U.S. patent application number 11/026724 was filed with the patent office on 2005-07-14 for method of thermal condensate reduction for optical devices.
Invention is credited to Krausse, George J..
Application Number | 20050152035 11/026724 |
Document ID | / |
Family ID | 26959473 |
Filed Date | 2005-07-14 |
United States Patent
Application |
20050152035 |
Kind Code |
A1 |
Krausse, George J. |
July 14, 2005 |
Method of thermal condensate reduction for optical devices
Abstract
The present invention provides a method and system to overcome
and eliminate the effects of condensation contamination of optical
surfaces that are induced by radiative cooling. The invention
counteracts the effects of radiative cooling on optical surfaces
and maintains an optical system within a very tight limit to the
ambient temperature by utilizing a resistive heater element that is
in contact with the optical components subject to condensation. In
thermal contact with this optical component is a solid-state
precision temperature sensor. In addition, there is a matching
solid-state precision temperature in thermal contact with the
ambient air but thermally isolated from the optical element.
Signals from these two sensors are applied to a comparator that
functions to generate a data signal when the optical surface
temperature is less than the ambient or reference temperature. This
data signal is used to activate a solid-state power switch that
applies a voltage to a resistive heating element. An offset may
also be applied to the reference temperature sensor allowing
compensation for the thermal resistance of the system comprised of
the optical component, optical component attachment heater and
temperature sensor.
Inventors: |
Krausse, George J.; (Bend,
OR) |
Correspondence
Address: |
William W. Cochran
Cochran Freund & Young LLC
Suite 230
3555 Stanford Road
Fort Collins
CO
80525
US
|
Family ID: |
26959473 |
Appl. No.: |
11/026724 |
Filed: |
December 30, 2004 |
Related U.S. Patent Documents
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Application
Number |
Filing Date |
Patent Number |
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11026724 |
Dec 30, 2004 |
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10279140 |
Oct 22, 2002 |
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6866391 |
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60335974 |
Nov 14, 2001 |
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Current U.S.
Class: |
359/512 |
Current CPC
Class: |
G02B 7/1815 20130101;
G02B 27/0006 20130101; G02B 7/008 20130101 |
Class at
Publication: |
359/512 |
International
Class: |
G11B 011/00; G02B
001/00 |
Claims
What is claimed is:
1. A method of reducing water vapor condensation on an optical
surface that is subject to condensation comprising; measuring the
ambient temperature of the air surrounding said optical surface;
measuring the surface temperature of said optical surface;
comparing said ambient temperature of the air surrounding said
optical surface to said surface temperature of said optical surface
to establish a temperature differential; increasing said surface
temperature of said optical surface to reduce said water vapor
condensation on said optical surfaces by introducing heat to said
optical surface with a heating element; regulating said amount of
heat applied to said optical surface by establishing a temperature
setpoint and a thermostatic range for the optical surface based
upon said temperature differential.
2. A method of claim 1 wherein said measuring of said ambient
temperature is performed with a surface mounted thermal sensor that
is thermally isolated from said optical surface.
3. A method of claim 1 wherein said measuring of the surface
temperature of said optical surface is performed with a surface
mounted thermal sensor in thermal communication with said optical
surface.
4. A method of claim 1 wherein said step of regulating said amount
of heat applied to said optical surface is performed by controlling
the duty cycle of said heating.
5. A method of reducing water vapor condensation on an optical
surface that is subject to condensation comprising; measuring the
ambient temperature of the air surrounding said optical surface
with a surface mounted thermal sensor that is thermally isolated
from said optical surface; measuring the surface temperature of
said optical surface with a surface mounted thermal sensor in
thermal communication with said optical surface; comparing said
ambient temperature of the air surrounding said optical surface to
said surface temperature of said optical surface to establish a
temperature differential; increasing said surface temperature of
said optical surface to reduce said water vapor condensation on
said optical surfaces by introducing heat to said optical surface
with a heating element; regulating said amount of heat applied to
said optical surface by establishing a temperature setpoint and a
thermostatic range for the optical surface based upon said
temperature differential.
6. A method of reducing water vapor condensation on an optical
surface of a telescope that is subject to condensation comprising;
measuring the ambient temperature of the air surrounding an optical
surface of said telescope; establishing a current ambient
temperature from said measurement of said ambient temperature;
measuring the surface temperature of said optical surface;
establishing a current optical surface temperature from said
measurement of said surface temperature; comparing said current
ambient temperature to said current surface temperature of said
optical surface to establish a temperature differential; generating
a data signal when said temperature differential reaches a selected
threshold; reducing said temperature differential sufficiently to
reduce said water vapor condensation on said optical surfaces by
heating said optical surface in response to said data signal;
maintaining said reduced temperature differential by controlling
the amount of said heating of said optical surface based upon
updated temperature measurements
7. A method of claim 6 wherein said measuring of said ambient
temperature is performed with a surface mounted thermal sensor that
is thermally isolated from said optical surface.
8. A method of claim 6 wherein said measuring of the surface
temperature of said optical surface is performed with a surface
mounted thermal sensor in thermal communication with said optical
surface.
9. A method of claim 6 wherein said step of reducing said
temperature differential sufficiently to reduce said water vapor
condensation on said optical surfaces by heating said optical
surface in response to said data signal further comprises;
compensating for the thermal resistance of the system comprising
said optical components, said heating and said temperature
sensors.
10. A method of reducing water vapor condensation on an optical
surface of a telescope that is subject to condensation comprising;
measuring the ambient temperature of the air surrounding an optical
surface of said telescope with a surface mounted thermal sensor
that is thermally isolated from said optical surface; establishing
a current ambient temperature from said measurement of said ambient
temperature; measuring the surface temperature of said optical
surface with a surface mounted thermal sensor in thermal
communication with said optical surface; establishing a current
optical surface temperature from said measurement of said surface
temperature; comparing said current ambient temperature to said
current surface temperature of said optical surface to establish a
temperature differential; generating a data signal when said
temperature differential reaches a selected lower limit threshold,
said data signal continues until a selected upper limit threshold
above said lower limit threshold is reached; activating a power
switch in response to said data signal that applies a voltage to a
resistive heating element mounted on, and in thermal contact with
said optical components; reducing said temperature differential
sufficiently to reduce said water vapor condensation on said
optical surfaces by controlling the amount of said voltage applied
to said resistive heating element; compensating for the thermal
resistance of the system comprising said optical components, said
resistive heating element and said temperature sensors; maintaining
said reduced temperature differential by controlling the amount of
said voltage applied to said resistive heating element based upon
updated temperature measurements.
11. A method of reducing water vapor condensation on an optical
surface that is subject to condensation comprising; measuring the
ambient temperature of the air surrounding an optical surface with
a thermal sensor that is thermally isolated from said optical
surface; establishing a current ambient temperature from said
measurement of said ambient temperature; measuring the ambient
relative humidity of the air surrounding said optical surface with
a hygrometric sensor; establishing a current ambient relative
humidity from said measurement of said ambient relative humidity;
measuring the surface temperature of said optical surface with
thermal sensor in thermal communication with said optical surface;
establishing a current optical surface temperature from said
measurement of said surface temperature; calculating a dew point
for said ambient air by comparing said current ambient relative
humidity to said current ambient temperature; generating a data
signal when said surface temperature of said optical surface is
lower than a selected threshold above said calculated dew point;
heating said optical components in response to said data signal to
increase said surface temperature of said optical surface to a
point greater than said selected threshold above said calculated
dew point.
12. A method of claim 11 wherein said measuring of said ambient
temperature is performed with a surface mounted thermal sensor that
is thermally isolated from said optical surface.
13. A method of claim 11 wherein said measuring of the surface
temperature of said optical surface is performed with a surface
mounted thermal sensor in thermal communication with said optical
surface.
14. A method of claim 11 further comprising the step; maintaining
said increased surface temperature of said optical surface by
controlling the amount of said heating based upon updated
temperature and relative humidity measurements.
15. A method of reducing water vapor condensation on an optical
surface of a telescope that is subject to condensation comprising;
measuring the ambient temperature of the air surrounding an optical
surface of said telescope with a surface mounted thermal sensor
that is thermally isolated from said optical surface; establishing
a current ambient temperature from said measurement of said ambient
temperature; measuring the ambient relative humidity of the air
surrounding an optical surface of said telescope with a hygrometric
sensor; establishing a current ambient relative humidity from said
measurement of said ambient relative humidity; measuring the
surface temperature of said optical surface with a surface mounted
thermal sensor in thermal communication with said optical surface;
establishing a current optical surface temperature from said
measurement of said surface temperature; calculating a dew point
for said ambient air by comparing said current ambient relative
humidity to said current ambient temperature; generating a data
signal when said surface temperature of said optical surface is
lower than a selected threshold above said calculated dew point;
activating a power switch in response to said data signal that
applies a voltage to a resistive heating element mounted on, and in
thermal contact with said optical components heating said optical
components to increase said surface temperature of said optical
surface to a point greater than said selected threshold above said
calculated dew point; compensating for the thermal resistance of
the system comprising said optical components, said resistive
heater and said temperature sensors; maintaining said increased
surface temperature of said optical surface by controlling the
amount of said heating based upon updated temperature and
relativity measurements.
Description
CROSS REFERENCE TO RELATED APPLICATIONS
[0001] This application is a divisional patent application and
claims the benefit of United States Nonprovisional patent
application Ser. No. 10/279,140 for "Thermal Condensate Reducer For
Optical Devices," which was filed on Oct. 22, 2002, by George J.
Krausse, the entire disclosure of which is herein specifically
incorporated by reference for all that it discloses and
teaches.
BACKGROUND OF THE INVENTION
[0002] 1. Field of the Invention
[0003] The present invention generally pertains to the reduction
and prevention of water vapor condensation on optical systems and
particularly to astronomical optical devices used in an outdoor
environment.
[0004] 2. Description of the Background
[0005] Optical devices in general, and astronomical optical devices
in particular, are highly sensitive to the effects of particulate
contamination degrading the ability of the optical surfaces to
refract and transmit light effectively. One of the most detrimental
and common forms of particulate contamination is the formation of
water condensate on lenses from the surrounding air. This condition
can occur in a situation where the relative humidity (RH) of the
viewing environment is very high or when the optical components are
at a temperature that is less than the surrounding air and
particularly if the components are below the dew point of the
ambient air.
SUMMARY OF THE INVENTION
[0006] The present invention overcomes the disadvantages and
limitations of the prior art by providing a method and system to
overcome and eliminate the effects of condensation contamination of
optical surfaces that are induced by radiative cooling. The
invention encompasses a method and system to precisely counteract
the effects of radiative cooling on optical surfaces and maintain
the temperature of an optical system within a very tight limit to
the ambient temperature.
[0007] The present invention may therefore comprise a method of
reducing water vapor condensation on an optical surface that is
subject to condensation comprising; measuring the ambient
temperature of the air surrounding the optical surface, measuring
the surface temperature of the optical surface, comparing the
ambient temperature of the air surrounding the optical surface to
the surface temperature of the optical surface to establish a
temperature differential, increasing the surface temperature of the
optical surface to reduce the water vapor condensation on the
optical surfaces by introducing heat to the optical surface with a
heating element, regulating the amount of heat applied to the
optical surface by establishing a temperature setpoint and a
thermostatic range for the optical surface based upon the
temperature differential.
[0008] The present invention may also comprise a method of reducing
water vapor condensation on an optical surface that is subject to
condensation comprising; measuring the ambient temperature of the
air surrounding an optical surface with a thermal sensor that is
thermally isolated from the optical surface, establishing a current
ambient temperature from the measurement of the ambient
temperature, measuring the ambient relative humidity of the air
surrounding the optical surface with a hygrometric sensor,
establishing a current ambient relative humidity from the
measurement of the ambient relative humidity, measuring the surface
temperature of the optical surface with thermal sensor in thermal
communication with the optical surface, establishing a current
optical surface temperature from the measurement of the surface
temperature calculating a dew point for the ambient air by
comparing the current ambient relative humidity to the current
ambient temperature, generating a data signal when the surface
temperature of the optical surface is lower than a selected
threshold above the calculated dew point, heating the optical
components in response to the data signal to increase the surface
temperature of the optical surface to a point greater than the
selected threshold above the calculated dew point.
[0009] The present invention may also comprise a system for
reducing water vapor condensation on an optical surface that is
subject to condensation comprising; a first temperature sensor for
measuring the surface temperature of the optical surface, a second
temperature sensor for measuring the ambient temperature of the air
surrounding the optical surface, a comparator for comparing the
first temperature sensor to the second temperature sensor and
establish a temperature differential from the comparison, a heating
element to transfer heat to the optical surface, a controller to
regulate the heating element by establishing a temperature setpoint
and a thermostatic range for the optical surface based upon the
temperature differential.
[0010] The present invention may also comprise a system for
reducing water vapor condensation on an optical surface of a
telescope that is subject to condensation comprising; a first
temperature sensor that measures the surface temperature of the
optical surface to provide a current surface temperature data
signal, a second temperature sensor that measures the ambient
temperature of the air surrounding the optical surface to provide a
current ambient temperature data signal, a hygrometric sensor for
measuring the ambient relative humidity of the air surrounding the
optical surface to provide a current ambient relative humidity data
signal, a controller that calculates a dew point of the ambient air
by comparing the current ambient relative humidity to the current
ambient temperature, a comparator that establishes a temperature
differential by comparing the current surface temperature data
signal to the dew point, a signal generator that generates a heater
control signal, a heating element that responds to the heater
control signal to transfer heat to the optical surface.
[0011] The method and system detailed in the disclosed embodiments
allow a user to maintain the temperature of optical surfaces to
within a tight temperature range of the ambient temperature, or to
maintain the temperature of optical surfaces at a set temperature
above the dew point, and thus, eliminate the condensation
associated with radiative cooling. The disclosed invention is
compact, self-contained, portable and adaptable to a wide variety
of optical surfaces. The invention has the further advantage of
being easy to use (set-and-forget) and can maintain the temperature
of a number of optical surfaces at once. The invention also has the
benefit of maintaining reduced thermal distortion from heating the
optical surface because of the tight temperature range that the
invention is able to maintain. The optical surfaces should not see
more than a few degrees temperature swing when the invention is in
operation, and therefore, extensive heating is minimized.
BRIEF DESCRIPTION OF THE DRAWINGS
[0012] In the drawings,
[0013] FIG. 1 is a block diagram of an embodiment of a method of
the reduction and prevention of condensation on optical
systems.
[0014] FIG. 2A is a partial circuit diagram detailing an embodiment
of a device for the reduction and prevention of condensation on
optical systems.
[0015] FIG. 2B is the remaining part of the circuit diagram
detailing an embodiment of a device for the reduction and
prevention of condensation on optical systems.
[0016] FIG. 3 is an illustration of a telescope with a condensate
reduction device.
[0017] FIG. 4 is an illustration of a surface mount printed circuit
board heater for a condensate reduction device.
DETAILED DESCRIPTION OF THE INVENTION
[0018] FIG. 1 is a block diagram illustrating the general concepts
of at least one embodiment of the present invention. One embodiment
disclosed herein has a resistive heater element is in contact with
the optical components that are subject to condensation although
any manner of transmitting heat can be used including radiative
methods such as irradiation. Also in thermal contact with this
optical component, is a solid-state precision temperature sensor.
In addition, there is a matching solid-state precision temperature
in thermal contact with the ambient air, but thermally isolated
from the optical element. Signals from these two sensors are
applied to a comparator which generates a data signal when the
optical temperature sensor is measuring an optical component
temperature that is less than the ambient or reference temperature.
This data signal is used to activate a solid-state power switch
that applies a voltage to a resistive heating element. An offset
may also be applied to the reference temperature sensor allowing
compensation for the thermal resistance of the system comprised of
the optical component, the optical component attachment heater and
temperature sensor.
[0019] In another embodiment, a thin flexible printed circuit board
populated with surface mount chip resistors and thermal sensors is
bonded to a flexible strap. The flexible strap is placed in thermal
contact with the optical component attachment and tightened so as
to secure a good thermal contact with the component. Electrical
wire leads are brought out to attach the circuit board to the
controller. Any number of heater straps can be utilized in a wide
variety of shapes and sizes to facilitate a multitude of optical
components that can be thermally controlled. Heating elements can
be designed in a number of configurations such as helical or
circumferential straps placed near the outer edge of an optical
component, as well as a wide variety of pad shapes that can be
placed on other surfaces such as the backs of mirrors.
[0020] Another embodiment may encompass, for example, a circular
heating pad mounted on the rear of the primary reflecting mirror of
a Newtonian telescope, a small rectangular heating pad on the back
side of the secondary mirror and a heating strap placed
circumferentially around the eyepiece. The spotting scope may have
a heating strap placed circumferentially around both the objective
lens holder and the eyepiece. Each heat element contains a
temperature sensor and is wired directly into the controller that
can independently calculate the ambient temperature offset for each
lens or mirror and adjust the heating to the individual components.
Numerous heating elements can be independently controlled with a
single controller.
[0021] An additional embodiment may include a hygrometer to monitor
the relative humidity of the ambient air and thus establish a dew
point. The electronic controller would then use this data to
maintain the optical system temperature at a point slightly greater
than the dew point.
[0022] Humidity is a general term that refers to the air's water
vapor content and the source for most condensation contamination.
Relative humidity is defined as the ratio of the amount of water
vapor actually in the air compared to the amount of water vapor the
air can hold at a particular temperature and pressure, or in other
terms, the ratio of the air's actual vapor pressure to its
saturation vapor pressure (capacity). In order for condensation to
occur, the ambient air surrounding the optics must become
saturated, even if the saturation only occurs within a very small
boundary layer near the optical surface. Saturation of air is an
atmospheric condition whereby the level of water vapor is the
maximum possible at the existing temperature and pressure, i.e.,
100% RH. When such a condition occurs, the air will seek an
equilibrium vapor pressure through micro and macroscopic
condensation.
[0023] Unfortunately, the steadiest, sharpest telescopic views are
often experienced under precisely the atmospheric conditions that
cause condensation to form. A common situation occurs when one
utilizes an astronomical viewing device such as a telescope,
binocular, charged coupled device (CCD) imaging or the like, in an
outdoor environment in cooler temperatures. Typically at night, the
RH will be high and increase as the air continues to cool through
the night and thus, the difference between the ambient air
temperature and the dew point decreases. Dew Point represents the
temperature to which air would have to be cooled (with no change in
air pressure or moisture content) for saturation to occur. A simple
example of condensation or "dew physics" occurs when you take a
beverage can out of the refrigerator. When placed at normal room
temperature where the can is colder than the air's dew point, it
drips with condensation. A similar situation occurs with telescopes
under a clear night sky.
[0024] The Second Law of Thermodynamics suggests that an optical
device would achieve equilibrium with the ambient air, and as long
as that air maintained moisture content above saturation, no
condensation would occur. On the contrary, if one were to take a
surface temperature measurement of the optics at a time when
equilibrium would be expected, one would find that the surface
temperature is actually several degrees cooler than the ambient air
temperature. Objects do try to achieve temperature equilibrium with
their environment as the Second Law says, but conduction is not the
only mechanism by which these objects are bound. Optical surfaces
like any other objects are also influenced by convection and more
importantly, radiation. The temperature differential at the surface
of these objects is caused by thermal radiant energy being
propagated to the cold night sky. The effective temperature of the
dark night sky is only a few degrees above absolute zero, and the
telescope in an open field is exposed to an entire celestial
hemisphere of thermal sink.
[0025] As the optical surfaces cool quickly by thermal radiation,
the surrounding boundary layer of air attempts to equilibrate the
temperature differential by transferring heat to the optics. As the
boundary layer air temperature decreases to or below the dew point,
saturation occurs and condensation begins to form on solid
surfaces. Because this phenomenon will continue until equilibrium
vapor pressure is achieved, mere wiping of the optical surfaces in
attempt to dry them is not feasible.
[0026] The greatest occurrences of optical contamination by
condensation are on the exposed parts that are thin or have a low
heat capacity and rapidly radiate energy. These are often essential
and common structures in optical and telescopic instruments. Prior
attempts to prevent condensation have been directed to shielding
optics from as much exposure to the night sky as is feasible.
Traditionally, a device called a dewcap can be placed extending
beyond a lens to serve as a radiative shield to the night sky. In
this configuration, the longer the dewcap, the more likely it is to
be effective.
[0027] The impact of condensation on telescopic optics has evolved
with time over the years. In the early '60s, most telescopes were
Newtonian reflector types. In this configuration, the entire tube
acts as a shield to the mirror positioned at the base and
condensation was not of great concern. An open-tube reflector,
however, would need a shroud along its entire length of open
framework to gain such a benefit. In the 1970's, with the advent of
Schmidt-Cassegrain telescopes, condensation became a much more
relevant factor. These instruments have thin corrector plates,
which quickly radiate heat and foster the formation of
condensation.
[0028] Throughout the 1980's, open-tube (Dobsonian) telescopes
proliferated through the market. These exposed reflectors were very
susceptible to condensation. The open systems combined with the
advent of high-performance eyepieces, which contain large amounts
of glass, exacerbated the problem of condensation. Eyepieces are
particularly prone to condensation because of the added humidity
from the observer's eye and breath. Because the massive optics
retain their heat longer than standard eyepieces, when they do
become contaminated, the efforts to remedy the situation are also
increased. The need for a means to overcome this contamination was
never more necessary.
[0029] As optics have evolved, various new mechanisms have been
introduced in the optical systems. The advent of CCD imaging
devices and autoguiders, have created an entirely new set of
condensation challenges. The high sensitivity CCD's, easily renders
these devices useless in the presence of even a moderate quantity
of condensation. Autoguiders can lose the ability to guide or track
when dew inhibits the imaging ability of the autoguiders.
[0030] With the advent of these new and complex optical and digital
electronic systems, the passive shielding of optical systems is no
longer able to affect a suitable a way to prevent condensation. An
active mechanism to remove, as well as prevent dew formation, is
needed. One of the most common means for dealing with condensation
or dewing of optics has been to apply heat to the effected
instrumentation. This has most commonly been performed with either
hot air or direct contact with an electric heating mechanism. Hot
air has been applied with "hair dryer" and "windshield defroster"
type devices for many years with very limited success. While these
devices can remove the condensate in a relatively quick and
efficient manner, the blast of hot air temporarily creates thermal
aberrations that limit the ability of the telescope. This
distortion is in addition to any introduction of thermal
deformation to the optics themselves. Air heaters produce
superficial and uneven heating of surfaces that can deform and
distort the images. Hot air is also only a temporary solution. The
moment that the hot air is removed from the optical surfaces, these
surfaces immediately begin to cool and initiate the radiative
cooling so that the condensation process begins once again. A
telescope can actually lose an entire magnitude of light grasp
before the unaided eye can detect condensate on the optical
surfaces. Contact heaters, which typically may comprise nichrome
wire heating elements or electrical resistors soldered in series
and placed against the optical surfaces, have had limited success
in dealing with condensation problems. In these devices, it is the
control of the heating element that has been deficient. These
heaters also cause thermal distortion of the optical surfaces and
can often be a danger to the user when controlled by a large DC or
120 volt AC power source.
[0031] Several commercial systems and numerous do-it-yourself plans
have been developed for removing dew on telescope optics. The
biggest drawback of current systems has been the lack of ability to
control and minimize the heat applied to the optics as well as the
ability to "set and forget" the heater. These systems typically
incorporate a heating mechanism with a rheostat, which is a simple
duty cycle adjustment for the power supply. The set point of the
device is estimated by the user and can often require constant
monitoring and readjustment to achieve the intended result. It is
also often very difficult or impossible for the user to maintain
optics at their optimal performance temperature which is the
ambient temperature. It is obvious that by simply heating the
optics, even with a fixed temperature control device, the desired
results are not achieved.
[0032] Referring again to FIG. 1, the block diagram illustrates the
manner in which condensation on optical elements can be reduced or
prevented. Optical element 100 is in thermal communication 110 with
both the optical planer heater element 120 and the optical element
temperature sensor 150. The temperature of the optical element 100
is measured by the optical element temperature sensor 150 and
electronically transmitted to the comparator 140. Ambient air
surrounding the optical device is measured by the ambient air
temperature sensor 160 and electronically transmitted to the
comparator 140. An offset 170 can be applied to the ambient air
temperature sensor 160 to allow compensation for the thermal
resistance of the system comprising the resistance of the optical
element 100, the optical planner heater element 120, and the
temperature sensor 150. A comparator circuit 140 analyzes the
temperature inputs and generates a data signal when the optical
element temperature is less than the ambient referenced
temperature. The status signal is used to activate the solid-state
power switch 130 and supply voltage from the conditioned power
supply 180 to the optical planar heater element 120, which is in
thermal communication with the optical element 100.
[0033] Illustrated in FIGS. 2A and 2B illustrate a circuit diagram
detailing an embodiment of a device for the reduction and
prevention of condensation on optical systems including a
controller 200 and the heater tape assembly 202. Integrated circuit
U1, 205 provides an output voltage at pin 2, 210 which is
proportional to the ambient air temperature. This voltage is
applied to pin 3, 220 of integrated circuit U3, 215 which is an
operational amplifier used as a comparator. Integrated circuit U4,
225 is a temperature stabilized voltage reference. The output of
integrated circuit U4, 225 provides a reference voltage for
integrated circuit U1, 205 and integrated circuit U2, 212 via
resistor R15, 230, resistor R18, 235, resistor R19, 240, and
resistor R20, 242. This network allows the user to set a thermal
offset to compensate for the thermal resistance between the heater
resistor R1, 245 and the optical element (not shown). As the
temperature of integrated circuit U2, 212 falls bellow the offset,
the output of integrated circuit U3, 215 raises to +12V. This turns
on power MOSFET Q1, 250 allowing current to flow thru resistor R1,
245 and heat resistor R1, 245 and the optical element. This
continues until the temperature of integrated circuit U2, 212 is
equal to the offset. This on-off action continues as long as power
is applied to the system, thus regulating the temperature of the
optical component to within approximately .+-.2 degrees C. of the
offset set point and tracks the air temperature. The light emitting
diode D2, 255 provides a heat on indication while diode D3, 260
provides a cooling indication.
[0034] FIGS. 2A and 2B illustrate a circuit diagram for controlling
a DC electric heating element. A variety of systems and methods for
controlling the amount, intensity and duration of the heat applied
to the optical surface have been contemplated and are not limited
by the disclosed embodiments. Constant heating at a constant level
can be applied in an on-off (go-no go) method where the heat is
only applied when the optical surface temperature is between a
lower and upper threshold limit, or variable heating (intensity or
duty cycle for example) can be applied based upon other thermal
factors such as how far away the current surface temperature is
from a temperature setpoint.
[0035] As shown in FIG. 3, a thin flexible printed circuit board
populated with surface mount chip resistors is encapsulated to form
a heater tape 300 and is bonded to a nylon strap 350 that can be
circumferentially mounted around an optical surface. A surface
mount thermal sensor 310 is also incorporated in the nylon strap
350 to register the temperature of the optical surface. The nylon
strap 350 is held in place by friction that is adjusted by tension
tabs 340. The heater control 320 is mounted above the tension tabs
340. The ambient air thermal sensor 330 is isolated from the
optical surface by thermal insulation 360 and measures ambient air
temperature. Electrical wire leads are brought out attaching all
the electrical components to the main controller.
[0036] A specific embodiment of the present invention can be
utilized in a wide variety of forms. The system can be embodied
using flexible straps or pads that can permanently or temporarily
attach to, or attach in proximity to the optical surfaces. The
flexible straps can be made out of a multitude of rigid and/or
non-rigid materials that may incorporate heater elements,
temperature and/or hygrometric sensors within single or multiple
straps. Heater elements can be conductive (i.e., AC or DC
electrical), radiative (i.e., infrared), or convective. Electrical
heater elements can be resistive heater tape, flexible printed
circuit boards populated with bonded surface mount chip resistors,
heating coils etc. Controller units can be dedicated to each
individual optical surface or multiple controllers can be combined
into a central controlling unit that can regulate the temperature
of any number of optical surfaces either independently or as a
single unit. Thermostatic setpoints and temperature ranges can be
programmed into the controller and set independently for each
optical surface or as a single parameter for all optical surfaces.
The aforementioned system can an aftermarket device that attaches
to existing optical equipment or can be incorporated into the
design and manufacture of new optical equipment such as telescopes,
binocular/monoculars scopes, mirrors, windows, viewing ports or any
other type of optical surface that is subject to condensation.
[0037] FIG. 4 is an illustration of a telescope with a condensate
reduction device in place. A typical refractor telescope
configuration is shown with the main features comprising a
telescope body 400, entraining and optical surface 410 on one end,
and an eyepiece holder 430 on the opposing end. The primary optical
surface 410 is heated by a surface mount sensor/heater assembly 435
comprising surface mount heater tape 450, surface mount thermal
sensor 440, the heater control 460 and an ambient air thermal
sensor 470. The eyepiece holder 430 is in connection with the
eyepiece 420 and retains an additional heater assembly 435, which
similarly contains (but does not show) surface mount heater tape,
surface mount thermal sensor, heater control and ambient air
thermal sensor. Each heater assembly 435 is connected to a 12-volt
power supply 480.
[0038] The foregoing description of the invention has been
presented for purposes of illustration and description. It is not
intended to be exhaustive or to limit the invention to the precise
form disclosed, and other modifications and variations may be
possible in light of the above teachings. The embodiment was chosen
and described in order to best explain the principles of the
invention and its practical application to thereby enable others
skilled in the art to best utilize the invention in various
embodiments and various modifications as are suited to the
particular use contemplated. It is intended that the appended
claims be construed to include other alternative embodiments of the
invention except insofar as limited by the prior art
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