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This Quick Selection Table outlines primary LPG performance specifications
to help you choose an appropriate model. More information about each model
is available from data sheets that describe each instrument in detail.
Click on the model number to view an online data sheet.
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| Model |
Spectral Peak |
Power Levels |
Pulse Width |
Risetime |
Rep Rate |
Notes |
| 6010G
|
450 nm |
100 µ2 |
25 nS to 10 mS, CW |
15 nS |
20 Hz to 10 MHz |
h |
| 6010C
|
560 nm |
5 µ2 |
75 nS to 10 mS, CW |
50 nS |
2 MHz to 20 MHz |
h |
| 6010A
|
660 nm |
200 µ |
15 nS to 10mS, CW |
10 nS |
20 Hz to 10 MHz |
h |
| 6010B
|
820 nm |
100 µ2 |
15 nS to 10mS, CW |
10 nS |
20 Hz to 10 MHz |
g |
| 6010E
|
850 nm |
100 µ2 |
15 nS to 10mS, CW |
10 nS |
20 Hz to 10 MHz |
g |
| 065
|
650 nm |
2 mW1 |
3 nS3 - 640 S, CW |
1 nS |
0.01 Hz to 100 MHz |
a,d,e |
| 085
|
850 nm |
2 mW1 |
3 nS3 - 640 S, CW |
1 nS |
0.01 Hz to 100 MHz |
a,d,e |
| 085M
|
850 nm |
18 mW1 |
3 nS3 - 640 S, CW |
1 nS |
0.01 Hz to 100 MHz |
a,d,e |
| 090
|
904 nm |
1.0 mW1 |
3 nS3 - 640 S, CW |
1 nS |
0.01 Hz to 100 MHz |
a,b,d |
| 106C
|
1064 nm |
1.0 mW1 |
3 nS3 - 640 S, CW |
1 nS |
0.01 Hz to 100 MHz |
a,b,d |
| 106H
|
1064 nm |
50 mW |
5 nS - 50 nS5 |
1 nS |
0.01 Hz to 2kHz |
c,d |
| 130
|
1310 nm |
1 mW1 |
3 nS3 - 640 S, CW |
1 nS |
0.01 Hz to 100 MHz |
a,b,d |
| 130M
|
1310 nm |
20 mW1 |
3 nS3 - 640 S, CW |
1 nS |
0.01 Hz to 100 MHz |
a,b,d |
| 155
|
1550 nm |
1 mW1 |
3 nS3 - 640 S, CW |
1 nS |
0.01 Hz to 100 MHz |
a,b,d |
| 155M
|
1550 nm |
20 mW1 |
3 nS3 - 640 S, CW |
1 nS |
0.01 Hz to 100 MHz |
a,b,d |
| 155H
|
1550 nm |
50 mW |
5 nS - 50 nS5 |
1 nS |
0.01 Hz to 2kHz |
c,d |
| 158H
|
1580 nm |
50 mW |
5 nS - 50 nS5 |
1 nS |
0.01 Hz to 2kHz |
c,d |
| Superscripts: 1Independently adjustable
peak and baseline levels of light. 2 Stabilized power
levels with optical feedback-typical tempco is 0.05%/°C. 3Also
sub nS impulse. 4The 201E can be externally driven to
500 MHz. Some laser diodes can follow the 500 MHz drive signal. 5Four
fixed widths, 10, 15, 20 and 25 nS are standard. Factory can provide other
widths. |
| Notes: a - These laser diodes can be modulated
around a bias level. Modulating bandwidths up to 500 MHz are standard. b
- ST connector, Single mode fiber 8/125 µ .21 NA. c - SMA 906
connector Multimode fiber, 100/140 µ 0.28 NA. d - Completely
programmable via GPIB and RS232. e - ST connector, Multimode fiber
50/125 µ 0.21 NA. f - These are laser diodes, packaged and
terminated to operate with our 6040/201E electrical drivers. They can be
pigtailed, collimated or be housed in a connector. The power out varies
with the output configuration. g - Fiber optic connector is SMA
906. The fiber is 100/120 µ fiber [a NA of 0.22 NA.] The source is
a LED. h - Fiber optic connector is SMA 905. Fiber connecting light
source is a 750 µ OD fiber bundle, each fiber with a 46 µ OD
[with a NA of 0.55 NA.] Source is a LED. |
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Model 6040
Mainframe with optical plug-in |
Impulse mode at 200 pS/cm |
Impulse, Pulse and Double Pulse at
1 ns/cm for Model 155 (106C, 090 similar) |
Model 6010G Blue Light
Pulse Generator |
Some important Light Pulse Generator Characteristics
Stable light source - Our light pulse generators
have excellent short and long-term stability, reportedly making them the leading
pulsed light standard for calibrating detectors and photomultiplier tubes. LPGs
test the response of detector elements and optical recievers.
Width and rate adjustibility - All of these
pulse generators offer a wide range of internal pulse width and rate control.
In addition, they can be externally triggered and driven. The external drive
mode allows the output to follow a user-controlled wavetrain.
pS jitter, nS delay resolution - The 6040-based
light pulse generators provide 25 pS jitter with 1 nS delay resolution, making
the generators useful calibrators for laser rangefinders.
Electrical Drivers - The 6040 mainframe/module
system allows electrical driver modules to be used in place of optical modules.
Electrical drive capabilities range from 150 pS risetime, 100 mA pulse to 10
nS risetime, 18 A pulses.
Last modified January 2003.
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