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BTS2048-UV-S-WP BiTec sensor spectroradiometer for high-quality outdoor UV measurements

The BTS2048-UV-S-WP is a high-quality spectroradiometer whose compact design and elaborate optical, electronic and mechanical interfaces make it ideal for high precision outdoor UV measurements. Due to its innovative filter and spectrometer design it is able to measure solar radiation with a very good straylight reduction performance. Accordingly, even the edge of the sun below 300 nm can be resolved for some orders of magnitude (see figure 2). With the included S-BTS2048 application software, precise measurements and data analysis (Erythema, ICNRIP, etc.) can be performed intuitively. In addition, the spectral range can be extended from the UV to the NIR with the complementary BTS2048-VL-TEC-WP. Applications in the whole Si spectral region (e.g. solar-cells) are possible.


BiTec sensor for high-end light measurement 

One of the outstanding features of this exceptional spectroradiometer is its BiTec sensor. It combines the special properties of a photodiode with those of a back-thinned CCD diode array. Through bilateral correction of measurement signals from both sensors, the BiTec sensor ensures precise radiometric and spectral-radiometric measurement values over a large dynamic range.


Spectrometer based on a high-quality back-thinned CCD detector 

The spectrometer unit is based on a CCD with usable spectral responsivity range between 190 nm and 430 nm. It has a 0.7 nm optical bandwidth and a pixel resolution of 0.13 nm/pixel. Due to the back-thinned technology, the CCD is substantially more sensitive as compared to conventional front-illuminated CCD chips. Furthermore, the CCD is one stage cooled (1TEC) to reduce the dark current and and thereby increase the signal to noise ratio.


Precise spectral radiometry (low straylight)

To facilitate optimum use of the CCD sensor‘s dynamic range and to overcome the problems of most array spectoradiometers in the UV range, a remote-controlled filter wheel (open, closed, optical filters) is located in the optical beam path. This filters combined with smart measurement and stray light correction routines enables high quality measurements of the BTS2048-UV-S. Results are comparable with double monochromator results (see figure). However, the measurement duration is significantly lower. Since the BTS2048-UV-S contains a filter wheel with 8 filter positions, a futher smart measurement routine for stray light reduction is implemented compared to the BTS2048-UV.


WP means weather proofed

The housing of the BTS2048-UV-S-WP is designed for outdoor measurements. The cooled back-thinned CCD and the spectrometer unit are temperature controlled in a second housing. In this housing, humidity is removed by an exchangeable cartridge. In order to avoid deposits of dust, rain or snow on the entrance optics on the entrance optics the quartz dome is blow-dried by warm air.


Diffuser window directly connected instead of light guide 

As for the input optics, the BTS2048-UV-S-WP has an incorporated diffuser window with a cosine corrected field of view. The fact that a light guide has not been used improves sensitivity and calibration stability which is a big advantage for outdoor use. The device‘s compact size is also of significant benefit. The f2 error of the cosine corrected field of view to less than 3% makes it possible to use the BTS2048-UV-S-WP for direct measurement in absolute radiometric quantities:

● Irradiance (W/m²)

● Spectral irradiance (W/(m² nm))


State of the art interface

The BTS2048-UV-S-WP is controlled via a USB 2.0 or Ethernet interface. With regards to the communication speed and cable length, the Ethernet port is superior to the USB2.0 interface. Furthermore, data preparation occurs in the BTS2048-UV-S-WP to optimize the data-transfer speed. For this purpose, an independent, high-performance microprocessor is incorporated. Data and power interface are of course of weather-proof design as well.


User software with flexible desktop structure 

The BTS2048-UV-S-WP‘s scope of delivery includes the S-BTS2048 user software. One of the characteristic features it has to offer is the flexible desktop that can be individually configured by the user.

This entails a potpourri of graphical and numerical display windows from which the user can choose:

● Freely definable numerical displays in decimal or scientific representation. Zoom function.

● Numerical display fields for radiometric, spectral and other measurands.

● Measurement protocol of the selected measurement parameters.

● Spectrum. Zoom function.

● Data logger. Zoom function.


Traceable calibration 

Calibration of the BTS2048-UV-S-WP, including its accessories, is performed by Gigahertz-Optik calibration laboratory for optical measurands with reference to national and international calibration standards. Due to the small dimensions of the device it can be shipped easily for re-calibration purposes.

 

BTS2048-UV-S-WP
Comparison of a solar measurement of the BTS2048-UV-S and a standard double monochromator. The BTS2048-UV-S achieves about the same quality in a measurement time of a few s compared to about 1.5 min of the double monochromator.
Entrance optic is blow-dried by warm air to prevent dirt, rain or snow
Side View of the BTS2048-UV-S-WP
S-BTS2048 software for the BTS2048-UV-S-WP
The WP version in a winter measurement campaign
General
Short description

CCD based spectroradiometer with large dynamic for CW-, Datalogger- and Single measurements of spectral irradiance and derivative quantities (spectrum, erythema, ICNIRP, etc.) in the UV spectral region for outdoor use.

Main features

Compact measurement device. Bi-Tec detector with back-thinned CCD-diodearray spectrometer (0.7 nm optical bandwidth, electronic Shutter, high dynamic) and SiC-Fotodiode. High stray light reduction. Filter wheel with aperture and optical filters. Entrance optic with diffuser which is cosine FOV. Weatherproof housing for outdoor use. Ethernet and USB interface.

Measurement range

Spectral: 3E-5 W/(m²nm) to 3E4 W/(m²nm) @325nm. Responsivity from 190 nm to 430 nm.

Integral: 2E5 W/m² to noise equivalent level by 5E-3 W/m²

typical applications

Diodearray spectrometer for scientific outdoor measurement tasks. Erythema, ICNIRP, solar-cells, etc.

Calibration

Factory calibrations traceable to PTB calibration standards.

Product
Measured Quantity

Spectral irradiance (W/(m² nm)), irradiance (W/m²), peak wavelength, center wavelength, centroid wavelength, Erythema, ICNIRP.

Input optics

Diffusor, cosine corrected field of view (f2 ≤ 3 %)

Filter wheel

8 positions (open, closed, optical filters). Use for remote dark current measurement and stray light reduction.

BiTec

Parallel measurement with diode and array is possible, thereby linearity correction of the array through the diode and online correction of the spectral mismatch of the diode through a*(sz(λ)) respectively F*(sz(λ)).

Calibration uncertainty

Spectral irradiance

(200 - 249) nm: ± 12 %
(250 - 339) nm: ± 7 %
(340 - 399) nm: ± 5 %
(400 - 430) nm: ± 4 %

Spectral irradiance responsivity (200 - 430) nm

Spectral Detector
Integration Time

2 μs - 60 s        *1

spectral range

(190 - 430) nm

Optical Bandwidth

0.8 nm

Pixel resolution

~0.13 nm/Pixel

Number of pixels

2048

Chip

Highly sensitive back-thinned CCD chip, one stage cooled (1TEC)

ADC

16bit (25 ns instruction cycle time)

Peak wavelength

± 0.05 nm

Band-pass correction

mathematical online band-pass correction is supported

Linearity

completely linearized chip >99.6%

Stray Light

Out of Bound method < 1E-4           *3

Bandpass method < 1E-5           *3

Base line noise

5 cts     *4

SNR

5000        *5

dynamic range

>9 Magnitudes

spectral irradiance responsivity range

(3E-5 - 3E4) W/(m²nm) @325nm        *6*7

typical measurement time

W/m² of a Halogen lampe from (250 - 400) nm

1 4,4 s
10 440 ms
100 44 ms
Measurement modes

Standard measurement mode: 200 nm to 430 nm

Out of Range stray light corrected measurement mode (OoR SLC): 200 nm to 430 nm

Stray light corrected bandpass mode for solar measurements (solar BP SLC): 285 nm to 420 nm

Universal stray light corrected bandpass measurement mode (BP SLC): 245 nm to 420 nm

Integral Detector
Filter

Spectral responsivity with radiometric matching. Online correction of the radiometric matching through spectral measurement data (spectral missmatch factor correction).

Measurement time

(0.1 - 6000) ms

Measurement range

seven (7) measurement ranges with transcendent offset correction

Calibration

Irradiance ± 6 %               *10

Measurement range

(5E-3  -  2E5) W/m²       *11

 

Graphs
spectral responsivity

responsivity BTS2048 UV

f2 Cosine Error

cos BTS2048 VL3

Miscellaneous
Microprocessor

32bit for device control,16bit for CCD array control, 8bit for photodiode control

Interface

USB V2.0, Ethernet (LAN UDP protocol), RS232, RS485

Data transfer

Standard for 2048 float array values via ethernet 7ms, via USB 2.0 140 ms

Input Interfaces

2x (0 - 25) VDC, 1x optocoupler isolated 5 V / 5 mA

Output Interfaces

2x open collector, max. 25 V, max. 500 mA

Trigger

Trigger input incorporated (different options, rising/falling edge, delayed, etc.)

Software

User software S-BTS2048
Optional software development kit S-SDK-BTS2048 for user software set-ups based on .dll‘s in C, C++,C# or in LabView.

Power Supply

With power supply: (90-295) V 150 W

Dimensions

Diameter: 160 mm

Height: 222 mm

(see detailed drawing)

Weight

2.85 kg

Mounting

3x M6 screw threads

temperature range

Storage: (-10 to 50) °C

Operation: (-25 to 50) °C           *9

Housing

Spectroradiometer unit: IP67

Outdoor housing itself: IPx5

Stability

inside WP housing (electronics): ≤ ± 1 °C

CCD Chip: ≤ ± 0.25 °C

Info

*1 It is recommended to perform a new dark signal measurement for every change in the integration time

*2 typical value, the uncertainty of the dominant wavelength depends on the spectral distribution of the LED

*3 typical value, measured 100nm left of the peak of a cold white broadband LED with and deep blue LED peak. The dynamic which can be resolved within one measurement depends on the number of averages and the light source. Typical for a solar measurement is a dynamic of 4.5 orders of magnitude resolution within one measurement.

*4 *5 typical value measured without averaging for a 4ms measurement time and full scale control of the array. Averaging results in quadratic rise of the S/N
i.e. quadratic fall of the base noise e.g. averaging to a factor 100 improves the S/N by a factor 10

*6 Minimum 500/1 S/N. Maximum at full scale control.

*7 Irradiation only allowed for a short time so as to avoid thermal damage

*8 during USB connection, not all functions are available due to the limited current supply e.g. no Ethernet and TEC cooling

*9 Device requires for temperature stabilization approx. 25min (power supply is needed for outdoor use). In measurement is performed in the warm-up phase, or if measurements are performed
under varying temperatures, dark signal measurement is required for each measurement.

*10 With a(Z) correction by a Deuterium lamp

*11 By a spectral power distribution of a deuterium lamp, maximum radiation only allowed for a short time so as to avoid thermal damage

Type Description File-Type Download
Datasheet BTS2048-UV-S-WP PDF
Produktname Product Image Description Show product
S-BTS2048 Application software for BTS2048 variants.
S-SDK-BTS2048 Software Development Kit for BTS2048 variants.
BTS2048-VL-TEC-WP Bi-technology sensor light meter for high quality solar VIS measurements.

Features: Weatherproofed, high spectral resolution, short measurement time, entrance optic with diffusor for irradiance and spectral irradiance, etc.
Article-Nr Modell Description Request / Compare
Product
15298728 BTS2048-UV-S-WP

Measuring device, users guide, software CD, calibration certificate.

Calibration
15300809 K-BTS2048-UV-S

Recalibration of the BTS2048-UV-S with calibration certificate

Software
15298470 S-SDK-BTS2048

Software development kit, software CD with users guide.

15298474 S-BTS2048

User software for BTS2048 and variants.

Accessories
15307929 BTS2048-XX-WP-Z02

tube for the measurement of the direct solar irradiance

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