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IUCAA Bulletin 2016
Editor : Editorial Assistant : Somak Raychaudhury Manjiri Mahabal ([email protected]) ([email protected]) A quarterly bulletin of the Inter-University Centre for Astronomy and Astrophysics ISSN 0972-7647 (An autonomous institution of the University Grants Commission) Available online at http://ojs.iucaa.ernet.in/ 27th IUCAA Foundation Day Lecture Introduction A Natural History of The 27th IUCAA Foundation Day Knowledge Lecture was delivered by the eminent A naturalist lives today in a world of Indian ecologist, Professor Madhav wounds, but for a connoisseur of Gadgil on December 29, 2015. Over a knowledge, ours is a golden age; the career spanning more than four decades, challenge before us is to deploy the strengths Professor Gadgil has championed the of our age to heal the wounds. Life is an effort towards the preservation of information-based, progressive and ecology in India, which includes cooperative enterprise, evolving organisms establishing the Centre for Ecological capable of handling greater and greater Sciences under the aegis of the Indian quantities, of increasingly more complex Institute of Science, Bengaluru in 1983 information, ever more effectively. Social and serving as the Head of the Western animals have taken this to new heights, with be unhappy in this as well as the nether Ghats Ecology Expert Panel of 2010, humans surpassing them, all thanks to the world. The ruling classes have always tried popularly known as the Gadgil language abilities, and the greatly enhanced to keep the populace ignorant as preached Commission. An alumnus of Harvard capacity to learn, teach, and to elaborate by Laozi, a contemporary of Buddha: The University, he is a recipient of the Padma memes, including mythologies and people are hard to rule when they have too Shri and Padma Bhushan from the scientific knowledge. -
Probing the Universe at Low Radio Frequencies Using the GMRT
The GMRT : a look at the Past, Present and Future Yashwant Gupta & Govind Swarup National Centre for Radio Astrophysics Pune India URSI GASS Montreal 2017 The GMRT : a look at the Past, Present and Future Yashwant Gupta & Govind Swarup National Centre for Radio Astrophysics Pune India URSI GASS Montreal 2017 Overview of today’s talk . Part I : the GMRT -- a historical perspective . Part II : the GMRT -- current status . Part III : future -- the upgraded GMRT Some history . It is the early 1980s… the VLA has recently become operational . Radio astronomy has shifted from the low frequencies, where it was born, to higher frequencies (cm and higher wavelengths) -- obvious reasons . Note, however, techniques like self-cal have been shown to work . In India, the radio astronomy group at the Tata Institute, under the leadership of Govind Swarup, is looking for the next big challenge… They have already : . Built the Ooty Radio Telescope in the late 1960s – still operational & producing international quality results (in fact, currently being upgraded with new receiver system!) . Built the Ooty Synthesis Radio Telescope (1980s) – short-lived but valuable learnings . Built up considerable experience in low frequencies (metre wavelengths) Birth of the GMRT . Motivation : bridge the gap in radio astronomy facilities at low frequencies and address science problems best studied at metre wavelengths . First concept : 1984 (started with large cylinders); evolved to 34 dishes of 45 metres by 1986 . Project cleared and funding secured by 1987 . Construction started : 1990; first antenna erected : 1992 . First light observations : 1997 – 1998 . Released for world-wide use : 2002 The GMRT : turning it ON Jan 1997 : First fringes with the prototype GMRT correlator Dec 1998 : first light pulsar observation with the GMRT Dedication of the GMRT The Giant Metrewave Radio Telescope was dedicated to the World Scientific Community by the Chairman of TIFR Council, Shri Ratan Tata. -
Prime Minister Dr Manmohan Singh Gives Away
ISSN 0409-7467 VOL 59 NO 1 15 JANUARY 2009 Prime Minister Dr Manmohan Singh gives away Shanti Swarup Bhatnagar Prizes for 2007 & 2008, CSIR Diamond Jubilee Technology Award for 2007 and CSIR Award for S&T Innovation for Rural Development for 2007 & 2008 Seen on the dais at the CSIR Award Presentation Function: Prime Minister Dr Manmohan Singh (centre), Minister for Science & Technology and Earth Sciences and Vice President, CSIR, Shri Kapil Sibal (left ) and Director General, CSIR, Prof. Samir K. Brahmachari Prime Minister of India and President, CSIR, Dr Manmohan Singh, gave away Shanti Swarup Bhatnagar Prizes for 2007 & 2008. CSIR Diamond Jubilee Technology Award for 2007 and CSIR Award for S&T Innovation for Rural Development for 2007 & 2008, at a glittering function held on 20 December 2008 in the Dr D.S. Kothari Auditorium, DRDO Bhawan, New Delhi. Attended by a galaxy of S&T personnel, the function was presided over by Shri Kapil Sibal, Minister for Science & Technology and Earth Sciences and Vice President, CSIR. Prof Samir K. Brahmachari, Director General, CSIR, proposed a vote of thanks. We bring in this issue, speeches of Dr Manmohan Singh, Shri Kapil Sibal and Prof. Brahmachari on the occasion along with the citations of the prize-winners. 15 JANUARY 2009 1 CSIR Award Function Speech of Prime Minister Dr Manmohan Singh am very pleased to be here in laboratories.” Iyour midst today to give away the It is this energy and this Shanti Swarup Bhatnagar Prizes for enthusiasm of our scientists that we the years 2007 & 2008. I honour and celebrate each year on congratulate each one of the award such events. -
00224Notice 10212019.Pdf
District-Gorakhpur, College Name-MADAN MOHAN MALAVIYA UNIVERSITY OF TECHNOLOGY, GORAKHPUR, Postmatric 2019-20 (Fresh) ALL Application For Session 2019-20 as on 18- 10-2019 Serial No.Registration No Name Father Name Date Of Birth Caste Course Course Branch YearType Student TypeClaim FeesStatus 1 580380501901323 AASHISH KUMAR MISHRA RAVI PRAKASH MISHRA 21/01/2001 GEN B.TECH/B.E.Bachelor of Technology (Electrical1 Regular EngineeringD/s 80900 ) Forwd 2 580380501901096 AASTHA SHUKLA RANG NATH SHUKLA 12/04/1999 GEN M.SC M.Sc. in Mathematics and1 ComputingRegular D/s 41900 Forwd 3 580380501901048 AAYUSH SRIVASTAV JAI SHANKAR LAL SRIVASTAV 14/12/1999 GEN B.TECH/B.E.Bachelor of Technology (Electrical1 Regular EngineeringD/s 80900 ) Forwd 4 580380501900555 ABHAY RAJ SINGH SURYA PRATAP SINGH 02/04/2000 GEN B.TECH/B.E.Bachelor of Technology (Mechanical1 Regular Engineering)Host 25900 Forwd 5 580380501900038 ABHIJEET KUMAR SINGH RAJEEV RANJAN SINGH 01/03/1998 GEN B.TECH/B.E.Bachelor of Technology (Computer3 Regular ScienceHost &80900 Engineering)Forwd 6 580380501900942 ABHINAV PRAKASH PANDEY GIRISH CHANDRA PANDEY 27/07/2000 GEN B.TECH/B.E.Bachelor of Technology (Electrical1 Regular EngineeringHost 25900 ) Forwd 7 580380501900314 ABHINAY SINGH UDAY PRATAP SINGH 25/08/1997 GEN MCA Master in Computer Applications1 Regular D/s 55900 Forwd 8 580380501901425 ABHISHEK MISHRA GYANENDRA DHAR MISHRA 10/10/1998 GEN B.TECH/B.E.Bachelor of Technology (Electranics2 Regular &D/s Communication)90000 Forwd 9 580380501900571 ABHISHEK PANDEY RAKESH PANDEY 29/01/2001 -
Details of Shareholders Whose Shares Are Liable to Be Transfer to Iepf Sr.No Fol Dpid Clid Name 1 Y000004 Yusufali Alibhaikarimj
DETAILS OF SHAREHOLDERS WHOSE SHARES ARE LIABLE TO BE TRANSFER TO IEPF SR.NO FOL DPID CLID NAME 1 Y000004 YUSUFALI ALIBHAIKARIMJEE JAWANJEE 2 M003118 MONICA DILAWARI 3 V003054 V CHANDRA SHEKHAR 4 K003086 KISHAN LAL JANGID 5 D003051 DIPTI P PATEL 6 N003058 NILA A PATEL 7 L003009 LACHMANDAS RAMCHAND 8 R003170 RASIKBHAI K SAVJANI 9 G003039 GITA ASHWIN BANKER 10 H003036 HATIM ARIAAR 11 B003056 BHAVANA KAPASI 12 R003173 RAVI D SAWANT 13 M003083 M A NARAYANAN 14 V003075 VIJAY MALLYA 15 N003055 NAYEEMUDDIN SYED 16 M003088 MAHABALAPPA NANDIHALLI SHANMUKHA 17 A003090 ABDUL AZEEZ 18 K003066 K JEGATHEESAN 19 A003126 ASOKAN KUNJURAMAN 20 0010146 JAGAN NATH PAL 21 0010188 PARTH KHAKHAR 22 0010953 SHIKAR CHAND JAIN 23 A000295 AVTAR SINGH 24 A005583 ARVINDBHAI ISHWAR BHAI PATEL 25 G003898 GUNVANTRAI C MEHTA 26 J000382 JEET SINGH 27 J004092 JAI PARKASH 28 M003185 M P SRIDHARAN 29 M003986 M.V.S. SURYANARAYANA 30 N003999 NAND LAL DHAWAN 31 P003628 PRADNYA PRAKASH PAI 32 P004247 PATEL NANDLAL JAGJIVANDAS 33 R003427 RAJENDRA SINGH NEGI 34 T003414 TRIPTI GUPTA 35 U003427 URMILA GOEL 36 0010970 KIRAN VIJAY JAIPURIA 37 A000311 ANANG UDAYA SINGH DEO 38 A003013 AMARJEET SINGH KAMBOJ 39 A003020 AMRIT PAL MITTAL 40 A003028 ANIL KUMAR CHOPRA 41 A003046 ARUN KR SULTANIA 42 A003066 ASHOK KUMAR GUPTA 43 A003983 ANIL GOYAL 44 A004030 A RAJA BABU 45 A004113 A T THOMAS 46 A004564 A. RAJA BABU 47 A004666 ANIL KUMAR LUKKAD 48 A004677 ASHA DEVI 49 A004915 ASHOK GUPTA 50 A005458 ANURAG JAIN 51 A005468 AGA REDDY VANTERU 52 B000031 BHAIRULAL GULABCHAND 53 B000049 BALMUKAND AGARWAL -
Ap-Rasc 2019)
2019 URSI Asia-Pacific Radio Science Conference (AP-RASC 2019) New Delhi, India 9-15 March 2019 Pages 1-730 IEEE Catalog Number: CFP19E09-POD ISBN: 978-1-5386-8551-8 1/2 Copyright © 2019, International Union of Radio Science All Rights Reserved *** This is a print representation of what appears in the IEEE Digital Library. Some format issues inherent in the e-media version may also appear in this print version. IEEE Catalog Number: CFP19E09-POD ISBN (Print-On-Demand): 978-1-5386-8551-8 ISBN (Online): 978-90-825987-5-9 Additional Copies of This Publication Are Available From: Curran Associates, Inc 57 Morehouse Lane Red Hook, NY 12571 USA Phone: (845) 758-0400 Fax: (845) 758-2633 E-mail: [email protected] Web: www.proceedings.com TABLE OF CONTENTS SPECTRUM MONITOR SYSTEM AT QTT SITE.......................................................................................................................................1 Qi Liu ; Yue Wang ; Ye Liu ; Na Wang ; Feng Liu ; Hao Yan ; Yang Wang RFI PREDICTION FOR QTT RESTRICTED AREA..................................................................................................................................5 Ye Liu ; Qi Liu ; Yang Wang ; Yue Wang PRECISE CLOCK COMPARISON BY MEANS OF SOFTWARE-DEFINED RADIO RECEIVER...................................................9 Yi-Jiun Huang ; Huang-Tien Lin GENERALIZED PROBABILITY DENSITY FUNCTION FOR INTERMODULATION DISTORTION COMPONENTS GENERATED BY POWER AMPLIFIER......................................................................................................................10 -
The Upgraded GMRT : Opening New Windows
The upgraded GMRT : Opening new windows Yashwant Gupta National Centre for Radio Astrophysics Pune India PHISC meeting NCRA Pune 6 Feb 2017 Plan of today's presentation . The upgraded GMRT (uGMRT) – goals & plans . Developments & current status of different aspects of the uGMRT . Status of (phased) release of the uGMRT to the user community The existing GMRT : An Overview . 30 dishes, 45 m diameter each . 12 dishes in a central 1 km x 1 km region (central square) . remaining along 3 arms of Y-shaped array . baselines : ~ 200 m (shortest); ~ 30 km (longest) . Frequency range : . 130-170 MHz . 225-245 MHz . 300-360 MHz . 580-660 MHz . 1000-1450 MHz . max instantaneous BW = 32 MHz . Effective collecting area (2-3% of SKA) : . 30,000 sq m at lower frequencies . 20,000 sq m at highest frequencies . Supports 2 modes of operation : . Interferometry, aperture synthesis . Array mode (incoherent & coherent) The existing GMRT : An Overview . 30 dishes, 45 m diameter each . 12 dishes in a central 1 km x 1 km region (central square) . remaining along 3 arms of Y-shaped array . baselines : ~ 200 m (shortest); ~ 30 km (longest) . Frequency range : . 130-170 MHz . 225-245 MHz . 300-360 MHz 1 km x . 580-660 MHz 1 km . 1000-1450 MHz . max instantaneous BW = 32 MHz 14 . Effective collecting area (2-3% of SKA) : km . 30,000 sq m at lower frequencies . 20,000 sq m at highest frequencies . Supports 2 modes of operation : . Interferometry, aperture synthesis . Array mode (incoherent & coherent) Dedication of the GMRT The Giant Metrewave Radio Telescope was dedicated to the World Scientific Community by the Chairman of TIFR Council, Shri Ratan Tata. -
Concept Note Indo-South African Flagship Programme in Astronomy
Concept Note Indo-South African Flagship Programme in Astronomy Preamble: The Indo-South Africa Flagship Workshop meetings took place at the Indian Institute of Astrophysics, Bangalore on 15th-16th September 2014, and at the Inter-University Centre for Astronomy and Astrophysics, Pune on 19th September, 2014 and were sanctioned by the Departments of Science and Technology of both countries. A list of participants is included in the appendix. 1. Introduction India and South Africa share common aspirations for scientific and technological development, and for the growth of human capital resources. The countries are members of the BRICS consortium, and have a current bi-lateral agreement to foster joint progress. Their shared goals are particularly apparent in the area of astronomy and astrophysics. Indo-African astronomy cooperation began with projects in radio astronomy in Nigeria and Mauritius in the 1980s, and the optical Nainital-Cape Survey, started in 1997. The Inter-University Centre for Astronomy and Astrophysics (IUCAA) joined SALT in 2007, and the National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research (NCRA) has recently joined the SKA. Astronomy captures the imagination of people everywhere, and touches a fundamental human desire to understand the universe that surrounds us and our place in it. It provides an ideal way to attract young learners into scientific and technical studies, developing the human capacity for the knowledge-based economy of the future. Its appeal transcends boundaries of class and race and speaks to all members of our societies. The goal of the Indo-South African Flagship Programme in Astronomy is to exploit these basic strengths for the mutual betterment of our peoples. -
To, Prof. Ajit Kembhavi, President, ASI CC
To, Prof. Ajit Kembhavi, President, ASI CC : Prof. Dipankar Banerjee, Secretary, ASI Subject : Formation of Working Group for Gender Equity Dear Sir, We, the undersigned, members of the Indian Astronomy & Astrophysics community (from a number of academic institutions), would like to request you for the formation of a working group for gender equity under the aegis of ASI. To this effect we hereby submit a formal proposal giving details of the rational behind such a working group and a brief outline of the role we would like the working group to play. We hope you would take cognizance of the fact that a significant fraction of our community feel that the formation of such a group is the need of the hour. For the Working Group to better serve the needs of the entire astronomy community, it would be advantageous if its constituted members reflect the diversity of the community in gender, age, affiliation, geographical region etc. In addition, in the interest of promoting equity in gender representation, we feel it is best chaired by a woman astronomer. Hoping to receive a positive response from you. Yours sincerely, The Proposers of the Working Group The Proposers : A core group of people (Preeti Kharb, Sushan Konar, Niruj Mohan, L. Resmi, Jasjeet Singh Bagla, Nissim Kanekar, Prajval Shastri, Dibyendu Nandi etc.) have been working towards sensitising the Indian Astronomical community about gender related issues and proposing the formation of a working group, with significant input from a number of others. However, a large section of the community have been supportive of this activity and would like to be a part of this initiative. -
Dynamics and Chaos in the Unified Scalar Field Cosmology
Dynamics and chaos in the unified scalar field Cosmology Georgios Lukes-Gerakopoulos,1,2 Spyros Basilakos,1 and George Contopoulos1 1Academy of Athens, Research Center for Astronomy, Soranou Efesiou 4, GR-11527, Athens, GREECE 2University of Athens,Department of Physics, Section of Astrophysics, Astronomy and Mechanics We study the dynamics of the closed scalar field FRW cosmological models in the framework of the so called Unified Dark Matter (UDM) scenario. Performing a theoretical as well as a numerical analysis we find that there is a strong indication of chaos in agreement with previous studies. We find that a positive value of the spatial curvature is essential for the appearance of chaoticity, though the Lyapunov number seems to be independent of the curvature value. Models that are close to flat (k 0+) exhibit a chaotic behavior after a long time while pure flat models do not exhibit any chaos.→ Moreover, we find that some of the semiflat models in the UDM scenario exhibit similar dynamical behavior with the Λ cosmology despite their chaoticity. Finally, we compare the measured evolution of the Hubble parameter derived from the differential ages of passively evolving galaxies with that expected in the semiflat unified scalar field cosmology. Based on a specific set of initial conditions we find that the UDM scalar field model matches well the observational data. PACS numbers: 98.80.-k, 11.10.Ef, 11.10.Lm Keywords: Scalar field; Cosmology; Chaotic scattering 1. INTRODUCTION question which has to be addressed: how can we esti- mate the amount of chaos? It has been shown that in chaotic scattering problems classical tools, like the Lya- There is by now convincing evidence that the avail- punov characteristic number, are unable to provide a able high quality cosmological data (Type Ia supernovae, clear answer whether an orbit is chaotic or not [22]. -
Tata Institute of Fundamental Research Deemed to Be University
Tata Institute of Fundamental Research Deemed to be University Annual Quality Assurance Report (AQAR) 2016-2017 Tata Institute of Fundamental Research AQAR 2016-17 Part A 1 Name of the Institution Tata Institute of Fundamental Research Name of the Head of the institution Prof. Sandip Trivedi Designation Director Does the institution function from own campus Yes Phone no./Alternate phone no. 2222782306 Mobile No 9892105000 Registered Email [email protected] Alternate Email [email protected] Address 1, Dr. Homi Bhabha Road, Navy Nagar, Colaba, City Mumbai State Maharashtra Pin Code 400005 2 Tata Institute of Fundamental Research AQAR 2016-17 2 Institutional status University Deemed to be University Type of Institution Co-education Location Urban Financial Status Centrally Funded Name of the IQAC Coordinator Prof. Amol Dighe Phone no. / Alternate No. 2222782432 Mobile 9967396593 IQAC email address [email protected] Alternate email address [email protected] 3 Website address Weblink of the AQAR: (Previous year) https://www.tifr.res.in/NAAC/tifrSSR.pdf 4 Whether Academic Calendar prepared during the year? Yes If yes, whether it is uploaded in the Institutional website Yes https://www.tifr.res.in/~sbp/new2015/Academic_Calendar_2017.pdf 5 Accreditation Details Cycle Grade CGPA Year of Accreditation Validity Period 1st A+ 3.68 2016 02 Dec 2016 to 01 Dec 2021 3 Tata Institute of Fundamental Research AQAR 2016-17 6 Date of Establishment of IQAC 15 Feb 2016 7 Internal Quality Assurance System 7.1 Quality initiatives by IQAC during the year for promoting quality culture Item /Title of the quality initiative by IQAC Date & Duration Number of participants/beneficiaries (1). -
The Council and the Governing Board
The Council Ved Prakash, Secretary, and the Governing Board University Grants Commission, New Delhi. S. G. Rajasekaran, The Council The Institute of Mathematical Sciences, Chennai. President V. S. Ramamurthy, Secretary to the Government of India, A.S. Nigavekar, Department of Science and Technology, New Delhi. Chairperson, University Grants Commission, New Delhi. C.V. Vishveshwara, Honorary Director, Vice-President Jawaharlal Nehru Planetarium, Bangalore. V.N. Rajasekharan Pillai, The following members have served in the Council for Vice-Chairperson, part of the year University Grants Commission, New Delhi. Arnab Rai Choudhuri, Members Indian Institute of Science, Bangalore. N. Mukunda, S. S. Dattagupta, [Chairperson, Governing Board], Director, Satyendra Nath Bose National Centre Centre for Theoretical Studies, for Basic Sciences, Kolkata. Indian Institute of Science, Bangalore. Deepak Dhar, Shishir K. Dube, Tata Institute of Fundamental Research, Mumbai. Director, Indian Institute of Technology, Kharagpur. G.K. Mehta, Vice-Chancellor, Ashok Kumar Gupta, University of Allahabad. J.K. Institute of Applied Physics, University of Allahabad. Janak Pandey, Vice-Chancellor, Kota Harinarayana, University of Allahabad. Vice-Chancellor, University of Hyderabad. R.R. Pandey, Vice-Chancellor, A.K. Kembhavi, Deendayal Upadhyay Gorakhpur University. IUCAA, Pune. S. R. Rajaraman, A.S. Kolaskar, School of Physical Sciences, Vice-Chancellor, Jawaharlal Nehru University, New Delhi. University of Pune. Nityananda Saha, R.A. Mashelkar, Vice-Chancellor, Director General, University of Kalyani. Council of Scientific and Industrial Research, New Delhi. S.S. Suryawanshi, Vice-Chancellor, G. Madhavan Nair, Swami Ramanand Teerth Marathwada Secretary to the Government of India, University, Nanded. Department of Space, Bangalore. J.A.K. Tareen, Rajaram Nityananda, Vice-Chancellor, Centre Director, University of Kashmir, Srinagar.