laser ranging technique for astrod i mission ◆ introduction ◆ key requirements of ground lr...
TRANSCRIPT
Laser Ranging Technique
for ASTROD I Mission
◆ Introduction
◆ Key Requirements of Ground LR Station for
ASTROD I
◆ Telescope Pointing and Pointing Ahead
◆ Day-Time Laser Ranging Technique
◆ Optical Layout of LR for the ASTROD I MissionXiong Yaoheng, Zheng Xiangming, Song Fenggan Yunnan Observatory, Chinese Academy of Sciences
Beijing 15/07/2006
◆◆ Introduction
Coordinates:
Latitude 25.0299 N
Longitude 102. 7972 E
Elevation 1991.83 m
One of suggested ground stations for ASTROD1 mission:
Yunnan Observatory 1.2mTelescope LR system
Specifications of 1.2m Telescope
Telescope Mounting: Alt-Az Focus: Coudé focus Focal Length: afocal, + a imaging lens Field of View: 3 Encoder resolution: 0. 36 Axis Accuracy: both Alt. and Az. 1 Pointing Accuracy: after modification , 1 Drive Mode: torque motor through friction disk for Az.; drive directly for Alt. Tracking Accuracy: 1 for stars
1.2m Laser Ranging System
• Range: 400 ~ 20,000km• Accuracy: ~ 3cm • Nd:YAG Laser 100mj/p, 200ps, 4Hz• Timing: GPS Resolution: 0.1s• Timing Interval Counter:
SR620, Resolution: 20ps
• Detector: SPAD (single photon avalanche photodiode)
• Operated from 1998
Servo-Control, Adaptive Optics & Laser →Ranging System
Laser Ranging System at Coudé Room
Right optical table (3.5m1.8m) is for ASTROD I mission
←
→
LAGEOS- 1
- 1500
- 1000
- 500
0
500
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11. 55 11. 6 11. 65 11. 7 11. 75 11. 8 11. 85 11. 9 11. 95 12 12. 05
UT
O-C(
ns)
LAGEOS-1, 5860 km
11h UT, Jan. 20, 2001 Echo Points:>1700
GPS36
- 200
0
200
400
600
800
1000
1200
1400
15. 1 15. 2 15. 3 15. 4 15. 5 15. 6 15. 7 15. 8
UT
O-C
(ns)
GPS 36, 20030 km 15h UT, Jan. 22, 2001 Echo
Points:>1130
AJ I SAI
- 3000
- 2000
- 1000
0
1000
2000
3000
4000
5000
23. 28 23. 3 23. 32 23. 34 23. 36 23. 38 23. 4 23. 42 23. 44 23. 46 23. 48 23. 5
UT
O-C
(ns)
TOPEX
- 1500
- 1000
- 500
0
500
1000
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3500
3. 96 3. 97 3. 98 3. 99 4 4. 01 4. 02 4. 03 4. 04
UT
O-C
(ns)
Day Time SLR: 23h16m UT, Fab.17, 2003 Echo Points: 377 AJISAI
Day Time SLR: 3h56m UT, Mar.6, 2003 Echo Points: 77 TOPEX
Evaluation of Laser Ranging Ranging Ability
laser pulse energy, receiving telescope diameter,
detector, telescope tracking and pointing accuracy
Ranging AccuracyAccidental errors: laser pulse width, time accuracy, time
interval counter accuracy
System error: correction of mass, system delay, ground
target calibration, atmospheric parameters and correction
New Trend of Laser Ranging
• LR Accuracy: Toward Millimeter• LR Data: KHz Laser, Million Echo for a Single Pass• LR Model: Passive Active (Transponder) Two-Way LR, Interplanetary LR (1~2AU)• Diffuse Reflective LR: Space Debris • Interferometric LR: Higher Ranging Accuracy• Chinese LLR: 2nd Phase of Chinese Lunar Mission
◆◆ Key Requirements of Ground LR Station for ASTROD I
(Pulse LR)(Pulse LR)
Telescope tracking and pointing accuracy: 1 Laser beam divergence: adjustable, better than 1 Timing: GPS
Receiver: SPAD or Avalanche Photodiode Array
Timing counter: Event Timer, resolution: 3ps
Coronagraph, Filtering ( spectral, spatial, temporal
)
Ground target calibration
Laser Requirements for Pulse LR
If ground station & S/C have specifications: Diode-pumped Nd:YAG laser, 532nm, 200mJ/p, 10
0ps, 100Hz, 1 laser beam divergence If ASTROD I S/C is in 1AU, with a 30cm telescope: 1.2m telescope can receive 3.9105photons/per p
ulse from the S/C S/C can receive 2.4104photons/per pulse from 1.2m LR system on the ground Pulse laser ranging accuracy can be less 3cm
◆◆ Key Requirements of Ground LR Station for ASTROD I (CW LR)(CW LR)
Diode-pumped CW Nd:YAG laser for interferometric laser ranging
100 fW Laser Phase Locking Optical comb
FADOF Filter
Laser Requirements for CW LR
If ground station & S/C have following specifications: 2 diode-pumped CW Nd:YAG lasers, 1.064 m, 1w, with a Fabry-Perot reference cavity: 1 laser locked to the cavity, the other laser pre-stabilized by this laser and phase-
locked to the incoming weak light, 1 laser beam divergence
If ASTROD I S/C is in 1AU, with a 30cm telescope: 1.2m telescope can receive 5105photons/per second from the
S/C S/C can receive 3.1104photons/per second from 1.2m LR syst
em on the ground CW laser ranging accuracy will be several mm
◆◆ Telescope Pointing and Pointing Ahead
For laser divergence and long distance range, such as ASTROD I mission, ground telescope must have the pointing and tracking accuracy of one arcsecond according to spacecraft ephemeris.
For a high tracking and pointing accuracy, telescope must have good axis, good encoders and a stable optical system. The system errors of telescope pointing can be moved using a mathematics model and through star observation & CCD image processing, to reach an accuracy of 1 (RMS).
Global Pointing ModelPointing Model
Using the Spherical Harmonic Function to 4th Terms: AsinZ = A0+A1cosZ+A2cosAsinZ+A3sinAsinZ+A4cos2Z+ A5cosAcosZsinZ+A6sinAcosZsinZ+A7cos3Z+ A8cosAsinZcos2Z+A9sinAsinZcos2Z+A10cos4+ A11cosAsinZcos3Z+A12sinAsinZcos3Z Z = B0 + B1cosZ + ……Through star observation in sky and image processing, to
solve Ai , B1 , i=0, 1, ……12. Then let A, Z be in all telescope pointing to reach its accuracy 1
Local Pointing ModelLocal Pointing Model
Telescope pointing accuracy will change with time, such as temperature, sunshine, humidity, wind direction. Global pointing model can not be kept a long time.
Local Pointing Model: Around the S/C orbit, we can do a simplified observation and modification using Hipparcos Catalogue (accuracy:1 mas) before every ASTROD I LR.
Advantage: 1. to make sure the telescope pointing accuracy 1 for t
he ASTROD I S/C that to be observed. 2. much less time will be needed to do the pointing model o
bservation.
AsinZ = C0 + C1(Z-Z0) + C2(A-A0)sinZ0 + C3
(Z-Z0)2 + C4(Z-Z0)(A-A0)sinZ0 + C5(A-A0)
2sin2Z0
Z = D0 + D1(Z-Z0) + D2(A-A0)sinZ0 ……
|A-A0 | 5° |Z-Z0| 5°
Telescope Pointing Ahead
The travel time of laser beam is more than
500 seconds for one AU distance from
ground station to the ASTROD I S/C.
Ground telescope must point ahead when
emits a laser beam to the S/C according to
its orbit ephemeris, and vice versa.
Calculation Telescope Pointing Ahead Angle
Calculating the orbit of spacecraft Using Newtonian Law
Physical model: When Calculating S/C orbit, following factors are considered: 9 large planets, Sun, Moon and 3 small planets: Ceres, Pallas, Vesta. Universal gravitation, post-Newtonian effect, and solar zonal harmonic term
rr
rij
ij
ijii 3
The Distance between Spacecraft and Earth
1.2m Telescope Pointing Ahead Angle
◆ Day-Time Laser Ranging
Technique The mean photoelectron ratio NB caused by
the sky background light on the detector is:
trrB qTANN 2
4
For 1.2m laser ranging system on daytime:NB= 6.1106 photoelectrons/sec
To reduce above sky background light, we need: Spatial & Spectral filterTiming gate
Spatial filter a pinhole shutter of 20-30 in receiving optical path Spectral filter the narrow band filter of 0.1nm for 1.064 m or
532nm in receiving optical path Fabry-Perot filter →high transmission coefficient →
60% Timing gate according to S/C ephemeris with a accuracy of 20ns f
or the detector in LR
Sunlight Shield System
Coronagraph- FADOF
The sunlight shield system consists of a
narrow-band interference filter, a FADOF
(Faraday Anomalous Dispersion Optical
Filter) filter, and a shutter
The Sun light should be less than 1 % of the
laser light at the photo-detector
◆ Optical Layout of LR for ASTROD I
1.2m telescopeOptical layout
←
Pulse Laser Ranging Optical Layout
Detector Counter GPS
Imaging
DiscriminatorFilter
FADOF PIN
Diode-PumpedNd: YAG Laser
Reflector
To Telescope
Beam Expander
GuidingPointing
Shutter
Pin-hole
Reflector Rotating Disk
Transmission Film
CW Laser Ranging
Transmit/Receive sharing same optical path model can not be used for CW laser beam at the 1.2m telescope
Two possible methods for CW laser ranging:
1. Attaching the CW laser device on the 1.2m telescope, depend on its size and cooling system
2. Another small telescope (=50cm) that close to 1.2m telescope transmits CW laser beam, and the 1.2m telescope receives the return photo-electrons.
Conclusion
Yunnan Observatory 1.2m Laser Ranging system in China is a ground station for the ASTROD1 mission
It’s ready! Requirements of LR for the ASTROD 1 mission are: Diode-pumped (Pulse or CW) Nd:YAG laser Detector (SPAD or avalanche photodiode array ) Event Timer Coronagraph, Filtering Weak Laser Phase lock and Optical comb
Thanks