JAXA s Venus Climate Orbiter (PLANET-C) overview. Launch: Jun 2010 Arrival: Dec 2010 Mission life: 2 years
|
|
|
- Blaise Kelley
- 5 years ago
- Views:
Transcription
1 JAXA s Venus Climate Orbiter (PLANET-C) overview Launch: Jun 2010 Arrival: Dec 2010 Mission life: 2 years
2 Venus and Earth They have almost the same size and mass. Surface environments are completely different. (Venus environment: CO 2 atmosphere, no ocean, 92bar, 740K, H 2 SO 4 cloud..) What differentiated these planets? How does the climate system work under different conditions?
3 Science goals Atmospheric dynamics Mechanism of super-rotation Meridional circulation Meso-scale processes Lightning Cloud physics Detection of active volcanism Inhomogeneity of surface material Zodiacal light
4 Hierarchy of Earth s meteorology Macro Meso Micro 1sec 10min 1hr 6hr 2d 20d 1yr 10yr Planetary Climate wave change Baroclinic instability Tropical cyclones Cloud cruster Inertio gravity wave Cumulus convection Gravity wave Boundary layer Wave breaking Boundary layer turbulence Interaction 10 4 km 10 3 km 10 2 km 10 km 1km 100 m 10 m
5 Hierarchy of Venus meteorology Macro Meso Micro 1sec 10min 1hr 6hr 2d 20d 1yr 10yr?????? Super-rotation?? Upscale cascade to super-rotation? 10 4 km 10 3 km 10 2 km 10 km 1km 100 m 10 m
6 Forbes (2002)
7 Concept of meteorological satellite Monitoring global structure Wide field of view (12 o ) Covering wide-range of time scales Continuous, systematic sampling (every 2 hours) Local time coverage Equatorial orbit Meso-scales / Wind vectors High spatial resolution (~10 km)
8 Spacecraft Mass 480 kg (including fuel) Science payload 34 kg Attitude control o Pointing accuracy 0.1 Stability 0.01o Oribit Periapsis 300km Apoapsis 13 Rv Period 30 hours 12o FOV
9 Science instruments (1) 1-μm camera (IR1) by Tokyo U. λ= 1.01 μm (near-ir window) Pixels: 1024x1024, Detector: Si-CSD/CCD Cloud (day/night) Active volcanism / surface emissivity (night) 2-μm camera (IR2) by Kumamoto U. λ= 1.73, 2.26, 2.32 μm (near-ir window), 2.02 μm (CO 2 absorption), 1.65 μm (zodiacal light) Pixels: 1024x1024, Detector: PtSi Cloud / Particle size Carbon monooxide (night) Cloud top height (day) Zodiacal light (cruising) Galileo (2.3μm)
10 Science instruments (2) UV imager (UVI) by Hokkaido U. λ= 283, 365 nm Pixels: 1024x1024, Detector: SiCCD SO 2 / Unknown UV absorber (day) Longwave IR camera (LIR) by Inst. of Polar Res. λ= 8-12 μm Pixels: 240x320, Detector: uncooled bolometer Cloud top temperature (day/night) Lightning and Airglow camera (LAC) by Tohoku U. λ= 777, 551, 553, 558, 630 nm Pixels: 8x8, Detector: APD (50kHz sampling) Lightning (night) O 2 /O airglow (night)
11 Science instruments (3) Sensor Digital Electronics unit (DE) by JAXA Controlling observation sequence of cameras Onboard calibration JPEG2000 data compression Ultra-stable oscillator (Radio science) by JAXA ~10-13, provided by Timetech Co. Temperature profiles H 2 SO 4 vapor profile Ionosphere To the earth Usuda deep space center Atmosphere X-band beacon Spacecraft motion
12 1-μm camera Lightning and airglow camera 2-μm camera Longwave IR camera Ultraviolet imager
13 Radio occultation Altitude coverage velocity (m s -1 ) (km) Sounding region 20 0 Unknown momentum transport Airglow (Visible) Cloud top temperature (IR) CO 2 absorption (Near-IR) SO 2/Unknown absorber (UV) Cloud layer Lightning Lower cloud (Near-IR) CO (Near-IR) Surface (Near-IR)
14 Observation sequence in each revolution 300km x 13 R Venus Period: 30 hours Inclination: 172 deg Temperature/H 2 SO 4 vapor by radio occultation Resolution: km Global images of atmosphere and ground surface (~24 hours) Limb images (~1 hour) Resolution: km Close-up images / Lightning / Airglow (~3 hours x 2) Resolution: 1-10 km
15 Orbital motion roughly synchronized with the super-rotational flow near the cloud base Spacecraft 60 m/s westward flow near the cloud base
16 Accurate derivation of eddy motions embedded in the background super-rotation Derivation of cloud motion vectors every 2 hours km Movement with time Cloud tracked winds on the Earth
17 3-D global meteorological data Dayside Nightside Temperature H 2 SO 4 vapor (RS) SO 2 / Unknown absorber (UVI) Cloud top height (IR2) Lower clouds (IR1) Cloud motion vectors 50 km 100 km 65 km km 0 km Airglow (LAC) Cloud top temperature (LIR) Lower clouds (IR1/IR2) Carbon monooxide (IR2) Lightning (LAC) Active volcanism / Surface material (IR1)
18 Optical sounding of ground surface Search for hot lava by taking global pictures at 1.01μm several times per orbit Emissivity distribution of the ground surface Cloud feature is distinguished from surface feature by taking motion pictures and using 1.7μm and 2.3μm images which reflect cloud feature but not the surface feature.
19 Schedule 2004 Proto Model (Phase-B) start 2006 Flight Model design/manufacturing start 2009 Final integration test 2010 Launch / Arrival at Venus M-V rocket of JAXA IR2 test model
PLANET-C: Venus Climate Orbiter mission from Japan. Takeshi Imamura Japan Aerospace Exploration Agency PLANET-C team
PLANET-C: Venus Climate Orbiter mission from Japan Takeshi Imamura Japan Aerospace Exploration Agency PLANET-C team Venus Climate Orbiter JAXA s 24th science spacecraft dedicated to the exploration of
PLANET-C: Venus Climate Orbiter mission -Updates- Takehiko Satoh (Kumamoto Univ / JAXA) George Hashimoto (Kobe Univ) PLANET-C team
PLANET-C: Venus Climate Orbiter mission -Updates- Takehiko Satoh (Kumamoto Univ / JAXA) George Hashimoto (Kobe Univ) PLANET-C team Venus Climate Orbiter JAXA s 24th science spacecraft dedicated to the
Toward Venus orbit insertion of Akatsuki
Toward Venus orbit insertion of Akatsuki Takeshi Imamura (JAXA, Japan) Lightning and Airglow Camera Mid-IR Camera UV Imager Ultra-Stable Oscillator 1µm Camera 2µm Camera Development and launch Objective:
Toward Venus orbit insertion of Akatsuki
Toward Venus orbit insertion of Akatsuki Takeshi Imamura (JAXA, Japan) Lightning and Airglow Camera Mid-IR Camera UV Imager Ultra-Stable Oscillator 1µm Camera 2µm Camera Development and launch Objective:
()*+,!-.-/01!023*),+4)5!6),!7580,-/+5895:! /;0!;+<9/+<9*9/.!95!/;0!759=0,-0
!!!!!!!! "#$%&!'! Lecture material:http://www.astrobio.k.u-tokyo.ac.jp/imamura/lecture/ ()*+,!-.-/01!023*),+4)5!6),!7580,-/+5895:! /;0!;+
Observation of Venus atmosphere in coordination with Akatsuki Venus orbiter
Solar system science using JCMT Observation of Venus atmosphere in coordination with Akatsuki Venus orbiter Hideo SAGAWA (Kyoto Sangyo University, JP) Brad SANDOR, Todd CLANCY (Space Science Institute,
PRESENT STATUS OF AKATSUKI
PRESENT STATUS OF AKATSUKI MASATO NAKAMURA, TAKEHIKO SATOH, TAKESHI IMAMURA, NOBUAKI ISHII AKATSIUKI PROJECT TEAM Akatsuki in Japanese Dawn: in English Venus shot on 1 st of January, 2015 in tn the morning
AKATSUKI RETURNS TO VENUS
AKATSUKI RETURNS TO VENUS MASATO NAKAMURA, NOBUAKI ISHII, TAKESHI IMAMURA, TAKEHIKO SATOH, TAKUMI ABE, CHIKAKO HIROSE, ATSUSHI YAMAZAKI, JUNICHI NAKATSUKA, TSUTOMU ICHIKAWA, TOMOAKI TODA, HIROYUKI TOYODA,
Aeolus. A Mission to Map the Winds of Mars. Anthony Colaprete Amanda Cook NASA Ames Research Center
Aeolus A Mission to Map the Winds of Mars Anthony Colaprete Amanda Cook NASA Ames Research Center Low-Cost Planetary Missions Conference 12, 2017 What is Aeolus? Science Aeolus will provide the very first
Venus atmosphere is enigmatic with many unsolved questions. Two prominent puzzles are:
Venus atmosphere is enigmatic with many unsolved questions. Two prominent puzzles are: How is it that Venus clouds rotate at a rate 50x that of the solid body and why has the atmospheric rotation rate
Venus many opportunities for small satellites & probes A new view of Earth s sister: Insights following seven years of observations with Venus Express
Venus many opportunities for small satellites & probes A new view of Earth s sister: Colin Wilson Oxford University Insights following seven years of observations with Venus Express Dmitriy Titov European
Abstract HISAKI (SPRINT A) satellite is an earth orbiting EUV spectroscopic mission and launched on 14 Sep Extreme ultraviolet spectroscope (EX
Pointing control of extreme ultraviolet spectroscope onboard the SPRINT A satellite F. Tsuchiya(1*), A. Yamazaki(2), G. Murakami(2), K. Yoshioka(2), T. Kimura(2), S. Sakai(2), K. Uemizu(3), T. Sakanoi(1),
Low Cost Planetary Missions Conference Picture: Etna lava flow, with Catania in the background
Low Cost Planetary Missions Conference 2013 Picture: Etna lava flow, with Catania in the background Venus Express: a low cost mission Mars Express Venus Express Astrium, ESA Astrium, ESA 2001: Call for
Overview of Venus orbiter, Akatsuki
Earth Planets Space, 63, 443 457, 2011 Overview of Venus orbiter, Akatsuki M. Nakamura 1, T. Imamura 1, N. Ishii 1,T.Abe 1, T. Satoh 1, M. Suzuki 1, M. Ueno 1, A. Yamazaki 1,N.Iwagami 2, S. Watanabe 3,
AKATSUKI s Second Journey to Venus. 7 October 2015 Chikako Hirose Japan Aerospace Exploration Agency
AKATSUKI s Second Journey to Venus 7 October 2015 Chikako Hirose Japan Aerospace Exploration Agency My STK usage history (2005-2009) JAXA conjunction assessment system JAXA CA system was developed in 2007
ATMOS 5140 Lecture 1 Chapter 1
ATMOS 5140 Lecture 1 Chapter 1 Atmospheric Radiation Relevance for Weather and Climate Solar Radiation Thermal Infrared Radiation Global Heat Engine Components of the Earth s Energy Budget Relevance for
Lectures 7 and 8: 14, 16 Oct Sea Surface Temperature
Lectures 7 and 8: 14, 16 Oct 2008 Sea Surface Temperature References: Martin, S., 2004, An Introduction to Ocean Remote Sensing, Cambridge University Press, 454 pp. Chapter 7. Robinson, I. S., 2004, Measuring
Atmosphere-Space Interactions Monitor (ASIM) on the International Space Station
Atmosphere-Space Interactions Monitor (ASIM) on the International Space Station Torsten Neubert Ib Lundgaard Rasmussen National Space Institute Overall Objective Thunderstorms and their relation to atmospheric
ESA s Juice: Mission Summary and Fact Sheet
ESA s Juice: Mission Summary and Fact Sheet JUICE - JUpiter ICy moons Explorer - is the first large-class mission in ESA's Cosmic Vision 2015-2025 programme. Planned for launch in 2022 and arrival at Jupiter
Juno Status and Earth Flyby Plans. C. J. Hansen
Juno Status and Earth Flyby Plans C. J. Hansen July 2013 Juno will improve our understanding of the history of the solar system by investigating the origin and evolution of Jupiter. To accomplish this
Kandis Lea Jessup 1 Franklin Mills 2 Emmanuel Marcq 3 Jean-Loup Bertaux 3 Tony Roman 4 Yuk Yung 5. Southwest Research Institute (Boulder CO) 2
"Coordinated HST, Venus Express, and Venus Climate Orbiter Observations of Venus", NASA program 12433. Kandis Lea Jessup 1 Franklin Mills 2 Emmanuel Marcq 3 Jean-Loup Bertaux 3 Tony Roman 4 Yuk Yung 5
LEARNING ABOUT THE OUTER PLANETS. NASA's Cassini spacecraft. Io Above Jupiter s Clouds on New Year's Day, Credit: NASA/JPL/University of Arizona
LEARNING ABOUT THE OUTER PLANETS Can see basic features through Earth-based telescopes. Hubble Space Telescope especially useful because of sharp imaging. Distances from Kepler s 3 rd law, diameters from
Purpose Mercury Na Atmosphere And Tail Venus (Dayside) Circulation Temperature Chemistry Venus (Nightside) Lightning Airglow Mars Dust Storm Chemistry
P2 157 The Circumpolar Stratospheric Telescope FUJIN for Observations of Planets Prof. Makoto TAGUCHI and Atsunori MAEDA (Rikkyo University) Dr. Yasuhiro SHOJI (ISAS/JAXA) Prof. Yukihiro TAKAHASHI,Masataka
APPENDIX B SUMMARY OF ORBITAL MECHANICS RELEVANT TO REMOTE SENSING
APPENDIX B SUMMARY OF ORBITAL MECHANICS RELEVANT TO REMOTE SENSING Orbit selection and sensor characteristics are closely related to the strategy required to achieve the desired results. Different types
Torben Königk Rossby Centre/ SMHI
Fundamentals of Climate Modelling Torben Königk Rossby Centre/ SMHI Outline Introduction Why do we need models? Basic processes Radiation Atmospheric/Oceanic circulation Model basics Resolution Parameterizations
Telescopes and the Atmosphere
Telescopes and the Atmosphere Our goals for learning How does Earth s atmosphere affect ground-based observations? Why do we put telescopes into space? How does Earth s atmosphere affect ground-based observations?
Jupiter. Jupiter is the third-brightest object in the night sky (after the Moon and Venus). Exploration by Spacecrafts
Jupiter Orbit, Rotation Physical Properties Atmosphere, surface Interior Magnetosphere Moons (Voyager 1) Jupiter is the third-brightest object in the night sky (after the Moon and Venus). Exploration by
Interpretation of Polar-orbiting Satellite Observations. Atmospheric Instrumentation
Interpretation of Polar-orbiting Satellite Observations Outline Polar-Orbiting Observations: Review of Polar-Orbiting Satellite Systems Overview of Currently Active Satellites / Sensors Overview of Sensor
Venus Upper Atmosphere Circulation Models and Coupling from Above and Below
Venus Upper Atmosphere Circulation Models and Coupling from Above and Below Stephen W. Bougher University of Michigan (bougher@umich.edu) (734-647-3585) 24-Feb-06 1 Current Picture of Upper Atmosphere
GCOM-C/SGLI and its Lunar Calibration
GCOM-C/SGLI and its Lunar Calibration Lunar Calibration Workshop December 1-4, 2014 JAXA/GCOM Proj. Yoshihiko Okamura (okamura.yoshihiko@jaxa.jp) 1. Overview of GCOM-C satellite and SGLI (1) Global Change
Thermal And Near infrared Sensor for carbon Observation (TANSO) On board the Greenhouse gases Observing SATellite (GOSAT) Research Announcement
Thermal And Near infrared Sensor for carbon Observation (TANSO) On board the Greenhouse gases Observing SATellite (GOSAT) Research Announcement Appendix A Outlines of GOSAT and TANSO Sensor GOSAT (Greenhouse
Status of Indian Satellite Meteorological Programme
Status of Indian Satellite Meteorological Programme Pradeep K Thapliyal Space Applications Centre (SAC) Indian Space research Organisation (ISRO) Ahmedabad (INDIA) Email: pkthapliyal@sac.isro.gov.in International
APPENDIX 2 OVERVIEW OF THE GLOBAL PRECIPITATION MEASUREMENT (GPM) AND THE TROPICAL RAINFALL MEASURING MISSION (TRMM) 2-1
APPENDIX 2 OVERVIEW OF THE GLOBAL PRECIPITATION MEASUREMENT (GPM) AND THE TROPICAL RAINFALL MEASURING MISSION (TRMM) 2-1 1. Introduction Precipitation is one of most important environmental parameters.
VENUS EXPRESS. The First European Mission to Venus. Gerhard Schwehm and Hakan Svedhem ESA/ESTEC
VENUS EXPRESS The First European Mission to Venus Gerhard Schwehm and Hakan Svedhem ESA/ESTEC Why is ESA going to Venus? Venus is a fascinating planet and an attractive target for planetary sciences. 1960-1990:
VIRTIS-Venus Express
VIRTIS-Venus Express - G. Piccioni, P. Drossart and the VIRTIS-VenusX Team Scientific Team Members by Countries I (1) (PI) Total 14 F (2) PO ES RU NL US D UK P Total (PI) 10 1 2 2 1 2 5 2 1 (1) G. Piccioni,
MAVEN Community Meeting IUVS: The Imaging UltraViolet Spectrograph
Mars Atmosphere and Volatile EvolutioN (MAVEN) MAVEN Community Meeting IUVS: The Imaging UltraViolet Spectrograph December 2, 2012 Nick Schneider IUVS Science Lead nick.schneider@lasp.colorado.edu Outline
Spectroscopy for planetary upper atmospheres きょくたん
Spectroscopy for planetary upper atmospheres きょくたん Spectrum of Venus atmosphere Spectrum of Jupiter and Io Figure 1. An EUV spectrum measured by Hisaki spacecraft. The spectrograph mixes spatial and spectral
Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.
Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric properties
Future Opportunities of Using Microwave Data from Small Satellites for Monitoring and Predicting Severe Storms
Future Opportunities of Using Microwave Data from Small Satellites for Monitoring and Predicting Severe Storms Fuzhong Weng Environmental Model and Data Optima Inc., Laurel, MD 21 st International TOV
Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres
Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds What is an atmosphere? Planetary Atmospheres Pressure Composition Greenhouse effect Atmospheric structure Color of the sky 1 Atmospheres
Planetary Temperatures
Planetary Temperatures How does Sunlight heat a planet with no atmosphere? This is similar to our dust grain heating problem First pass: Consider a planet of radius a at a distance R from a star of luminosity
PSWS meeting Multi-wavelength observations of Jupiter's aurora during Juno s cruise phase T. Kimura (RIKEN)
PSWS meeting 2017 Multi-wavelength observations of Jupiter's aurora during Juno s cruise phase T. Kimura (RIKEN) Background p a Bagenal+14 Planetary parameters p a Earth Jupiter Saturn Spin period (hr)
Venus Express: Results, Status and Future Plans
Venus Express: Results, Status and Future Plans Håkan Svedhem ESA/ESTEC Present Status The spacecraft and its payload in general is in a good condition, with the following remarks: One of the two coolers
12a. Jupiter. Jupiter Data (Table 12-1) Jupiter Data: Numbers
12a. Jupiter Jupiter & Saturn data Jupiter & Saturn seen from the Earth Jupiter & Saturn rotation & structure Jupiter & Saturn clouds Jupiter & Saturn atmospheric motions Jupiter & Saturn rocky cores Jupiter
GCOM-C SGLI calibration and characterization. Hiroshi Murakami JAXA/EORC Satellite instrument pre- and post-launch calibration
GCOM-C SGLI calibration and characterization Hiroshi Murakami JAXA/EORC Satellite instrument pre- and post-launch calibration 1 1. SGLI sensor system and onboard calibration system Target: Improvement
The current status of FY-3D
The current status of FY-3D Xiang Fang National Satellite Meteorological Center, China Meteorological Administration (NSMC/CMA) OUTLINE Overview Key instruments onboard FY-3D Products and data service
Updates on CMA FENGYUN Meteorological Satellite Programs
Updates on CMA FENGYUN Meteorological Satellite Programs Peng ZHANG National Satellite Meteorological Center, China Meteorological Administration (NSMC/CMA) 29 Nov. - 5 Dec. 2017, Darmstadt, Germany 1.
Preparation for FY-4A. (Submitted by Xiang Fang, CMA)
WORLD METEOROLOGICAL ORGANIZATION COMMISSION FOR BASIC SYSTEMS OPEN PROGRAMME AREA GROUP ON INTEGRATED OBSERVING SYSTEMS EXPERT TEAM ON SATELLITE UTILIZATION AND PRODUCTS ET-SUP-8/Doc. 10.3 (2.IV.2014)
Satellite Position Determination of LEO Spacecraft
Satellite Position Determination of LEO Spacecraft S.C.Rathnakara ISRO Satellite Centre 5 th September, 2007 International Committee on Global Navigation Satellite Systems(ICG) Things to follow Brief background
Atmospheric Lidar The Atmospheric Lidar (ATLID) is a high-spectral resolution lidar and will be the first of its type to be flown in space.
www.esa.int EarthCARE mission instruments ESA s EarthCARE satellite payload comprises four instruments: the Atmospheric Lidar, the Cloud Profiling Radar, the Multi-Spectral Imager and the Broad-Band Radiometer.
Imaging the Earth from the Moon FUV Imaging of the Earth s Space Weather. Dr. Larry J. Paxton (office)
Imaging the Earth from the Moon FUV Imaging of the Earth s Space Weather Dr. Larry J. Paxton 240 228 6871 (office) Larry.paxton@jhuapl.edu Making Observations of the Earth from the Moon Makes Sense Once
Appendix B. A proposition for updating the environmental standards using real Earth Albedo and Earth IR Flux for Spacecraft Thermal Analysis
19 Appendix B A proposition for updating the environmental standards using real Earth Albedo and Earth IR Romain Peyrou-Lauga (ESA/ESTEC, The Netherlands) 31 st European Space Thermal Analysis Workshop
Application of Radio Occultation Data in Analyses and Forecasts of Tropical Cyclones Using an Ensemble Assimilation System
Application of Radio Occultation Data in Analyses and Forecasts of Tropical Cyclones Using an Assimilation System Hui Liu, Jeff Anderson, and Bill Kuo NCAR Acknowledgment: C. Snyder, Y. Chen, T. Hoar,
Scott Bolton OPAG February 1, 2016
Scott Bolton OPAG February 1, 2016 Juno Status Launched August 2011 Earth flyby October 2013 Jupiter arrival July 4, 2016 Spacecraft is healthy and all instruments are working. Juno Science Juno Science
HY-2A Satellite User s Guide
National Satellite Ocean Application Service 2013-5-16 Document Change Record Revision Date Changed Pages/Paragraphs Edit Description i Contents 1 Introduction to HY-2 Satellite... 1 2 HY-2 satellite data
Atmosphere, Ocean and Climate Dynamics Fall 2008
MIT OpenCourseWare http://ocw.mit.edu 12.003 Atmosphere, Ocean and Climate Dynamics Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. Contents
Presentation by Indian Delegation. to 49 th STSC UNCOPUOS. February 2012 Vienna
Presentation by Indian Delegation to 49 th STSC UNCOPUOS February 2012 Vienna ASTROSAT Astrosat is India s first dedicated multiwavelength astronomy satellite with a capability to observe target sources
The time variation of atomic oxygen around Io during volcanic active event observed by Hisaki/EXCEED
Symposium on planetary Science 2017 2017/2/21 The time variation of atomic oxygen around Io during volcanic active event observed by Hisaki/EXCEED Ryoichi Koga* [1], Fuminori Tsuchiya [1], Masato Kagitani
CMA Consideration on early-morning orbit satellite
CMA Consideration on early-morning orbit satellite National Satellite Meteorological Center,CMA Yang Jun CGMS 40 in Lugano, 5-9 Nov., 2012 Outline Background Gap analysis on the sounding data coverage
JUICE/Laplace Mission Summary & Status
JUICE/Laplace Mission Summary & Status C. Erd JUICE Instrument WS, Darmstadt 9/11/2011 Activities during the Reformulation Phase 1. Feasible JGO s/c as a starting point a. no re-design of s/c necessary
Report of the Venera-D Joint Science Definition Team: "Together to Venus"
Report of the Venera-D Joint Science Definition Team: "Together to Venus" L. Zasova1, D. Senske2, T. Economou3, N. Eismont1, L. Esposito4, M. Gerasimov1, N. Ignatiev1, M. Ivanov5, I. Khatuntsev1, O. Korablev1,
VELOX-CI: Advanced Application of GPS for Radio Occultation and Satellite Attitude Determination
VELOX-CI: Advanced Application of GPS for Radio Occultation and Satellite Attitude Determination Yung-Fu Tsai, Guo Xiong Lee and Kay Soon Low Satellite Research Centre (SaRC) School of Electrical and Electronic
GOSAT update. June Prepared by JAXA EORC Presented by David Crisp
CEOS AC-VC GOSAT update June Prepared by JAXA EORC Presented by David Crisp GOSAT & GOSAT-2 Organization ORGANIZATION GOSAT is the joint project of JAXA, MOE (Ministry of the Environment) and NIES (National
Interacciones en la Red Iberica
2a Reunion Red Iberica MM5 Grupo 12: interacciones, modelo mm5 y proyectos actuales Lidia Cucurull UCAR - NOAA/NCEP Washington DC, USA http://www.cosmic.ucar.edu Lidia.Cucurull@noaa.gov cucurull@ucar.edu
Orbit Design Marcelo Suárez. 6th Science Meeting; Seattle, WA, USA July 2010
Orbit Design Marcelo Suárez Orbit Design Requirements The following Science Requirements provided drivers for Orbit Design: Global Coverage: the entire extent (100%) of the ice-free ocean surface to at
Venus Monitoring Camera for Venus Express
Venus Monitoring Camera for Venus Express W.J. Markiewicz 1, D. Titov 1,4, B. Fiethe 2, T. Behnke 3, I. Szemerey 1, H. Perplies 1, M. Wedemeier 1, I. Sebastian 1, W. Boogaerts 1, C. Dierker 2, D. Osterloh
Large Area Imaging Survey of Near-Infrared Sky with Korean Compact Space Telescopes
Large Area Imaging Survey of Near-Infrared Sky with Korean Compact Space Telescopes Science & Technology Satellite Series (KARI) (2000 ~ 2013. 02) 1 st Satellite: FIMS (Far-ultraviolet IMaging Spectrograph)
Silicate Atmospheres, Clouds, and Fractional Vaporization of Hot Earth-like Exoplanets
Silicate Atmospheres, Clouds, and Fractional Vaporization of Hot Earth-like Exoplanets Laura Schaefer and Bruce Fegley, Jr. Planetary Chemistry Laboratory Department of Earth and Planetary Sciences Washington
General Comments about the Atmospheres of Terrestrial Planets
General Comments about the Atmospheres of Terrestrial Planets Mercury Very little atmosphere Contents: vaporized micrometeorites, solar wind Sky is black Venus Very thick (10% density of water), dense
DWTS The Doppler Wind and Temperature Sounder
DWTS The Doppler Wind and Temperature Sounder Quantifying the Neutral Drivers of Weather and Space Weather Dave Fritts Larry Gordley GLOBAL ATMOSPHERIC TECHNOLOGIES AND SCIENCES (GATS) Outline - Need for
Outline. Planetary Atmospheres. General Comments about the Atmospheres of Terrestrial Planets. General Comments, continued
Outline Planetary Atmospheres Chapter 10 General comments about terrestrial planet atmospheres Atmospheric structure & the generic atmosphere Greenhouse effect Magnetosphere & the aurora Weather & climate
ROCSAT-3 Constellation Mission
ROCSAT-3 Constellation Mission, An-Ming Wu, Paul Chen National Space Program Office 8F, 9 Prosperity 1st Road, Science Based Industrial Park, Hsin-Chu, Taiwan vicky@nspo.org.tw, amwu@nspo.org.tw, paulchen@nspo.org.tw
AST 105 Intro Astronomy The Solar System
AST 105 Intro Astronomy The Solar System STRUCTURE OF A PLANET S ATMOSPHERE If you remember this. X-rays Ultraviolet Heating & Destruction Heating & Destruction Visible Infrared Transmission and Scattering
esa ACE+ An Atmosphere and Climate Explorer based on GPS, GALILEO, and LEO-LEO Occultation Per Høeg (AIR/DMI) Gottfried Kirchengast (IGAM/UG)
ACE+ An Atmosphere and Climate Explorer based on GPS, GALILEO, and LEO-LEO Occultation Per Høeg (AIR/DMI) Gottfried Kirchengast (IGAM/UG) OPAC-1, September, 2002 1 Objectives Climate Monitoring global
Lecture 4: Radiation Transfer
Lecture 4: Radiation Transfer Spectrum of radiation Stefan-Boltzmann law Selective absorption and emission Reflection and scattering Remote sensing Importance of Radiation Transfer Virtually all the exchange
Wind Imaging Spectrometer and Humidity-sounder (WISH): a Practical and Effective NPOESS P3I Sensor
Wind Imaging Spectrometer and Humidity-sounder (WISH): a Practical and Effective NPOESS P3I Sensor Jeffery J. Puschell Raytheon Space and Airborne Systems Hung-Lung Huang University of Wisconsin, Madison
Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.
Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric
Technology Reference Studies
In the proceedings of the 8th ESA Workshop on Advanced Space Technologies for Robotics and Automation 'ASTRA 2004' ESTEC, Noordwijk, The Netherlands, November 2-4, 2004 Technology Reference Studies P.
Winds in the martian upper atmosphere from MGS aerobraking density profiles
Winds in the martian upper atmosphere from MGS aerobraking density profiles Paul Withers*, Steve Bougher, and Gerry Keating AGU Fall Meeting 2002 #P61C-0353 (* = Postdoc job wanted) The Importance of Winds
Neutral Winds in the Upper Atmosphere. Qian Wu National Center for Atmospheric Research
Neutral Winds in the Upper Atmosphere Qian Wu National Center for Atmospheric Research Outline Overview of the upper atmosphere. Ozone heating. Neutral wind tides (the strongest dynamic feature). Why do
Observing Habitable Environments Light & Radiation
Homework 1 Due Thurs 1/14 Observing Habitable Environments Light & Radiation Given what we know about the origin of life on Earth, how would you recognize life on another world? Would this require a physical
Vicky Chu, Jer Ling, Tom Lin, Joe Fong, Feng-Tai Huang, Guey-Shin Chang. April 15, 2011
FORMOSAT-7/COSMIC-2 Overview Vicky Chu, Jer Ling, Tom Lin, Joe Fong, Feng-Tai Huang, Guey-Shin Chang April 15, 2011 Program Status AIT-TECRO Agreement on FORMOSAT-7/COSMIC-2 joint program has been signed
Electromagnetic Radiation and Scientific Instruments. PTYS April 1, 2008
Electromagnetic Radiation and Scientific Instruments PTYS 206-2 April 1, 2008 Announcements Deep Impact 6 PM Wednesday Night Pizza, no beer Watch at home if you can t watch here. It will be discussed in
Electromagnetic Radiation. Radiation and the Planetary Energy Balance. Electromagnetic Spectrum of the Sun
Radiation and the Planetary Energy Balance Electromagnetic Radiation Solar radiation warms the planet Conversion of solar energy at the surface Absorption and emission by the atmosphere The greenhouse
Remote Sensing in Meteorology: Satellites and Radar. AT 351 Lab 10 April 2, Remote Sensing
Remote Sensing in Meteorology: Satellites and Radar AT 351 Lab 10 April 2, 2008 Remote Sensing Remote sensing is gathering information about something without being in physical contact with it typically
NASA Future Magnetospheric Missions. J. Slavin & T. Moore Laboratory for Solar & Space Physics NASA GSFC
NASA Future Magnetospheric Missions J. Slavin & T. Moore Laboratory for Solar & Space Physics NASA GSFC Future Magnetospheric Missions Strategic Missions Radiation Belt Storm Probes (LWS/2011) Magnetospheric
Solar Orbiter. T.Appourchaux, L.Gizon and the SO / PHI team derived from M.Velli's and P.Kletzkine's presentations
Solar Orbiter T.Appourchaux, L.Gizon and the SO / PHI team derived from M.Velli's and P.Kletzkine's presentations 2 nd Solar-C definition meeting, Tokyo, Japan Content Science Objectives of Solar Orbiter
EUMETSAT products and services for monitoring storms - New missions, more data and more meteorological products
EUMETSAT products and services for monitoring storms - New missions, more data and more meteorological products Jochen Grandell 1 EUM/RSP/VWG/17/921460 Outline Overview of EUMETSAT missions Current...and
FUNDAMENTALS OF REMOTE SENSING FOR RISKS ASSESSMENT. 1. Introduction
FUNDAMENTALS OF REMOTE SENSING FOR RISKS ASSESSMENT FRANÇOIS BECKER International Space University and University Louis Pasteur, Strasbourg, France; E-mail: becker@isu.isunet.edu Abstract. Remote sensing
Robotic Lunar Exploration Scenario JAXA Plan
Workshop May, 2006 Robotic Lunar Exploration Scenario JAXA Plan Tatsuaki HASHIMOTO JAXA 1 Question: What is Space Exploration? Answers: There are as many answers as the number of the people who answer
Weather & Climate. Sanjay S. Limaye Space Science & Engineering Center University of Wisconsin-Madison
Weather & Climate Sanjay S. Limaye Space Science & Engineering Center University of Wisconsin-Madison 1 What is Weather? Webster s New Collegiate Dictionary: state of the atmosphere with respect to heat
Aeolus ESA s Wind Lidar Mission: Objectives, Design & Status
Aeolus ESA s Wind Lidar Mission: Objectives, Design & Status Anne Grete Straume on behalf of Anders Elfving European Space Agency/ESTEC Working Group on Space-based Lidar Winds Boulder, 28/04/2015 Atmospheric
Lectures 7 and 8: 13, 18 Feb Sea Surface Temperature
Lectures 7 and 8: 13, 18 Feb 2008 Sea Surface Temperature References: Martin, S., 2004, An Introduction to Ocean Remote Sensing, Cambridge University Press, 454 pp. Chapter 7. Robinson, I. S., 2004, Measuring
Planetary Science from a balloon-based Observatory. January 25-26, 2012 NASA Glenn Research Center
Planetary Science from a balloon-based Observatory January 25-26, 2012 NASA Glenn Research Center Additional info can be found at http://spaceflightsystems.grc.nasa.gov/sspo/sp/balloon_platform/ Outline
Leonid Meteor Observer in LEO: A Proposal for a University Microsatellite for the 2001 Leonids
Leonid Meteor Observer in LEO: A Proposal for a University Microsatellite for the 2001 Leonids Kazuya Yoshida* Hajime Yano** *Tohoku University **Institute of Space and Astronautical Science (ISAS) JAPAN
Escaping the Zodi Light! Harvey Moseley! NASA/GSFC! The View from 5 AU! March 26, 2010!
Escaping the Zodi Light! Harvey Moseley! NASA/GSFC! The View from 5 AU! March 26, 2010! The Galaxy and the Zodi Light are the dominant sources of diffuse light in the night sky! Both are much brighter
Weather in the Solar System
Weather in the Solar System Sanjay S. Limaye Space Science and Engineering Center University of Wisconsin-Madison 8 February 2002 What is Weather? Webster s New Collegiate Dictionary: state of the atmosphere
Thermal And Near infrared Sensor for carbon Observation (TANSO) onboard the Greenhouse gases Observing SATellite (GOSAT) Research Announcement
Thermal And Near infrared Sensor for carbon Observation (TANSO) onboard the Greenhouse gases Observing SATellite (GOSAT) Research Announcement Appendix C Operation Policies of GOSAT and Basic Observation
Pfs results at Mars. By V.Formisano and the PFS Team
Pfs results at Mars By V.Formisano and the PFS Team Table of content 0- Generalities 1- Published results 1.1 Temperature fields over Olimpus 1.2 Comparison with ISO SWS 1.3 Polar vortex 1.4 Polar ice
Data and formulas at the end. Real exam is Wednesday May 8, 2002
ATMS 31: Physical Climatology Practice Mid Term Exam - Spring 001 page 1 Atmospheric Sciences 31 Physical Climatology Practice Mid-Term Examination: Would be Closed Book Data and formulas at the end. Real