PERIPHERAL EQUIPMENT
Light-emitting
phenomenon
¶Input
section
Streak camera
•Trigger
unit
§Optical
trigger
6
Optical Trigger
(PIN diode head)
•
PIN Diode Head C1083-01 (for Low Repetition)
7
Input Section
•
Spectroscopes C5094 and C5095
Spectral response
Rise time
400 nm to 1100 nm
0.8 ns
Dimensions/weight Head: 100 (W)
×
160 to 235 (H)
×
50 (D) mm/400 g
Power supply unit: 100 (W)
×
83(H)
×
100 (D) mm/400 g
Power supply
+22.5 V (battery)
C5094
Optical layout
Focal distance
F value
Incident light slit width
Grating
Reciprocal dispersion
C5095
•
PIN Diode Head C1808-03 (for High Repetition)
Czerny-Turner model
(with toroidal mirror for aberration correction)
250 mm
500 mm
4
8
Variable between 10
µ
m to 2,000
µ
m
Up to 3 can be installed simultaneously
2.5 nm/mm
1.5 nm/mm
(when using 1200 gr/mm) (when using 1200 gr/mm)
Wavelength resolution
< reciprocal dispersion
×
0.06
The following are needed in order to connect these units to the C5680:
• A spectroscope mounting table
• A spectroscope adaptor
• A light source for wavelength axis calibration (mercury lamp, etc.)
•
Fiber-optic Input Optics System (FC Connector) A6368
1 mW (f=80 MHz,
λ=800
mm, FWHM<1 ps)
Minimum input level
Saturation output level Approx. 1.5 Vp-p (50
Ω)
<100 MHz
Frequency band
Power supply
INPUT Voltage range 100 V to 240 V Input
power supply frequency range 50/60 Hz
This fiber-optic input optics system can be connected in place of
theincident light slit in the C5680.
•
Objective Lens
Connecting a C-mount adaptor to the incident light slit section of the
C5680 enables attachment of a C-mount objective lens. F-mount ob-
jective lenses can also be attached using an FC converter.
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