Preliminary Results of Laser Ranging to Un-cooperative Targets at Shanghai SLR Station Yang FuMin, Zhang ZhongPing, Chen JuPing, Chen WanZhen, Wu ZhiBo,

Slides:



Advertisements
Similar presentations
Laser Retro-reflector Arrays on the Compass Satellites Chen WanZhen, Yang FuMin, Wang YuanMing, Li Pu Shanghai Observatory, Chinese Academy of Sciences.
Advertisements

Test Beam at IHEP,CAS ZHANG Liang sheng, Test Beam Group Introduction BEPC/BES Ⅱ will be upgraded as BEPC Ⅱ / BES Ⅲ, it is necessary to do beam test for.
7. Radar Meteorology References Battan (1973) Atlas (1989)
Chapter 22 Electromagnetic Waves. Units of Chapter 22 Changing Electric Fields Produce Magnetic Fields; Maxwell’s Equations Production of Electromagnetic.
FDWAVE : USING THE FD TELESCOPES TO DETECT THE MICRO WAVE RADIATION PRODUCED BY ATMOSPHERIC SHOWERS Simulation C. Di Giulio, for FDWAVE Chicago, October.
The Future of Satellite Communications Joel Klooster ENGR 302 May, 2002.
Calibration for LHAASO_WFCTA Yong Zhang, LL Ma on behalf of the LHAASO collaboration 32 nd International Cosmic Ray Conference, Beijing 2011.
Lecture 12 Content LIDAR 4/15/2017 GEM 3366.
Upgrading Plans of the Chinese SLR Network Upgrading Plans of the Chinese SLR Network Yang FuMin(1), Wu Bin(1), Zhang ZhongPing(1), Guo TangYong(2), Zhao.
An Optical Receiver for Interplanetary Communications Jeremy Bailey.
1 Extreme Ultraviolet Polarimetry Utilizing Laser-Generated High- Order Harmonics N. Brimhall, M. Turner, N. Herrick, D. Allred, R. S. Turley, M. Ware,
The Preliminary Results of Laser Time Transfer (LTT) Experiment Yang Fumin(1), Huang Peicheng(1), Ivan Prochazka(2), Zhang Zhongping(1), Chen Wanzhen(1),
Ground Target kHz Laser Ranging with Submillimeter Precision Lukas Kral, Karel Hamal, Ivan Prochazka (1) Georg Kirchner, Franz Koidl (2) presented at kHz.
Introduction to LIDAR Mapping Technology
1 Progress of Changchun SLR You ZHAO, Cunbo FAN, Xinwei HAN, Gang ZHAO, Ziang ZHANG, Xue DONG Changchun Observatory/NAOC, CAS, , China.
Photon counting detectors for future space missions Ivan Prochazka, Josef Blazej Ulrich Schreiber * presented at 16 th International Workshop on Laser.
1 Development of Any Frequency Fire Rate SLR Control System Cunbo FAN, Xue DONG, Xingwei HAN, You ZHAO Changchun Observatory, , China.
PULSE REPETITION RATE OPTMIZATION IN SLR STATIONS TO PROVIDE MINIMUM SYSTEMATIC ERROR OF RANGING M.A. Sadovnikov M.A. Sadovnikov Institute for Precision.
Radar Many in a series of McGourty- Rideout Productions.
NGSLR: Sharing Eye-safe Kilohertz SLR with Transponder Ranging Jan McGarry, Tom Zagwodzki NASA Goddard Space Flight Center Tom Varghese, Cybioms John Degnan,
I. Prochazka 1, J. Kodet 1,2, J. Blazej 1 K.G. Kirchner 3, F. Koidl 3 Presented at Workshop on Laser solutions for Orbital Space Debris April 2015,Laboratoire.
Review Doppler Radar (Fig. 3.1) A simplified block diagram 10/29-11/11/2013METR
30. Nov I.Will, G. Klemz, Max Born Institute: Optical sampling system Optical sampling system for detailed measurement of the longitudinal pulse.
Radar equation review 1/19/10. Radar eq (Rayleigh scatter) The only variable is h, the pulse length Most radars have a range of h values. Rewrite the.
Chapter 9 Electromagnetic Waves. 9.2 ELECTROMAGNETIC WAVES.
Dense Wavelength Division Multiplexing (DWDM) Technology
A New Method of Through Wall Moving Target Detection and Imaging using UWB-SP Radar Shiyou Wu, Yanyun Xu, Jie Chen, Shengwei Meng, Guangyou Fang, Hejun.
DMP Product Portfolio Femtosecond Lasers Trestles Ti:Sapphire lasers …… fs; nm, mW Mavericks Cr:Forsterite lasers
Real-Time Phase-Stamp Range Finder with Improved Accuracy Akira Kimachi Osaka Electro-Communication University Neyagawa, Osaka , Japan 1August.
12 April 2007 Lidar Measurements of Atmospheric State Parameters in the Mesosphere and Lower Thermosphere Jonathan Friedman Arecibo Observatory Seminar.
IPBSM status and plan ATF project meeting M.Oroku.
Laser Ranging Technique for ASTROD I Mission
B. Gentry/GSFCSLWG 06/29/05 Scaling Ground-Based Molecular Direct Detection Doppler Lidar Measurements to Space Using Wind Profile Measurements from GLOW.
LIGO-G D Enhanced LIGO Kate Dooley University of Florida On behalf of the LIGO Scientific Collaboration SESAPS Nov. 1, 2008.
Mike Newchurch 1, Shi Kuang 1, John Burris 2, Steve Johnson 3, Stephanie Long 1 1 University of Alabama in Huntsville, 2 NASA/Goddard Space Flight Center,
Electric and magnetic fields fluctuating together can form a propagating electromagnetic wave. An electromagnetic wave is a transverse wave, the electric.
The Second International Workshop on Ultra-high-energy cosmic rays and their sources INR, Moscow, April 14-16, 2005 from Extreme Universe Space Observatory.
Scaling Surface and Aircraft Lidar Results for Space-Based Systems (and vice versa) Mike Hardesty, Barry Rye, Sara Tucker NOAA/ETL and CIRES Boulder, CO.
System Operations Eastbourne, October 2005 Towards the 1-mm: -A realistic goal ? -A vision ? -A myth ? -???
Fig. 3 Wind measurements experimental setup Lidar (light detection and ranging) operates using the same concept of microwave RADAR, but it employs a lot.
A New E-Band (60 – 90 GHz) Fourier Transform Millimeter-wave Spectrometer DeWayne T. Halfen and Lucy M. Ziurys Department of Chemistry Department of Astronomy.
Spaceborne 3D Imaging Lidar John J. Degnan Geoscience Technology Office, Code Code 900 Instrument and Mission Initiative Review March 13, 2002.
Frequency Scanned Interferometer Demonstration System Tim Blass, Jason Deibel, Sven Nyberg, Keith Riles, Haijun Yang University of Michigan, Ann Arbor.
Wavelength and Frequency E = h c =  c = speed of light (3 x 10 8 m/s) = frequency (s -1 )  = wavelength (m) E = energy (Joules or J) h  = Planck’s constant.
A Thermospheric Lidar for He 1083 nm, Density and Doppler Measurements
IPS Observations in China: Past, Now and Future Lijia Liu National Astronomical Observatories, Chinese Academy of Sciences (NAOC) (Given by Mario M. Bisi,
Ivan Procházka, Jan Kodet presented at : seminart ACES – ELT Meeting, Fundamental Station Wettzell, Technische Univ.Muenchen, Germany May 8, 2009 Czech.
Einstein’s photon theory Photons = corpuscular theory E = hf E = Photon energy (Joules) h = Planck’s constant = x Js f = frequency of oscillations.
Use LL1 & LL6 to detect microwave radiation equipping the empty pixels with microwave radio receivers Pixels without photomultipliers (removed to be installed.
LIGO- G D Experimental Upper Limit from LIGO on the Gravitational Waves from GRB Stan Whitcomb For the LIGO Scientific Collaboration Informal.
I. Prochazka 1, J. Kodet 1,2, J. Blazej 1 K.G. Kirchner 3, F. Koidl 3 Presented at 2015 ILRS Technical Workshop, Matera, Italy, October 26 – 30,
ELT delays absolute calibration Ivan Procházka (1), Josef Blazej (1), Anja Schlicht (2) Prepared for ESA Webex meeting(s) March 2015 (1) Czech Technical.
The High Altitude Observatory (HAO) at the National Center for Atmospheric Research (NCAR) The National Center for Atmospheric Research is sponsored by.
1 Progress of the Thomson Scattering Experiment on HSX K. Zhai, F.S.B. Anderson, D.T. Anderson HSX Plasma Laboratory, UW-Madison Bill Mason PSL, UW-Madison,
INTEGRATION OF IFE BEAMLET ALIGNMENT, TARGET TRACKING AND BEAM STEERING Graham Flint March 3, 2005.
OSETI with MAGIC IntroductionIntroduction Radio SETIRadio SETI Optical SETIOptical SETI OSETI with MAGICOSETI with MAGIC SummarySummary July 2004.
I.Prochazka,et al, KOM ESOC, Darmstadt, April 2016 SPACE SITUATIONAL AWARENESS PROGRAMME P2-SST-VII EXPERT COORDINATION CENTRES (PHASE 1) Contribution.
Demonstration for cm-size space debris REDUCTION/REMEDIATION from the International Space Station Toshikazu Ebisuzaki, S. Wada, L.W. Pitrowski, M. Casolino.
上海天文台 Shanghai Astronomical Observatory CVN in Chang’e-3 lunar exploration mission ZHENG Weimin Shanghai Astronomical Observatory, Chinese.
METR Advanced Atmospheric Radiation Dave Turner Lecture 11.
Using Planck’s Constant…. Picture credit: He was a German physicist and is considered as the founder.
1 Opto-Acoustic Imaging 台大電機系李百祺. 2 Conventional Ultrasonic Imaging Spatial resolution is mainly determined by frequency. Fabrication of high frequency.
Yb:YAG Regenerative Amplifier for A1 Ground Laser Hut Rui Zhang ACCL Division V, RF-Gun Group Nov 20, 2015 SuperKEKB Injector Laser RF Gun Review.
Visit for more Learning Resources
Methods of transfer of ultra-stable frequencies to radio telescope
James Donahue EE 444 Fall LiDAR James Donahue EE 444 Fall
Validation of airborne 1
Wavelength and Frequency
National Institute for Environmental Studies, Tsukuba, Japan
ULTRA Meeting – Torino Gennaio
Presentation transcript:

Preliminary Results of Laser Ranging to Un-cooperative Targets at Shanghai SLR Station Yang FuMin, Zhang ZhongPing, Chen JuPing, Chen WanZhen, Wu ZhiBo, Zhang HaiFeng Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, China Ivan Prochazka Czech Technical University in Prague, Czech Republic

Goals Investigation of the key techniques of un-cooperative target laser ranging Experimental laser ranging to un-cooperative targets

The returned signal strength of laser ranging on un- cooperative targets can be estimated by: Estimate of the returned signal strength

Where n 0 : Average number of photoelectrons received by detector λ: Wavelength of laser, 532nm η q : Quantum efficiency of the C-SPAD detector, 0.2 h: Planck constant, 6.624× J·S c: Light speed, 2.998×10 8 m/s E t : Energy of laser pulse, 2J Ar: Effective area of receive telescope, 0.245m 2 ρ: Reflectivity of the target’s surface r: Equivalent radius of the target, 1m cos(  ): Suppose the targets are spherical, cos(  )=1

We have, n 0 =0.198 (Photoelectron)  t : Divergency of laser beam from telescope, 12 arcsec R: Range of the targets, 800Km T: Atmospheric transmission, T 2 =0.6 Kt: Eff. of transmitting optics, 0.60 Kr: Eff. of receiving optics, 0.60  : Attenuation factor, 13dB

The probability of detection can be estimated: So we can get 18 return signals in 5 second by the laser with 20Hz repetition.

1: HR mirror 2: E-Q Switch 3: Polarizer 4: YAG rod 5: Output mirror 6: Isolator 7: Compensator 8: Reflect mirror 9: Frequency doubler 10: Optical coupler 11: Imaging lens Beams combination Amplifier Unit 2 Amplifier Unit 1Isolator Oscillator Diagram of the 40W laser (2J, 20Hz, 10ns)

Photo of the laser

Inner view of the laser

Laser firing at Shanghai

Some results of un-cooperative target laser ranging at the Shanghai SLR station

Returns from the discard Soviet rocket (ID B) on July 7, 2008 Number of point: 127 RMS: 76cm

Returns from the discard US rocket (ID G) on July 17, 2008 Number of point: 79 RMS: 83cm

Returns from the discard US rocket (ID G) on July 18, 2008 Number of point: 170 RMS: 68cm

Ranging data of ID B on July 7, 2008 Time (s) Range (Km)

Ranging data of ID G on July 17, 2008 Time (s) Range (Km)

Ranging data of ID G on July 18, 2008 Time (s) Range (Km)

Statistics of returns (5-second bin) on July 7, returns in 5 seconds were obtained when tracking well, and roughly coincide with the estimation of the returns signal strength. Time (5-second bin) Number of returns

Future Plan Upgrading of the prediction of the targets (now the error of range prediction is about 1km, too difficult to obtain the returns) Automatically scanning of range gate and rapidly identify the return signals To track smaller targets and assessing the ranging capability of the system

The laser returns from the un-cooperative targets have been obtained at the Shanghai SLR Station in July These targets are the discard Soviet and US rockets with the ID B and G respectively. The return signals from the targets with the range of 900km were quite strong. Summary

Thank You!