FY11 NOAA Congressional Justification
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NSF Current Newsletter Highlights Research and Education Efforts Supported by the National Science Foundation
March 2012 Each month, the NSF Current newsletter highlights research and education efforts supported by the National Science Foundation. If you would like to automatically receive notifications by e-mail or RSS when future editions of NSF Current are available, please use the links below: Subscribe to NSF Current by e-mail | What is RSS? | Print this page | Return to NSF Current Archive Robotic Surgery Systems Shipped to Medical Research Centers A set of seven identical advanced robotic-surgery systems produced with NSF support were shipped last month to major U.S. medical research laboratories, creating a network of systems using a common platform. The network is designed to make it easy for researchers to share software, replicate experiments and collaborate in other ways. Robotic surgery has the potential to enable new surgical procedures that are less invasive than existing techniques. The developers of the Raven II system made the decision to share it as the best way to move the field forward--though it meant giving competing laboratories tools that had taken them years to develop. "We decided to follow an open-source model, because if all of these labs have a common research platform for doing robotic surgery, the whole field will be able to advance more quickly," said Jacob Rosen, Students with components associate professor of computer engineering at the University of of the Raven II surgical California-Santa Cruz. Rosen and Blake Hannaford, director of the robotics systems. Credit: University of Washington Biorobotics Laboratory, led the team that Carolyn Lagattuta built the Raven system, initially with a U.S. -
Effect of the Solar Wind Density on the Evolution of Normal and Inverse Coronal Mass Ejections S
A&A 632, A89 (2019) Astronomy https://doi.org/10.1051/0004-6361/201935894 & c ESO 2019 Astrophysics Effect of the solar wind density on the evolution of normal and inverse coronal mass ejections S. Hosteaux, E. Chané, and S. Poedts Centre for mathematical Plasma-Astrophysics (CmPA), Celestijnenlaan 200B, KU Leuven, 3001 Leuven, Belgium e-mail: [email protected] Received 15 May 2019 / Accepted 11 September 2019 ABSTRACT Context. The evolution of magnetised coronal mass ejections (CMEs) and their interaction with the background solar wind leading to deflection, deformation, and erosion is still largely unclear as there is very little observational data available. Even so, this evolution is very important for the geo-effectiveness of CMEs. Aims. We investigate the evolution of both normal and inverse CMEs ejected at different initial velocities, and observe the effect of the background wind density and their magnetic polarity on their evolution up to 1 AU. Methods. We performed 2.5D (axisymmetric) simulations by solving the magnetohydrodynamic equations on a radially stretched grid, employing a block-based adaptive mesh refinement scheme based on a density threshold to achieve high resolution following the evolution of the magnetic clouds and the leading bow shocks. All the simulations discussed in the present paper were performed using the same initial grid and numerical methods. Results. The polarity of the internal magnetic field of the CME has a substantial effect on its propagation velocity and on its defor- mation and erosion during its evolution towards Earth. We quantified the effects of the polarity of the internal magnetic field of the CMEs and of the density of the background solar wind on the arrival times of the shock front and the magnetic cloud. -
Predicting the Magnetic Vectors Within Coronal Mass Ejections Arriving at Earth: 2
Space Weather RESEARCH ARTICLE Predicting the magnetic vectors within coronal mass ejections 10.1002/2015SW001171 arriving at Earth: 1. Initial architecture Key Points: N. P.Savani1,2, A. Vourlidas1, A. Szabo2,M.L.Mays2,3, I. G. Richardson2,4, B. J. Thompson2, • First architectural design to predict A. Pulkkinen2,R.Evans5, and T. Nieves-Chinchilla2,3 a CME’s magnetic vectors (with eight events) 1 2 • Modified Bothmer-Schwenn CME Goddard Planetary Heliophysics Institute (GPHI), University of Maryland, Baltimore County, Maryland, USA, NASA 3 initiation rule to improve reliability Goddard Space Flight Center, Greenbelt, Maryland, USA, Institute for Astrophysics and Computational Sciences (IACS), of chirality Catholic University of America, Washington, District of Columbia, USA, 4Department of Astronomy, University of • CME evolution seen by remote Maryland, College Park, Maryland, USA, 5College of Science, George Mason University, Fairfax, Vancouver, USA sensing triangulation is important for forecasting Abstract The process by which the Sun affects the terrestrial environment on short timescales is Correspondence to: predominately driven by the amount of magnetic reconnection between the solar wind and Earth’s N. P. Savani, magnetosphere. Reconnection occurs most efficiently when the solar wind magnetic field has a southward [email protected] component. The most severe impacts are during the arrival of a coronal mass ejection (CME) when the magnetosphere is both compressed and magnetically connected to the heliospheric environment. Citation: Unfortunately, forecasting magnetic vectors within coronal mass ejections remain elusive. Here we report Savani, N. P., A. Vourlidas, A. Szabo, M.L.Mays,I.G.Richardson,B.J. how, by combining a statistically robust helicity rule for a CME’s solar origin with a simplified flux rope Thompson, A. -
Arxiv:2101.07771V4 [Stat.AP] 9 Jun 2021
Received Jan-19-2021; Revised Jun-02-2021; Accepted XX-XX-XXX DOI: xxx/xxxx SURVEY Critical Risk Indicators (CRIs) for the electric power grid: A survey and discussion of interconnected effects Che-Castaldo, Judy P.*1 | Cousin, Rémi2 | Daryanto, Stefani3 | Deng, Grace4 | Feng, Mei-Ling E.1 | Gupta, Rajesh K.5 | Hong, Dezhi5 | McGranaghan, Ryan M.6 | Owolabi, Olukunle O.7 | Qu, Tianyi8 | Ren, Wei3 | Schafer, Toryn L. J.4 | Sharma, Ashutosh9,10 | Shen, Chaopeng9 | Sherman, Mila Getmansky8 | Sunter, Deborah A.7 | Tao, Bo3 | Wang, Lan11 | Matteson, David S.4 1Conservation & Science Department, Lincoln Park Zoo, Illinois, USA Abstract 2International Research Institute for Climate The electric power grid is a critical societal resource connecting multiple infrastruc- and Society, Earth Institute / Columbia University, New York, USA tural domains such as agriculture, transportation, and manufacturing. The electrical 3Department of Plant and Soil Sciences, grid as an infrastructure is shaped by human activity and public policy in terms of College of Agriculture, Food and Environment / University of Kentucky, demand and supply requirements. Further, the grid is subject to changes and stresses Kentucky, USA due to diverse factors including solar weather, climate, hydrology, and ecology. The 4 Department of Statistics and Data Science, emerging interconnected and complex network dependencies make such interactions Cornell University, New York, USA 5Halicioglu Data Science Institute and increasingly dynamic, posing novel risks, and presenting new challenges to manage Department of Computer Science & the coupled human-natural system. This paper provides a survey of models and meth- Engineering, University of California, San ods that seek to explore the significant interconnected impact of the electric power Diego, California, USA 6Atmosphere Space Technology Research grid and interdependent domains. -
Cmes, Solar Wind and Sun-Earth Connections: Unresolved Issues
CMEs, solar wind and Sun-Earth connections: unresolved issues Rainer Schwenn Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany [email protected] In recent years, an unprecedented amount of high-quality data from various spaceprobes (Yohkoh, WIND, SOHO, ACE, TRACE, Ulysses) has been piled up that exhibit the enormous variety of CME properties and their effects on the whole heliosphere. Journals and books abound with new findings on this most exciting subject. However, major problems could still not be solved. In this Reporter Talk I will try to describe these unresolved issues in context with our present knowledge. My very personal Catalog of ignorance, Updated version (see SW8) IAGA Scientific Assembly in Toulouse, 18-29 July 2005 MPRS seminar on January 18, 2006 The definition of a CME "We define a coronal mass ejection (CME) to be an observable change in coronal structure that occurs on a time scale of a few minutes and several hours and involves the appearance (and outward motion, RS) of a new, discrete, bright, white-light feature in the coronagraph field of view." (Hundhausen et al., 1984, similar to the definition of "mass ejection events" by Munro et al., 1979). CME: coronal -------- mass ejection, not: coronal mass -------- ejection! In particular, a CME is NOT an Ejección de Masa Coronal (EMC), Ejectie de Maså Coronalå, Eiezione di Massa Coronale Éjection de Masse Coronale The community has chosen to keep the name “CME”, although the more precise term “solar mass ejection” appears to be more appropriate. An ICME is the interplanetry counterpart of a CME 1 1. -
Solar Wind Properties and Geospace Impact of Coronal Mass Ejection-Driven Sheath Regions: Variation and Driver Dependence E
Solar Wind Properties and Geospace Impact of Coronal Mass Ejection-Driven Sheath Regions: Variation and Driver Dependence E. K. J. Kilpua, D. Fontaine, C. Moissard, M. Ala-lahti, E. Palmerio, E. Yordanova, S. Good, M. M. H. Kalliokoski, E. Lumme, A. Osmane, et al. To cite this version: E. K. J. Kilpua, D. Fontaine, C. Moissard, M. Ala-lahti, E. Palmerio, et al.. Solar Wind Properties and Geospace Impact of Coronal Mass Ejection-Driven Sheath Regions: Variation and Driver Dependence. Space Weather: The International Journal of Research and Applications, American Geophysical Union (AGU), 2019, 17 (8), pp.1257-1280. 10.1029/2019SW002217. hal-03087107 HAL Id: hal-03087107 https://hal.archives-ouvertes.fr/hal-03087107 Submitted on 23 Dec 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. RESEARCH ARTICLE Solar Wind Properties and Geospace Impact of Coronal 10.1029/2019SW002217 Mass Ejection-Driven Sheath Regions: Variation and Key Points: Driver Dependence • Variation of interplanetary properties and geoeffectiveness of CME-driven sheaths and their dependence on the E. K. J. Kilpua1 , D. Fontaine2 , C. Moissard2 , M. Ala-Lahti1 , E. Palmerio1 , ejecta properties are determined E. -
Ten Years of PAMELA in Space
Ten Years of PAMELA in Space The PAMELA collaboration O. Adriani(1)(2), G. C. Barbarino(3)(4), G. A. Bazilevskaya(5), R. Bellotti(6)(7), M. Boezio(8), E. A. Bogomolov(9), M. Bongi(1)(2), V. Bonvicini(8), S. Bottai(2), A. Bruno(6)(7), F. Cafagna(7), D. Campana(4), P. Carlson(10), M. Casolino(11)(12), G. Castellini(13), C. De Santis(11), V. Di Felice(11)(14), A. M. Galper(15), A. V. Karelin(15), S. V. Koldashov(15), S. Koldobskiy(15), S. Y. Krutkov(9), A. N. Kvashnin(5), A. Leonov(15), V. Malakhov(15), L. Marcelli(11), M. Martucci(11)(16), A. G. Mayorov(15), W. Menn(17), M. Mergè(11)(16), V. V. Mikhailov(15), E. Mocchiutti(8), A. Monaco(6)(7), R. Munini(8), N. Mori(2), G. Osteria(4), B. Panico(4), P. Papini(2), M. Pearce(10), P. Picozza(11)(16), M. Ricci(18), S. B. Ricciarini(2)(13), M. Simon(17), R. Sparvoli(11)(16), P. Spillantini(1)(2), Y. I. Stozhkov(5), A. Vacchi(8)(19), E. Vannuccini(1), G. Vasilyev(9), S. A. Voronov(15), Y. T. Yurkin(15), G. Zampa(8) and N. Zampa(8) (1) University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence, Italy (2) INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy (3) University of Naples “Federico II”, Department of Physics, I-80126 Naples, Italy (4) INFN, Sezione di Naples, I-80126 Naples, Italy (5) Lebedev Physical Institute, RU-119991 Moscow, Russia (6) University of Bari, I-70126 Bari, Italy (7) INFN, Sezione di Bari, I-70126 Bari, Italy (8) INFN, Sezione di Trieste, I-34149 Trieste, Italy (9) Ioffe Physical Technical Institute, RU-194021 St. -
Examining Emerging Risks
CAS Professional Education IN FOCUS: TAMING CATS‐MANAGING NATURAL AND MAN‐MADE CATASTROPHE RISKS BALTIMORE, MD EXAMINING EMERGING RISKS Alan D. Roth, Ph.D. Chief Risk Officer, Advanced Fusion Systems, LLC TOPICS TO BE COVERED • CLIMATE CHANGE • WATER SCARCITY • FOOD SCARCITY • FUEL SCARCITY • SOLAR STORMS • EMP • PANDEMICS • CYBER WARFARE CLIMATE CHANGE Is it real? This is from NASA Where? –is also important! We need to consider: • Pacific Decadal Oscillation • North Atlantic Oscillation • Southern Oscillation: El Niño and La Niña • Arctic Oscillation • Trade winds • Meridional Overturning Circulation (aka Conveyor Belt) Temperature from 1884 to 2011 Ocean currents are varied http://www.jpl.nasa.gov/news/news.cfm?release=2012‐099 El Niño/Southern Oscillation (ENSO) NOAA: North Atlantic Oscillation NOAA: North Atlantic Oscillation Arctic Oscillation The state of atmospheric circulation over the Arctic. Red is low pressure, blue is high pressure. Influences weather patterns at lower latitudes. Effect of changes in temperature distribution on extremes ”MANAGING THE RISKS OF EXTREME EVENTS AND DISASTERS TO ADVANCE CLIMATE CHANGE ADAPTATION: SUMMARY FOR POLICYMAKERS” Special Report of the IPCC 2012 page 6 The. Different changes in temperature distributions between present and future climate and their effects on extreme values of the distributions: (a) effects of a simple shift of the entire distribution toward a warmer climate; (b) effects of an increase in temperature variability with no shift in the mean; (c) effects of an altered shape of the distribution, in this example a change in asymmetry toward the hotter part of the distribution. (courtesy IPCC) Arctic Sea Ice Extent thru Sept. ‘12 Ice Decreasing at an Increasing Rate 2007 vs 2012 Abrupt Climate Change 23 Times! Courtesy Rihichar d B. -
REFERENCE SHEET for NWS TAUNTON WARNING/ADVISORY THRESHOLDS (Last Updated: March 7, 2017)
REFERENCE SHEET FOR NWS TAUNTON WARNING/ADVISORY THRESHOLDS (Last Updated: March 7, 2017) The following are National Weather Service criteria for issuing Watches/Warnings/Advisories: Watches: 50% confidence of meeting Warning criteria (generally within 36-48+ hours). Advisories and Warnings: 80% confidence in the event occurrence (generally within 24-36 hours). TYPE OF ISSUANCE WHEN ISSUED FOR SOUTHERN NEW ENGLAND WINTER WEATHER ADVISORY More than one predominant hazard Winter weather event having more than one predominant hazard (ie., snow and ice, snow and sleet, or snow, ice & sleet) meeting or exceeding advisory criteria for at least one of the precipitation elements, but remaining below warning criteria. Snow, Ocean Effect Snow, and/or Sleet 3 inches averaged over a forecast zone in 12 hours Snow and Blowing Snow Sustained or frequent gusts of 25 to 34 mph accompanied by falling and blowing snow occasionally reducing visibility to ≤ 1/4 mile for ≥ 3 hours Blowing Snow Widespread or localized blowing snow reducing visibility to ≤ ¼ mile with winds < 35 mph Black Ice A Special Weather Statement will usually be issued when sufficient moisture is expected to cause a thin layer of ice on road surfaces, typically on cloudless nights (“black ice”). At forecaster discretion a formal Winter Weather Advisory may be issued instead. FREEZING RAIN ADVISORY Any accretion of freezing rain or freezing drizzle on road surfaces WIND CHILL ADVISORY Wind chill index between -15°F and -24°F for at least 3 hours using only the sustained wind WINTER STORM WARNING More than one predominant hazard Winter weather event having more than one predominant hazard {ie. -
Astrophysics in 2006 3
ASTROPHYSICS IN 2006 Virginia Trimble1, Markus J. Aschwanden2, and Carl J. Hansen3 1 Department of Physics and Astronomy, University of California, Irvine, CA 92697-4575, Las Cumbres Observatory, Santa Barbara, CA: ([email protected]) 2 Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, Organization ADBS, Building 252, 3251 Hanover Street, Palo Alto, CA 94304: ([email protected]) 3 JILA, Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder CO 80309: ([email protected]) Received ... : accepted ... Abstract. The fastest pulsar and the slowest nova; the oldest galaxies and the youngest stars; the weirdest life forms and the commonest dwarfs; the highest energy particles and the lowest energy photons. These were some of the extremes of Astrophysics 2006. We attempt also to bring you updates on things of which there is currently only one (habitable planets, the Sun, and the universe) and others of which there are always many, like meteors and molecules, black holes and binaries. Keywords: cosmology: general, galaxies: general, ISM: general, stars: general, Sun: gen- eral, planets and satellites: general, astrobiology CONTENTS 1. Introduction 6 1.1 Up 6 1.2 Down 9 1.3 Around 10 2. Solar Physics 12 2.1 The solar interior 12 2.1.1 From neutrinos to neutralinos 12 2.1.2 Global helioseismology 12 2.1.3 Local helioseismology 12 2.1.4 Tachocline structure 13 arXiv:0705.1730v1 [astro-ph] 11 May 2007 2.1.5 Dynamo models 14 2.2 Photosphere 15 2.2.1 Solar radius and rotation 15 2.2.2 Distribution of magnetic fields 15 2.2.3 Magnetic flux emergence rate 15 2.2.4 Photospheric motion of magnetic fields 16 2.2.5 Faculae production 16 2.2.6 The photospheric boundary of magnetic fields 17 2.2.7 Flare prediction from photospheric fields 17 c 2008 Springer Science + Business Media. -
Workshop on the Impacts of Flooding
Workshop on the Impacts of Flooding Proceed/rigs of a Workshop held in Rockhamptori, Australia, 27 Septeinber 1991. , Edited by G.T. Byron Queensland Department of. ti Environment tand Heritage ’ Great Barrier Reef Marine Park Authority ‘, , ,’ @ Great Barrier Reef Marine Park Authority ISSN 0156-5842 ISBN 0 624 12044 7 Published by GBRMPA April 1992 The opinions expressed in th.is document are not necessarily those of the Great Barrier Reef Marine Park Authority or the Queensland Department of Env/ionment an!d Heritage. Great Barrier Reef Environment and P.O. Box 155 P.O. Box1379 North Quay , Townsville Queens’land 4002 Queensland 48 TABLE OF CONTENTS : PREFACE iv 1 EXECUTIVE SUMMARY V PART A: FORUM PAPERS Jim Pearce MLA Opening Address 1 Peter Baddiley Fitzroy River Basin 3 Rainfalls and The 1991 Flood Event Mike Keane Assessment of the 1991 16 Fitzroy River Flood How much water? J.P. O’Neill, G.T.Byron and Some Physical Characteristics 36 S.C.Wright and Movement of 1991 Fitzroy River flood plume PART B: WORKSHOP PAPERS GROUP A - WATER RELATED’ISSUES Jon E. Brodie and Nutrient Composition of 56 Alan Mitchell the January 1991 Fitzroy River Plume Myriam Preker The Effects of the 1991 75 Central Queensland Floodwaters around Heron Island, Great Barrier Reef i > d.T.Byron and J.P.O’Neill Flood Induced Coral Mortality 76 on Fringing Reefs in Keppel Bay J.S. Giazebrook and Effects of low salinity on 90 R. Van Woesik the tissues of hard corals Acropora spp., Pocillopora sp and Seriatopra sp from the Great Keppel region M. -
Spearfish Fire Department Policies and Procedures
SPEARFISH FIRE DEPARTMENT POLICIES AND PROCEDURES Page 1 of 5 Volume: Operation Section: 20.00 Number: 20.09 Subject: Weather Watches, Warnings, Advisory’s and Spotter Activation Date Issued: 8 August 2019 Originator: Assistant Chief R. Mathis Rescinds: 28 March 2017 Approval: Assistant Chief R. Mathis I. Purpose This procedure provides guidance for safety and general procedures when responding to Weather Spotter activations. II. SCOPE This policy applies to all personnel. III. DEFINITIONS Winter Storm Watch A Winter Storm Watch is issued when there is the potential for significant and hazardous winter weather within 48 hours. It does not mean that significant and hazardous winter weather will occur...it only means it is possible. Significant and hazardous winter weather is defined as a combination of: 1) 5 inches or more of snow/sleet within a 12-hour period or 7 inches or more of snow/sleet within a 24-hour period AND/OR 2) Enough ice accumulation to cause damage to trees or powerlines AND/OR 3) a life threatening or damaging combination of snow and/or ice accumulation with wind. Blizzard Warning A Blizzard Warning means that the following conditions are occurring or expected within the next 12 to 18 hours. 1) Snow and/or blowing snow reducing visibility to 1/4 mile or less for 3 hours or longer AND 2) Sustained winds of 35 mph or greater or frequent gusts to 35 mph or greater. There is no temperature requirement that must be met to achieve blizzard conditions. Winter Storm Warning A Winter Storm Warning is issued when a significant combination of hazardous winter weather is occurring or imminent.