The New Grand Minimum New Skills Have Been Developed by Actuaries If They Are to Understand the Changes in Risks That Are Occurring in the New Solar Grand Minimum
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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. -
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. -
Statistical Properties of Superactive Regions During Solar Cycles 19–23⋆
A&A 534, A47 (2011) Astronomy DOI: 10.1051/0004-6361/201116790 & c ESO 2011 Astrophysics Statistical properties of superactive regions during solar cycles 19–23 A. Q. Chen1,2,J.X.Wang1,J.W.Li2,J.Feynman3, and J. Zhang1 1 Key Laboratory of Solar Activity of Chinese Academy of Sciences, National Astronomical Observatories, Chinese Academy of Sciences, PR China e-mail: [email protected]; [email protected] 2 National Center for Space Weather, China Meteorological Administration, PR China 3 Helio research, 5212 Maryland Avenue, La Crescenta, USA Received 26 February 2011 / Accepted 20 August 2011 ABSTRACT Context. Each solar activity cycle is characterized by a small number of superactive regions (SARs) that produce the most violent of space weather events with the greatest disastrous influence on our living environment. Aims. We aim to re-parameterize the SARs and study the latitudinal and longitudinal distributions of SARs. Methods. We select 45 SARs in solar cycles 21–23, according to the following four parameters: 1) the maximum area of sunspot group, 2) the soft X-ray flare index, 3) the 10.7 cm radio peak flux, and 4) the variation in the total solar irradiance. Another 120 SARs given by previous studies of solar cycles 19–23 are also included. The latitudinal and longitudinal distributions of the 165 SARs in both the Carrington frame and the dynamic reference frame during solar cycles 19–23 are studied statistically. Results. Our results indicate that these 45 SARs produced 44% of all the X class X-ray flares during solar cycles 21–23, and that all the SARs are likely to produce a very fast CME. -
Space Weather — History and Current Status
Space Weather — History and Current Status Ji Wu National Space Science Center, CAS Oct. 3, 2017 1 Contents 1. Beginning of Space Age and Dangerous Environment 2. The Dynamic Space Environment so far We Know 3. The Space Weather Concept and Current Programs 4. Looking at the Future Space Weather Programs 2 1.Beginning of Space Age and Dangerous Environment 3 Space Age Kai'erdishi Korolev Oct. 4, 1957, humanity‘s first artificial satellite, Sputnik-1, has launched, ushering in the Space Age. 4 Space Age Explorer 1 was the first satellite of the United States, launched on Jan 31, 1958, with scientific object to explore the radiation environment of geospace. 5 Unknown Space Environment Sputnik-2 (Nov 3, 1957) detected the Earth's outer radiation belt in the far northern latitudes, but researchers did not immediately realize the significance of the elevated radiation because Sputnik 2 passed through the Van Allen belt too far out of range of the Soviet tracking stations. Explorer-1 detected fewer cosmic rays in its orbit (which ranged from 220 miles from Earth to 1,563 miles) than Van Allen expected. 6 Space Age - unknown and dangerous space environment 7 Satellite failures due to the unknown and Particle dangerous space environment Radiation! Statistics show that the space radiation environment is one of the main causes of satellite failure. The space radiation environment caused about 2,300 satellite failures of all the 5000 failure events during the 1966-1994 period collected by the National Geophysical Data Center. Statistics of the United States in 1996 indicate that the space environment caused more than 40% of satellite failures in 1958-1986, and 36% in 1986-1996. -
Space Weather and Aviation Impacts
Space Weather and Aviation Impacts Char Dewey NOAA/National Weather Service Salt Lake City, UT @DeweyWx [email protected] IWAWS 2020 Space Weather and Aviation Impacts What is space weather? How space weather affects Earth and aviation; hazards and impacts How to monitor conditions and be space weather-aware Space Weather 101 Space Weather 101 Weather originating from the Sun and traveling the 93 million miles to reach Earth and our atmosphere, interacting with systems on and orbiting Earth. Observations come from satellite sources with instruments that monitor space weather. Model data (some now operational!) developing. Coronal Mass Ejections (CME), Solar Energetic Particles (SEP), and Solar Flares. Space Weather 101 Active regions on the sun are where solar activity begins; where sunspots are located on the solar disk. Magnetic “instability” where solar storming forms. Space Weather 101 Coronal Mass Ejections (CME) An eruption of plasma particles and electromagnetic radiation from the solar corona, often following solar flares. Originate from active regions on the Sun’s surface (sunspots). Very slow to reach the Earth from 12 hours to days or a week. Space Weather Impacts Coronal Mass Ejections (CME) Impacts: Geomagnetic storming compresses Earth’s magnetosphere on the day-side, extending night-side “tail” and reconnecting, focusing energy at the poles and resulting in Aurora. Increase electrons in the ionosphere at high-latitude regions, exposing to higher radiation values. Space Weather 101 Solar Energetic Particles (SEP) High-energy particles; protons, electrons Originate from solar flare or shock wave (CME) reaching the Earth from 20 minutes to many hours, depending the location it leaves the solar disk. -
On Polar Magnetic Field Reversal in Solar Cycles 21, 22, 23, and 24
On Polar Magnetic Field Reversal in Solar Cycles 21, 22, 23, and 24 Mykola I. Pishkalo Main Astronomical Observatory, National Academy of Sciences, 27 Zabolotnogo vul., Kyiv, 03680, Ukraine [email protected] Abstract The Sun’s polar magnetic fields change their polarity near the maximum of sunspot activity. We analyzed the polarity reversal epochs in Solar Cycles 21 to 24. There were a triple reversal in the N-hemisphere in Solar Cycle 24 and single reversals in the rest of cases. Epochs of the polarity reversal from measurements of the Wilcox Solar Observatory (WSO) are compared with ones when the reversals were completed in the N- and S-hemispheres. The reversal times were compared with hemispherical sunspot activity and with the Heliospheric Current Sheet (HCS) tilts, too. It was found that reversals occurred at the epoch of the sunspot activity maximum in Cycles 21 and 23, and after the corresponding maxima in Cycles 22 and 24, and one-two years after maximal HCS tilts calculated in WSO. Reversals in Solar Cycles 21, 22, 23, and 24 were completed first in the N-hemisphere and then in the S-hemisphere after 0.6, 1.1, 0.7, and 0.9 years, respectively. The polarity inversion in the near-polar latitude range ±(55–90)˚ occurred from 0.5 to 2.0 years earlier that the times when the reversals were completed in corresponding hemisphere. Using the maximal smoothed WSO polar field as precursor we estimated that amplitude of Solar Cycle 25 will reach 116±12 in values of smoothed monthly sunspot numbers and will be comparable with the current cycle amplitude equaled to 116.4. -
The Sun-Climate Connection John A
The Sun-Climate Connection John A. Eddy National Solar Observatory Tucson, Arizona Surely the oldest of all suspected solar-terrestrial connections—and by far the most important in terms of potential societal impacts—are probable links between solar variations and regional or global climate. Dramatic advances in recent years in both solar physics and in climatology have moved this age-old question out of the closet and into the light of more rigorous tests and examination. They also allow us to frame it more clearly in the context of other, competing or interactive climate change mechanisms. For the Sun, these advances include, among others, the results from a quarter century of radiometric monitoring of solar irradiance from space; the exploitation of naturally-sequestered cosmogenic isotope records to extend the known history of solar activity hundreds of thousands of years into the past; and success in defining the impacts of variations in solar ultraviolet radiation on stratospheric chemistry and dynamics. Similar seminal advances in what we know of climate and climatic change include vast improvements in our knowledge of the interactive climate system and in our ability to model and test possible forcing mechanisms; and the recovery and accumulation of longer and more extensive records of environmental changes of the past. In 2003, the NASA Living With a Star Program commissioned an interdisciplinary Task Group, which I chaired, to consider what is now known or suspected of the effects of solar variations on terrestrial climate; to frame the outstanding questions that currently limit progress; and to define current needs in Sun- Climate research. -
Redefining the Limit Dates for the Maunder Minimum J
Redefining the limit dates for the Maunder Minimum J. M. Vaquero1,2 and R. M. Trigo2,3 1Departamento de Física, Universidad de Extremadura, Avda. Santa Teresa de Jornet, 38, 06800 Mérida (Badajoz), Spain (e-mail: [email protected]) 2CGUL-IDL, Universidade de Lisboa, Lisbon, Portugal 3Departamento de Eng. Civil da Universidade Lusófona, Lisbon, Portugal Abstract. The Maunder Minimum corresponds to a prolonged minimum of solar activity a phenomenon that is of particular interest to many branches of natural and social sciences commonly considered to extend from 1645 until 1715. However, our knowledge of past solar activity has improved significantly in recent years and, thus, more precise dates for the onset and termination of this particularly episode of our Sun can be established. Based on the simultaneous analysis of distinct proxies we propose a redefinition of the Maunder Minimum period with the core "Deep Maunder Minimum" spanning from 1645 to 1700 (that corresponds to the Grand Minimum state) and a wider "Extended Maunder Minimum" for the longer period 1618-1723 that includes the transition periods. Gustav Spörer was the first to show in 1887 that there was a period of very low solar activity that ended in 1716. However the confirmation on the prolonged hiatus of solar activity would be attributed to the English astronomer Edward Walter Maunder who provided evidence that very few sunspots had been observed between 1645 and 1715 (Maunder 1922). John Allen Eddy, who popularized the name of this period as "Maunder Minimum" (MM), corroborated these dates after a thorough analysis of all available records of solar activity proxies including records of sunspot and aurorae observations from the 17th- and 18th-century astronomers and carbon-14 record (Eddy 1976). -
Solar Activity and Transformer Failures in the Greek National Electric Grid
J. Space Weather Space Clim. 3 (2013) A32 DOI: 10.1051/swsc/2013055 Ó I.P. Zois, Published by EDP Sciences 2013 RESEARCH ARTICLE OPEN ACCESS Solar activity and transformer failures in the Greek national electric grid Ioannis Panayiotis Zois* Testing Research and Standards Centre, Public Power Corporation, 9 Leontariou street, GR 153 51, Kantza, Pallini, Athens, Attica, Greece *Corresponding author: [email protected] Received 3 August 2012 / Accepted 27 October 2013 ABSTRACT Aims: We study both the short term and long term effects of solar activity on the large transformers (150 kV and 400 kV) of the Greek national electric grid. Methods: We use data analysis and various statistical methods and models. Results: Contrary to com- mon belief in PPC Greece, we see that there are considerable both short term (immediate) and long term effects of solar activity onto large transformers in a mid-latitude country like Greece. Our results can be summarised as follows: 1. For the short term effects: During 1989–2010 there were 43 ‘‘stormy days’’ (namely days with for example Ap 100) and we had 19 failures occurring during a stormy day plus or minus 3 days and 51 failures occurring during a stormy day plus or minus 7 days. All these failures can be directly related to Geomagnetically Induced Currents (GICs). Explicit cases are briefly pre- sented. 2. For the long term effects, again for the same period 1989–2010, we have two main results: (i) The annual number of transformer failures seems to follow the solar activity pattern. Yet the maximum number of transformer failures occurs about half a solar cycle after the maximum of solar activity. -
Nonaxisymmetric Component of Solar Activity and the Gnevyshev-Ohl Rule
Solar Physics DOI: 10.1007/•••••-•••-•••-••••-• Nonaxisymmetric Component of Solar Activity and the Gnevyshev-Ohl rule E.S.Vernova1 · M.I. Tyasto1 · D.G. Baranov2 · O.A. Danilova1 c Springer •••• Abstract The vector representation of sunspots is used to study the non- axisymmetric features of the solar activity distribution (sunspot data from Greenwich–USAF/NOAA, 1874–2016).The vector of the longitudinal asym- metry is defined for each Carrington rotation; its modulus characterizes the magnitude of the asymmetry, while its phase points to the active longitude. These characteristics are to a large extent free from the influence of a stochastic component and emphasize the deviations from the axisymmetry. For the sunspot area, the modulus of the vector of the longitudinal asymmetry changes with the 11-year period; however, in contrast to the solar activity, the amplitudes of the asymmetry cycles obey a special scheme. Each pair of cycles from 12 to 23 follows in turn the Gnevyshev–Ohl rule (an even solar cycle is lower than the following odd cycle) or the “anti-Gnevyshev–Ohl rule” (an odd solar cycle is lower than the preceding even cycle). This effect is observed in the longitudinal asymmetry of the whole disk and the southern hemisphere. Possibly, this effect is a manifes- tation of the 44-year structure in the activity of the Sun. Northern hemisphere follows the Gnevyshev–Ohl rule in Solar Cycles 12–17, while in Cycles 18–23 the anti-rule is observed. Phase of the longitudinal asymmetry vector points to the dominating (active) longitude. Distribution of the phase over the longitude was studied for two periods of the solar cycle, ascent-maximum and descent-minimum, separately. -
Arxiv:1901.09083V2 [Astro-Ph.SR] 3 Jun 2019 2 University of Maryland, Department of Astronomy, College Park, MD 20742, USA
Solar Physics DOI: 10.1007/•••••-•••-•••-••••-• What the Sudden Death of Solar Cycles Can Tell us About the Nature of the Solar Interior Scott W. McIntosh 1 · Robert J. Leamon 2,3 · Ricky Egeland 1 · Mausumi Dikpati 1 · Yuhong Fan 1 · Matthias Rempel 1 c Springer •••• Abstract We observe the abrupt end of solar activity cycles at the Sun's Equa- tor by combining almost 140 years of observations from ground and space. These \terminator" events appear to be very closely related to the onset of magnetic activity belonging to the next Solar Cycle at mid-latitudes and the polar-reversal process at high latitudes. Using multi-scale tracers of solar activity we examine the timing of these events in relation to the excitation of new activity and find that the time taken for the solar plasma to communicate this transition is of the order of one solar rotation { but could be shorter. Utilizing uniquely com- prehensive solar observations from the Solar Terrestrial Relations Observatory (STEREO) and Solar Dynamics Observatory (SDO) we see that this transitional event is strongly longitudinal in nature. Combined, these characteristics suggest that information is communicated through the solar interior rapidly. A range of possibilities exist to explain such behavior: for example gravity waves on the solar tachocline, or that the magnetic fields present in the Sun's convection zone could be very large, with a poloidal field strengths reaching 50 kG { considerably larger than conventional explorations of solar and stellar dynamos estimate. Regardless of the mechanism responsible, the rapid timescales demonstrated by the Sun's global magnetic field reconfiguration present strong constraints on first-principles numerical simulations of the solar interior and, by extension, other stars. -
SOLAR CYCLE 23: an ANOMALOUS CYCLE? Giuliana De Toma and Oran R
The Astrophysical Journal, 609:1140–1152, 2004 July 10 # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. SOLAR CYCLE 23: AN ANOMALOUS CYCLE? Giuliana de Toma and Oran R. White High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80301; [email protected], [email protected] and Gary A. Chapman, Stephen R. Walton, Dora G. Preminger, and Angela M. Cookson San Fernando Observatory, Department of Physics and Astronomy, California State University at Northridge, 18111 Nordhoff Street, Northridge, CA 91330; [email protected], [email protected], [email protected], [email protected] Received 2004 January 24; accepted 2004 March 19 ABSTRACT The latest SOHO VIRGO total solar irradiance (TSI) time series is analyzed using new solar variability measures obtained from full-disk solar images made at the San Fernando Observatory and the Mg ii 280 nm index. We discuss the importance of solar cycle 23 as a magnetically simpler cycle and a variant from recent cycles. Our results show the continuing improvement in TSI measurements and surrogates containing infor- mation necessary to account for irradiance variability. Use of the best surrogate for irradiance variability due to photospheric features (sunspots and faculae) and chromospheric features (plages and bright network) allows fitting the TSI record to within an rms difference of 130 ppm for the period 1986 to the present. Observations show that the strength of the TSI cycle did not change significantly despite the decrease in sunspot activity in cycle 23 relative to cycle 22. This points to the difficulty of modeling TSI back to times when only sunspot observations were available.