Atmospheric Lidar (ATLID): Pre-Launch Testing and Calibration of the European Space Agency Instrument That Will Measure Aerosols and Thin Clouds in the Atmosphere
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Toward Non-Invasive Measurement of Atmospheric Temperature Using Vibro-Rotational Raman Spectra of Diatomic Gases
remote sensing Article Toward Non-Invasive Measurement of Atmospheric Temperature Using Vibro-Rotational Raman Spectra of Diatomic Gases Tyler Capek 1,*,† , Jacek Borysow 1,† , Claudio Mazzoleni 1,† and Massimo Moraldi 2,† 1 Department of Physics, Michigan Technological University, Houghton, MI 49931, USA; [email protected] (J.B.); [email protected] (C.M.) 2 Dipartimento di Fisica e Astronomia, Universita’ degli Studi di Firenze, via Sansone 1, I-50019 Sesto Fiorentino, Italy; massimo.moraldi@fi.infn.it * Correspondence: [email protected] † These authors contributed equally to this work. Received: 8 October 2020; Accepted: 15 December 2020; Published: 17 December 2020 Abstract: We demonstrate precise determination of atmospheric temperature using vibro-rotational Raman (VRR) spectra of molecular nitrogen and oxygen in the range of 292–293 K. We used a continuous wave fiber laser operating at 10 W near 532 nm as an excitation source in conjunction with a multi-pass cell. First, we show that the approximation that nitrogen and oxygen molecules behave like rigid rotors leads to erroneous derivations of temperature values from VRR spectra. Then, we account for molecular non-rigidity and compare four different methods for the determination of air temperature. Each method requires no temperature calibration. The first method involves fitting the intensity of individual lines within the same branch to their respective transition energies. We also infer temperature by taking ratios of two isolated VRR lines; first from two lines of the same branch, and then one line from the S-branch and one from the O-branch. Finally, we take ratios of groups of lines. -
Planetary Science Division Status Report
Planetary Science Division Status Report Jim Green NASA, Planetary Science Division January 26, 2017 Astronomy and Astrophysics Advisory CommiBee Outline • Planetary Science ObjecFves • Missions and Events Overview • Flight Programs: – Discovery – New FronFers – Mars Programs – Outer Planets • Planetary Defense AcFviFes • R&A Overview • Educaon and Outreach AcFviFes • PSD Budget Overview New Horizons exploresPlanetary Science Pluto and the Kuiper Belt Ascertain the content, origin, and evoluFon of the Solar System and the potenFal for life elsewhere! 01/08/2016 As the highest resolution images continue to beam back from New Horizons, the mission is onto exploring Kuiper Belt Objects with the Long Range Reconnaissance Imager (LORRI) camera from unique viewing angles not visible from Earth. New Horizons is also beginning maneuvers to be able to swing close by a Kuiper Belt Object in the next year. Giant IcebergsObjecve 1.5.1 (water blocks) floatingObjecve 1.5.2 in glaciers of Objecve 1.5.3 Objecve 1.5.4 Objecve 1.5.5 hydrogen, mDemonstrate ethane, and other frozenDemonstrate progress gasses on the Demonstrate Sublimation pitsDemonstrate from the surface ofDemonstrate progress Pluto, potentially surface of Pluto.progress in in exploring and progress in showing a geologicallyprogress in improving active surface.in idenFfying and advancing the observing the objects exploring and understanding of the characterizing objects The Newunderstanding of Horizons missionin the Solar System to and the finding locaons origin and evoluFon in the Solar System explorationhow the chemical of Pluto wereunderstand how they voted the where life could of life on Earth to that pose threats to and physical formed and evolve have existed or guide the search for Earth or offer People’sprocesses in the Choice for Breakthrough of thecould exist today life elsewhere resources for human Year forSolar System 2015 by Science Magazine as exploraon operate, interact well as theand evolve top story of 2015 by Discover Magazine. -
New Opportunities for Ice Sheet Observations
Remote Sens. 2015, 7, 9371-9389; doi:10.3390/rs70709371 OPEN ACCESS remote sensing ISSN 2072-4292 www.mdpi.com/journal/remotesensing Article The Sentinel-1 Mission: New Opportunities for Ice Sheet Observations Thomas Nagler 1,*, Helmut Rott 1,2, Markus Hetzenecker 1, Jan Wuite 1 and Pierre Potin 3 1 ENVEO IT GmbH, Technikerstrasse 21a, A-6020 Innsbruck, Austria; E-Mails: [email protected] (H.R.); [email protected] (M.H.); [email protected] (J.W.) 2 Institute for Meteorology and Geophysics, University of Innsbruck, A-6020 Innsbruck, Austria 3 European Space Agency/ESRIN, via Galileo Galilei, I-00044 Frascati, Italy; E-Mail: [email protected] * Author to whom correspondence should be addressed; E-Mail: [email protected]; Tel.: +43-512-507-48300; Fax: +43-512-507-48319. Academic Editors: Nicolas Baghdadi and Prasad S. Thenkabail Received: 28 May 2015 / Accepted: 14 July 2015 / Published: 22 July 2015 Abstract: The Sentinel satellite constellation series, developed by the European Space Agency, represents the dedicated space component of the European Copernicus program, committed to long-term operational services in a wide range of application domains. Here, we address the potential of the Sentinel-1 mission for mapping and monitoring the surface velocity of glaciers and ice sheets. We present an ice velocity map of Greenland, derived from synthetic aperture radar (SAR) data acquired in winter 2015 by Sentinel-1A, the first satellite of the Copernicus program in orbit. The map is assembled from about 900 SAR scenes acquired in Interferometric Wide swath (IW) mode, applying the offset tracking technique. -
CHAPTER CONTENTS Page CHAPTER 5
CHAPTER CONTENTS Page CHAPTER 5. SPECIAL PROFILING TECHNIQUES FOR THE BOUNDARY LAYER AND THE TROPOSPHERE .............................................................. 640 5.1 General ................................................................... 640 5.2 Surface-based remote-sensing techniques ..................................... 640 5.2.1 Acoustic sounders (sodars) ........................................... 640 5.2.2 Wind profiler radars ................................................. 641 5.2.3 Radio acoustic sounding systems ...................................... 643 5.2.4 Microwave radiometers .............................................. 644 5.2.5 Laser radars (lidars) .................................................. 645 5.2.6 Global Navigation Satellite System ..................................... 646 5.2.6.1 Description of the Global Navigation Satellite System ............. 647 5.2.6.2 Tropospheric Global Navigation Satellite System signal ........... 648 5.2.6.3 Integrated water vapour. 648 5.2.6.4 Measurement uncertainties. 649 5.3 In situ measurements ....................................................... 649 5.3.1 Balloon tracking ..................................................... 649 5.3.2 Boundary layer radiosondes .......................................... 649 5.3.3 Instrumented towers and masts ....................................... 650 5.3.4 Instrumented tethered balloons ....................................... 651 ANNEX. GROUND-BASED REMOTE-SENSING OF WIND BY HETERODYNE PULSED DOPPLER LIDAR ................................................................ -
Fraunhofer Lidar Prototype in the Green Spectral Region for Atmospheric Boundary Layer Observations
Remote Sens. 2013, 5, 6079-6095; doi:10.3390/rs5116079 OPEN ACCESS Remote Sensing ISSN 2072-4292 www.mdpi.com/journal/remotesensing Article Fraunhofer Lidar Prototype in the Green Spectral Region for Atmospheric Boundary Layer Observations Songhua Wu *, Xiaoquan Song and Bingyi Liu Ocean Remote Sensing Institute, Ocean University of China, 238 Songling Road, Qingdao 266100, China; E-Mails: [email protected] (X.S.); [email protected] (B.L.) * Author to whom correspondence should be addressed; E-Mail: [email protected]; Tel.: +86-532-6678-2573. Received: 8 October 2013; in revised form: 27 October 2013 / Accepted: 13 November 2013 / Published: 18 November 2013 Abstract: A lidar detects atmospheric parameters by transmitting laser pulse to the atmosphere and receiving the backscattering signals from molecules and aerosol particles. Because of the small backscattering cross section, a lidar usually uses the high sensitive photomultiplier and avalanche photodiode as detector and uses photon counting technology for collection of weak backscatter signals. Photon Counting enables the capturing of extremely weak lidar return from long distance, throughout dark background, by a long time accumulation. Because of the strong solar background, the signal-to-noise ratio of lidar during daytime could be greatly restricted, especially for the lidar operating at visible wavelengths where solar background is prominent. Narrow band-pass filters must therefore be installed in order to isolate solar background noise at wavelengths close to that of the lidar receiving channel, whereas the background light in superposition with signal spectrum, limits an effective margin for signal-to-noise ratio (SNR) improvement. This work describes a lidar prototype operating at the Fraunhofer lines, the invisible band of solar spectrum, to achieve photon counting under intense solar background. -
Venona Special Studies
- 1 - Venona Project Special Studies Transcribed by Students of the Mercyhurst College Institute for Intelligence Studies Arranged by John Earl Haynes, Library of Congress, 2010 COVER NAMES IN NEW YORK TRAFFIC p. 2 UNIDENTIFIED COVER NAMES IN NEW YORK TRAFFIC p. 86 COVER NAMES IN SAN FRANCISCO TRAFFIC p. 92 COVER NAMES IN WASHINGTON TRAFFIC p. 123 ADDITIONAL COVERNAMES AND RELATED INFORMATION IN DIPLOMATIC TRAFFIC p. 127 REVISED TRANSLATION OF MESSAGE ON ANTENNA-LIBERAL'S WIFE ETHEL p. 135 THE COVERNAMES "ANTENNA" AND "LIBERAL" IN . MESSAGES p. 139 ESSAGES IN . INVOLVING THE COVERNAME"ENORMOZ" AND THE NAMES OF NUCLEAR PHYSICISTS, ETC. p. 147 UNDATED REPORT OF MEREDITH GARDNER p. 155 DEVELOPMENT OF THE “G--“HOMER” [“GOMER”] CASE p. 158 THE KOMAR (KRAVCHENKO) AFFAIR IN . MESSAGES p. 161 REVISED TRANSLATION OF TWO . MESSAGES ON CHANGES IN COVERNAMES p. 170 THE COVERNAME "KARAS" IN. TRAFFIC p. 178 THE COVERNAMES "TÉNOR", "BAS", AND "CHETÁ" (? IN . TRAFFIC p. 181 - 2 - Special Study Cover Names in New York Traffic - 3 - cover-name Message number Date Publication reference S/ or 3/NBF/ 19 N.Y. to M. 812 29053 JKI 06 T1022 1B-1910 0027A ABRAM N.Y. to M. 992 24063 JKR 14 T872√ 1B-7518 0005A JACK SOBLE 1086 06073 JKV 48 T873√ 2A-0011 1957 29113 NNNNNN T939√ 625 04054 JHD 48 T916√ 851 15064 JIJ 40 T10.1√ 1146 10084 JHM 41 T123√ 1251 02094 JHN 12 T301√ (to ChEKh) 0005B 1353 23094 JHO 42 T289√ 1449 12104 JIL 37 T106√ 1754 14124 JHZ 49 T6√ 48 11015 JHV 37 (NSA)T1941 AVGUR 2A-0013 1638 (AUGUR) N.Y. -
Atmospheric Dynamics Mission. the Phase-A Studies Were All Completed in June 1999
ESA SP-1233 (4) July 1999 Reports for Mission Selection THE FOUR CANDIDATE EARTH EXPLORER CORE MISSIONS Atmospheric Dynamics Mission ESA SP-1233 (4) – The Four Candidate Earth Explorer Core Missions – ATMOSPHERIC DYNAMICS _________________________________________________________________ Report prepared by: Earth Sciences Division Scientific Co-ordinator: Paul Ingmann Earth Observation Preparatory Programme Technical Co-ordinator: Joachim Fuchs Cover: Richard Francis & Carel Haakman Published by: ESA Publications Division c/o ESTEC, Noordwijk, The Netherlands Editor: Bruce Battrick Copyright: © 1999 European Space Agency ISBN 92-9092-528-0 Price: 70 DFl CONTENTS 1 INTRODUCTION................................................................................................................................5 2 BACKGROUND AND SCIENTIFIC JUSTIFICATION...............................................................9 2.1 GLOBAL WIND PROFILE MEASUREMENTS FOR CLIMATE AND NWP........................................9 2.2 THE NEED FOR ATMOSPHERIC WIND FIELDS FOR ATMOSPHERIC ANALYSES .........................10 2.3 POTENTIAL IMPROVEMENT OF NWP BY ENHANCED WIND OBSERVATIONS ...........................14 2.4 THE NEED FOR ATMOSPHERIC WIND FIELDS FOR CLIMATE STUDIES......................................22 2.5 FUTURE STUDIES AND PERSPECTIVES AIMING AT IMPROVING THE WIND FIELD KNOWLEDGE IN THE POST-2000 TIME FRAME ................................................................................................31 2.6 CONCLUSIONS ON NWP AND CLIMATE STUDIES ......................................................................33 -
Campaigns / the Living Planet Programme / Observing the Earth / Our Activities / ESA
Campaigns / The Living Planet Programme / Observing the Earth / Our Activities / ESA → EUROPEAN SPACE ABOUT US OUR ACTIVITIES CONNECT WITH US FOR MEDIA FOR EDUCATORS FOR KIDS AGENCY ESA OBSERVING THE EARTH LIVING PLANET CAMPAIGNS About Campaigns ESA > Our Activities > Observing the Earth > The Living Planet Programme > Campaigns Recent campaigns Cryovex DomeC-air DOMEX-3 IceSAR-2012 Campaigns blog KaSAR SMOS-ice Services Subscribe Campaigns photo gallery Contact us ARCTIC TREK FOR CRYOSAT A short video from Cold Facts explains why going to the Arctic to collect snow and ice measurements ensures confidence in the data from ESA’s CryoSat mission Campaigns data Archive LATEST NEWS Focus on Gabon forests for Biomass 03 March 2016 Gabon on the radar 22 July 2015 Revealing mountains hiding under ice 29 April 2015 Ice venturers yield results for CryoSat 18 March 2015 Plant power from above 03 February 2015 http://www.esa.int/Our_Activities/Observing_the_Earth/The_Living_Planet_Programme/Campaigns[19/04/2016 12:58:52] Campaigns / The Living Planet Programme / Observing the Earth / Our Activities / ESA Air quality under new scrutiny 28 October 2014 News Archive LATEST ARTICLES MOST-VIEWED ARTICLES MOST-VIEWED IMAGES MOST-VIEWED VIDEOS · Sentinel-1 sees rice paddy drop in… · Live updates: Rosetta mission… · Welcome to a comet · Europe’s solar eclipse seen f… · Interstellar dust intercepted at S… · Touchdown! Rosetta’s Philae p… · ROLIS descent image · Rosetta’s twelve-year journey… · Nansen gives birth to two icebergs · Pioneering Philae completes m… · First comet panoramic · Ambition the film · First light for ExoMars · Rosetta to deploy lander on 1… · OSIRIS spots Philae drifting … · Reconstructing Philae’s flight · Busy spacecraft and experiment sch… · Black hole-star pair orbiting… · Comet panoramic – lander orie… · Timelapse: Canary Islands to … FAQ JOBS AT ESA SITE MAP CONTACTS TERMS AND CONDITIONS http://www.esa.int/Our_Activities/Observing_the_Earth/The_Living_Planet_Programme/Campaigns[19/04/2016 12:58:52]. -
The Hera Mission
Dr. Patrick Michel Hera Investigation Team PI Université Côte d’Azur Observatoire de la Côte d’Azur CNRS, Lagrange Laboratory Nice, France The Hera Mission ESA UNCLASSIFIED - For Official Use Hera main aspects Role of space missions at ESA in NEO hazard mitigation • Understanding the problem (deflection modeling and simulations) 2001 • Ground versus space solutions analyses • Assessment of space component options 2002- • 6 parallel phase-0 studies (3 space telescopes, 3 rendezvous) Euneos Nero Earthguard 1 2004 • ESA’s NEO Mission Advisory Panel (NEOMAP) established • Kinetic impactor validation ranked highest importance 2004- • Don Quijote mission selected and studied up to phase-A level 2006 • SANCHO / Proba-IP orbiter up to phase A level studies, small deep-space Don Quijote Ishtar Simone 2008- mission to investigate impactor’s result 2009 • AIDA proposed by NASA: USA/impactor + ESA/impact assessment • ESA phase 0 and phase A studies on the observer spacecraft "AIM” (GSP) 2011- Proba-IP 2016 • Phase B1 study and “consolidation phase” for mission definition (GSTP) • HERA: impact observer spacecraft reformulation and optimization AIM 2017- • Phase B1 implementation + payload + technology breadboards (GSTP+SSA) Several concepts 2019 • DART phase-C kick-off on 15 May 2018 Hera iterated AIDA: An International Planetary Defense Mission U.S. National Research Council Committee “Defending Planet Earth: Near-Earth Object Surveys and Hazard Mitigation Strategies” Recommendation: “If [U.S.] Congress chooses to fund mitigation research at an appropriately high level, the first priority for a space mission in the mitigation area is an experimental test of a kinetic impactor along with a characterization, monitoring, and verification system, such as the Don Quixote mission that was previously considered, but not funded, by the European Space Agency. -
Securing the Copernicus Programme Why EU Earth Observation Matters
Briefing April 2017 Securing the Copernicus programme Why EU earth observation matters SUMMARY The Copernicus programme is a user-driven programme which provides six free-of- charge operational services (atmosphere monitoring, marine environment monitoring, land monitoring, climate change, emergency management and security) to EU, national, and regional institutions, as well as to the private sector. The programme builds on the initiative on global monitoring for environment and security launched in 2001. It aims at filling the gaps in European earth observation capacities. Data is provided from space infrastructures, particularly the sentinel missions developed under the programme, and in situ infrastructure supported by the Member States. Copernicus services are mainly operated by European Union (EU) agencies. Copernicus requires a high level of continuity in data and service provision. A strong political commitment at EU level is required to provide adequate funding for the development of the operational earth observation missions and services. The EU – under the framework programme for research and operational programmes – and the European Space Agency (ESA) have invested more than €7 billion in Copernicus since 2002. By the end of 2017, four of the six sentinel missions should be fully deployed and the last of the six services should become fully operational. As Copernicus reaches its full operational stage, the focus of the programme is shifting towards the uptake of the services and the development of a downstream sector that would provide additional commercial services to the users. This aspect is a key priority of the space strategy adopted by the European Commission in October 2016. The development of the downstream sector is dependent on the long-term continuity of service, to be ensured by improved governance of the programme and renewed long- term political and financial commitments for the next EU budgetary period. -
First Provisional Land Surface Reflectance Product From
remote sensing Letter First Provisional Land Surface Reflectance Product from Geostationary Satellite Himawari-8 AHI Shuang Li 1,2, Weile Wang 3, Hirofumi Hashimoto 3 , Jun Xiong 4, Thomas Vandal 4, Jing Yao 1,2, Lexiang Qian 5,*, Kazuhito Ichii 6, Alexei Lyapustin 7 , Yujie Wang 7,8 and Ramakrishna Nemani 9 1 School of Geography and Resources, Guizhou Education University, Guiyang 550018, China; [email protected] (S.L.); [email protected] (J.Y.) 2 Guizhou Provincial Key Laboratory of Geographic State Monitoring of Watershed, Guizhou Education University, Guiyang 550018, China 3 NASA Ames Research Center—California State University Monterey Bay (CSUMB), Moffett Field, CA 94035, USA; [email protected] (W.W.); [email protected] (H.H.) 4 NASA Ames Research Center—Bay Area Environmental Research Institute (BAERI), Moffett Field, CA 94035, USA; [email protected] (J.X.); [email protected] (T.V.) 5 School of Geographical Sciences, Guangzhou University, Guangzhou 510006, China 6 Center for Environmental Remote Sensing, Chiba University, Chiba 263-8522, Japan; [email protected] 7 NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA; [email protected] (A.L.); [email protected] (Y.W.) 8 Joint Center for Earth systems Technology (JCET), University of Maryland-Baltimore County (UMBC), Baltimore, MD 21228, USA 9 Goddard Space Flight Center—NASA Ames Research Center, Moffett Field, CA 94035, USA; [email protected] * Correspondence: [email protected] Received: 11 October 2019; Accepted: 2 December 2019; Published: 12 December 2019 Abstract: A provisional surface reflectance (SR) product from the Advanced Himawari Imager (AHI) on-board the new generation geostationary satellite (Himawari-8) covering the period between July 2015 and December 2018 is made available to the scientific community. -
Observations of Atmospheric Aerosol and Cloud Using a Polarized Micropulse Lidar in Xi’An, China
atmosphere Article Observations of Atmospheric Aerosol and Cloud Using a Polarized Micropulse Lidar in Xi’an, China Chao Chen 1,2,3,4, Xiaoquan Song 1,* , Zhangjun Wang 1,2,3,4,*, Wenyan Wang 5, Xiufen Wang 2,3,4, Quanfeng Zhuang 2,3,4, Xiaoyan Liu 1,2,3,4 , Hui Li 2,3,4, Kuntai Ma 1, Xianxin Li 2,3,4, Xin Pan 2,3,4, Feng Zhang 2,3,4, Boyang Xue 2,3,4 and Yang Yu 2,3,4 1 College of Information Science and Engineering, Ocean University of China, Qingdao 266100, China; [email protected] (C.C.); [email protected] (X.L.); [email protected] (K.M.) 2 Institute of Oceanographic Instrumentation, Qilu University of Technology (Shandong Academy of Sciences), Qingdao 266100, China; [email protected] (X.W.); [email protected] (Q.Z.); [email protected] (H.L.); [email protected] (X.L.); [email protected] (X.P.); [email protected] (F.Z.); [email protected] (B.X.); [email protected] (Y.Y.) 3 Shandong Provincial Key Laboratory of Marine Monitoring Instrument Equipment Technology, Qingdao 266100, China 4 National Engineering and Technological Research Center of Marine Monitoring Equipment, Qingdao 266100, China 5 Xi’an Meteorological Bureau of Shanxi Province, Xi’an 710016, China; [email protected] * Correspondence: [email protected] (X.S.); [email protected] (Z.W.) Abstract: A polarized micropulse lidar (P-MPL) employing a pulsed laser at 532 nm was developed by the Institute of Oceanographic Instrumentation, Qilu University of Technology (Shandong Academy Citation: Chen, C.; Song, X.; Wang, of Sciences).