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Red Hat Satellite 6.7 Provisioning Guide
Red Hat Satellite 6.7 Provisioning Guide A guide to provisioning physical and virtual hosts on Red Hat Satellite Servers. Last Updated: 2021-05-14 Red Hat Satellite 6.7 Provisioning Guide A guide to provisioning physical and virtual hosts on Red Hat Satellite Servers. Red Hat Satellite Documentation Team [email protected] Legal Notice Copyright © 2021 Red Hat, Inc. The text of and illustrations in this document are licensed by Red Hat under a Creative Commons Attribution–Share Alike 3.0 Unported license ("CC-BY-SA"). An explanation of CC-BY-SA is available at http://creativecommons.org/licenses/by-sa/3.0/ . In accordance with CC-BY-SA, if you distribute this document or an adaptation of it, you must provide the URL for the original version. Red Hat, as the licensor of this document, waives the right to enforce, and agrees not to assert, Section 4d of CC-BY-SA to the fullest extent permitted by applicable law. Red Hat, Red Hat Enterprise Linux, the Shadowman logo, the Red Hat logo, JBoss, OpenShift, Fedora, the Infinity logo, and RHCE are trademarks of Red Hat, Inc., registered in the United States and other countries. Linux ® is the registered trademark of Linus Torvalds in the United States and other countries. Java ® is a registered trademark of Oracle and/or its affiliates. XFS ® is a trademark of Silicon Graphics International Corp. or its subsidiaries in the United States and/or other countries. MySQL ® is a registered trademark of MySQL AB in the United States, the European Union and other countries. -
Weather Reporting -- Volume C2
WEATHER REPORTING MESSAGES MÉTÉOROLOGIQUES МЕТЕОРОЛОГИЧЕСКИЕ СООБЩЕНИЯ INFORMES METEOROLOGICOS VOLUME/TOM/VOLUMEN C2 TRANSMISSION PROGRAMMES PROGRAMMES DE TRANSMISSION ЛPOГPAMMЬI ЛEPEДY PROGRAMAS DE TRANSMISIÓN 2012 Weather y Climate y Water World Meteorological Organization Organisation météorologique mondiale Всемирная Метеорологическая Организация Organización Meteorológica Mundial WMO/OMM/BMO No. 9 WEATHER REPORTING MESSAGES MÉTÉOROLOGIQUES МЕТЕОРОЛОГИЧЕСКИЕ СООБЩЕНИЯ INFORMES METEOROLOGICOS VOLUME/TOM/VOLUMEN C2 TRANSMISSION PROGRAMMES PROGRAMMES DE TRANSMISSION ЛPOГPAMMЬI ЛEPEДY PROGRAMAS DE TRANSMISIÓN 2012 Edition World Meteorological Organization Organisation météorologique mondiale Всемирная Метеорологическая Организация Organización Meteorológica Mundial WMO/OMM/BMO No. 9 COPYRIGHT © World Meteorological Organization © Organisation météorologique mondiale The right of publication in print, electronic and any other L’OMM se réserve le droit de publication en version imprimée form and in any language is reserved by WMO. Short extracts ou électronique ou sous toute autre forme et dans n’importe from WMO publications may be reproduced without quelle langue. De courts extraits des publications de l’OMM authorization, provided that the complete source is clearly peuvent être reproduits sans autorisation, pour autant que la indicated. Editorial correspondence and requests to publish, source complète soit clairement indiquée. La correspondance reproduce or translate this publication in part or in whole relative au contenu rédactionnel -
586 World Political
22_Biz_in_Global_Econ MAPS 12/14/04 2:56 PM Page 586 WORLD POLITICAL MAP ARCTIC OCEAN Barrow GREENLAND Fort Yukon Port Radium Fairbanks ICELAND Nome Baker Lake Nuuk Reykjavik Rankin Inlet Torshavn Anchorage Cordova Fort Chipewyan Churchill Juneau Inukjuak Fort McMurray Bear Lake Dawson Creek Thompson Grande Prairie Flin Flon Su Prince Rupert Prince George Unalaska Prince Albert Dublin Labrador City U. K. Red Deer IRELAND Londo Saskatoon CANADA Kamloops Calgary Cork Moosonee Swift Current Vancouver Brandon Timmins Amos Williston Spokane Grand Forks Seattle Nantes Butte Duluth Ottawa Montreal Minneapolis Portland Bayonne Twin Falls MilWawkee Detroit Scottsbluff Chicago Buffalo Boston Valladolid Porto Omaha Madrid Provo New York Reno Denver Kansas City Baltimore PORTUGAL Philadelphia SPAIN Oakland U. S. A. St. Louis Washington D. C. Ponta Delgada Lisbon Sevilla San Francisco Norfolk Gibraltar Las Vegas Albuquerque Memphis Charlotte Rabat Los Angeles Atlanta Casablanca Tucson Dallas Birmingham San Diego ATLANTIC MOROCCO Houston New Orleans Jacksonville Canary Islands ALG Tampa WESTERN THE BAHAMAS MEXICO SAHARA Havana Mexico City CUBA DOM. REP. MAURITANIA Araouan JAMAICA Nouakchott BELIZE HAITI MALI HONDURAS SENEGAL Dakar GUATEMALA GAMBIA Bamako EL SALVADOR NICARAGUA BURKIN Caracas GUINEA BISSAU GUINEA Conakry GHANA IVORY T COSTA RICA Freetown VENEZUELA Georgetown COAST PACIFIC PANAMA Paramaribo SIERRA LEONE Bogota GUYANA Monrovia FRENCH GUIANA A SURINAME LIBERIA Abidjan COLOMBIA EQU SAO TOM ECUADOR Quito Belem Manaus Fortaleza Talara PERU -
THE PLANETARY REPORT DECEMBER SOLSTICE 2016 VOLUME 36, NUMBER 4 Planetary.Org
THE PLANETARY REPORT DECEMBER SOLSTICE 2016 VOLUME 36, NUMBER 4 planetary.org A PEAK YEAR 2016 YEAR IN PICTURES PRESERVING OUR PAST C ROCKET ROAD TRIP C CALLING CHARTER MEMBERS Calling All Charter Members Envisioning a New Outreach Program A PLANETARY SOCIETY charter member is a I contacted Robin Young, the Society’s person whose membership began in 1980 or donor relations coordinator, and we began TOP LEFT A special evening reception and 1981 and who remains active today. We charter an e-mail dialog that led to a conference call fundraiser opened The members have a long-term perspective about between Robin, Society Chief Development Planetary Society’s The Planetary Society and the importance of Officer Richard Chute, and myself. We brain- 35th Anniversary its ongoing goals and plans, and we can be stormed on potential ways in which charter celebrations on October a power base of talent, ability, and ideas for members, working together under the direc- 23, 2015. At Pasadena’s the Society. However, there has not been a tion and guidance of a Planetary Society staff famed Huntington Library, cofounder format for us to organize and work together member, could make a wide variety of impor- Louis D. Friedman on projects for The Planetary Society. tant contributions. told stories about The At the Society’s 35th Anniversary celebra- The concept is nebulous at this point, but Planetary Society’s tions in Pasadena last year, several of us charter we would like to know whether the general inception and early members got acquainted and our conversa- idea of a task force of charter members days to our charter members, friends, tions almost always led to our remembrances working together on a project appeals to you. -
Southern Hemisphere Mid- and High-Latitudinal AOD, CO, NO2, And
Ahn et al. Progress in Earth and Planetary Science (2019) 6:34 Progress in Earth and https://doi.org/10.1186/s40645-019-0277-y Planetary Science RESEARCH ARTICLE Open Access Southern Hemisphere mid- and high- latitudinal AOD, CO, NO2, and HCHO: spatiotemporal patterns revealed by satellite observations Dha Hyun Ahn1, Taejin Choi2, Jhoon Kim1, Sang Seo Park3, Yun Gon Lee4, Seong-Joong Kim2 and Ja-Ho Koo1* Abstract To assess air pollution emitted in Southern Hemisphere mid-latitudes and transported to Antarctica, we investigate the climatological mean and temporal trends in aerosol optical depth (AOD), carbon monoxide (CO), nitrogen dioxide (NO2), and formaldehyde (HCHO) columns using satellite observations. Generally, all these measurements exhibit sharp peaks over and near the three nearby inhabited continents: South America, Africa, and Australia. This pattern indicates the large emission effect of anthropogenic activities and biomass burning processes. High AOD is also found over the Southern Atlantic Ocean, probably because of the sea salt production driven by strong winds. Since the pristine Antarctic atmosphere can be polluted by transport of air pollutants from the mid-latitudes, we analyze the 10-day back trajectories that arrive at Antarctic ground stations in consideration of the spatial distribution of mid-latitudinal AOD, CO, NO2, and HCHO. We find that the influence of mid-latitudinal emission differs across Antarctic regions: western Antarctic regions show relatively more back trajectories from the mid-latitudes, while the eastern Antarctic regions do not show large intrusions of mid-latitudinal air masses. Finally, we estimate the long-term trends in AOD, CO, NO2, and HCHO during the past decade (2005–2016). -
Articles Upon the Hox Family by Comparing Averages of Days Impacted by These Events with Averages of Non-Impacted 3945–3977, Doi:10.5194/Acp-13-3945-2013, 2013
Atmos. Chem. Phys., 15, 2889–2902, 2015 www.atmos-chem-phys.net/15/2889/2015/ doi:10.5194/acp-15-2889-2015 © Author(s) 2015. CC Attribution 3.0 License. Stratospheric and mesospheric HO2 observations from the Aura Microwave Limb Sounder L. Millán1,2, S. Wang2, N. Livesey2, D. Kinnison3, H. Sagawa4, and Y. Kasai4 1Joint Institute for Regional Earth System Science and Engineering, University of California, Los Angeles, California, USA 2Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA 3National Center for Atmospheric Research, Boulder, Colorado, USA 4National Institute of Information and Communications Technology, Koganei, Tokyo, Japan Correspondence to: L. Millán ([email protected]) Received: 18 June 2014 – Published in Atmos. Chem. Phys. Discuss.: 8 September 2014 Revised: 17 February 2015 – Accepted: 24 February 2015 – Published: 13 March 2015 Abstract. This study introduces stratospheric and meso- sphere where O3 chemistry is controlled by catalytic cycles spheric hydroperoxyl radical (HO2) estimates from the Aura involving the HOx (HO2, OH and H) family (Brasseur and Microwave Limb Sounder (MLS) using an offline retrieval Solomon, 2005): (i.e. run separately from the standard MLS algorithm). This new data set provides two daily zonal averages, one during X C O3 ! XO C O2 (R1) daytime from 10 to 0.0032 hPa (using day-minus-night dif- O C XO ! O2 C X; (R2) ferences between 10 and 1 hPa to ameliorate systematic bi- ases) and one during nighttime from 1 to 0.0032 hPa. The where the net effect of these two reactions is simply vertical resolution of this new data set varies from about 4 km O C O ! 2O (R3) at 10 hPa to around 14 km at 0.0032 hPa. -
Planetary Defence Activities Beyond NASA and ESA
Planetary Defence Activities Beyond NASA and ESA Brent W. Barbee 1. Introduction The collision of a significant asteroid or comet with Earth represents a singular natural disaster for a myriad of reasons, including: its extraterrestrial origin; the fact that it is perhaps the only natural disaster that is preventable in many cases, given sufficient preparation and warning; its scope, which ranges from damaging a city to an extinction-level event; and the duality of asteroids and comets themselves---they are grave potential threats, but are also tantalising scientific clues to our ancient past and resources with which we may one day build a prosperous spacefaring future. Accordingly, the problems of developing the means to interact with asteroids and comets for purposes of defence, scientific study, exploration, and resource utilisation have grown in importance over the past several decades. Since the 1980s, more and more asteroids and comets (especially the former) have been discovered, radically changing our picture of the solar system. At the beginning of the year 1980, approximately 9,000 asteroids were known to exist. By the beginning of 2001, that number had risen to approximately 125,000 thanks to the Earth-based telescopic survey efforts of the era, particularly the emergence of modern automated telescopic search systems, pioneered by the Massachusetts Institute of Technology’s (MIT’s) LINEAR system in the mid-to-late 1990s.1 Today, in late 2019, about 840,000 asteroids have been discovered,2 with more and more being found every week, month, and year. Of those, approximately 21,400 are categorised as near-Earth asteroids (NEAs), 2,000 of which are categorised as Potentially Hazardous Asteroids (PHAs)3 and 2,749 of which are categorised as potentially accessible.4 The hazards posed to us by asteroids affect people everywhere around the world. -
The Space-Based Global Observing System in 2010 (GOS-2010)
WMO Space Programme SP-7 The Space-based Global Observing For more information, please contact: System in 2010 (GOS-2010) World Meteorological Organization 7 bis, avenue de la Paix – P.O. Box 2300 – CH 1211 Geneva 2 – Switzerland www.wmo.int WMO Space Programme Office Tel.: +41 (0) 22 730 85 19 – Fax: +41 (0) 22 730 84 74 E-mail: [email protected] Website: www.wmo.int/pages/prog/sat/ WMO-TD No. 1513 WMO Space Programme SP-7 The Space-based Global Observing System in 2010 (GOS-2010) WMO/TD-No. 1513 2010 © World Meteorological Organization, 2010 The right of publication in print, electronic and any other form and in any language is reserved by WMO. Short extracts from WMO publications may be reproduced without authorization, provided that the complete source is clearly indicated. Editorial correspondence and requests to publish, reproduce or translate these publication in part or in whole should be addressed to: Chairperson, Publications Board World Meteorological Organization (WMO) 7 bis, avenue de la Paix Tel.: +41 (0)22 730 84 03 P.O. Box No. 2300 Fax: +41 (0)22 730 80 40 CH-1211 Geneva 2, Switzerland E-mail: [email protected] FOREWORD The launching of the world's first artificial satellite on 4 October 1957 ushered a new era of unprecedented scientific and technological achievements. And it was indeed a fortunate coincidence that the ninth session of the WMO Executive Committee – known today as the WMO Executive Council (EC) – was in progress precisely at this moment, for the EC members were very quick to realize that satellite technology held the promise to expand the volume of meteorological data and to fill the notable gaps where land-based observations were not readily available. -
IBM Cloud Satellite: Delivering True Hybrid Multicloud Capabilities
Produced by TIMOTHYH/ADOBE IBM Cloud Satellite: delivering true hybrid multicloud capabilities without geographical boundaries Produced by True hybrid capabilities delivered via public cloud and on-premise systems IBM Cloud Satellite enables organisations to enjoy the benefits of consistent and flexible public cloud services wherever in the world they want them, confident in the knowledge that compliance with local security and regulations is being managed by IBM Cloud rganisations are increasingly moving IT workloads to the cloud to achieve “Consistency benefits including flexibility, scale and consistent application performance O wherever their operations are located. means the same set of services, But for many IT leaders, retaining some applications and data in-house is essential – perhaps for regulatory compliance or local security needs. wherever you need According to TechTarget’s annual IT priorities research, 34% of European IT them, whether on leaders are increasing their cloud spending in 2020, even though 46% of the IBM Cloud, on organisations surveyed say that on-premise systems will remain their primary environment. Not surprisingly, therefore, a quarter of IT chiefs are prioritising someone else’s hybrid cloud. cloud, on-premise, But hybrid setups can suffer from inconsistent user experiences and fragmented or in a third-party visibility. Systems management can be challenging in a mixed cloud and on-premise environment, and more so when using multiple public cloud providers. datacentre” IBM Cloud aims to tackle this issue with its new offering, IBM Cloud Satellite, Dave Tropeano, which brings the benefits of cloud to in-house IT systems, delivering services IBM Cloud that are consistent, flexible and compliant with security and regulatory rules, while ensuring organisations are not restricted by location. -
The Planetary Report, to Make Those Discoveries Acces 20 Questions and Sible to All of Our Members
- --_.- .. .. _-- The Volume XIV On the Cover : Skywatchers will be poised to observe the heavenly Table of Number 1 stri ng of pearls kn own as comet Shoemaker-Levy 9 January/February 1994 thi s July when it crashes into Jupi te r's swirling atmo Contents sphere. This is an en largement of an image captured by the Hubble Space Tel escope (HSl) on July 1,1993, showing the reg ion of the brig htest nucleus of the comet, torn apart when it came too cl ose to Jupiter in 1992. This "bright nucleus " is actually a group of at least four separate pieces. The span of th is enti re Features image covers abou t 64,000 kilomete rs (40,000 miles). North is at the lower right. Image: H.A. Weaver and Bodies at the 16 Readers' T.E. Smith, Space Te lescope Science Institute, NASA 4 Brink Service Decades ago legendary planetary scientist The new mathematical field of chaos is Gerard P. Kuiper theorized that a band of difficult to penetrate, yet its somewhat comets orbited at the edge of our solar whimsical name and surprising predic From system. Telescopes of his time couldn't tions intrigue even the mathematically test this hypothesis, but now, working unsophisticated. Our featured book looks The with new equipment, astronomers have at chaos' applications to understanding discovered the first evidence that Kuiper our solar system. Editor was right. World Jupiter Watch: 17 Watch es, we have changed the 8 The Celestial Necklace It's a time of birth and death for NASA: Y design of The Planetary Breaks Its program to search for extraterrestrial Report; your eyes do not deceive This July, comet Shoemaker-Levy 9 will radio signals has been canceled by Congress, you. -
Extreme Weather Events
Extreme weather events Introduction The further a particular weather event lies from the typical range of that type of event, the more it is likely to be described as an extreme event, irrespective of whether it concerns a violent storm, unusual temperatures, heavy precipitation, drought or flood. 2012 seems to have been a year of extreme weather events (‘superstorm’ Sandy in the USA, high rainfall and floods in the UK, etc.). Other years in the last decade have also contained droughts and wildfires (in the USA and Australia), hurricane Katrina (USA), floods (Pakistan) and heat waves (Russia and France). At the same time it is becoming increasingly accepted that human activity, principally the burning of fossil fuels, is changing the global climate and causing the atmosphere to warm. The average global temperature of the lowermost atmosphere has increased markedly since about 1980. Are the two observations, which operate on different timescales1, connected? Are extreme weather events really becoming more common and/or more severe, or are they perhaps part of the climate’s natural variability? The aim of this document is to investigate these two questions. Some basic physics of a warmer atmosphere As air warms its humidity is able to rise and so the atmosphere carries more water vapour. For example, the water content of the atmosphere increases by 7% for each degree Centigrade rise in temperature, although globally precipitation is expected to rise by only about 2%/°C because relative humidity is typically not expected to change on the global scale.8 1 climate change is defined as changes occurring at least over a few decades whereas extreme weather typically lasts from days to months. -
Ice& Stone 2020
Ice & Stone 2020 WEEK 51: DECEMBER 13-19 Presented by The Earthrise Institute # 51 Authored by Alan Hale COMET OF THE WEEK: The Great Comet of 1680 Perihelion: 1680 December 18.49, q = 0.006 AU The Great Comet of 1680 over Rotterdam in The Netherlands, during late December 1680 as painted by the Dutch artist Lieve Verschuier. This particular comet was undoubtedly one of the brightest comets of the 17th Century, but it is also one of the most important comets in history from a scientific perspective, and perhaps even from the perspective of overall human history. While there were certainly plenty of superstitions attached to the comet’s appearance, the scientific investigations made of it were among the beginnings of the era in European history we now call The Enlightenment, and indeed, in a sense the Great Comet of 1680 can perhaps be considered as one of the sparks of that era. The significance began with the comet’s discovery, which was made on the morning of November 14, 1680, by a German astronomer residing in Coburg, Gottfried Kirch – the first comet ever to be discovered by means of a telescope. It was already around 4th magnitude at that time, and located near the star Regulus in the constellation Leo; from that point it traveled eastward and brightened rapidly, being closest to Earth (0.42 AU) on November 30. By that time it was a conspicuous naked-eye object with a tail 20 to 30 degrees long, and it remained visible for another week before disappearing into morning twilight.