
TL;DR: The first search for ν_{μ}→ν_{e} transitions by the NOvA experiment finds 6 events in the Far Detector, compared to a background expectation of 0.99±0.11(syst) events based on the Near Detector measurement.
Abstract: We report results from the first search for ν_{μ}→ν_{e} transitions by the NOvA experiment. In an exposure equivalent to 2.74×10^{20} protons on target in the upgraded NuMI beam at Fermilab, we observe 6 events in the Far Detector, compared to a background expectation of 0.99±0.11(syst) events based on the Near Detector measurement. A secondary analysis observes 11 events with a background of 1.07±0.14(syst). The 3.3σ excess of events observed in the primary analysis disfavors 0.1π<δ_{CP}<0.5π in the inverted mass hierarchy at the 90% C.L.

242 citations


Authors

Showing all 5433 results

NameH-indexPapersCitations
Pulickel M. Ajayan1761223136241
Maxime Dougados134105469979
Sabu Thomas102155451366
Philippe Ravaud10161841409
David P. Salmon9941943935
Jérôme Bertherat8543824794
Luc Mouthon8456426238
Xavier Bertagna7428518738
Alfred Mahr7322922581
Nicolas Roche7262922845
Charles Chapron7137818048
Benoit Terris6123413353
François Goffinet6053214433
Xavier Puéchal6031613240
Pascal Laugier5848210518
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
202318
2022106
2021753
2020613
2019503
2018439