Sun-Earth System Interaction Studies Over Vietnam: an International Cooperative Project
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A PROFILE Dr. Vijay Bhatkar Is One of Most Acclaimed and Internationally Acknowledged
DR. VIJAY BHATKAR: A PROFILE www.vijaybhatkar.org Dr. Vijay Bhatkar is one of most acclaimed and internationally acknowledged scientists of India. He is presently the Chancellor of Nalanda University. In this responsibility, he has committed himself to resurrecting the glory of ancient Nalanda, in the context of 21st century. Prior to Nalanda responsibility, he was the Chairman of Board of Governors of IIT Delhi from 2012 to 2017. He is best known as the architect of India’s national initiative in supercomputing, where he led the development of India’s first supercomputer Param in 1990, under the technology denial regime. Currently he is steering the National Supercomputing Mission of developing Exascale Architecture Supercomputing for India. Dr. Bhatkar is also widely known for bringing ICT to the masses through a wide range of path-breaking initiatives, such as the celebrated GIST multilingual technology covering India’s 22 official languages with 10 diverse scripts that has dissolved the language barrier on computers once for all; MKCL’s computer literacy programme that made a world mark by creating 10 million computer literates within a decade; Education to Home (ETH) initiative for bringing the benefits of ICT to school education. In the 80’s, Dr Bhatkar substantially contributed to the ushering of electronics revolution in India. He is also credited with the creation of several national research labs and institutions, notably amongst them being C-DAC, ER&DC Trivandrum, IIITM-K, TechnoPark, MKCL, IsquareIT, ETH Research Lab and Multiversity. Simultaneously, he has mentored several innovation-based start-ups. Dr. Bhatkar has served as a member of the Scientific Advisory Committee to PM, Member of the Governing Council of CSIR and a member of the IT Task Force constituted by PM in 1998. -
Theory, Modeling, and Integrated Studies in the Arase (ERG) Project
Seki et al. Earth, Planets and Space (2018) 70:17 https://doi.org/10.1186/s40623-018-0785-9 FULL PAPER Open Access Theory, modeling, and integrated studies in the Arase (ERG) project Kanako Seki1* , Yoshizumi Miyoshi2, Yusuke Ebihara3, Yuto Katoh4, Takanobu Amano1, Shinji Saito5, Masafumi Shoji2, Aoi Nakamizo6, Kunihiro Keika1, Tomoaki Hori2, Shin’ya Nakano7, Shigeto Watanabe8, Kei Kamiya5, Naoko Takahashi1, Yoshiharu Omura3, Masahito Nose9, Mei‑Ching Fok10, Takashi Tanaka11, Akimasa Ieda2 and Akimasa Yoshikawa11 Abstract Understanding of underlying mechanisms of drastic variations of the near-Earth space (geospace) is one of the current focuses of the magnetospheric physics. The science target of the geospace research project Exploration of energiza‑ tion and Radiation in Geospace (ERG) is to understand the geospace variations with a focus on the relativistic electron acceleration and loss processes. In order to achieve the goal, the ERG project consists of the three parts: the Arase (ERG) satellite, ground-based observations, and theory/modeling/integrated studies. The role of theory/modeling/integrated studies part is to promote relevant theoretical and simulation studies as well as integrated data analysis to combine diferent kinds of observations and modeling. Here we provide technical reports on simulation and empirical models related to the ERG project together with their roles in the integrated studies of dynamic geospace variations. The simu‑ lation and empirical models covered include the radial difusion model of the radiation belt electrons, GEMSIS-RB and RBW models, CIMI model with global MHD simulation REPPU, GEMSIS-RC model, plasmasphere thermosphere model, self-consistent wave–particle interaction simulations (electron hybrid code and ion hybrid code), the ionospheric electric potential (GEMSIS-POT) model, and SuperDARN electric feld models with data assimilation. -
National Supercomputing Mission
02 April, 2020 National Supercomputing Mission Part of: GS Prelims and GS-III- S&T India has produced just three supercomputers since 2015 under the National Supercomputing Mission (NSM). National Supercomputing Mission The National Supercomputing Mission was announced in 2015, with an aim to connect national academic and R&D institutions with a grid of more than 70 high-performance computing facilities at an estimated cost of ?4,500 crores over the period of seven years. It supports the government's vision of 'Digital India' and 'Make in India' initiatives. The mission is being implemented by the Department of Science and Technology (Ministry of Science and Technology) and Ministry of Electronics and Information Technology (MeitY), through the Centre for Development of Advanced Computing (C-DAC), Pune and Indian Institute of Science (IISc), Bengaluru. It is also an effort to improve the number of supercomputers owned by India. These supercomputers will also be networked on the National Supercomputing grid over the National Knowledge Network (NKN). The NKN connects academic institutions and R&D labs over a high-speed network. Under NSM, the long-term plan is to build a strong base of 20,000 skilled persons over the next five years who will be equipped to handle the complexities of supercomputers. Key Points Progress of NSM: NSM’s first supercomputer named Param Shivay has been installed in IIT-BHU, Varanasi, in 2019. It has 837 TeraFlop High-Performance Computing (HPC) capacity. The second supercomputer with a capacity of 1.66 PetaFlop has been installed at IIT-Kharagpur. The third system, Param Brahma, has been installed at IISER-Pune, which has a capacity of 797 TeraFlop. -
Param Shavak
CENTRE FOR DEVELOPMENT OF ADVANCED COMPUTING PARAM SHAVAK User Manual www.cdac.in PARAM SHAVAK USER MANUAL PARAM SHAVAK USER MANUAL www.cdac.in i PARAM SHAVAK USER MANUAL Copyright Notice Copyright © 2014 Centre for Development of Advanced Computing All Rights Reserved. Any technical documentation that is made available by C-DAC (Centre for Development of Advanced Computing) is the copyrighted work of C-DAC and is owned by C-DAC. This technical documentation is being delivered to you as is, and C-DAC makes no warranty as to its accuracy or use. Any use of the technical documentation or the information contained therein is at the risk of the user. This document may include technical or other inaccuracies or typographical errors. C-DAC reserves the right to make changes without prior notice. Trademarks CDAC, CDAC logo, PARAM Shavak and PARAM Shavak logo are trademarks or registered trademarks of Centre for Development of Advanced Computing. The CentOS Mark is a trademark of Red Hat, Inc. Ubuntu® is a registered trademark of Canonical Ltd. Intel® and Intel® products are trademarks or registered trademarks of Intel® Corporation and are hereby acknowledged. Other brands and product names mentioned in this manual may be trademarks or registered trademarks of their respective companies and are hereby acknowledged. Intended Audience This document is meant for PARAM Shavak users. This document assumes that they have the following skills depending on the target platform: Basic Linux Commands ii PARAM SHAVAK USER MANUAL Typographic Conventions Symbol Meaning Blue underlined text A hyperlink or link you can click to go to a related section in this document or to a URL in your web browser. -
Locations of Chorus Emissions Observed by the Polar Plasma Wave Instrument K
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 115, A00F12, doi:10.1029/2009JA014579, 2010 Click Here for Full Article Locations of chorus emissions observed by the Polar Plasma Wave Instrument K. Sigsbee,1 J. D. Menietti,1 O. Santolík,2,3 and J. S. Pickett1 Received 18 June 2009; revised 20 November 2009; accepted 17 December 2009; published 8 June 2010. [1] We performed a statistical study of the locations of chorus emissions observed by the Polar spacecraft’s Plasma Wave Instrument (PWI) from March 1996 to September 1997, near the minimum of solar cycles 22/23. We examined how the occurrence of chorus emissions in the Polar PWI data set depends upon magnetic local time, magnetic latitude, L shell, and L*. The Polar PWI observed chorus most often over a range of magnetic local times extending from about 2100 MLT around to the dawn flank and into the dayside magnetosphere near 1500 MLT. Chorus was least likely to be observed near the dusk flank. On the dayside, near noon, the region in which Polar observed chorus extended to larger radial distances and higher latitudes than at other local times. Away from noon, the regions in which chorus occurred were more restricted in both radial and latitudinal extent. We found that for high‐latitude chorus near local noon, L* provides a more reasonable mapping to the equatorial plane than the standard L shell. Chorus was observed slightly more often when the magnitude of the solar wind magnetic field BSW was greater than 5 nT than it was for smaller interplanetary magnetic field strengths. -
Air Quality Over Major Cities of Saudi Arabia During Hajj Periods of 2019 and 2020
Chapman University Chapman University Digital Commons Biology, Chemistry, and Environmental Sciences Science and Technology Faculty Articles and Faculty Articles and Research Research 2-2-2021 Air Quality Over Major Cities of Saudi Arabia During Hajj Periods of 2019 and 2020 Ashraf Farahat Akshansha Chauhan Mohammed Al Otaibi Ramesh P. Singh Follow this and additional works at: https://digitalcommons.chapman.edu/sees_articles Part of the Atmospheric Sciences Commons, Environmental Indicators and Impact Assessment Commons, and the Environmental Monitoring Commons Air Quality Over Major Cities of Saudi Arabia During Hajj Periods of 2019 and 2020 Comments This article was originally published in Earth Systems and Environment in 2021. https://doi.org/10.1007/ s41748-021-00202-z This scholarship is part of the Chapman University COVID-19 Archives. Creative Commons License This work is licensed under a Creative Commons Attribution 4.0 License. Copyright The authors Earth Systems and Environment https://doi.org/10.1007/s41748-021-00202-z ORIGINAL ARTICLE Air Quality Over Major Cities of Saudi Arabia During Hajj Periods of 2019 and 2020 Ashraf Farahat1 · Akshansha Chauhan2 · Mohammed Al Otaibi3 · Ramesh P. Singh4 Received: 25 October 2020 / Accepted: 13 January 2021 © The Author(s) 2021 Abstract Mecca and Madinah are two holy cities where millions of people in general, visit throughout the years, during Hajj (Mus- lim’s pilgrimage) time number of people visit these holy cities from diferent parts of the world is very high. However, the Government of Saudi Arabia only allowed 1000 pilgrims during the 2020 Hajj especially when the world is sufering from COVID-19. -
The Near-Earth Plasma Environment
Space Sci Rev (2012) 168:23–112 DOI 10.1007/s11214-012-9872-6 The Near-Earth Plasma Environment Robert F. Pfaff Jr. Received: 1 March 2012 / Accepted: 3 March 2012 / Published online: 20 June 2012 © US Government 2012 Abstract An overview of the plasma environment near the earth is provided. We describe how the near-earth plasma is formed, including photo-ionization from solar photons and impact ionization at high latitudes from energetic particles. We review the fundamental characteristics of the earth’s plasma environment, with emphasis on the ionosphere and its interactions with the extended neutral atmosphere. Important processes that control iono- spheric physics at low, middle, and high latitudes are discussed. The general dynamics and morphology of the ionized gas at mid- and low-latitudes are described including electro- dynamic contributions from wind-driven dynamos, tides, and planetary-scale waves. The unique properties of the near-earth plasma and its associated currents at high latitudes are shown to depend on precipitating auroral charged particles and strong electric fields which map earthward from the magnetosphere. The upper atmosphere is shown to have profound effects on the transfer of energy and momentum between the high-latitude plasma and the neutral constituents. The article concludes with a discussion of how the near-earth plasma responds to magnetic storms associated with solar disturbances. Keywords Ionosphere · Upper atmosphere · Electric fields 1 Introduction In this article we discuss the near-earth plasma environment, for which the ionosphere is the natural focus. Because this ionized gas co-exists with the neutral atmospheric gas to which it is coupled, the ionized/neutral gas system is more properly considered a partially ionized gas rather than a medium consisting of two distinct, independent fluids. -
THE BACKGROUND the Crude Market from As Recently As 2015, Saudi Energy Officials Competing Suppliers” Dismissed Suggestions That the Kingdom
FEATURE ENERGY ENERGY FEATURE BEYOND What are the implications of an increase in Saudi crude oil production capacity? BY JIM KRANE COMBINATION OF FACTORS IS encouraging Saudi Arabia A to consider raising crude oil production capacity beyond the current ceiling of 12.5 million barrels per day. The kingdom has managed to maintain a constant share of global crude oil markets, even as it copes with growing domestic demand for oil and a spate of investments in refineries, inside and outside the kingdom. Longer term, the threat of peak global oil demand – perhaps in response to climate change “Saudi Arabia finds itself – enhances the attractions of a shorter time horizon to depletion. However, an oscillating between increase in Saudi crude oil production cutting crude oil would have consequences for markets and competing forms of energy, as well production to prop up as for the kingdom's geopolitical stature. prices and maintaining The wide range of potential outcomes suggests that a major capacity increase is high levels of exports a risky strategy. to defend its share of THE BACKGROUND the crude market from As recently as 2015, Saudi energy officials competing suppliers” dismissed suggestions that the kingdom 40 Vol. 18/31, September 2017 anbusiness.com 41 FEATURE ENERGY ENERGY FEATURE would seek to raise its crude oil production “Even though costs based on what we see as projection and capacity above its theoretical maximum are among the world’s call on Saudi oil, we don’t see anything of 12.5 million barrels per day (m b/d). like that, even by 2030 or 2040. -
LCSH Section E
E (The Japanese word) E. J. Pugh (Fictitious character) E-waste [PL669.E] USE Pugh, E. J. (Fictitious character) USE Electronic waste BT Japanese language—Etymology E.J. Thomas Performing Arts Hall (Akron, Ohio) e World (Online service) e (The number) UF Edwin J. Thomas Performing Arts Hall (Akron, USE eWorld (Online service) UF Napier number Ohio) E. Y. Mullins Lectures on Preaching Number, Napier BT Centers for the performing arts—Ohio UF Mullins Lectures on Preaching BT Logarithmic functions E-journals BT Preaching Transcendental numbers USE Electronic journals E-zines (May Subd Geog) Ë (The Russian letter) E.L. Kirchner Haus (Frauenkirch, Switzerland) UF Ezines BT Russian language—Alphabet USE In den Lärchen (Frauenkirch, Switzerland) BT Electronic journals E & E Ranch (Tex.) E. L. Pender (Fictitious character) Zines UF E and E Ranch (Tex.) USE Pender, Ed (Fictitious character) E1 (Mountain) (China and Nepal) BT Ranches—Texas E-lists (Electronic discussion groups) USE Lhotse (China and Nepal) E-605 (Insecticide) USE Electronic discussion groups E2ENP (Computer network protocol) USE Parathion E. London Crossing (London, England) USE End-to-End Negotiation Protocol (Computer E.1027 (Roquebrune-Cap-Martin, France) USE East London River Crossing (London, England) network protocol) UF E1027 (Roquebrune-Cap-Martin, France) E. London River Crossing (London, England) E10 Motorway Maison en bord du mer E.1027 (Roquebrune- USE East London River Crossing (London, England) USE Autoroute E10 Cap-Martin, France) Ê-luan Pi (Taiwan) E22 Highway (Sweden) Villa E.1027 (Roquebrune-Cap-Martin, France) USE O-luan-pi, Cape (Taiwan) USE Väg E22 (Sweden) BT Dwellings—France E-mail art E190 (Jet transport) E.A. -
The Atmospheric Global Electric Circuit: an Overview
The atmospheric global electric circuit: An overview Devendraa Siingha,b*, V. Gopalakrishnana,, R. P. Singhc, A. K. Kamraa, Shubha Singhc, Vimlesh Panta, R. Singhd, and A. K. Singhe aIndian Institute of Tropical Meteorology, Pune-411 008, India bInstitute of Environmental Physics, University of Tartu, 18, Ulikooli Street, Tartu- 50090, Estonia cDepartment of Physics, Banaras Hindu University, Varanasi-221 005, India dIndian Institute of Geomagnetism, Mumbai-410 218, India ePhysics Department, Bundelkhand University, Jhansi, India Abstract: Research work in the area of the Global Electric Circuit (GEC) has rapidly expanded in recent years mainly through observations of lightning from satellites and ground-based networks and observations of optical emissions between cloud and ionosphere. After reviewing this progress, we critically examine the role of various generators of the currents flowing in the lower and upper atmosphere and supplying currents to the GEC. The role of aerosols and cosmic rays in controlling the GEC and linkage between climate, solar-terrestrial relationships and the GEC has been briefly discussed. Some unsolved problems in this area are reported for future investigations. ----------------------------------------------------------------------------------------------------------- - *Address for corrspondence Institute of Environmental Physics, University of Tartu, 18, Ulikooli Street Tartu-50090, Estonia e-mail; [email protected] [email protected] Fax +37 27 37 55 56 1 1. Introduction The global electric circuit (GEC) links the electric field and current flowing in the lower atmosphere, ionosphere and magnetosphere forming a giant spherical condenser (Lakhina, 1993; Bering III, 1995; Bering III et al., 1998; Rycroft et al., 2000; Siingh et al., 2005), which is charged by the thunderstorms to a potential of several hundred thousand volts (Roble and Tzur, 1986) and drives vertical current through the atmosphere’s columnar resistance. -
International Civil Aviation Organization
METWARN/I TF/2 – WP/6 Agenda Item 2 (a) 19/04/12 International Civil Aviation Organization THE SECOND MEETING OF ASIA/PACIFIC METEOROLOGICAL ADVISORIES AND WARNINGS IMPLEMENTATION TASK FORCE (METWARN/I TF/2) Bangkok, Thailand, 19 – 20 April 2012 Agenda Item 2: Review educational material a) Monitor the developments of IAVWOPSG and METWSG with reference to guidance on radioactive cloud and Tsunami GLOBAL PROGRESS ON GUIDANCE ON RADIOACTIVE CLOUD (Presented by the Secretariat) SUMMARY This paper presents an update on the global progress on guidance on radioactive cloud information. This paper relates to: Strategic Objectives: A. Safety Global Plan Initiatives: GPI-18 Aeronautical information GPI-19 Meteorological Systems 1. INTRODUCTION 1.1 The Twentieth Meeting of the Asia/Pacific Air Navigation Planning and Implementation Regional Group (APANPIRG/20) Conclusion 20/69 calls for further guidance on the issuance of SIGMET on radioactive cloud. The International Airways Volcano Watch Operations Group (IAVWOPSG) determined that additional Standards were not necessary (IAVWOPSG/5 Decision 5/23 refers) and that guidance be included in Part II of the Manual on Volcanic Ash, Radioactive Material and Toxic Chemical Clouds (Doc 9691) (IAVWOPSG/5 Conclusion 5/24 refers). METWARN/I TF/2 – WP/6 -2- Agenda Item 2a 19/04/12 2. DISCUSSION 2.1 The IAVWOPSG/6 meeting in Dakar, Senegal, 19 to 23 September 2011, concluded that ad-hoc groups continue with tasks identified to address key issues concerning the importance, complexity and lack of expertise on radioactive clouds. The meeting report and conclusions from IAVWOPSG/6 are provided in the Attachment for review by the METWARN/I TF/2 and can be accessed on the web at http://www2.icao.int/en/anb/met/iavwopsg/Lists/Meetings/DispForm.aspx?ID=6. -
C-DAC Activities on Many Cores and Accelerators
CC--DACDAC HPCHPC ActivitiesActivities && ExperienceExperience onon AcceleratorsAccelerators Goldi Misra Group Coordinator & Head HPC Solutions Group C-DAC, India Thematic R & D Areas of C-DAC • High Performance Computing & Grid Computing • Hardware, Software, Systems, Applications, Research, Technology, Infrastructure • Multilingual Computing and Heritage Computing • Tools, Fonts, Products, Solutions, Research, Technology Development • Health Informatics • Hospital Information System, Telemedicine, Decision Support System, Tools, Traditional Knowledge-base and DSS for Medicine • Software Technologies including FOSS • FOSS, Multimedia, ICT for masses, E-Governance, Geomatics, ICT4D • Professional Electronics including VLSI & Embedded Systems • Digital Broadband and Wireless Systems, Network Technologies, Power Electronics, Real- Time Systems, Control Electronics, Embedded Systems, VLSI/ASIC Design, Agri Electronics, Strategic Electronics • Cyber Security & Cyber Forensics • Cyber Security tools, technologies & solution development, Research & Training Education and Training forms an important component of C-DAC activities cutting across the above Thematic Areas Kaleidoscope of C-DAC Products Spectrum of HPC Activities Technologies Trainings Systems Spectrum of HPC Activities Solutions National Facilities Applications PARAM Series of Supercomputers PARAM YUVA Indian Supercomputing Scenario C-DAC’s PARAM 8000, India’s first Gigascale 1990 Supercomputer ANUPAM- BARC PARAM – C-DAC ANURAG- DRDO Flowsolver- NAL Parallel 1990 Initiatives -2000 Several HPC Facilities setup including those at C-DAC, IISc, BARC, 2000 NAL, CMMACS, DRDO, NCMRWF -2007 C-DAC’s PARAM Padma, India’s first Terascale Supercomputer 2002 Launched (Rank 171 in Top 500 List) CRL’s EKA ranks 4th in Top 500 List 2007 9 Terascale Systems from India in Top 500 List C-DAC’s PARAM Yuva Launched (Rank 68 in Top 500 List) 2008 Only 4 systems from India in Top 500 List as against 41 systems from China 2010 India’s best system ranked 47 in Top 500 List India Govt.