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CE318-TS9 automatic solar photometer

NegotiableUpdate on 05/06
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Overview

The CE318-TS9 automatic solar photometer is used for global climate change monitoring, atmospheric and environmental monitoring, aerosol optical thickness, atmospheric turbidity measurement, particle spectrum distribution, aerosol physical and optical properties research, satellite calibration and radiometric correction, and peak air pollution forecasting.

Product Details

CE318-TS9 automatic solar photometerUsed for global climate change monitoring, atmospheric and environmental monitoring, aerosol optical thickness, atmospheric turbidity measurement, particle spectrum distribution, aerosol physics and optical properties research, satellite calibration and radiation correction, and peak air pollution forecasting.


Product Introduction

High precision fully automatic multi band photometer for network measurementCE318-TS9 automatic solar photometerIt reflects the optical properties of the atmosphere by observing the reflection of the sun, sky, moon, and ground. It is a photometer that can be observed both during the day and at night, providing quantitative and physical optical property data of aerosols. Due to its low energy consumption, self powering, and robust design, reliability, long lifespan, and low maintenance costs can meet the needs of continuous monitoring. The instrument was developed for NASA in 1992 and has been continuously improved to meet the growing demands of AERONET (AErosol ROBOTIC NETwork). AERONET is a global joint network for aerosol measurement, jointly operated by NASA. Other independent networks such as PHOTONS in France, AEROCAN in Canada, RIMA in Spain, AGSNET in Australia, CARSNET in China, and SONET are all running CE318.


Product Features

Accuracy and stability of measurement

Full time observation during day and night

● Automatic tracking, aiming, high-resolution tracking accuracy

Widely deployed and adopted by the technology industry with scientifically validated standard instruments

Standardized automated measurement mode can also be manually operated for measurement

● Strictly regulated field of view

● GPS automatic time, latitude, and longitude with minimal regular maintenance

Over 1000 instruments operate reliably around the world


Reliable operation under any climatic conditions

Stable and continuous operation under * * climate conditions

● Strengthen lightning protection

Durable and corrosion-resistant (with a service life of over 15 years)


Flexible usability

Self powered is suitable for long-term networked observation and on-site operation

● Realize long-term unmanned automatic operation through solar power supply

● Data transmission: serial port, GPRS/SIM, Wireless, SD card/USB


Product Application

Aerosol characteristics and quantification

Satellite calibration for aerosol measurement

Real time measurement of volcanic ash columns

● Particle size determination

Measurement of atmospheric optical properties in satellite imagery

Measurement of Ocean Water Color

● Determination of precipitation

● Air quality monitoring


Technical specifications


model

description

optical filter

CE318-TS9

Standard Edition

340, 380, 440, 500, 675, 870, 937, 1020, 1640 nm

CE318-TP9

Polarization version

340, 380, 440, 500, 675, 870, 937, 1020, 1640 nm, Three polarization directions for analyzing particle shape

CE318-TU9

BRDF measurement of 9-band

380, 440, 550, 675, 740, 870, 937, 1020, 1640 nm

CE318-TU12

BRDF measurement of 12 bands

415, 440, 490, 555, 675, 702, 740, 782, 870, 937, 1020, 1640 nm

CE318-TV12-OC

SEAPRISM

Sea surface radiation measurement

400, 412.5, 442.5, 490, 510, 560, 620, 665, 779, 865, 937, 1020 nm

CE318-TV12-LC

SEAPRISM

Lake surface radiation measurement

412.5, 442.5, 490, 510, 560, 620, 665, 681, 709, 865, 937, 1020 nm





















optical probe

Full size digital counting accuracy:<0.1%

Bandwidth/Field of View: 10nm/1.0 °

*Small scattering angle: 2 °

Detector: Si (UV+visible): 340-1020nm

InGaAs(IR):1020-1640nm

Optical filter drift:<1%/year


robot arm

Azimuth angle: 0~360 °

Height angle: 0~180 °

Resolution: 0.003 °

Sun Moon automatic tracking accuracy:<0.01 °


power supply

External power supply: power adapter 110-240V

Independent self powered: total energy consumption with solar panels<2W

Battery: 12V/8Ah


control box

Firmware: Compatible with all photometer models and all available scenarios, multiple measurement programs

Data encoding: 32-bit

User interface: touch keyboard, backlit display, direct reading

Input/output connector: detachable

Automatic communication output: RS232 (100m), USB, GPRS/SIM

Storage: Flash memory (4M): 6 to 8 weeks of data storage, used for automatic transmission of multi interface free settings; SD card (8GB): Manual copy lifetime storage

Additional measurement: Rain sensor shutdown self-protection, GPS, Barometer, temperature and humidity sensor

Monitoring software: PhotodData instrument startup, wavelength selection, scanning mode and scene configuration, measurement plan, data analysis, data visualization, data storage (raw data, K8, ASCII files)


Overall dimensions

Package dimensions

External instrument box: 66 × 52 × 47cm

Instrument box body: 59 × 48 × 33cm

Bracket and field protection box: 100 × 60 × 60cm

package weight

Instrument box: 29Kg

Bracket and field protection box: 35Kg

Dimensions after installation: 130 × 50 × 50cm

Weight after installation: 50Kg


data product

Data display, storage, statistics, and editing, BOUGUER-HANGLEY curve, aerosol optical thickness (AOT) for each channel, estimation of water vapor content, Angstrom index, etc. By utilizing data, the following information can be further obtained:

● Volume distribution of aerosol particle spectrum

● Composite refractive index

● Aerosol scale distribution

● Phase function for each scattering angle

Asymmetric parameters

● Single scattering albedo