350-1100 nm Silicon 3 W Divergent Beam 1.6 inch ID Integrating Sphere

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Overview

The 3A-IS integrating sphere photodiode laser measurement sensor is for divergent beams up to +/-40 degrees. It has a 12 mm aperture and can measure optical power from 1 µW to 3 W. It covers the spectral range from 350 to 1100 nm.

1.6 inch ID integrating sphere for divergent beam
Silicon photodiode for 350 to 1100 nm spectral range
1 µW to 3 W power measurement range
12 mm diameter aperture

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Products

		Compare	Model	Compatibility	sortOrder	rankScore	ranking	Drawings, CAD & Specs		Type	Sphere Size	Aperture Size	Spectral Range	Maximum Average Power	Availability	Featured Item	Price		Brand
		7Z02404 3A-IS Integrating Sphere, Silicon, 1 µW to 3 W, Ø12 mm, 350-1100 nm $1,973 In Stock	7Z02404 3A-IS Integrating Sphere, Silicon, 1 µW to 3 W, Ø12 mm, 350-1100 nm	UNIVERSAL	0.0	1.0	0.0		0.0	Divergent Beam	1.6 in.	Ø12 mm	350-1100 nm	3 W	In Stock		$1,973		Ophir

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Specifications

Product Name

3A-IS
Type

Divergent Beam
Sphere Size

1.6 inch Inner Diameter
Aperture Size

Ø12 mm
Detector Type

Silicon Photodiode
Spectral Range

350-1100 nm
Minimum Power

1 µW
Maximum Average Power

3 W

Maximum Pulse Energy

100 µJ
Maximum Average Power Density

0.2 kW/cm²
Response Time

0.2 s
Dimensions

68 x 95 x 46 mm (LxWxD)
Cable Length

1.5 m
CE Compliance

Yes
UKCA Compliance

Yes
China RoHS Compliance

Yes

Specifications

Product Name

3A-IS
Type

Divergent Beam
Sphere Size

1.6 inch Inner Diameter
Aperture Size

Ø12 mm
Detector Type

Silicon Photodiode
Spectral Range

350-1100 nm
Minimum Power

1 µW
Maximum Average Power

3 W

Maximum Pulse Energy

100 µJ
Maximum Average Power Density

0.2 kW/cm²
Response Time

0.2 s
Dimensions

68 x 95 x 46 mm (LxWxD)
Cable Length

1.5 m
CE Compliance

Yes
UKCA Compliance

Yes
China RoHS Compliance

Yes

Features

Integrating Spheres for Divergent Light Sources

Integrating spheres are used when we have divergent light sources. As shown in the illustration, an integrating sphere has its inner surface coated with a surface that highly reflects (typically 99%) in a scattering, nonspecular way. Thus when a divergent beam hits the walls of the integrating sphere, the light is reflected and scattered many times until the light hitting any place on the walls of the sphere has the same intensity.

A detector placed in the sphere thus gets the same intensity as anywhere else and the power the detector detects is thus proportional to the total incident power independent of the beam divergence. (The detector is so arranged that it only sees scattered light and not the incident beam). An ideal integrating sphere has a surface with reflective properties are Lambertian. This means that light incident on the surface is scattered uniformly in all directions in the 2pi steradians solid angle above the surface. The surface used by Ophir closely approximates a Lambertian surface.

Two Integrating Spheres in Series

The 3A-IS series has two 50 mm integrating spheres in series with a photodiode detector. The two series spheres scramble up the light very well thus giving output very independent of incident beam divergence angle. The two spheres in series also insure that the light hitting the detector is greatly reduced in intensity thus allowing use up to 3 Watts even though photodiodes saturate at about 1 mW. There are two models, the 3A-IS with a silicon photodiode for 400-1100 nm and the 3A-ISIRG with an InGaAs detector for 800-1700 nm.

Choose the Right Sensor Using the LED Sensor Finder

Choosing the right sensor to measure LEDs or similar sources, whose beams are usually divergent and have a broadened spectrum, can be tricky. The LED Sensor Finder will help you get it right.

Calibration Factors - Laser Power/Energy Meter

When a power/energy meter is in "Calibrate" mode, various "Factors" are displayed to the user. This video explains the meaning of each of these factors.

Measuring Power of LEDs: UV, Visible and NIR

Measuring the emitted power of an LED can be tricky. It is different in some important ways from measuring the power of a laser beam. This video shows you how to use the Ophir 3A-IS Integrating Sphere Sensor, along with the Auxiliary LED accessory, to easily make accurate measurements in LED applications.

Measuring Beams Coming Out of A Fiber

When you need to measure a beam coming out of a fiber, there are some parameters that might have a somewhat different meaning than they do when referring to "regular" beam measurements. Missing some of these points could lead to incorrect measurement, and possible equipment damage. This video clarifies some issues you'll need to keep in mind so you can set up -- and perform -- this measurement correctly.

Calibration Stability of 3A-IS Integrating Sphere Sensors

The Ophir integrating sphere sensors, models 3A-IS and 3A-IS-IRG have a white diffuse reflecting coating on the inside of the integrating sphere. The sensitivity of the sensor is quite sensitive to the reflectivity of the coating. If the coating absorption goes up 1%, it can cause a 5% change in reading. Therefore, care must be taken not to soil or damage the white coating of the sensors. Also it may be a good idea to send the sensors for recalibration yearly.

Features

Integrating Spheres for Divergent Light Sources

Two Integrating Spheres in Series

Choose the Right Sensor Using the LED Sensor Finder

Choosing the right sensor to measure LEDs or similar sources, whose beams are usually divergent and have a broadened spectrum, can be tricky. The LED Sensor Finder will help you get it right.

Calibration Factors - Laser Power/Energy Meter

When a power/energy meter is in "Calibrate" mode, various "Factors" are displayed to the user. This video explains the meaning of each of these factors.

Measuring Power of LEDs: UV, Visible and NIR

Measuring Beams Coming Out of A Fiber

Calibration Stability of 3A-IS Integrating Sphere Sensors

Frequently Asked Questions

Are there any special problems with the calibration stability of integrating sphere sensors?
Answer
The Ophir integrating sphere sensors, models 3A-IS and 3A-IS-IRG have a white diffuse reflecting coating on the inside of the integrating sphere. The sensitivity of the sensor is quite sensitive to the reflectivity of the coating. If the coating absorption goes up 1%, it can cause a 5% change in reading. Therefore, care must be taken not to soil or damage the white coating of the sensors. Also it may be a good idea to send the sensors for recalibration yearly.

Integrating spheres are used when you have divergent light sources. How do they work?
Answer
Integrating Sphere Theory
Integrating spheres are used when we have divergent light sources. As shown in the illustration, an integrating sphere has its inner surface coated with a surface that highly reflects (typically 99%) in a scattering, nonspecular way. Thus when a divergent beam hits the walls of the integrating sphere, the light is reflected and scattered many times until the light hitting any place on the walls of the sphere has the same intensity.

A detector placed in the sphere thus gets the same intensity as anywhere else and the power the detector detects is thus proportional to the total incident power independent of the beam divergence. (The detector is so arranged that it only sees scattered light and not the incident beam). An ideal integrating sphere has a surface with reflective properties are Lambertian. This means that light incident on the surface is scattered uniformly in all directions in the 2pi steradians solid angle above the surface. The surface used by Ophir closely approximates a Lambertian surface.

Step 1 – Starting position

3A-IS Series
The 3A-IS series has two 50mm integrating spheres in series with a photodiode detector. The two series spheres scramble up the light very well thus giving output very independent of incident beam divergence angle. The two spheres in series also insure that the light hitting the detector is greatly reduced in intensity thus allowing use up to 3 Watts even though photodiodes saturate at about 1mW. There are two models, the 3A-IS with a silicon photodiode for 400 – 1100nm and the 3A-ISIRG with an InGaAs detector for 800 – 1700nm

When using the fiber optic adaptor, how do we handle power loss due to the fiber relative to calibration?
Answer
All Ophir power meters, including photodiode power meters, have an air gap between the fiber tip and the sensor. Therefore they measure the power emitted by the fiber into the air and do not take into account any reflection losses there are in the fiber. Therefore, if in actual use, the fiber will be coupled with no loss to another element, then the losses should be added to the reading. These losses are usually about 4%. Thus if the reading on the Ophir meter is say 100 mW, then in lossless use, the real power will be 104 mW.

I wish to increase the accuracy of the measurement. Can I get the auxiliary LED in a different wavelength than 390nm?
Answer
Not at this time. Contact Ophir to discuss your particular application.

Do I need to recalibrate my instrument? How often must it be recalibrated?
Answer
Unless otherwise indicated, Ophir sensors and meters should be recalibrated within 18 months after initial purchase, and then once a year after that.

There are several models of IS6 integrating sphere detectors. how can I select the right one?
Answer
There is a simple to use selection guide.

How much variation in water temperature or flow rate is allowed in Ophir water cooled sensors?
Answer
Ophir water cooled sensors measure the heat flow across the thermopile disc and therefore are quite insensitive to the water temperature or flow rate within the given specified limits. However, sudden changes in the water temperature or water flow rate can cause a disturbance to the reading until the flow rate/temperature stabilizes again. Therefore we specify in our water cooled sensors that the water temperature should not change faster than 1 °C/min. Likewise, sudden changes in flow rate (e.g. switching another device connected to the same water line on and off) can results in temporary disturbances in the power reading.

What is the purpose of the auxiliary LED accessory for the 3A-IS integrating sphere?
Answer
The auxiliary LED is used to increase accuracy in cases where the source under measurement is reflective or protrudes into the integrating sphere. The auxiliary LED is used to measure this effect and calibrate it out.

Among the Integrating Sphere accessories offered, there are “Port Plugs” (white), and “Port Covers” (black). What’s the difference?
Answer
An unused port should be closed, to prevent unwanted light from entering the sphere. Closing it with a diffuse white port plug, however, adds the surface area of that plug to the (diffuse white) effective area of the sphere that is doing the “integrating”. For a calibrated integrating sphere sensor, this change in the behavior of the sphere changes its calibration, and results in incorrect readings. In such applications, a black “Port Cover” should be used.

The damage thresholds for your Integrating Sphere sensors are only given for the sphere surface – what about for the detector?
Answer
The damage threshold is given in the datasheet for the sphere inner surface rather than for the detector itself, because the sphere surface will reach its damage threshold long before the detector will. A beam entering the sphere will first hit the inner surface on the opposite side of the sphere, and if at that point the power density is too high it will damage the inner surface of the sphere. From that first "meeting" of the beam with the white diffuse reflective inner sphere surface, it will be diffusely reflected multiple times. Since there is no direct line of sight between the entrance port and the detector, any light reaching the detector has already been uniformly distributed around the inner surface of the sphere, but light in that "first impact" on the sphere wall has not yet been uniformly distributed. Therefore, the "damage threshold" for the device is the maximum power density of the beam as it first hits the inner wall.

Frequently Asked Questions

Are there any special problems with the calibration stability of integrating sphere sensors?
Answer
The Ophir integrating sphere sensors, models 3A-IS and 3A-IS-IRG have a white diffuse reflecting coating on the inside of the integrating sphere. The sensitivity of the sensor is quite sensitive to the reflectivity of the coating. If the coating absorption goes up 1%, it can cause a 5% change in reading. Therefore, care must be taken not to soil or damage the white coating of the sensors. Also it may be a good idea to send the sensors for recalibration yearly.

Integrating spheres are used when you have divergent light sources. How do they work?
Answer
Integrating Sphere Theory
Integrating spheres are used when we have divergent light sources. As shown in the illustration, an integrating sphere has its inner surface coated with a surface that highly reflects (typically 99%) in a scattering, nonspecular way. Thus when a divergent beam hits the walls of the integrating sphere, the light is reflected and scattered many times until the light hitting any place on the walls of the sphere has the same intensity.

A detector placed in the sphere thus gets the same intensity as anywhere else and the power the detector detects is thus proportional to the total incident power independent of the beam divergence. (The detector is so arranged that it only sees scattered light and not the incident beam). An ideal integrating sphere has a surface with reflective properties are Lambertian. This means that light incident on the surface is scattered uniformly in all directions in the 2pi steradians solid angle above the surface. The surface used by Ophir closely approximates a Lambertian surface.

Step 1 – Starting position

3A-IS Series
The 3A-IS series has two 50mm integrating spheres in series with a photodiode detector. The two series spheres scramble up the light very well thus giving output very independent of incident beam divergence angle. The two spheres in series also insure that the light hitting the detector is greatly reduced in intensity thus allowing use up to 3 Watts even though photodiodes saturate at about 1mW. There are two models, the 3A-IS with a silicon photodiode for 400 – 1100nm and the 3A-ISIRG with an InGaAs detector for 800 – 1700nm

When using the fiber optic adaptor, how do we handle power loss due to the fiber relative to calibration?
Answer
All Ophir power meters, including photodiode power meters, have an air gap between the fiber tip and the sensor. Therefore they measure the power emitted by the fiber into the air and do not take into account any reflection losses there are in the fiber. Therefore, if in actual use, the fiber will be coupled with no loss to another element, then the losses should be added to the reading. These losses are usually about 4%. Thus if the reading on the Ophir meter is say 100 mW, then in lossless use, the real power will be 104 mW.

I wish to increase the accuracy of the measurement. Can I get the auxiliary LED in a different wavelength than 390nm?
Answer
Not at this time. Contact Ophir to discuss your particular application.

Do I need to recalibrate my instrument? How often must it be recalibrated?
Answer
Unless otherwise indicated, Ophir sensors and meters should be recalibrated within 18 months after initial purchase, and then once a year after that.

There are several models of IS6 integrating sphere detectors. how can I select the right one?
Answer
There is a simple to use selection guide.

How much variation in water temperature or flow rate is allowed in Ophir water cooled sensors?
Answer
Ophir water cooled sensors measure the heat flow across the thermopile disc and therefore are quite insensitive to the water temperature or flow rate within the given specified limits. However, sudden changes in the water temperature or water flow rate can cause a disturbance to the reading until the flow rate/temperature stabilizes again. Therefore we specify in our water cooled sensors that the water temperature should not change faster than 1 °C/min. Likewise, sudden changes in flow rate (e.g. switching another device connected to the same water line on and off) can results in temporary disturbances in the power reading.

What is the purpose of the auxiliary LED accessory for the 3A-IS integrating sphere?
Answer
The auxiliary LED is used to increase accuracy in cases where the source under measurement is reflective or protrudes into the integrating sphere. The auxiliary LED is used to measure this effect and calibrate it out.

Among the Integrating Sphere accessories offered, there are “Port Plugs” (white), and “Port Covers” (black). What’s the difference?
Answer
An unused port should be closed, to prevent unwanted light from entering the sphere. Closing it with a diffuse white port plug, however, adds the surface area of that plug to the (diffuse white) effective area of the sphere that is doing the “integrating”. For a calibrated integrating sphere sensor, this change in the behavior of the sphere changes its calibration, and results in incorrect readings. In such applications, a black “Port Cover” should be used.

The damage thresholds for your Integrating Sphere sensors are only given for the sphere surface – what about for the detector?
Answer
The damage threshold is given in the datasheet for the sphere inner surface rather than for the detector itself, because the sphere surface will reach its damage threshold long before the detector will. A beam entering the sphere will first hit the inner surface on the opposite side of the sphere, and if at that point the power density is too high it will damage the inner surface of the sphere. From that first "meeting" of the beam with the white diffuse reflective inner sphere surface, it will be diffusely reflected multiple times. Since there is no direct line of sight between the entrance port and the detector, any light reaching the detector has already been uniformly distributed around the inner surface of the sphere, but light in that "first impact" on the sphere wall has not yet been uniformly distributed. Therefore, the "damage threshold" for the device is the maximum power density of the beam as it first hits the inner wall.

Accessories

Fiber Adapter Mounting Bracket

A mounting bracket is needed to connect most power and energy sensors to a fiber adapter (SC, ST, FC or SMA). This bracket can be used for integrating sphere models 3A-IS and 3A-IS-IRG.

	Compare	Description	Compatibility	Drawings, CAD & Specs	Avail.	Price
		7Z08213 Fiber Adapter Mounting Bracket, 3A-IS Photodiode Sensors	UNIVERSAL		Contact Us	$127

Fiber Connector Adapters

These adapters allow for power measurement of connectorized fiber-optic cables. The sensor may need an additional mounting bracket to connect to these fiber adapters.

Description	Compatibility	Avail.	Price
7Z08227 SC Fiber Connector Adapter, Power and Energy Sensors	UNIVERSAL	In Stock	$302
7Z08226 ST Fiber Connector Adapter, Power and Energy Sensors	UNIVERSAL	In Stock	$264
7Z08229 FC Fiber Connector Adapter, Power and Energy Sensors	UNIVERSAL	In Stock	$153
1G01236A SMA Fiber Connector Adapter, Power and Energy Sensors	UNIVERSAL	In Stock	$74

Extended Warranty for Sensor

Customers that purchase the above items also consider the following items. Ophir-Spiricon meters and sensors include a standard manufacturers warranty for one year. Add a one year Extended Warranty to your meter or sensor, which includes one recalibration.