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Your Free Digital Flight Simulation Magazine
Vol.2 Issue 7 June 2019 Your Free digital Flight Simulation magazine 2 Welcome once again. Summer is upon us with mixed weather but hopefully it will be fine for the Bray Air Display on 27th and 28th July. Check their website for what’s on in the air and on the ground. Flight Sim Show 2019 in Cosford, UK will be a two day event for the first time which should increase attendance. We are unsure whether we will exhibit, so keep an eye on the show website. Microsoft have announced their re-entry into the Flight Sim market with ‘Microsoft Flight Simulator’ for PC and X-Box. I don’t think it will be on par with Prepar3d as it has become very popular since its update to 64bit. However, it may mean more business for the add-on publishers. In this issue, John McNeely expresses his opinion on updates and buggy software in ‘Testing Times’. In addition to his Plane Talking column, Published by Ian Broni reports on his visit to ‘DAKS Over Normandy’. John Melville reviews The PC Pilots Ireland the Carenado A42 500 Series and Brian Church reviews the new Navigraph Charts. pcpilotsireland.com The next issue is due September 2019. Contributors Terry McGee Terry McGee [email protected] https://brayairdisplay.com Ian Broni [email protected] John Melville [email protected] John McNeely [email protected] Brian Church [email protected] Aerosoft www.aerosoft.com Simmarket www.simmarket.com Chillblast www.chillblast.com www.flightsimshow.com Contents: Page Aerosoft Advert 2 Testing Times 31 Editorial 3 Flightsim Apps 34 Front Cover 4 Plane -
UC Irvine UC Irvine Previously Published Works
UC Irvine UC Irvine Previously Published Works Title Astrophysics in 2006 Permalink https://escholarship.org/uc/item/5760h9v8 Journal Space Science Reviews, 132(1) ISSN 0038-6308 Authors Trimble, V Aschwanden, MJ Hansen, CJ Publication Date 2007-09-01 DOI 10.1007/s11214-007-9224-0 License https://creativecommons.org/licenses/by/4.0/ 4.0 Peer reviewed eScholarship.org Powered by the California Digital Library University of California Space Sci Rev (2007) 132: 1–182 DOI 10.1007/s11214-007-9224-0 Astrophysics in 2006 Virginia Trimble · Markus J. Aschwanden · Carl J. Hansen Received: 11 May 2007 / Accepted: 24 May 2007 / Published online: 23 October 2007 © Springer Science+Business Media B.V. 2007 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: general · Planets and satellites: general · Astrobiology · Star clusters · Binary stars · Clusters of galaxies · Gamma-ray bursts · Milky Way · Earth · Active galaxies · Supernovae 1 Introduction Astrophysics in 2006 modifies a long tradition by moving to a new journal, which you hold in your (real or virtual) hands. The fifteen previous articles in the series are referenced oc- casionally as Ap91 to Ap05 below and appeared in volumes 104–118 of Publications of V. -
Détection Et Modélisation De Binaires Sismiques Avec Kepler
Frédéric MARCADON Détection et modélisation de binaires sismiques avec Kepler Directeur de thèse : Thierry APPOURCHAUX Institut d’Astrophysique Spatiale Orsay – 20 mars 2018 Introduction à l’astérosismologie Astérosismologie avec K2 Intérêt des étoiles binaires Introduction générale Missions CoRoT et Kepler : détection d’exoplanètes par la méthode des transits et caractérisation des étoiles hôtes par l’astérosismologie. Astérosismologie : outil de diagnostic de la structure interne des étoiles et de détermination de leurs propriétés physiques (masse et âge). Observation des variations de luminosité des étoiles au cours du temps par photométrie (courbes de lumière). Frédéric MARCADON Détection et modélisation de binaires sismiques avec Kepler 1 / 36 Introduction à l’astérosismologie Astérosismologie avec K2 Intérêt des étoiles binaires Sommaire 1 Introduction à l’astérosismologie 2 Astérosismologie avec K2 3 Intérêt des étoiles binaires 4 Binaires sismiques avec Kepler 5 Analyse orbitale de HD 188753 6 Modélisation de HD 188753 7 Conclusions et perspectives Frédéric MARCADON Détection et modélisation de binaires sismiques avec Kepler 2 / 36 Introduction à l’astérosismologie Astérosismologie avec K2 Intérêt des étoiles binaires Sommaire 1 Introduction à l’astérosismologie 2 Astérosismologie avec K2 3 Intérêt des étoiles binaires 4 Binaires sismiques avec Kepler 5 Analyse orbitale de HD 188753 6 Modélisation de HD 188753 7 Conclusions et perspectives Frédéric MARCADON Détection et modélisation de binaires sismiques avec Kepler 2 / 36 Introduction à l’astérosismologie Astérosismologie avec K2 Intérêt des étoiles binaires Théorie des oscillations stellaires Astérosismologie : étude des oscillations des étoiles permettant de sonder leur structure interne. Différents types d’ondes se propageant à l’intérieur de l’étoile : les ondes acoustiques générées dans la zone convective et dont la force de rappel est la pression (modes p). -
Study on State Asset Management in the EU
Study on State asset management in the EU Final study report for Pillar 2 – Portugal Contract: ECFIN/187/2016/740792 Written by KPMG and Bocconi University February 2018 EUROPEAN COMMISSION Directorate-General for Economic and Financial Affairs Directorate Fiscal policy and policy mix and Directorate Investment, growth and structural reforms European Commission B-1049 Brussels 2 Portugal This Country fiche presents a quantitative overview of the mix of non-financial assets owned by the Portuguese General government. A recap and a summary table on sources of data and valuation methods used to map and assess (as far as possible) non-financial assets owned by the Portuguese General government is reported in the Appendix (Table C). 1. OVERVIEW OF NON-FINANCIAL ASSETS In 2015, the estimated value of Non-financial assets owned by the Portuguese General government was equal to 119.6 Eur Bn, accounting for about 82.9% of the estimated value of all assets (including Financial assets) owned by the General government1. Figure 1 General government’s Financial and Non-financial assets (Eur Bn), Portugal, 2015 Source: KPMG elaboration. Data on Gross Domestic Product were directly retrivied from Eurostat on 19th September 2017. (1) Estimated values refer to 2015 as the latest available year for both financial assets and all clusters of non-financial assets. (2) In this chart, the “estimated value” of financial assets is reported in terms of Total Assets of the country’s PSHs as weighted by the stake(s) owned by the Public sector into the PSHs themselves2. (3) Values of Dwellings, and Buildings other than dwellings were directly retrieved from Eurostat, while values for other Non-financial assets were estimated according to the valuation approaches explained in the Methodological Notes for Pillar 2. -
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. -
A Comparative Study of Long Distance Aircraft
European Aviation Safety Agency Safety Analysis and Research Department Executive Directorate 2008 Annual Safety Recommendations review Executive Directorate- Safety Analysis and Research Page 1/48 © European Aviation Safety Agency, 2008. All rights reserved. Proprietary document. Printed copies are not controlled. Confirm revision status through the EASA-Internet/Intranet. European Aviation Safety Agency Annual Safety Recommendations review 2008 SAR-002-2009 2008 Annual Safety Recommendations review Document ref. Status Date SAR-002-2008 20 August 2009 Contact name and address for enquiries: European Aviation Safety Agency Safety Analysis and Research Postfach 10 12 53 50452 Köln - Germany Information on EASA is available at: www.easa.europa.eu Disclaimer: Neither the European Aviation Safety Agency, nor any person acting on behalf of the European Aviation Safety Agency is responsible for the use which might be made of the following information. Authorisation : Name Signature Date Zsofia Olah 05 March 2009 Prepared Dominique Verdoni Reviewed 1 Bernard Bourdon Reviewed 2 Authorised John Vincent Executive Directorate- Safety Analysis and Research Page 2/48 © European Aviation Safety Agency, 2008. All rights reserved. Proprietary document. Printed copies are not controlled. Confirm revision status through the EASA-Internet/Intranet. European Aviation Safety Agency Annual Safety Recommendations review 2008 SAR-002-2009 Table of Contents 1 Introduction...........................................................................................................5 -
¿Cuánto Sabés Sobre El Universo?
¿CUÁNTO SABÉS SOBRE EL UNIVERSO? Apuntes básicos sobre Astronomía - 2014 Autores: Dra. Eugenia Díaz-Giménez / Dr. Ariel Zandivarez Instituto de Astronomía Teórica y Experimental (CONICET) Observatorio Astronómico de Córdoba (UNC) Imagen: Aldo Mottino / Estación Astrofísica de Bosque Alegre 2 Índice INTRODUCCIÓN.............................................................................................................................5 0.1 LA LUZ..................................................................................................................................5 0.2 LAS IMÁGENES ASTRONÓMICAS......................................................................................8 CAPÍTULO 1: Sistema Solar y otros sistemas planetarios.......................................................11 1.1 HISTORIA DE LA CONCEPCIÓN DEL SISTEMA SOLAR..................................................11 1.2 FORMACIÓN DEL SISTEMA SOLAR.................................................................................13 1.3 MOVIMIENTO DE LOS OBJETOS DEL SISTEMA SOLAR.................................................13 1.4 CARACTERÍSTICAS DE LOS OBJETOS DEL SISTEMA SOLAR......................................14 1.4.1 SOL..............................................................................................................................16 1.4.2 MERCURIO..................................................................................................................17 1.4.3 VENUS.........................................................................................................................17 -
Habitable Zones with Stable Orbits for Planets Around Binary Systems
Mon. Not. R. Astron. Soc. 000, 1–?? (—-) Printed 23 May 2014 (MN LATEX style file v2.2) Habitable Zones with Stable Orbits for Planets around Binary Systems Luisa G. Jaime1?, Luis Aguilar2, and Barbara Pichardo1 1Instituto de Astronom´ıa, Universidad Nacional Autonoma´ de Mexico,´ Apdo. postal 70-264, Ciudad Universitaria, Mexico´ 2Instituto de Astronom´ıa, Universidad Nacional Autonoma´ de Mexico,´ Apdo. postal 877, 22800 Ensenada, Mexico´ Accepted. Received ; in original form ABSTRACT A general formulation to compute habitable zones around binary stars is presented. A habitable zone in this context must satisfy two separate conditions: a radiative one and one of dynamical stability. For the case of single stars, the usual concept of circumstellar habitable zone is based on the radiative condition only, as the dynamical stability condition is taken for granted (assuming minimal perturbation from other planets). For the radiative condition, we extend the simple formulation of the circumstellar habitable zone for single stars, to the case of eccentric stellar binary systems, where two sources of luminosity at different orbital phases contribute to the irradiance of their planetary circumstellar and circumbinary regions. Our approach considers binaries with eccentric orbits and guarantees that orbits in the computed habitable zone remain within it at all orbital phases. For the dynamical stability condition, we use the approach of invariant loops developed by Pichardo et al. (2005) to find regions of stable, non-intersecting orbits, which is a robust method to find stable regions in binary stars, as it is based in the existence of integrals of motion. We apply the combined criteria to calculate habitable zones for 64 binary stars in the solar neighborhood with known orbital parameters, including some with discovered planets. -
THE STAR FORMATION NEWSLETTER an Electronic Publication Dedicated to Early Stellar Evolution and Molecular Clouds
THE STAR FORMATION NEWSLETTER An electronic publication dedicated to early stellar evolution and molecular clouds No. 159 — 22 January 2006 Editor: Bo Reipurth ([email protected]) Abstracts of recently accepted papers Physical Conditions in Orion’s Veil II: A Multi-Component Study of the Line of Sight Towards the Trapezium N. P. Abel1, G. J. Ferland1, C. R. O’Dell2, G. Shaw1 and T. H. Troland1 1 University of Kentucky, Department of Physics and Astronomy, Lexington, KY 40506, USA 2 Department of Physics and Astronomy, Vanderbilt University, Box 1807-B, Nashville, TN 37235, USA E-mail contact: [email protected] Orion’s Veil is an absorbing screen that lies along the line of sight to the Orion H II region. It consists of two or more layers of gas that must lie within a few parsecs of the Trapezium cluster. Our previous work considered the Veil as a whole and found that the magnetic field dominates the energetics of the gas in at least one component. Here we use high-resolution STIS UV spectra that resolve the two velocity components in absorption and determine the conditions in each. We derive a volume hydrogen density, 21 cm spin temperature, turbulent velocity, and kinetic temperature, for each. We combine these estimates with magnetic field measurements to find that magnetic energy significantly dominates turbulent and thermal energies in one component, while the other component is close to equipartition between turbulent and magnetic energies. We observe molecular hydrogen absorption for highly excited v, J levels that are photoexcited by the stellar continuum, and detect blueshifted S III and P III absorption lines. -
I Melkeveien Side 12: Galaktisk Leksikon Over Annerledesverdener
Astronomi_2012_3_Astronomi_2012_3.qxd 27.04.12 11:52 Side 1 Et øye på Merkur 24 42. årgang Stjernen som blåser såpebobler 30 Juni 2012 3 Kr. 59,– Lyse netter og solrike sommerdager 40 Sommerfullmånen: Synet som færre enn 1 av 100 mennesker får oppleve i sin fulle prakt 46 Stjernebilder og mytologi: Musikanten som spilte så bra at han døde av det 48 De merkeligste planetene i Melkeveien Side 12: Galaktisk leksikon over annerledesverdener Norske blinkskudd: Universets ukjente materie skaper hodebry Interpress Norge Sol, måne, planeter Men nå vet forskerne mer Returuke: 28 og fjerne galakser om hva den ikke er Side 56 Side 22 Astronomi_2012_3_Astronomi_2012_3.qxd 27.04.12 11:52 Side 2 ASTRONOMI Innhold Utgiver: Norsk Astronomisk Selskap Postboks 1029 Blindern, 0315 Oslo Org.nr. 987 629 533 ISSN 0802-7587 De merkeligste Abonnementsservice: Bli medlem / avslutte medlemskap / melde adresseforandring / gi beskjed planetene om manglende blad: «Astronomi», c/o Ask Media AS, Postboks 130, 2261 Kirkenær i Melkeveien Org.nr. 990 684 219 Tlf. 46 94 10 00 (kl. 09.00-15.00) Faks 62 94 87 05 e-post: [email protected] Girokonto: 7112.05.74951 Ask Media fører abonnements register for en rekke tidsskrifter. Vær vennlig å oppgi at henvendelsen gjelder bladet Astronomi. Vi gjør oppmerksom på at Ask Media kun fører medlemsregiste- ret for NAS og ikke har mulighet til å besvare astronomi-spørsmål. Henvendelser til Norsk Astronomisk Selskap: Se kontaktinfo side 53 Redaktør: Bidrag, artikler, bilder, annonser o.l.: «Astronomi», v/Trond Erik Hillestad, Riskeveien 10, 3157 Barkåker Tlf. 99 73 73 85 [email protected] Layout: Eureka Design AS v/ Bendik Nerstad Hele tiden oppdages det fjerne planeter som på en eller annen måte setter rekord. -
Safetaxi Full Coverage List – 21S5 Cycle
SafeTaxi Full Coverage List – 21S5 Cycle Australia Australian Capital Territory Identifier Airport Name City Territory YSCB Canberra Airport Canberra ACT Oceanic Territories Identifier Airport Name City Territory YPCC Cocos (Keeling) Islands Intl Airport West Island, Cocos Island AUS YPXM Christmas Island Airport Christmas Island AUS YSNF Norfolk Island Airport Norfolk Island AUS New South Wales Identifier Airport Name City Territory YARM Armidale Airport Armidale NSW YBHI Broken Hill Airport Broken Hill NSW YBKE Bourke Airport Bourke NSW YBNA Ballina / Byron Gateway Airport Ballina NSW YBRW Brewarrina Airport Brewarrina NSW YBTH Bathurst Airport Bathurst NSW YCBA Cobar Airport Cobar NSW YCBB Coonabarabran Airport Coonabarabran NSW YCDO Condobolin Airport Condobolin NSW YCFS Coffs Harbour Airport Coffs Harbour NSW YCNM Coonamble Airport Coonamble NSW YCOM Cooma - Snowy Mountains Airport Cooma NSW YCOR Corowa Airport Corowa NSW YCTM Cootamundra Airport Cootamundra NSW YCWR Cowra Airport Cowra NSW YDLQ Deniliquin Airport Deniliquin NSW YFBS Forbes Airport Forbes NSW YGFN Grafton Airport Grafton NSW YGLB Goulburn Airport Goulburn NSW YGLI Glen Innes Airport Glen Innes NSW YGTH Griffith Airport Griffith NSW YHAY Hay Airport Hay NSW YIVL Inverell Airport Inverell NSW YIVO Ivanhoe Aerodrome Ivanhoe NSW YKMP Kempsey Airport Kempsey NSW YLHI Lord Howe Island Airport Lord Howe Island NSW YLIS Lismore Regional Airport Lismore NSW YLRD Lightning Ridge Airport Lightning Ridge NSW YMAY Albury Airport Albury NSW YMDG Mudgee Airport Mudgee NSW YMER -
Dynamical Evolution of Planets Orbiting Two Stars
TATOOINE'S FUTURE: DYNAMICAL EVOLUTION OF PLANETS ORBITING TWO STARS Keavin Moore A THESIS SUBMITTED TO THE FACULTY OF GRADUATE STUDIES IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE Graduate Program in Physics and Astronomy York University Toronto, Ontario September 2017 c Keavin Moore, 2017 ii Abstract Science fiction has long teased our imaginations with tales of planets with two suns. How these planets form and evolve, and their survival prospects, are active fields of research. Expanding on previous work, four new Kepler candidate circumbinary planet systems were evolved through the complex common-envelope phase. The dynamical response of the planets to this dramatic evolutionary phase was simulated using open-source binary star evolution and numerical integrator codes. All four systems undergo at least one common-envelope phase; one experience two and another, three. Their planets tend to survive the common-envelope phase, regardless of relative inclination, and migrate to wider, more eccentric orbits; orbital expansion can occur well within a single planetary orbit. During the secondary common-envelope phases, the planets can gain sufficient eccentricity to be ejected from the system. Depending on the mass-loss rate, the planets either migrate adiabatically outward within a few orbits, or non-adiabatically to much more eccentric orbits. Their final orbital configurations are consistent with those of post-common-envelope circumbinary planet candidates, suggesting a possible origin for the latter. The results from this work provide a basis for future observations of post-common-envelope circumbinary systems. iii Acknowledgements Space has fascinated me since I was a kid; I remember watching the first Star Wars and realizing just how much more the night sky was than just a black sheet with tiny dots of light.