Cimel CE318-T, Руководство пользователя

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CE318-T Photometer
User Operation Manual
Revision V4.10 October 2021
51
870 nm SKY 1020 nm SKY POL IR 0-1-2-3 1640 i nm SKY
702 nm AUR 442 nm AUR
675 nm SKY 1640 i nm SKY 870 nm SKY 415 nm AUR 412 nm AUR
440 nm SKY 1640 i nm SKY POL IR 0-1-2-3 675 nm SKY 1020 nm SKY 400 nm / 681 nm AUR
500 nm SKY 870 nm SKY 440 nm SKY 1640 i nm SKY 1020 nm SKY
380 nm SKY 870 nm SKY POL IR 0-1-2-3 550 nm SKY 870 nm SKY 865 nm SKY
Sensor head T (°C) 675 nm SKY 1020 i nm SKY 675 nm SKY 779 nm / 709 nm SKY
675 nm SKY POL VIS 0-1-2-3 380 nm SKY 440 nm SKY 665 nm SKY
440 nm SKY 740 nm SKY 500 nm SKY 620 nm SKY
440 nm SKY POL VIS 0-1-2-3 Sensor head T (°C) 555 nm SKY 560 nm SKY
500 nm SKY 1020i nm SKY 1020 i nm SKY
500 nm SKY POL VIS 0-1-2-3 782 nm SKY 510 nm SKY
380 nm SKY 740 nm SKY 490 nm SKY
380 nm SKY POL UV 0-1-2-3 702 nm SKY 442 nm SKY
340 nm SKY 415 nm SKY 412 nm SKY
340 nm SKY POL UV 0-1-2-3 Sensor head T (°C) 779 nm / 709 nm SKY
Sensor head T (°C) Sensor head T (°C)
BCLSKY : The BCLSKY scenario consists in performing sky and 3 Black
measurements. The number of sky measurements is defined by NBCLSKY in the
settings menu, which by default is 10.
BLACK : The black scenario consists in measuring the electronic background of the
device. Light path is closed on the two channels by positioning the filter-wheel between
two filters.
Important note: The signal measured is the dark current. It is subtracted to the full
signal measured. It is also an indicator for a possible electronic failure if too big.
Measures are done in the following order:
•
AUREOLE gain, silicon channel (canal 1)
•
AUREOLE gain, InGaAs channel (canal 2)
•
SKY gain, silicon channel
•
SKY gain, InGaAs channel
SKY CALIBRATE : The SKY CALIBRATE scenario consists in performing 3 SKY and
1 BLACK scenario.
HYBRID (Standard, Polarized): The scenario is a combination of the Almucantar /
Principal Plane scenario to optimize the range of scattering angle.