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SECTION 1 - - INTRODUCTION

1.1

RANGE AND PERFORMANCE

The range of these telescopes is nominally 500 feet (with appropriate customer supplied electronics)
for personnel and farther for vehicles.  HOWEVER, range is dependent on the thermal contrast
between the target and the background.  You will find that this varies throughout the day, with weather
conditions, and even with the clothing of the target.  If your application involves detecting someone
crossing through a field of grass, you will find that the undulation of the grass on a windy day will
appear on the analog output signals.  Thus the system is limited by the thermal contrast of the target
against the background as well as thermal background noise.

For shorter range (~200 ft) or more covert applications, Eltec suggests the Model 8502M3 or 8502M7.
The Model 8502M3 is a short range version of the Model 860M5 and the Model 8502M7 is a short
range version of the Model 860M6.  The short range and long range versions are pin for pin compatible
and use the same connector.  The short and long range versions differ with regard to directionality
(refer to the Directionality Considerations section for the appropriate Model).

Performance will greatly depend on the amplification you use with the telescope’s analog output
including your bandpass filtering.  Many feel that human motion is sufficiently detected through the
frequency range of 0.3 to 3 Hz.  Yet, the conditions of your application may require a broadening of
that range - - with a consequent increase in noise.  Eltec recommends that you AC-couple the
telescope’s analog output.  The current draw per channel should be typically 8 microamps.

1.2

BASICS OF PASSIVE INFRARED (PIR) DETECTION

Each person, object or animal emits infrared energy as a function of its surface temperature and size.
For temperatures around ambient the maximum of the radiated energy is in the region of 10 microns
(20 times the wavelength of visible light).  Thermal changes, relative to the background, within the
telescope’s field of view as produced by a moving target generate a signal which will trigger an alarm.

PIR detection has become the most widely used approach for indoor intrusion detection and Eltec
provides a proven high reliability sensor for both indoor and outdoor applications.

PIR detection does not require an emitter, but makes use of radiation which is already there - 100%
natural and harmless. The fact that no radiation is emitted also means that:

A sensor unit cannot be detected by any technical means.  Like the human eye, it is completely
passive in operation.

No license is required as for microwaves.

No eye protection required as with many active IR devices.

Neighboring units will not interfere with each other.

Directional information can be obtained utilizing an internal two channel detector and appropriate
external electronic circuit.

1.3

DESCRIPTION

These telescopes are specifically designed for use as a component in a total security system for long
range detection of people and vehicles.  Eltec’s passive infrared thermal telescopes have been

Page 1

Summary of Contents for IR-EYE 860M1

Page 1: ...mate with Contractor Developed Signal Processing or Legacy Systems Model 860M1 Model 860M5 Model 860M6 Please note These telescopes do not provide either relay or TTL outputs They are made available for special signal processing systems For units that do provide relay and TTL outputs see Eltec Models 864 and 864M3 ...

Page 2: ...THIS PAGE LEFT INTENTIONALLY BLANK ...

Page 3: ...SE ALARM SOURCES SECTION 2 INSTALLATION AND OPERATION 2 1 INTRODUCTION AND PRECAUTIONS 2 2 UNPACKING 2 3 POWER REQUIREMENTS 2 4 CONNECTION TO EXTERNAL EQUIPMENT 2 5 TAMPER SENSE MODEL 860M5 AND 860M6 ONLY 2 6 AMPLIFICATION REQUIREMENTS 2 7 MECHANICAL OUTLINE 2 8 MOUNTING 2 9 MOUNTING AND ACCESSORIES 2 10 OPERATION 2 11 ALIGNMENT 2 12 WALK TESTING 2 13 WALK TESTING FIELD OF VIEW 2 14 MAINTENANCE 2 ...

Page 4: ... application may require a broadening of that range with a consequent increase in noise Eltec recommends that you AC couple the telescope s analog output The current draw per channel should be typically 8 microamps 1 2 BASICS OF PASSIVE INFRARED PIR DETECTION Each person object or animal emits infrared energy as a function of its surface temperature and size For temperatures around ambient the max...

Page 5: ...rature contrast can be as little as 1o C or less either positive or negative for a person at the nominal distance of 500ft to trigger the alarm A precison mirror focuses the radiation onto a twin channel pyroelectric detector which will produce a defined signal from a moving target Two stage optical filtering restricts the radiation to the atmospheric window 8 14 microns where the effects of the n...

Page 6: ...nfrared signal attenuation can almost be neglected for points 1 to 9 on the International Visibility Scale see Table 1 corresponding to dense fog and perfectly pure air respectively Only for visibility 0 very dense fog will the attenuation be significant but detection range will still be typically up to 50 more than the distance the human eye will see Page 3 DISTANCE COVERAGE X SIZE Y SIZE 100 ft ...

Page 7: ...vided into portions of 300 ft each being covered by one telescope see Fig 1 4 This kind of set up will give reliable detection under virtually all climatic conditions It is important to note that the range of the telescope is not limited by but a function of size and temperature of the target A car or an airplane may trigger an alarm when crossing the field of view at a mile distance depending on ...

Page 8: ...g wave infrared See Fig 1 8 1 9 POTENTIAL FALSE ALARM SOURCES Various sources may affect the performance of an outdoor security system For instance DO NOT aim the telescope into the horizon straight out UNLESS you are aiming into a wall the side of a building or an embankment that is within your monitored perimeter Although the telescope will detect a person at 500 feet under most conditions it ma...

Page 9: ...trips the first thing to check after verifying that there is proper voltages to electronics and telescope is the aiming to make sure that detection of motion of distant objects is not the source of unwanted alarm signals REFER TO OPERATION AND ALIGNMENT SECTIONS Passive infrared detection can perform exceptionally well under almost all conditions Page 6 Figure 1 9 Grounding with Actual Terrain Tel...

Page 10: ... damaged or broken Use precautions in lightning storms In lightning prone areas take measures to arrest lightning discharges and electrostatic buildup 2 2 UNPACKING Remove the unit from the shipping container and carefully check for signs of damage Any such damage should be reported to your supplier or to the Technical Support staff at Eltec Instruments directly Do not attempt to install a damaged...

Page 11: ...3µF C6 1 54K R4 3 3µF C3 V 5 TO 15V GND ANALOG OUTPUT 100K 100µF C1 ANALOG OUTPUT 13K R5 13K R10 6 81M R7 6 81M R2 C2 2 2nF 1Hz TO 10Hz SINGLE SUPPLY AMP WITH GAIN OF 500 NOTES ALL CAPACITORS ARE 10 10V ALUM EXCEPT FOR C2 AND C5 CAPACITORS C1 AND C4 MUST HAVE A LEAKAGE 1µA ALL RESISTORS ARE 1 1 4W MFLM AMPLIFIER MAY HAVE TURN ON TIME OF SEVERAL MINUTES OFFSET WILL BE ONE HALF OF V ADJUST RATIO OF ...

Page 12: ...r stable mounting and easy aiming the following accessories can be supplied Page 9 Double Mounting Bracket No AO54M1 The part clasping the telescope is fixed to a platform with a nut for adjustment of the elevation The other part is fixed to the pole with 360 o rotation capability for aiming the telescope to any desired direction Suitable for pole diameters of 1 5 to 3 0 inches Mounting Bracket No...

Page 13: ...lescope does not alarm through the trouble period when blinded then the actual field of view should be verified by walk testing to insure that the telescope is not picking up distant vehicles or motion from an adjacent area In addition many telescope users have used the scope output to trigger a recording CCTV system with time date stamp for alarm source verification This approach is highly recomm...

Page 14: ...SEMBLY WILL COMPROMISE THE SEAL AND VOID THE WARRANTY 2 15 MODEL 860M1 860M5 860M6 SPECIFICATIONS Mechanical Weight 2 lbs 12 oz Size 3 50 8 89 cm dia x 12 93 32 84 cm long Enclosure Painted PVC hermetically sealed Color O D Green other colors available as special order Optical Nominal Range 500 ft 152 m with appropriate customer supplied electronics Spectral Response 8 to 14 microns double filtere...

Page 15: ...cinstruments com ELTEC INSTRUMENTS INC 07 2017 Printed in U S A Form DS860M1 5 6 E 07 2017 NOTICE The information provided herein is believed to be reli able However ELTEC Instruments Inc assumes no responsibility for inaccuracies or omissions Due to industry components being incorporated into ELTEC s devices and ELTEC continually striving for product improvement specifications may change without ...

Page 16: ...4 10 km 0 4 0 7 Moderate rain very light snow thin haze 7 Good 10 20 km 0 7 0 8 Light rain no precipitation 8 Very Good 20 50 km 0 8 0 9 No precipitation 9 Exceptional 50 km 0 9 1 0 Perfectly pure air Notes 1 The transmittance refers to λ 0 61 µ 2 The values for 0 3 points are rough estimates due to meager experimental data Bramson Infrared Radiation Plenum Press N Y 1968 TABLE 1 ELTEC Instruments...

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