Influence of Solar Minimum on Cosmic Ray Flux, Mutations in Viruses and Pandemics Like COVID-19
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→ Investigating Solar Cycles a Soho Archive & Ulysses Final Archive Tutorial
→ INVESTIGATING SOLAR CYCLES A SOHO ARCHIVE & ULYSSES FINAL ARCHIVE TUTORIAL SCIENCE ARCHIVES AND VO TEAM Tutorial Written By: Madeleine Finlay, as part of an ESAC Trainee Project 2013 (ESA Student Placement) Tutorial Design and Layout: Pedro Osuna & Madeleine Finlay Tutorial Science Support: Deborah Baines Acknowledgements would like to be given to the whole SAT Team for the implementation of the Ulysses and Soho archives http://archives.esac.esa.int We would also like to thank; Benjamín Montesinos, Department of Astrophysics, Centre for Astrobiology (CAB, CSIC-INTA), Madrid, Spain for having reviewed and ratified the scientific concepts in this tutorial. CONTACT [email protected] [email protected] ESAC Science Archives and Virtual Observatory Team European Space Agency European Space Astronomy Centre (ESAC) Tutorial → CONTENTS PART 1 ....................................................................................................3 BACKGROUND ..........................................................................................4-5 THE EXPERIMENT .......................................................................................6 PART 1 | SECTION 1 .................................................................................7-8 PART 1 | SECTION 2 ...............................................................................9-11 PART 2 ..................................................................................................12 BACKGROUND ........................................................................................13-14 -
Apocalypse Now? Initial Lessons from the Covid-19 Pandemic for the Governance of Existential and Global Catastrophic Risks
journal of international humanitarian legal studies 11 (2020) 295-310 brill.com/ihls Apocalypse Now? Initial Lessons from the Covid-19 Pandemic for the Governance of Existential and Global Catastrophic Risks Hin-Yan Liu, Kristian Lauta and Matthijs Maas Faculty of Law, University of Copenhagen, Copenhagen, Denmark [email protected]; [email protected]; [email protected] Abstract This paper explores the ongoing Covid-19 pandemic through the framework of exis- tential risks – a class of extreme risks that threaten the entire future of humanity. In doing so, we tease out three lessons: (1) possible reasons underlying the limits and shortfalls of international law, international institutions and other actors which Covid-19 has revealed, and what they reveal about the resilience or fragility of institu- tional frameworks in the face of existential risks; (2) using Covid-19 to test and refine our prior ‘Boring Apocalypses’ model for understanding the interplay of hazards, vul- nerabilities and exposures in facilitating a particular disaster, or magnifying its effects; and (3) to extrapolate some possible futures for existential risk scholarship and governance. Keywords Covid-19 – pandemics – existential risks – global catastrophic risks – boring apocalypses 1 Introduction: Our First ‘Brush’ with Existential Risk? All too suddenly, yesterday’s ‘impossibilities’ have turned into today’s ‘condi- tions’. The impossible has already happened, and quickly. The impact of the Covid-19 pandemic, both directly and as manifested through the far-reaching global societal responses to it, signal a jarring departure away from even the © koninklijke brill nv, leiden, 2020 | doi:10.1163/18781527-01102004Downloaded from Brill.com09/27/2021 12:13:00AM via free access <UN> 296 Liu, Lauta and Maas recent past, and suggest that our futures will be profoundly different in its af- termath. -
Riley Et Al., 2015
The Astrophysical Journal, 802:105 (14pp), 2015 April 1 doi:10.1088/0004-637X/802/2/105 © 2015. The American Astronomical Society. All rights reserved. INFERRING THE STRUCTURE OF THE SOLAR CORONA AND INNER HELIOSPHERE DURING THE MAUNDER MINIMUM USING GLOBAL THERMODYNAMIC MAGNETOHYDRODYNAMIC SIMULATIONS Pete Riley1, Roberto Lionello1, Jon A. Linker1, Ed Cliver2, Andre Balogh3, Jürg Beer4, Paul Charbonneau5, Nancy Crooker6, Marc DeRosa7, Mike Lockwood8, Matt Owens8, Ken McCracken9, Ilya Usoskin10, and S. Koutchmy11 1 Predictive Science, 9990 Mesa Rim Road, Suite 170, San Diego, CA 92121, USA; [email protected], [email protected], [email protected] 2 National Solar Observatory, Sunspot, NM 88349, USA; [email protected] 3 Imperial College, South Kensington Campus, Department of Physics, Huxley Building 6M68, London, SW7 2AZ, UK; [email protected] 4 Surface Waters, Eawag, Ueberlandstrasse 133, P.O. Box 611, 8600 Duebendorf, Switzerland; [email protected] 5 Département de Physique, Université de Montréal, C.P. 6128 Centre-Ville, Montréal, Qc, H3C-3J7, Canada; [email protected] 6 Center for Space Physics, Boston University, 725 Commonwealth Avenue, Boston, MA 02215, USA; [email protected] 7 Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover St., B/252, Palo Alto, CA 94304, USA; [email protected] 8 University of Reading, Department of Meteorology, Reading, Berkshire, RG6 6BB, UK; [email protected], [email protected] 9 100 Mt. Jellore Lane, Woodlands, NSW, 2575, Australia; [email protected] 10 Sodankyla Geophysical Observatory, FIN-90014, University of Oulu, Finland; ilya.usoskin@oulu.fi 11 Institut d’Astrophysique de Paris, CNRS and UPMC, Paris, France; [email protected] Received 2014 September 29; accepted 2015 January 29; published 2015 March 30 ABSTRACT Observations of the Sun’s corona during the space era have led to a picture of relatively constant, but cyclically varying solar output and structure. -
A Spectral Solar/Climatic Model H
A Spectral Solar/Climatic Model H. PRESCOTT SLEEPER, JR. Northrop Services, Inc. The problem of solar/climatic relationships has prove our understanding of solar activity varia- been the subject of speculation and research by a tions have been based upon planetary tidal forces few scientists for many years. Understanding the on the Sun (Bigg, 1967; Wood and Wood, 1965.) behavior of natural fluctuations in the climate is or the effect of planetary dynamics on the motion especially important currently, because of the pos- of the Sun (Jose, 1965; Sleeper, 1972). Figure 1 sibility of man-induced climate changes ("Study presents the sunspot number time series from of Critical Environmental Problems," 1970; "Study 1700 to 1970. The mean 11.1-yr sunspot cycle is of Man's Impact on Climate," 1971). This paper well known, and the 22-yr Hale magnetic cycle is consists of a summary of pertinent research on specified by the positive and negative designation. solar activity variations and climate variations, The magnetic polarity of the sunspots has been together with the presentation of an empirical observed since 1908. The cycle polarities assigned solar/climatic model that attempts to clarify the prior to that date are inferred from the planetary nature of the relationships. dynamic effects studied by Jose (1965). The sun- The study of solar/climatic relationships has spot time series has certain important characteris- been difficult to develop because of an inadequate tics that will be summarized. understanding of the detailed mechanisms respon- sible for the interaction. The possible variation of Secular Cycles stratospheric ozone with solar activity has been The sunspot cycle magnitude appears to in- discussed by Willett (1965) and Angell and Kor- crease slowly and fall rapidly with an. -
COVID-19: Make It the Last Pandemic
COVID-19: Make it the Last Pandemic Disclaimer: The designations employed and the presentation of the material in this publication do not imply the expression of any opinion whatsoever on the part of the Independent Panel for Pandemic Preparedness and Response concerning the legal status of any country, territory, city of area or of its authorities, or concerning the delimitation of its frontiers or boundaries. Report Design: Michelle Hopgood, Toronto, Canada Icon Illustrator: Janet McLeod Wortel Maps: Taylor Blake COVID-19: Make it the Last Pandemic by The Independent Panel for Pandemic Preparedness & Response 2 of 86 Contents Preface 4 Abbreviations 6 1. Introduction 8 2. The devastating reality of the COVID-19 pandemic 10 3. The Panel’s call for immediate actions to stop the COVID-19 pandemic 12 4. What happened, what we’ve learned and what needs to change 15 4.1 Before the pandemic — the failure to take preparation seriously 15 4.2 A virus moving faster than the surveillance and alert system 21 4.2.1 The first reported cases 22 4.2.2 The declaration of a public health emergency of international concern 24 4.2.3 Two worlds at different speeds 26 4.3 Early responses lacked urgency and effectiveness 28 4.3.1 Successful countries were proactive, unsuccessful ones denied and delayed 31 4.3.2 The crisis in supplies 33 4.3.3 Lessons to be learnt from the early response 36 4.4 The failure to sustain the response in the face of the crisis 38 4.4.1 National health systems under enormous stress 38 4.4.2 Jobs at risk 38 4.4.3 Vaccine nationalism 41 5. -
Level and Length of Cyclic Solar Activity During the Maunder Minimum As Deduced from the Active-Day Statistics
A&A 577, A71 (2015) Astronomy DOI: 10.1051/0004-6361/201525962 & c ESO 2015 Astrophysics Level and length of cyclic solar activity during the Maunder minimum as deduced from the active-day statistics J. M. Vaquero1,G.A.Kovaltsov2,I.G.Usoskin3, V. M. S. Carrasco4, and M. C. Gallego4 1 Departamento de Física, Universidad de Extremadura, 06800 Mérida, Spain 2 Ioffe Physical-Technical Institute, 194021 St. Petersburg, Russia 3 Sodankylä Geophysical Observatory and ReSoLVE Center of Excellence, University of Oulu, 90014 Oulu, Finland e-mail: [email protected] 4 Departamento de Física, Universidad de Extremadura, 06071 Badajoz, Spain Received 25 February 2015 / Accepted 25 March 2015 ABSTRACT Aims. The Maunder minimum (MM) of greatly reduced solar activity took place in 1645–1715, but the exact level of sunspot activity is uncertain because it is based, to a large extent, on historical generic statements of the absence of spots on the Sun. Using a conservative approach, we aim to assess the level and length of solar cycle during the MM on the basis of direct historical records by astronomers of that time. Methods. A database of the active and inactive days (days with and without recorded sunspots on the solar disc) is constructed for three models of different levels of conservatism (loose, optimum, and strict models) regarding generic no-spot records. We used the active day fraction to estimate the group sunspot number during the MM. Results. A clear cyclic variability is found throughout the MM with peaks at around 1655–1657, 1675, 1684, 1705, and possibly 1666, with the active-day fraction not exceeding 0.2, 0.3, or 0.4 during the core MM, for the three models. -
Relation Between Sunspots and Covid19 – a Proof for Panspermia
International Research Journal of Engineering and Technology (IRJET) e-ISSN: 2395-0056 Volume: 07 Issue: 11 | Nov 2020 www.irjet.net p-ISSN: 2395-0072 RELATION BETWEEN SUNSPOTS AND COVID19 – A PROOF FOR PANSPERMIA Janani T1 1Department of Biotechnology, Kumaraguru College of Technology, Coimbatore, Tamilnadu, India ---------------------------------------------------------------------***---------------------------------------------------------------------- Abstract - The novel viral or the bacterial pandemics and epidemics are not new to this earth. Often these disease-causing pathogens are of unknown origin and often identified as an infection which is transmitted from other animals. They are frequently found as the mutated form of the original strain or completely a newly developed strain. The causes for this mutation are many which comprises of both natural and artificial sources. The time of occurrence of these pandemic and epidemic astonishingly coincides with the sun spot extremum (often minimum). It is observed that whenever there is a sun spot extremum there was a novel microbial pandemic or epidemic. The current COVID19 pandemic is also suggested to be due to such sunspot extremum as the sun cycle is currently at its sun spot minimum. This review aims at providing the facts of relation between sunspots and the novel corona virus pandemic and there by stating this occurrence as a proof for panspermia. Key Words: Pandemic, Epidemic, COVID19, Sunspot, Solar Cycle, Solar minimum, Panspermia 1. INTRODUCTION 1.1 SUNSPOTS: Sunspots are the dark regions in the sun’s surface due to the concentration of magnetic field in that region. These regions are relatively colder to the other regions of the sun’s surface. Hotter region emits more light than the colder region hence these regions appear to be darker and called the spots of the sun. -
The Maunder Minimum and the Variable Sun-Earth Connection
The Maunder Minimum and the Variable Sun-Earth Connection (Front illustration: the Sun without spots, July 27, 1954) By Willie Wei-Hock Soon and Steven H. Yaskell To Soon Gim-Chuan, Chua Chiew-See, Pham Than (Lien+Van’s mother) and Ulla and Anna In Memory of Miriam Fuchs (baba Gil’s mother)---W.H.S. In Memory of Andrew Hoff---S.H.Y. To interrupt His Yellow Plan The Sun does not allow Caprices of the Atmosphere – And even when the Snow Heaves Balls of Specks, like Vicious Boy Directly in His Eye – Does not so much as turn His Head Busy with Majesty – ‘Tis His to stimulate the Earth And magnetize the Sea - And bind Astronomy, in place, Yet Any passing by Would deem Ourselves – the busier As the Minutest Bee That rides – emits a Thunder – A Bomb – to justify Emily Dickinson (poem 224. c. 1862) Since people are by nature poorly equipped to register any but short-term changes, it is not surprising that we fail to notice slower changes in either climate or the sun. John A. Eddy, The New Solar Physics (1977-78) Foreword By E. N. Parker In this time of global warming we are impelled by both the anticipated dire consequences and by scientific curiosity to investigate the factors that drive the climate. Climate has fluctuated strongly and abruptly in the past, with ice ages and interglacial warming as the long term extremes. Historical research in the last decades has shown short term climatic transients to be a frequent occurrence, often imposing disastrous hardship on the afflicted human populations. -
Predicting Maximum Sunspot Number in Solar Cycle 24 Nipa J Bhatt
J. Astrophys. Astr. (2009) 30, 71–77 Predicting Maximum Sunspot Number in Solar Cycle 24 Nipa J Bhatt1,∗, Rajmal Jain2 & Malini Aggarwal2 1C. U. Shah Science College, Ashram Road, Ahmedabad 380 014, India. 2Physical Research Laboratory, Navrangpura, Ahmedabad 380 009, India. ∗e-mail: [email protected] Received 2008 November 22; accepted 2008 December 23 Abstract. A few prediction methods have been developed based on the precursor technique which is found to be successful for forecasting the solar activity. Considering the geomagnetic activity aa indices during the descending phase of the preceding solar cycle as the precursor, we predict the maximum amplitude of annual mean sunspot number in cycle 24 to be 111 ± 21. This suggests that the maximum amplitude of the upcoming cycle 24 will be less than cycles 21–22. Further, we have estimated the annual mean geomagnetic activity aa index for the solar maximum year in cycle 24 to be 20.6 ± 4.7 and the average of the annual mean sunspot num- ber during the descending phase of cycle 24 is estimated to be 48 ± 16.8. Key words. Sunspot number—precursor prediction technique—geo- magnetic activity index aa. 1. Introduction Predictions of solar and geomagnetic activities are important for various purposes, including the operation of low-earth orbiting satellites, operation of power grids on Earth, and satellite communication systems. Various techniques, namely, even/odd behaviour, precursor, spectral, climatology, recent climatology, neural networks have been used in the past for the prediction of solar activity. Many investigators (Ohl 1966; Kane 1978, 2007; Thompson 1993; Jain 1997; Hathaway & Wilson 2006) have used the ‘precursor’ technique to forecast the solar activity. -
Solar Wind Variation with the Cycle I. S. Veselovsky,* A. V. Dmitriev
J. Astrophys. Astr. (2000) 21, 423–429 Solar Wind Variation with the Cycle I. S. Veselovsky,* A. V. Dmitriev, A. V. Suvorova & M. V. Tarsina, Institute of Nuclear Physics, Moscow State University, 119899 Moscow, Russia. *e-mail: [email protected] Abstract. The cyclic evolution of the heliospheric plasma parameters is related to the time-dependent boundary conditions in the solar corona. “Minimal” coronal configurations correspond to the regular appearance of the tenuous, but hot and fast plasma streams from the large polar coronal holes. The denser, but cooler and slower solar wind is adjacent to coronal streamers. Irregular dynamic manifestations are present in the corona and the solar wind everywhere and always. They follow the solar activity cycle rather well. Because of this, the direct and indirect solar wind measurements demonstrate clear variations in space and time according to the minimal, intermediate and maximal conditions of the cycles. The average solar wind density, velocity and temperature measured at the Earth's orbit show specific decadal variations and trends, which are of the order of the first tens per cent during the last three solar cycles. Statistical, spectral and correlation characteristics of the solar wind are reviewed with the emphasis on the cycles. Key words. Solar wind—solar activity cycle. 1. Introduction The knowledge of the solar cycle variations in the heliospheric plasma and magnetic fields was initially based on the indirect indications gained from the observations of the Sun, comets, cosmic rays, geomagnetic perturbations, interplanetary scintillations and some other ground-based methods. Numerous direct and remote-sensing space- craft measurements in situ have continuously broadened this knowledge during the past 40 years, which can be seen from the original and review papers. -
Global Catastrophic Risks Survey
GLOBAL CATASTROPHIC RISKS SURVEY (2008) Technical Report 2008/1 Published by Future of Humanity Institute, Oxford University Anders Sandberg and Nick Bostrom At the Global Catastrophic Risk Conference in Oxford (17‐20 July, 2008) an informal survey was circulated among participants, asking them to make their best guess at the chance that there will be disasters of different types before 2100. This report summarizes the main results. The median extinction risk estimates were: Risk At least 1 million At least 1 billion Human extinction dead dead Number killed by 25% 10% 5% molecular nanotech weapons. Total killed by 10% 5% 5% superintelligent AI. Total killed in all 98% 30% 4% wars (including civil wars). Number killed in 30% 10% 2% the single biggest engineered pandemic. Total killed in all 30% 10% 1% nuclear wars. Number killed in 5% 1% 0.5% the single biggest nanotech accident. Number killed in 60% 5% 0.05% the single biggest natural pandemic. Total killed in all 15% 1% 0.03% acts of nuclear terrorism. Overall risk of n/a n/a 19% extinction prior to 2100 These results should be taken with a grain of salt. Non‐responses have been omitted, although some might represent a statement of zero probability rather than no opinion. 1 There are likely to be many cognitive biases that affect the result, such as unpacking bias and the availability heuristic‒‐well as old‐fashioned optimism and pessimism. In appendix A the results are plotted with individual response distributions visible. Other Risks The list of risks was not intended to be inclusive of all the biggest risks. -
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