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Digital Age – the Implementers 1 July – 31 December 2020
Digital Age – The Implementers 1 July – 31 December 2020 ”Digitalisation has a huge impact on the way we live, work and communicate. In some fields, Europe has to catch up – like for business to consumers – while in others we are frontrunners – such as in business to business. We have to make our single market fit for the digital age, we need Renew to make the most of artificial intelligence and big data, EPP S&D Europe we have to improve on cybersecurity and we have to work hard for our technological sovereignty.” — Ursula von der Leyen President of the European Commission Bjoern Seibert Ilze Juhansone Lorenzo Mannelli Klaus Welle François Roux Jeppe Tranholm-Mikkelsen Head of cabinet Secretary General Head of cabinet Secretary General Head of cabinet Secretary General Executive Vice-President Margrethe Vestager will coordinate the agenda on a Europe fit for the digital age. Ursula von der Leyen David Sassoli Charles Michel Renew S&D Europe COMP Margrethe Vestager Kim Jørgensen Oliver Guersent Irene Tinagli Claudia Lindemann EPP Commissioner Head of Cabinet Director General ECON Committee Chair ECON Secretariat Peter Altmaier Norbert Schultes Federal Minister of Economics Permanent Representation GROW and Energy Kerstin Jorna Greens/EFA Renew Director General Europe EPP Petra de Sutter Panos Konstantopoulos CONNECT IMCO Committee Chair IMCO Secretariat with ITRE with ITRE Thierry Breton Valère Moutarlier Roberto Viola Cristian- Peter Andreas Scheuer Stefanie Schröder Silviu Bușoi Traung Federal Minister of Transport Margrethe Commissioner -
Joint Comments on Treatment of Biomass (PDF)
October 31, 2018 Joint Comments of Clean Air Task Force, Natural Resources Defense Council, Center for Biological Diversity, Clean Air Council, Clean Wisconsin, Conservation Law Foundation, Dogwood Alliance, Partnership for Policy Integrity, and Sierra Club on the Treatment of Biomass-Based Power Generation in EPA’s Proposed Emission Guidelines for Greenhouse Gas Emissions from Existing Electric Utility Generating Units; Revisions to Emission Guideline Implementing Regulations; Revisions to New Source Review Program (83 Fed. Reg. 44746 (August 31, 2018) Docket No. EPA-HQ-OAR-2017-0355 Submitted via regulations.gov Environmental and public health organizations Clean Air Task Force, Natural Resources Defense Council, Center for Biological Diversity, Clean Air Council, Clean Wisconsin, Conservation Law Foundation, Dogwood Alliance, Partnership for Policy Integrity, and Sierra Club hereby submit the following comments on the “best system of emission reduction” and other issues EPA’s proposed rule “Emission Guidelines for Greenhouse Gas Emissions from EXisting Electric Utility Generating Units; Revisions to Emission Guideline Implementing Regulations; Revisions to New Source Review Program,” 83 Fed. Reg. 44,746 (Aug. 31, 2018). [I] Overview Climate change continues to intensify and threaten public health and welfare. A recent report from the Intergovernmental Panel on Climate Change (IPCC) concludes that if greenhouse gas (GHG) emissions continue at the current rate, the atmosphere will warm by as much as 1.5°C (or 2.7°F) by 2040.1 “Climate-related risks to health, livelihoods, food security, water supply, human security, and economic growth are projected to increase with global warming of 1.5°C and increase further with 2°C.”2 The power sector was responsible for 29 percent of the climate-warming GHGs emitted in the United States in 2017,3 making it imperative that the U.S. -
Del Progetto Einstein@Home, Scoprono Una Nuova Pulsar Nei Dati Del Radio Telescopio Di Arecibo
Gente comune, ‘’scienziati’’ del progetto Einstein@Home, scoprono una nuova pulsar nei dati del radio telescopio di Arecibo. I computer inattivi sono un po’ come il parco giochi degli astronomi: tre persone comuni, un tedesco ed una coppia in America, hanno scoperto una pulsar nascosta nei dati raccolti dall’osservatorio di Arecibo. Questa e’ la prima scoperta dello spazio profondo da parte di Einstein@Home, un progetto che utilizza il tempo di calcolo donato da 250 000 volontari in 192 differenti paesi. I volontari mettono a disposizione i propri computer quando non li stanno usando (Science Express, Aug. 12, 2010.). I volontari i cui computer hanno fatto la scoperta sono Chris ed Helen Colvin, di Ames, nell’Iowa, USA, e Daniel Gebhardt dell’universita’ di Mainz , dipartimento di informatica musicale, Germania. I loro computer, assieme agli altri 500 000 sparsi in tutto il mondo, analizzano dati per Einstein@Home (in media ogni volontario contribuisce con due computer). La nuova pulsar, chiamata PSR J2007+2722, e’ una stella di neutroni che ruota su se’ stessa 41 volte al secondo. La pulsar si trova nella Via Lattea nella costellazione Vulpecula a circa 17 000 anni luce dalla Terra. A differenza delle altre pulsar che ruotano velocemente e stabilmente come lei, J2007+2722 se ne sta tutta sola nello spazio senza nessun’altra stella compagna ad orbitarle attorno. Gli astronomi ritengono che J2007+2722 sia particolarmente interessante perche’ e’ probabilmente una pulsar riciclata che ha perso durante la propria evoluzione la stella compagna. Questa ipotesi, seppure la piu’ interessante, rimane tuttavia una ipotesi e altri scenari sono possibili, per esempio che J2007+2722 sia una pulsar giovane nata con un campo magnetico piu’ basso del normale. -
Max Planck Society's Careful Planning Reaps Benefits
briefing Within the east German research insti- “We were not treated unfairly, according tutes of the Leibniz Society, three-quarters of to western rules,” he says. “But the rules were institute directors, and over a third of depart- ost see the against us. For example, the selection process ment heads, come from west Germany. The West German was in English, whereas we could have done directors of the three new national research M better in Russian, and publication record was centres are west Germans, and 55 per cent of ‘takeover’ as having a major criterion, whereas we had had few department heads are from west Germany chances to publish in western journals.” with a further eight per cent coming from been inevitable There were also cultural differences. “We abroad. all spoke German, yet after 40 years of cultur- Even more extreme ratios exist in the 20 peared for the good of east Germany’s scien- al divide it was hard to really talk to each Max Planck institutes, with only three of the tific future, he says. At his own Institute for other,” says Horst Franz Kern, dean of sci- 240 institute directors and department Plant Biochemistry, from which he retired as ence at the University of Marburg, who heads being east Germans. In contrast to director at the end of 1997, “even those hired chaired the Wissenschaftsrat’s committee on universities and other research organiza- on temporary grant money come increas- biology and medicine at the time of the tions, 40 per cent of these top jobs are occu- ingly from west Germany”. -
Solar Orbiter and Sentinels
HELEX: Heliophysical Explorers: Solar Orbiter and Sentinels Report of the Joint Science and Technology Definition Team (JSTDT) PRE-PUBLICATION VERSION 1 Contents HELEX Joint Science and Technology Definition Team .................................................................. 3 Executive Summary ................................................................................................................................. 4 1.0 Introduction ........................................................................................................................................ 6 1.1 Heliophysical Explorers (HELEX): Solar Orbiter and the Inner Heliospheric Sentinels ........ 7 2.0 Science Objectives .............................................................................................................................. 8 2.1 What are the origins of the solar wind streams and the heliospheric magnetic field? ............. 9 2.2 What are the sources, acceleration mechanisms, and transport processes of solar energetic particles? ........................................................................................................................................ 13 2.3 How do coronal mass ejections evolve in the inner heliosphere? ............................................. 16 2.4 High-latitude-phase science ......................................................................................................... 19 3.0 Measurement Requirements and Science Implementation ........................................................ 20 -
The Digital Agenda the Context
GERMAN PRESIDENCY OF THE EU THE DIGITAL AGENDA THE CONTEXT The COVID-19 crisis has reinforced the importance of digital transformation at European level. With the global competitiveness of the EU being at stake, Germany assumes the Presidency with a renewed sense to drive Europe’s digital future forward. In the upcoming months, the German government’s key priority will be to strengthen the EU’s ‘digi- tal sovereignty’. With this leitmotiv, the Presidency will focus on rolling out a resilient European digital and data infrastructure ecosystem, implement several steps of the EU’s strategy for “A Europe Fit for the Digital Age” and boost competencies in key digital technologies through coordinated R&D and in- vestment efforts. An important challenge will be to ensure effective cross-ministerial coordination on digital policies af- fecting the European Green Deal, health, transport, and consumer protection policies. KEY INITIATIVES AND FILES THE KEY HUB • Strengthen the EU’s digital sovereignty following lessons Peter Altmaier learnt from the COVID-19 pandemic by laying the groundwork • Born in 1958 for the roll out of the European cloud project GAIA-X. • Federal Minister for • Support the implementation of the EU’s strategy for A Economic Affairs and Energy Europe Fit for the Digital Age with a focus on data availabil- ity and security, AI, and digital skills. This includes achieving • Member of Christian Democratic progress on the European Data Strategy with the launch of Union of Germany (CDU) guidelines for the governance of Common European Data Spaces, promoting a human-centred and ethical approach • Presiding over the Ministerial Council for to AI at EU level and discussing the European Commission’s telecommunications / digital affairs and key Digital Education Action Plan. -
Max Planck Institute for Intelligent Systems
Max Planck Institute for Intelligent Systems Stuttgart Center for Electron Microscopy – StEM Heisenbergstrasse 3, D-70569, Stuttgart, Germany www.mf.mpg.de/StEM International Workshop at Ringberg Castle, Lake Tegernsee, Germany July 27th – July 29th, 2011 Programme – updated version Current topics in Transmission Electron Microscopy: “Plasmonics” and “Tomography” Wednesday, July 27th, 2011 15:00 – 15:10 Opening and Welcome Peter A. van Aken Plasmonics (Chair: Peter van Aken) 15:10 – 15:50 Ralf Vogelgesang, Stuttgart Near-field optics of nanoplasmonic structures 15:50 – 16:30 Duncan Alexander, Lausanne Cathodoluminescence and EELS of photonic crystals 16:30 – 17:00 Coffee break 17:00 – 17:40 Jorge Bravo-Abad, Madrid Molding the flow of Terahertz radiation using holey metamaterials 18:30 Dinner After 20:00 Posters & Beer Thursday, July 28th, 2011 Plasmonics (Chair: Wilfried Sigle/Peter van Aken) 09:00 – 09:40 Marcus Rommel, Stuttgart Electron beam lithography 09:40 – 10:20 Maria Eugenia Toimil-Molares, Darmstadt Preparation and characterization of metallic nanorods 10:20 – 11:00 Coffee break 11:00 – 11:40 Toon Coenen, Amsterdam Angle-resolved cathodoluminescence spectroscopy on plasmonic nanoantennas 11:40 – 12:20 Wilfried Sigle, Stuttgart TEM methods for valence-loss spectroscopy 12:30 Lunch page 2, Programme International Workshop at Ringberg Castle, Lake Tegernsee, Germany Thursday, July 28th, 2011 Plasmonics (Chair: Christoph Koch) 14:00 – 14:40 Burcu Ögüt, Stuttgart EFTEM and FEM simulation of plasmonic modes in nanoslits 14:40 – 15:20 Javier Garcia de Abajo, Madrid Valence electron loss theory 15:20 – 16:00 Coffee break 16.00 – 16:40 Paul A. Midgley, Cambridge UK Electron spectroscopy of plasmons in silver nanocubes and other geometries 16:40 – 17:20 Falk Roeder, Dresden Inelastic holography for investigating surface plasmons 18:30 Dinner Friday, July 29th, 2011 Tomography (Chair: Fritz Phillipp) 09:00 – 09:40 Rafal E. -
Research Environment
Bingen 25 km (16 miles) Selected Academic Institutions Research Environment Wiesbaden 8 km Goethe University Frankfurt Ernst Strüngmann Institute for Cognitive Wiesbaden University of Applied Sciences Brain Research of the Max Planck Society Frankfurt Institute for Advanced Studies Ingelheim Max Planck Institute for Biophysics 12 km Max Planck Institute for Brain Research Selected Research Companies Boehringer Ingelheim AEterna Zentaris Inc BayerCrop Science SCHOTT AG Roman-Germanic Museum Merz JGU Campus (Institute of the Leibniz Society) Sanofi-Aventis Johannes Gutenberg University (JGU) Museum of Natural History Mainz Max Planck Institute for Chemistry Mainz Institute of European History Mainz Max Planck Institute for Polymer Research (Institute of the Leibniz Society) Max Planck Graduate Center with the JGU Frankfurt Helmholtz Institute Mainz 35 km University School of Music Frankfurt Airport 23 km Selected Research Companies Catholic University of Applied Sciences Mainz GENterprise Genomics GmbH University School of Art Academic Institutions Selected Research Companies Academic Institutions Mainz University of Applied Sciences University Medical School Ganymed Pharmaceuticals AG Darmstadt University of Applied Sciences Institute of Translational Oncology (TRON) Darmstadt Technical University Selected Research Companies Academy of Sciences and Literature Mainz Merck KGaA IBM Mainz 0 1 2 km IMM Institute of Microtechnology Mainz Darmstadt 30 km 0 1 mile Facts about Mainz Facts about Frankfurt Facts about Darmstadt Facts about Wiesbaden -
Abstract Book
Table of Contents: Item: Page Background Information a Committees b Sponsors c Hotel d Conference Venue e Local Area f Social Programme g Timetable h Conference Programme & List of Posters i - xviii Programme Abstracts 1 – 63 Poster Abstracts P1 – P231 a SOHO 17: 10 Years of SOHO and Beyond Background: The Solar and Heliospheric Observatory (SOHO) is a mission of international cooperation between ESA and NASA to study the Sun, from its deep core to the outer corona, the solar wind, and the interaction with the interstellar medium. It was launched a decade ago on 2 December 1995, and in April 2006 it will have completed 10 years of successful scientific operations. In celebration of this milestone, we are organizing a meeting to review the many and varied scientific accomplishments of SOHO. An important focus of the meeting will be the conceptual and theoretical advances that coordinated multi- instrument and multi-mission observations of the Sun have helped us make in the last decade, and to examine the role that the continued observations of SOHO will play within the context of future missions. The meeting will cover the full breadth of SOHO science, organised around the following seven sessions: 1) Solar Interior: From Exploration to Experimentation Invited speakers: D. Gough, S. Basu, T. Corbard 2) Magnetic Variability: From the Tachocline to the Heliosphere Invited speakers: L. Gizon, S. Tobias, Z. Mikic 3) Atmospheric Heating and Solar Wind Origin: MHD vs. Plasma Physics Invited speakers: J. Klimchuk, V. Hansteen, G. Poletto 4) Solar Variability and its Effects on the Heliosphere and the Earth Invited speakers: P. -
An Insight Into Space Weather Ashish Mishra1*, Mukul Kumar1,2* 1 Department of Physics, Indian Institute of Science Education and Research Bhopal, India
Advanced Journal of Graduate Research ISSN:2456-7108 Volume 2, Issue 1, pp. 46-57, July 2017 GRADUATE REVIEW ARTICLE An Insight into Space Weather Ashish Mishra1*, Mukul Kumar1,2* 1 Department of Physics, Indian Institute of Science Education and Research Bhopal, India. 2 State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China. doi : https://doi.org/10.21467/ajgr.2.1.46-57 ABSTRACT * Corresponding Author email: The present article gives a brief overview of space weather and 1 [email protected] its drivers. The space weather is of immense importance for the 2 [email protected] spaceborne and ground-based technological systems. The Article History satellites, the power grids, telecommunication and in severe Received: 27 November 2017 conditions the human lives are at risk. The article covers the Revised: 26 December 2017 effects of solar transient activities (e.g. Solar flares, Coronal mass Accepted: 27 December 2017 ejections and Solar winds etc.) and their consequences on the Published: 27 December 2017 Earth’s atmosphere. The space weather is the change in the conditions of interplanetary space because of the solar transient Student(s) activities. We also discussed the importance of the solar wind • Ashish Mishra which is a continuous flow of the charged energy particles from the Sun to the Earth in respect of the space weather. This article Academic Year: 2015-16, 1st Semester also put light on the Sun-Earth connection and effects of the Course Level: Bachelor Degree space weather on it. The Earth’s magnetosphere, formed by the Course Name: BS-MS dual degree program interaction of solar wind and Earth’s magnetic field behaves like 4th Year / 8th Semester Course year: a shield for the Earth against the solar wind. -
Programme 70Th Lindau Nobel Laureate Meeting 27 June - 2 July 2021
70 Programme 70th Lindau Nobel Laureate Meeting 27 June - 2 July 2021 Sessions Speakers Access Background Scientific sessions, Nobel Laureates, Clear guidance Everything else social functions, young scientists, to all viewing there is to know partner events, invited experts, and participation for a successful networking breaks moderators options meeting 2 Welcome Two months ago, everything was well on course to celebrate And yet: this interdisciplinary our 70th anniversary with you, in Lindau. anniversary meeting will feature But with the safety and health of all our participants being the most rich and versatile programme ever. of paramount importance, we were left with only one choice: It will provide plenty of opportunity to educate, inspire, go online. connect – and to celebrate! Join us. 4 PARTICIPATING LAUREATES 4 PARTICIPATING LAUREATES 5 Henry A. Joachim Donna George P. Hartmut Michael M. Adam Hiroshi Kissinger Frank Strickland Smith Michel Rosbash Riess Amano Jeffrey A. Peter Richard R. James P. Randy W. Brian K. Barry C. Dean Agre Schrock Allison Schekman Kobilka Barish John L. Harvey J. Robert H. J. Michael Martin J. Hall Alter Grubbs Kosterlitz Evans F. Duncan David J. Ben L. Edmond H. Carlo Brian P. Kailash Elizabeth Haldane Gross Feringa Fischer Rubbia Schmidt Satyarthi Blackburn Robert B. Reinhard Aaron Walter Barry J. Harald Takaaki Laughlin Genzel Ciechanover Gilbert Marshall zur Hausen Kajita Christiane Serge Steven Françoise Didier Martin Nüsslein- Haroche Chu Barré-Sinoussi Queloz Chalfie Volhard Anthony J. Gregg L. Robert J. Saul Klaus William G. Leggett Semenza Lefkowitz Perlmutter von Klitzing Kaelin Jr. Stefan W. Thomas C. Emmanuelle Kurt Ada Konstantin S. -
Generation and Dissipation of Alfvén-Cyclotron Turbulence in the Solar Corona and Solar Wind and Related Ion Differential Heating and Acceleration
Generation and dissipation of Alfvén-cyclotron turbulence in the solar corona and solar wind and related ion differential heating and acceleration Dissertation zur Erlangung des mathematisch-naturwissenschaftlichen Doktorgrades “Doctor rerum naturalium” der Georg-August-Universität Göttingen vorgelegt von Yana Georgieva Maneva aus Sofia, Bulgarien Göttingen 2010 Bibliografische Information der Deutschen Nationalbibliothek Die Deutsche Nationalbibliothek verzeichnet diese Publikation in der Deutschen Nationalbibliografie; detaillierte bibliografische Daten sind im Internet über http://dnb.d-nb.de abrufbar. Referent: Prof. Dr. Stefan Dreizler Korreferent: Prof. Dr. Eckart Marsch Tag der mündlichen Prüfung: 24.09.2010 ISBN 978-3-942171-39-7 uni-edition GmbH 2010 http://www.uni-edition.de c Yana Georgieva Maneva This work is distributed under a Creative Commons Attribution 3.0 License Printed in Germany Contents Summary 5 1 Introduction 7 1.1 The solar corona and the solar wind - overview and plasma parameters . .7 1.1.1 Solar corona . .7 1.1.2 Solar wind: types and origin . .9 1.1.3 Plasma composition and collisional conditions . 11 1.2 Observations of Alfvén waves in the solar corona and fast solar wind . 16 1.3 Motivation, scope and outline of the present work . 18 2 Plasma kinetics in the corona and the solar wind 23 2.1 Common features, observed in the corona and the fast solar wind . 24 2.1.1 Velocity distributions . 25 2.1.2 Temperature profiles and kinetic temperature ratios . 27 2.1.3 Ion anisotropies and differential streaming . 30 3 Analytical description of nonlinear couplings in multi-species plasmas 35 3.1 Parametric instabilities .