ESA) Organisation, Programmes, Ambitions
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ESA Missions AO Analysis
ESA Announcements of Opportunity Outcome Analysis Arvind Parmar Head, Science Support Office ESA Directorate of Science With thanks to Kate Isaak, Erik Kuulkers, Göran Pilbratt and Norbert Schartel (Project Scientists) ESA UNCLASSIFIED - For Official Use The ESA Fleet for Astrophysics ESA UNCLASSIFIED - For Official Use Dual-Anonymous Proposal Reviews | STScI | 25/09/2019 | Slide 2 ESA Announcement of Observing Opportunities Ø Observing time AOs are normally only used for ESA’s observatory missions – the targets/observing strategies for the other missions are generally the responsibility of the Science Teams. Ø ESA does not provide funding to successful proposers. Ø Results for ESA-led missions with recent AOs presented: • XMM-Newton • INTEGRAL • Herschel Ø Gender information was not requested in the AOs. It has been ”manually” derived by the project scientists and SOC staff. ESA UNCLASSIFIED - For Official Use Dual-Anonymous Proposal Reviews | STScI | 25/09/2019 | Slide 3 XMM-Newton – ESA’s Large X-ray Observatory ESA UNCLASSIFIED - For Official Use Dual-Anonymous Proposal Reviews | STScI | 25/09/2019 | Slide 4 XMM-Newton Ø ESA’s second X-ray observatory. Launched in 1999 with annual calls for observing proposals. Operational. Ø Typically 500 proposals per XMM-Newton Call with an over-subscription in observing time of 5-7. Total of 9233 proposals. Ø The TAC typically consists of 70 scientists divided into 13 panels with an overall TAC chair. Ø Output is >6000 refereed papers in total, >300 per year ESA UNCLASSIFIED - For Official Use -
Call for M5 Missions
ESA UNCLASSIFIED - For Official Use M5 Call - Technical Annex Prepared by SCI-F Reference ESA-SCI-F-ESTEC-TN-2016-002 Issue 1 Revision 0 Date of Issue 25/04/2016 Status Issued Document Type Distribution ESA UNCLASSIFIED - For Official Use Table of contents: 1 Introduction .......................................................................................................................... 3 1.1 Scope of document ................................................................................................................................................................ 3 1.2 Reference documents .......................................................................................................................................................... 3 1.3 List of acronyms ..................................................................................................................................................................... 3 2 General Guidelines ................................................................................................................ 6 3 Analysis of some potential mission profiles ........................................................................... 7 3.1 Introduction ............................................................................................................................................................................. 7 3.2 Current European launchers ........................................................................................................................................... -
ESA Solar System Missions
Small Missions and the Science Programme of ESA Alvaro Gimenez, Director of Science and Robotic Exploration 26 February 2014 2 2 Astro-H suzaku corot Science Programme building blocks “Large” (Ariane 5-class) missions 1. High innovation content 2. European flagships 3. 1 B€ class 4. 3 per 20 years Herschel XMM-Newton Rosetta BepiColombo L3 L2 JUICE BepiColombo GAIA Herschel Rosetta XMM STSP 1980 1990 2000 2010 2020 2030 2040 H2000 H2000+ CV 2040 2035 2030 2025 2020 2015 2010 2005 2000 1995 1990 0 2 4 6 8 10 Science Programme building blocks “Medium” (Soyuz-class) missions 1. Makes use of current cutting-edge technology 2. Programme workhorse 3. 500 M€ class Planck 4. 3-4 per 10 years Euclid Solar Orbiter Mars Express 2040 2030 2020 2010 2000 1990 1980 0 5 10 15 20 Science Programme building blocks Missions of Opportunity 1. Moderate-size participation of the ESA Science Programme in missions led by partners 2. Format can vary 3. Increase flight and science opportunities for European scientists COROT ASTRO-H Hinode Double Star Science Programme building blocks Small missions a. New Programme element, still “experimental” b. Fast and with ESA CaC = 0.1 yearly budget c. Increase flight opportunities for European scientists d. Example: CHEOPS PLATO EUCLID SOLAR JUICE Astro H ORBITER µSCOPE Cheops ExoMars JWST BEPI LISA PF GAIA COLOMBO Akari Proba 2 Chandrayaan PLANCK Hinode HERSCHEL COROT ROSETTA Double Star SMART INTEGRAL Suzaku 1 SOHO VENUS MARS XMM F 2 CLUSTER → EXPRESS EXPRESS NEWTON CLUSTER HUYGENS ULYSSES ISO Time II HST 2030 2025 2020 2015 2010 2005 2000 1995 1990 1985 0 2 4 6 8 10 12 Small missions a. -
Observation of Pc 3/5 Magnetic Pulsations Around the Cusp at Mid Altitude
1 OBSERVATION OF PC 3/5 MAGNETIC PULSATIONS AROUND THE CUSP AT MID ALTITUDE Liu Yonghua(1), Liu Ruiyuan(1), B. J. Fraser(2), S. T. Ables(2), Xu Zhonghua(1), Zhang Beichen(1), Shi Jiankui(3), Liu Zhenxing(3), Huang Dehong(1), Hu Zejun(1), Chen Zhuotian(1), Wang Xiao(3), Malcolm Dunlop(4), A. Balogh(5) (1) Polar Research Institute of China, 451 Jinqiao Rd., Shanghai 200136, P. R. CHINA, [email protected] (2) The University of Newcastle, University Drive, Callaghan NSW 2308, AUSTRALIA, [email protected] (3)The Center of Space Science & Applied Research, Chinese Academy of Science, Post Box8701, Beijing 100080, jkshi@@center.cssar.ac.cn (4) The Rutherford Appleton Laboratory, Chilton, DIDCOT, Oxfordshire, OX11 0QX, UK, [email protected] (5)Space and Atmospheric Physics Group, Imperial College, London, [email protected] ABSTRACT transmitted straightforwardly from solar wind to the ionosphere (Bolshakova & Troitskaia, 1984). So far most Since launched in year 2000 the Cluster mission has research work on such topic are on basis of observation passed the region around the cusp at mid-altitude (~6Re) at ground or/and data from satellite located in the for many times, where ULF wave activities are rich in. upstream of solar wind or in the magnetosheath. To my From 0800 to 1300UT on October 30 2002 the Cluster knowledge, few authors take a study based on the spacecrafts ran along an orbit of southern cusp- measurement at the mid-altitude of the cusp. It seems plasmasphere-northern cusp that provides an excellent reasonable to assume that such a measurement be a direct observation of ULF waves in dayside magnetosphere. -
China's Space Industry and International Collaboration
China’s Space Industry and International Collaboration Presenter: Ju Jin Title: Minister Counselor,the Embassy of P.R.China Date: Feb 27,2008 Brief History • 52 years since 1956, first space institute established • Learning from Soviet Union until 1960 • U.S.A.’s close door policy until now • China’s self-reliance Policy Major Achievements • 12 series of Long March Launching Rockets • >100 Launches • >80 satellites in remote sensing, telecommunication, GPS, scientific experiment • Manned space flights——Shenzhou 5 (2003) and Shenzhou 6 (2005) • Lunar Exploration Project——Chang’e 1 (2007) LM-2F Launch Vehicle • Stages 1 & 2 & 4 strap-on boosters • 58.3 meters long • Launch Mass: 480 tons • Total Thrust : 600 tons • Reliability & Safety Index: 0.97 & 0.997 • 10 Sub-Systems Manned Space Flight--Shenzhou 6 Manned Space Flight--Shenzhou 6 Lunar Probe Project--Change-1 First Lunar Surface Photos Lunar Probe Project—Change 1 • 3 Years • 17,000 Scientists and Engineers • Young Team averaged in the age of 30s • 100% China-Made • Technology Breakthroughs – All-direction Antenna – Ultra-violet Sensor International Exchange and Cooperation: Main Activities Over the recent years, China has signed cooperation agreements on the peaceful use of outer space and space project cooperation agreements with Argentina, Brazil, Canada, France, Malaysia, Pakistan, Russia, Ukraine, the ESA and the European Commission, and has established space cooperation subcommittee or joint commission mechanisms with Brazil, France, Russia and Ukraine. China and the ESA z Sino-ESA Double Star Satellite Exploration of the Earth's Space Plan. z "Dragon Program," involving cooperation in Earth observation satellites, having so far conducted 16 remote-sensing application projects in the fields of agriculture, forestry, water conservancy, meteorology, oceanography and disasters. -
Prism Vol. 9, No. 2 Prism About Vol
2 021 PRISMVOL. 9, NO. 2 | 2021 PRISM VOL. 9, NO. 2 NO. 9, VOL. THE JOURNAL OF COMPLEX OPER ATIONS PRISM ABOUT VOL. 9, NO. 2, 2021 PRISM, the quarterly journal of complex operations published at National Defense University (NDU), aims to illuminate and provoke debate on whole-of-government EDITOR IN CHIEF efforts to conduct reconstruction, stabilization, counterinsurgency, and irregular Mr. Michael Miklaucic warfare operations. Since the inaugural issue of PRISM in 2010, our readership has expanded to include more than 10,000 officials, servicemen and women, and practi- tioners from across the diplomatic, defense, and development communities in more COPYEDITOR than 80 countries. Ms. Andrea L. Connell PRISM is published with support from NDU’s Institute for National Strategic Studies (INSS). In 1984, Secretary of Defense Casper Weinberger established INSS EDITORIAL ASSISTANTS within NDU as a focal point for analysis of critical national security policy and Ms. Taylor Buck defense strategy issues. Today INSS conducts research in support of academic and Ms. Amanda Dawkins leadership programs at NDU; provides strategic support to the Secretary of Defense, Chairman of the Joint Chiefs of Staff, combatant commands, and armed services; Ms. Alexandra Fabre de la Grange and engages with the broader national and international security communities. Ms. Julia Humphrey COMMUNICATIONS INTERNET PUBLICATIONS PRISM welcomes unsolicited manuscripts from policymakers, practitioners, and EDITOR scholars, particularly those that present emerging thought, best practices, or train- Ms. Joanna E. Seich ing and education innovations. Publication threshold for articles and critiques varies but is largely determined by topical relevance, continuing education for national and DESIGN international security professionals, scholarly standards of argumentation, quality of Mr. -
Thermal Test Campaign of the Solar Orbiter STM
46th International Conference on Environmental Systems ICES-2016-236 10-14 July 2016, Vienna, Austria Thermal Test Campaign of the Solar Orbiter STM C. Damasio1 European Space Agency, ESA/ESTEC, Noordwijk ZH, 2201 AZ, The Netherlands A. Jacobs2, S. Morgan3, M. Sprague4, D. Wild5, Airbus Defence & Space Limited,Gunnels Wood Road, Stevenage, SG1 2AS, UK and V. Luengo6 RHEA System S.A., Av. Pasteur 23, B-1300 Wavre, Belgium Solar Orbiter is the next solar-heliospheric mission in the ESA Science Directorate. The mission will provide the next major step forward in the exploration of the Sun and the heliosphere investigating many of the fundamental problems in solar and heliospheric science. One of the main design drivers for Solar Orbiter is the thermal environment, determined by a total irradiance of 13 solar constants (17500 W/m2) due to the proximity with the Sun. The spacecraft is normally in sun-pointing attitude and is protected from severe solar energy by the Heat Shield. The Heat Shield was tested separately at subsystem level. To complete the STM thermal verification, it was decided to subject to Solar orbiter platform without heat shield to thermal balance test that was performed at IABG test facility in November- December 2015 This paper will describe the Thermal Balance Test performed on the Solar Orbiter STM and the activities performed to correlate the thermal model and to show the verification of the STM thermal design. Nomenclature AU = Astronomical Unit CE = Cold Element FM = Flight Model HE = Hot Element IABG = Industrieanlagen -
LISA, the Gravitational Wave Observatory
The ESA Science Programme Cosmic Vision 2015 – 25 Christian Erd Planetary Exploration Studies, Advanced Studies & Technology Preparations Division 04-10-2010 1 ESAESA spacespace sciencescience timelinetimeline JWSTJWST BepiColomboBepiColombo GaiaGaia LISALISA PathfinderPathfinder Proba-2Proba-2 PlanckPlanck HerschelHerschel CoRoTCoRoT HinodeHinode AkariAkari VenusVenus ExpressExpress SuzakuSuzaku RosettaRosetta DoubleDouble StarStar MarsMars ExpressExpress INTEGRALINTEGRAL ClusterCluster XMM-NewtonXMM-Newton CassiniCassini-H-Huygensuygens SOHOSOHO ImplementationImplementation HubbleHubble OperationalOperational 19901990 19941994 19981998 20022002 20062006 20102010 20142014 20182018 20222022 XMM-Newton • X-ray observatory, launched in Dec 1999 • Fully operational (lost 3 out of 44 X-ray CCD early in mission) • No significant loss of performances expected before 2018 • Ranked #1 at last extension review in 2008 (with HST & SOHO) • 320 refereed articles per year, with 38% in the top 10% most cited • Observing time over- subscribed by factor ~8 • 2,400 registered users • Largest X-ray catalogue (263,000 sources) • Best sensitivity in 0.2-12 keV range • Long uninterrupted obs. • Follow-up of SZ clusters 04-10-2010 3 INTEGRAL • γ-ray observatory, launched in Oct 2002 • Imager + Spectrograph (E/ΔE = 500) + X- ray monitor + Optical camera • Coded mask telescope → 12' resolution • 72 hours elliptical orbit → low background • P/L ~ nominal (lost 4 out 19 SPI detectors) • No serious degradation before 2016 • ~ 90 refereed articles per year • Obs -
Cryogenics in Space
— 37 — Cryogenics in space Nicola RandoI Abstract Cryogenics plays a key role on board space-science missions, with a range of applications, mainly in the domain of astrophysics. Indeed a tremendous progress has been achieved over the last 20 years in cryogenics, with enhanced reliability and simpler operations, thus matching the needs of advanced focal-plane detectors and complex science instrumentation. In this article we provide an overview of recent applications of cryogenics in space, with specific emphasis on science missions. The overview includes an analysis of the impact of cryogenics on the spacecraft system design and of the main technical solutions presently adopted. Critical technology developments and programmatic aspects are also addressed, including specific needs of future science missions and lessons learnt from recent programmes. Introduction H. Kamerlingh-Onnes liquefied 4He for the first time in 1908 and discovered superconductivity in 1911. About 100 years after such achievements (Pobell 1996), cryogenics plays a key role on board space-science missions, providing the environ- ment required to perform highly sensitive measurements by suppressing the thermal background radiation and allowing advantage to be taken of the performance of cryogenic detectors. In the last 20 years several spacecraft have been equipped with cryogenic in- strumentation. Among such missions we should mention IRAS (launched in 1983), ESA’s ISO (launched in 1995) (Kessler et al 1996) and, more recently, NASA’s Spitzer (formerly SIRTF, launched in 2006) (Werner 2005) and the Japanese mis- sion Akari (IR astronomy mission launched in 2006) (Shibai 2007). New missions involving cryogenics are the ESA missions Planck (dedicated to the mapping of the cosmic background radiation) and Herschel (far infrared and sub-millimetre observatory), carrying instruments operating at temperatures of 0.1 K and 0.3 K, respectively (Crone et al 2006). -
The High Energy Astrophysics Division Newsletter
SPRING 2017 The High Energy Astrophysics Division Newsletter In this Issue: View from the Chair — special advertising section — hidden black holes revealed, and others — second running — finding a path through spacetime — announcing mysteries under the ice — performance enhancements for Chandra — milestones for XMM — the hunt continues for Swift — ULXNS — on the trail of the wild neutrino with INTEGRAL — searching at home with Fermi — energetic electrons seen at the ISS — news from the cosmos — of scientific interest — a Universe of learning — NICER launch prep — SRG progress — the wisdom of Athena — the slant on IXPE — the XARM — building CTA — all-seeing Lynx — in memoriam From the Chair for the discovery of merging black hole binaries, and for beginning the new era of gravitational-wave astronomy. CHRIS REYNOLDS (U. MD) Prof. González will give the Rossi Prize Lecture at the All systems are go for our 16th Divisional meeting to 231st AAS meeting to be held at National Harbor, MD be held in Sun Valley, Idaho, 20-24 August 2017! Regis- in January 2018. Please join me in congratulating all of tration and abstract submission is now open and we’re this year’s HEAD prize winners. looking forward to an exciting scientific program cover- ing all aspects of high-energy astrophysics, kicked off by The past few months has been eventful in the world a total solar eclipse! of high-energy astrophysics missions. NICER and ISS- CREAM are at the Kennedy Space Center and ready for One of the most important aspects of these meet- launch to the International Space Station. Further in the ings is the chance to honor a new batch of HEAD future, NASA has formally selected the Imaging X-ray Po- prize winners. -
NASA HQ Update on IXO
NASA HQ Update on IXO IXO Facility Science Team Meeting GSFC, 20 August 2008 Michael Salamon Astrophysics Division, NASA HQ Recent History of IXO • Stern and Southwood at NASA/ESA bilateral informally agree that Con-X and XEUS must find a path forward to a single, merged mission (Paris, Sept 2007). • Southwood letter to Stern (Jan 2008) invites NASA to participate in XEUS study as a starting point leading to possible interagency partnership. • Morse/Favata letter (May 2008): • Con-X is highest priority large-class mission following JWST (2000 Decadal), to be revisited in 2010 Decadal. • XEUS selected as one of three CV L-class competing missions (Outer Planets, XEUS, LISA) with downselection in 2009 and 2011. • Limited resources in both agencies and considerable overlap in science goals argue for finding a joint mission approach. • Agreement for a joint mission study (not the mission itself). • Formation of coordination group (CG) composed of ESA, NASA, and JAXA representatives. • First task of CG is to determine the existence of possible joint mission scenarios. • Once found, study the joint mission scenario to the level required by the selection process milestones of the agencies involved. • No consideration to be given by the CG of which agency might lead the merged mission. IXO Coordination Group • IXO-CG initially charged to find a joint mission scenario for further joint study by the agencies (ESA, NASA, JAXA). • IXO-CG now charged with definition of science requirements for the IXO concept, scientific supervision of study activities, reporting to Agencies. • IXO-CG jointly chaired by the ESA and NASA study scientists. -
We Need Your Colouring Skills!
We need your colouring skills! What do you think the colours of Mercury are? DID YOU KNOW? ercury • Mercury is the smallest planet in our solar system. • It is only slightly larger than the Earth’s Moon. • One day on Mercury is as long as 59 days on Earth. • A year on Mercury is as long as 88 Earth days • Temperatures on Mercury are extreme, reaching 430°C during the day, and -180°C at night. DID YOU KNOW? The Erth Depending on where you are on the globe, you could be spinning through space at just over 1,000 miles per hour. Water covers 70 percent of Earth's surface. 1 million Earths could fit in the Sun. Earth's atmosphere is composed of about 78 percent nitrogen, 21 percent oxygen, 0.9 percent argon, and 0.1 percent other gases. Earth is the only planet not named after a god. We need your colouring skills! What colours will you choose? We need your colouring skills! What do you think the colours of Jupiter are? DID YOU KNOW? Jupiter • Jupiter is the largest planet in the solar system. • Jupiter is as large as 1,300 Earths. • It's the 3rd brightest object in the night sky. • There's a big red spot on Jupiter, which is in fact a storm that has been raging for more than 350 years. DID YOU KNOW? Saturn • Saturn is the 2nd largest planet in the Solar System. • 764 Earths could fit inside Saturn. • Saturn's rings are made of ice and rock. They span 175,000 miles We need your and yet they’re only 20 metres thick.