Upload
sabina-hamilton
View
214
Download
1
Tags:
Embed Size (px)
Citation preview
System Operations
Eastbourne,
October 2005
Towards the 1-mm:- A realistic goal ?- A vision ?- A myth ?- ???
System Operations: Accuracy
Eastbourne,
October 2005
How to reach the 1 mm ACCURACY ? Is it possible ?
How to reach the 1 mm STABILITY ? Is it possible ?
Which developments are necessary ? Recommended ?
Is the 1 mm a realistic / achievable goal ?
Simple answer:
Yes, but we do not know WHEN
Eastbourne, October 2005
1 mm: What we need …
Good LASER: SSDPL (Solid State Diode Pumped)
Short Pulse Duration: 10 ps
Good Event Timer:
A032-ET (Riga): < 10 ps RMS, < 2 ps nonlinearity, kHz ...
Dassault Modules (Graz E.T.): < 3 ps RMS, < 2 ps nonlinearity
Good detector: C-SPAD, Time Walk Compensated;
Good satellites: ZERO Signature; PLUS strong return signal !
Grace A, Grace B, Champ: No sat signature, good signal
LARET-C: Zero signature, but weak signal
Eastbourne, October 2005
1 mm: Needs a good laser …
UPGRADE THE LASER:
Switch to Solid State Lasers (e.g. kHz);
Excellent Pulse uniformity;
Excellent Stability (shot-to-shot, day-by-day);
Short Pulses (10 ps in Graz) => better accuracy;
We do not see any disadvantage ...
Change from „TUBES“ to „SOLID STATE“ !!!
October 2005
1 mm: Needs strong signals …
With a 10-ps laser, good ET, strong-signal / zero signature sat.:
2 – 3 mm Single Shot RMS precision;
With VERY strong returns (> 300 pe / return): 1 mm SS RMS
Measure Return Signal Strength of EACH return:
C-SPAD: Use Time Difference Comp. / Uncomp. Output
Select returns with > 300 pe only 1 mm RMS
In CALs to 4 km Retro Target: Routinely achieved;
Current project ongoing in Graz; results in Canberra expected
Eastbourne,
October 2005
CAL RMS: From 10 Hz to kHz
SLR Graz: Routine - Calibrations 2003-2005;10 Hz: 500 Returns; kHz: 10 000 Returns
0.00.5
1.01.5
2.02.53.0
3.54.0
4.55.0
2003 2003.5 2004 2004.5 2005 2005.5
CA
L R
MS
[m
m]
CAL RMS [mm]
Eastbourne,
October 2005
CAL P-M: From 10 Hz to kHz
SLR Graz: Routine - Calibrations 2003-2005;10 Hz: 500 Returns; kHz: 10 000 Returns / CAL
-4
-3
-2
-1
0
1
2
3
4
2003 2003.5 2004 2004.5 2005 2005.5
Pe
ak
min
us
Me
an
[m
m] CAL Peak minus Mean [mm]
Eastbourne,
October 2005
1 mm with flash lamp laser ?
Old 10-Hz-Laser system in Graz (but with E.T. etc.):
Peak-minus-Mean: about ± 2 mm variations;
Too big; => difficult to reach the 1 mm goal !!!
With new Solid State Laser (kHz):
Peak-minus-Mean: MUCH better, very stable !!!
about ± 0.3 mm variations only ...
Eastbourne,
October 2005
1 mm: Needs a good satellite …
Use Retros / panels WITHOUT satellite signatures !!!
GRACE-A
GRACE-B
CHAMP
???
2-3 mm SS RMS
Eastbourne,
October 2005
1 mm Accuracy / Stability
All previous comparisons:
From 10 Hz Flash Lamp to 2 kHz Solid State Laser
All other Equipment: Same ...
Event Timer (Graz E.T. / Dassault Modules)
Same C-SPAD; same other equipment ....
Conclusion again:
Change from „TUBES“ to „SOLID STATE“ !!!
Eastbourne, October 2005
Laser Pulse Width and Accuracy
Wide range of pulse widths used in SLR:
10 ps: Graz / kHz / Solid State Laser;
35 –50 ps: Standard Lasers; Flash Lamp Pumped;
110 ps: e.g. Herstmonceux Flash Lamp Pumped;
300 ps: SLR 2000
Any other ?
What is the „best“/„optimum“/„desired“ pulse width ?
Eastbourne, October 2005
Laser Pulse Width Selection
10 ps: Present optimum; no reason for shorter pulses …
No significant contribution to overall systematics anymore;
Excellent for Single-Photon-Detectors;
Allowa to see – and to handle - Single Retros ….
300 ps: Can be eye-safe at e.g. 50 cm dia, if < 150 µJ / pulse
Relatively big contribution to overall systematics;
1mm goal for Lageos => difficult with SPE signals<
Satellite signature problem slightly increasing;
Less problems with LEOs / MultiPhoton Detection