SEMI-ACTIVE FOCUS AND THERMAL COMPENSATION OF A CENTRALLY-OBSCURED REFLECTIVE TELESCOPE

Abstract: A semi-active focus and thermal compensation system (20) and improved three mirror anastigmat telescope (10). The telescope has a primary mirror (12), a secondary mirror (13) suspended between the input window and the primary mirror by support struts (14), a tertiary mirror (16), and optional fold mirror (15). The system includes a plurality of heating elements (22) respectively disposed on each of the support struts. A first temperature sensor (23) disposed on the secondary mirror, a second temperature sensor (24) (disposed on the primary mirror) generates a reference temperature, and a plurality of third temperature sensors (25) are disposed on each of the support struts. A temperature compensation controller (21) is coupled to the heating elements and temperature sensors and controls the heat output of the plurality of heating elements to heat the support struts and control the position of the secondary mirror.

Description: SEMI-ACTIVE FOCUS AND THERMAL COMPENSATION OF A CENTRALLY-OBSCURED REFLECTIVE TELESCOPE BACKGROUND The ptesent invention ielates generally to centrally-obscured ieflective telescopes, and more particulai ly, to such as a cenh ally-obscured reΩectn e telescope having a semi-active focus and thermal compensation system that also may be used foi boiestght correction (line-of sight control) 5 A centrally obscured reflet tive telescope, such as a thtee mirror anasttgmat telescope, for example, includes a pr imary mirror a secondar y mir ror , and a tertiary mn ror T he telescope is generally paired with focusing optics or an iinagci that focuses an image produced by the telescope onto a detectoi The telescope may be pi tected by a window located in object space I he secondary minor is suspended between the ] () window and the primary mrrror by means of a plurality of suppor t sti nts The window is exposed to external temperatures and there is a temperature gradient between the exter ior of the indow and the primary mir ror T he thr ee miπoi anastigmat telescope pro\ ιdes optimum per formance only w ithin a narrow isothermal range Many applications require the secondary mir ror to be 1 located near the window where external temper atures are extreme (high altitude in aircraft, ior example), and the ιty temperature must be contiolled, lesulπng in a lai ge thermal gradient near the window To minimize system and window si/e the secondary mirror is generally located close to the w indow, and is thus within this gr adient aiea T echniques used to heat the window oi othei wise minimi/e the 20 temperature giadient take substantial power, cause gimbal disturbances due to airflow and the like Furtheimore these techniques do not eliminate asymmetric temperatures if the l elative angle of the telescope wrth respect to the wrndow is not constant (gimbal pointing) This will cause boresrght shift The problem rs that the telescope must be matntamed rsotheimal in ordei to remain in focus In particular , rn order for the telescope to remarn in focus, the relative curvatures of the primary and secondary miirors must be maintained as well as the separation between the pπmary and secondary mirrors Due to a drfficult ther mal envir onment and local power drssipation, this has not been possible using external cavity tempeiature control One pπor approach to compensate for temperature var iations in lved the use of a mechanical drive system that displaces the focal plane This approach is difficult to align initially, and is susceptible to shifts T he primary issue is that movement of the focal plane, or primary and secondary minors along the optical axis by as little as fϊfty- milhonths of an inch will result in defocusing of the telescope Actuator drives, position sensors and servo controls are required Mechanical elements aie degraded by dm, temperature variations, shock and vibration, corrosion, lubi icant degradation, calibration drift rth temperature, hysteresis and friction Furthermor e, there may be optical prescription errors, and the like, that cannot be corrected by such mechanrca! drive system These effects make it almost impossible to c ontr ol the r elatrve positions of the focal plane, primary and secondary miirois with suf ficient accuracy to focus the telescope It would therefore be an advantage to hav e an ιmpι ed centt ally-obscui ed reflective telescope that embodies a focus and theπnal compensation that improves upon conventional approaches Accordingly, it <s an objective of the present invention to provide for an improved centrally-obscured reflective telescope having a semi active focus and thermal compensation system ft is a furthei obiective of the present inv ention to provide for an improved centrally-obscur ed reflective telescope hav ing a semi active focus and thermal compensatton system that may be used for boresrght coπection (line of-sight conti ol) SUMMARY OF THE INVENTION I o meet the above and other objectiv es the present invention provides tor a centrally-obscured reflectiv e telescope, such as a three mπroi anastigmat telescope, for example, that employs a semi activ e focus and thermal compensation system An exemplary three mirror anastigmat telescope comprises an insulated housing ha ing a ca ity and an input window The telescope also comprises a primary mirror, a secondary nun or, and a tertiary mirror The tertiary mnroi is not required for all embodiments ot the centr ally obscured reflectiv e telescope The secondary mirror is suspended between the input window and the primary mirror by means of a plurality of support struts. A cylindrical housing or barrel has the support struts secured to one end thereof and is secured to the primary mirror at the other end. The telescope is generally mated to focussing optics, such as an imager. A fold mirror may be used to reflect light from the secondary mirror onto the tertiary mirror which couples the light to the focussing optics or imager. A cavity heater may be provided in the cavity for heating the interior of the cavity. The semi-active focus and thermal compensation system comprises a temperature compensation controller that is coupled to heating elements disposed on various components of the telescope. The temperature compensation controller" is coupled to a temperature sensor disposed on each of the support struts, to a temperature sensor disposed on the secondary mirror, to a temperature sensor on disposed the primary mirror, and to a plurality of temperature sensors disposed around the cylindrical housing or barrel. The temperature sensors may comprise thermistors, for example. In general, it is desirable to have the temperature sensor on each support strut aligned with temperature sensors on the cylindrical housing or barrel. As was mentioned in the Background section, to keep the telescope in focus, the relative curvatures of the primary and secondary mirrors must be maintained and the separation between the primary and secondary mirrors must be held constant. The semi-active focus and thermal compensation system senses temperatures of the support struts, the barrel, and the primary and secondary mirrors using the temperature sensors. The primary mirror is used as a reference, although another component may be selected. The barrel and the support struts are selectively heated by the heating elements under control of the temperature compensation controller to control their relative lengths which in turn controls the position of the secondary mirror relative to the primary mirror and hence the focus and boresight of the telescope using servo-type balance. The secondary mirror is selectively heated to control its curvature relative to the primary mirror. These temperature control actions maintain the relative curvatures of the primary and secondary mirrors and the separation between the primary and secondar y mirrors relatively constant in order to keep the telescope in focus. The heating elements are tailored to expected gradients and are shielded from the optical path of the telescope. The temperature compensation controller provides closed loop feedback control of the strut, barrel and mirror temperatures, and thus, focus and theπnal characteristics of the telescope. The temperature compensation controller may control the heating elements in an analog (hardwired) fashion, or the healers may be software controlled, depending upon requirements. l he heating elements attached to the support struts, bar rel and secondary mrrror athermalr e the telescope, provide focus control, and mitigate boresight drift This is accomplished by multipoint temperature sensing and proportional heater power control using the temperature compensatron controller The semi-active focus and thermal compensation system may be operated in a balance mode, pi ovrdrng only athei malrza- tion, or actrve boresight correctron and focus control may be provided by the controllei BRIEF DESCRIPTION OF THE DRAWINGS The various features and advantages of the present inv ention may be more readily under stood with relerence to the following detailed description taken in conjunction wrth the accompanying drawings, herein like reference numerals designate like structur al elements, and in w hich Fig 1 illustrates a parttally cutaway side view of a reduced to pr actice embodiment of a centrally obscured reflective telescope employing an exemplary embodiment of a semr-active focus and thermal compensation system in accordance with the pimcrples of the present invention, Fig. la is a partially cutaway perspective vrew of the c entr ally-obscured reflective telescope shown in Fig 1 , Fig 2 illustrates details of the semi active focus and thermal compensation system used in the centrally obscured reflectiv e telescope shown in Tig 1 , Fig 3 shows a plan iew of an exemplary surface heating element that may be employed in the semi-activ e focus and thermal compensation system, Figs 4a and 4b show plan and sectional views of an exemplary embedded heating element that may be employed rn the semi activ e focus and theπnal compensation s tem, Fig 5 illustrates an uncorrected telescope housing gradient obtained w ithout using the present rnventton, Fig 6 illustrates a corrected telescope housing gt adicnt obtained using the pr esent invention, and Fig 7 illustr ates boresight col lection achieved using the pr esent inv ention DE TAILED DESCRIPTION Referring to the drawing figures, Fig 1 illustrates a partial cutaway side v iew of an exemplary centrally-obscured reflective telescope 10 comprising an exemplary embodiment of a semr-active focus and thermal compensation sy tem 20 in accordance w ith the principles of the pi esent in ention Fig l a is a partially cutaway pei spectiv e v iew of the exemplary centrally -obscured reflectiv e telescope 10 show n in Fig 1 Fig 2 shows a front view of the centrally-obscured reflective telescope 10 shown in Fig. 1 and illustrates details of the semi-active focus and thermal compensation system 20. The exemplary centrally-obscured reflective telescope 10 is illustrated as a three mir ror anastigmat telescope 10. Although the present invention is shown and described with reference to a centrally-obscured reflective telescope 10 having a Cassegrain configuration, it is to be understood that other configurations may be used The exemplary telescope 10 comprises an telescope housing 1 1 (a portion of which rs shown) which may be insulated, having an internal cavity 12 and an input window 13. The telescope 10 comprises three powered mui ois including a pπmary mirror 13, a secondary mirror 14, an optional ternary mirroi 16, and includes an optional flat fold mirror 15 An inner housing 1 8 oi banel 18 has the support str uts 17 secured to one end thereof and is secured to the pnmary min or 13 at the other end thereof. The secondary mirror 14 is suspended between the input window 1 1 and the pr imary mirror 13 by means of a plurality of support struts 17 The above-mentioned optical components are disposed within the cavity 13 of the telescope housing 1 1 or on an optical bench (not shown) A cavity heater 19 may be provided in the cavity 13 for heating the interror of the cavity 13. The telescope 10 is typically mated to focussing optics, such as an imager (gener ally shown). A fold mrrror is used to improve packaging of the telescope 10 and to leflect light from the secondary mirror 14 onto the tertiary mirror 16 which couples the Irght to the focussing optics or tmager. The semr-active focus and thermal compensation system 20 comprises a temperature compensatron controller 21 that is coupled to a plui ahty of temperature sensors and heating elements that are respectively disposed on various components of the telescope 10. One or more first temperature sensors 24 ai e disposed on the primary min or 13 that generate a reference temperature fTpj5 ), a second temperature sensor 23 is drsposed on the secondary mirroi 14, and one or more thud tempei atui e sensors 25 are disposed on the support struts 17 A pluiahty of fourth temperature sensois 26 may be disposed around the periphery of the bairel 1 8, that αi e typically located in r espectiv e quadrants thereot. A temperature sensor 27 may also be disposed on the tertiary mtrroi 1 6 The tempeiature sensoi s 23, 24, 25, 26, 27 may comprise thermistors, foi example. In general, it is preferable to have the third temperature sensor 25 on each support strut 17 aligned with temperature sensors on the ban el 1 A secondary mnror heating element 3 1 may be disposed on the secondary mirror 14. The secondary mnror heating element 3 1 is used to control the curvature of the secondary' mirror 14. One or more strut heating elements 32 are disposed on each of the support stnits 1 7 The strut heating elements 32 ai e is used to contr ol the relative lengths of the respective support struts 17 A plurality of strip heating elements 33 may be disposed around the periphery of the barrel 18, that are typically located in respective quadrants thereof The cavity heater 19 may be used to heat the inter ror of the cavrty 13 , including the barrel 18, instead of the plurality of stnp heating elements 33 The various heating elements may be secured to the their respective components using an adhesive film, for example In a preferred embodiment, the temperature sensors 23 27 are located as follows The temperature sensors 23, 24, 27 are disposed on each of the pow ered min or s 13, 14, 16 (primary min or 13 secondary mirror 14, tertiary mn ror 16) The curvature of the powered mirrors 13 14, 16 are sensitive to tempei atui e, and can be col l ected by mathematically predicting curvatui e as a function of temperature and contr oll ng the temperatures of the respective 13, 14, 16 The second temper ature sensoi 24 are disposed on the primary minor 1 3 and generate the reference temperature (TR £F) The temperature sensors 23-27 are mapped into a focus algorithm employed in the conn oiler 21 using analysrs of the growth of the telescope 10 due to temperature gradients Active corrections are input from these temperature sensors 23-27 In the preferred embodiment, the cavity heater 19 is used to heat the interior of the cavity 13 and the barrel 1 Therefore, the plurality of strip heating elements 33 on the bai rel 18 are not used The fourth tempei ature sensoi s 26 are thus disposed on an unheated structure (I e , the barrel 18) Foi example, in a reduced to practice embodiment of the system 20. eight or more fourth temperature sensors 26 are disposed on the banel 18 T he controller 21 of the semi-active focus and thermal compensation system 20 senses temperatures of the support struts 17, the bαπel 1 8, primary min or 1 3, the secondary mirror 14, and optionally the tertiary minor 16 using the r espective temperature sensors 25, 26, 23, 24, 27 The support struts 17 that support the secondary mirror 14 are heated by the strut heating elements ^2 under control of the temperature compensation c onttoller 21 to control the position (focus and boresight) of the secondary mirroi 14 using serv o-type control The strut heating elements 32 are tailor ed to expected temperanue gradients and are shielded from the optrcal path ol the telescope 10 1 he conti ollcr 21 prov ides closed loop feedback control of the strut, banel and min or temperatures and thus the locus and thermal chai actei isttcs of the telescope 10 The contr oller 2 1 may control the strut heating elements M, strip heating elements 33 and mirror heating elements 1 34 in an analog ( hai d ired) fashion Alternatively the heating elements 1 -34 may be sol tware controlled The temperatures sensed by the temperature sensor s 23 27 r e instantaneous and autonomous in that, as the system 20 operates, it is subject to thermal transient such as tum-on, solai load, active components mounted in close pioximity, local air temperature, and the hke If the controller 21 is operating with a given sample fiequency, the stnits 17 can be continuously commanded to refocus and the curvature of the secondary mrrτor 14 can be adjusted to provrde the cot rect curvature Two temperature sensor 24 were used on the primary mirror 1 of a reduced to-prαctrce telescope 10 The pi imary mrrror 13 has the hrghest sensitivity (defocus/ ϋ C) and this is used as the first correction term ( 1 REF^ rn the calculatron performed by the algorrthm. The outputs of the two sensors 25 were aver ged In developing the telescope 10, the secondary mrπ or heatmg element 3 1 was installed on the secondary mirror 14 However , it was determined that this heating element 31 was not required Notwithstanding this, such α heating element 1 may be used in certain applications, to provide additional coπection tei m loi the focus algorithm It is to be understood that the leduced to-pi αctrce embodiment of the telescope 10 shown in Fig 1 is afocal (not fo used) An imager is used to focus light to α point or focal plane Thus, the output beam from the telescope 10 has paiallel limit rays as shown in Frg 1 . Fig 3 shows a plan view of α first exemplary heatmg element 32 that may be employed rn the semr-actrvc focus and thermal compensation system 20 The first heating element 32 is a thermo-fotl type heating element 32 The thei o f oil type heating element 32 comprises α loil filament 41 that is disposed on a dielectric substr ate 42 One end of the foil filament 41 is coupled to a heater output of the temperature compensation controller 2 1 while the othei end is coupled to gi ound Figs 4a and 4b show plan and sectional views of a second exemplary heatmg element 32 that may be employed in the semi-active locus and thermal compensation system 20 The second heating element 32 may be an embedded type heating element 32 The embedded ty pe heating element 32 comprises a filament 4 1 that is embedded within the support strut 17 The filament 41 may be disposed in a slot, tor example rn the support strut 17 hich is filled with a filler material 43 to encapsulate the filament 1 The filler mater ral 43 may compπse a flexible epoxy based compound, tor example One end of the filament 4 1 is c oupled to a heatei output of the tcmpei atuie compensation controller 2 1 while the other end is coupled to giound The strut heating elements 32 attached to the suppor t str uts 17 tor the secondaiy mirror 14 atheπnalrze the telescope 10, pro ide focus conti ol, and mitigate boiesight drill This is accomplished by multipoint tempei ature sensing of the heated elements (support stiuts 17) and the secondary mirroi 23 and proportional heater power conti ol provided by the temperature compensatron controller 21 The semi-active focus and thermal compensatron system 20 may be operated rn α balanced mode, provrdmg only athermalizatton Alternatively active boiesight correc tion and focus control may be provided by the controller 21 Thus wrll be discussed with teference to Figs 5-7 The illustrations in Figs 5-7 are not drawn to scale Fig. 5 illustrates an uncoπected telescope housing gradient obtained vvrthout using the present invention The secondary mirror 14 is coupled by way of struts 17 that ar e unsensed As a consequence, the focus and boresight of the telescope 10 are uncompensated and the image produced by the telescope 10 will not be focused at the desired location Tig 6 illustrate^ α corrected telescope housing gradient obtained using the present invention By sensing the temperalm es of the sti uts 1 7 and mirroi s 1 , 14, 16 the controllei 21 can adjust the respective temperatures provided by the heating elements 32 to change then respective lengths and thercfoie maintain focus and boiesight ot the telescope 10 Fig 7 illustrates boiesight coπection achieved using the present invention The nominal positions of the struts 17 and secondary mirror 14 are shown in solid lines The adjusted (compensated) positions ot the struts 17 and secondary min or 14 ai e shown in dashed lines By using the controller 21 to adjust the respective temperatures provided by the heating elements 32 coupled to the struts 17 for example, the respec- trve lengths of the struts 17 are controlled to correct the boiesight of the telescope 10 One benefit of using the present inventron is that mateπals having ditfeient coefficients of theimαl expansion may be used This is desirable from a mantifactui ing producibrlrty an cost standpoint For example, the mirroi 1 3, 14 , 1 6 used in the reduced to practice embodiment of the telescope 1 were 606 1 - ' I 6 1 aluminum The secondary support struts 17 and barrel 18 weie made oi A356 oi A357 cast aluminum If all ol the components of the telescope 1 were aligned and focused at 68 r F, and it the coefficients of thermal expansion of each component matched all ot the other components, and rl the entire telescope 10 remained isother mal, then it would alway s be in toctrs This ould also establish the initial boresight Most practical systems, ho evei , are made tiom the most suitable material for that component Theiefoie, the coefficients of ther mal expansion are typically not identical πthermore, most systems expeπence both theπnal gradients and thermal ti ansients Even in scientific instruments (astronomy) these are a problem In military and commercial systems, w hich are usually tightly packaged and w eight critical, the thermal problems may be sev ere If the stntts 17 aie u^ed to correct a theπnal gradient in the telescope 10, they simultaneously coπ ect both focus and boresight as was discussed with reference to Figs 5-7 For practical purposes, the struts 17 need to be heated slightly above the temperature of the remaining components If one side of the struts 17 are allowed to cool and the other side is heated, a boresight shift is induced such as is lllustiated in Fig 7 Thus, by applying temperature commands in an appropriate way, full X/Y tilting of the secondary min or 14 may be achieved This may be done open loop (fixed offsets in the software command, foi example) or usrng feedback from another alignment references, providing an autoahgnment system Other features may be included in order to enhance the semr-active focus sy stem 20 pi ovided by the pr esent invention It may be desnable to alter the heat transfer characteristics of the telescope 10 Typical methods include adding fin area to the banel 1 , for example, to more closely couple rt to the local arr temperature, or to add theπnal insulation to decouple the component from the air (such as on the secondary minor 14, for example) Also, actrve heatmg of the banel 18 may be performed Hie addition of strip heaters 33 in each quadrants of the banel 18 may be done, although it was not necessary rn the reduced to-practrce embodrment of the telescope 10 shown in Fig 1 It is to be understood that the reduced to practice embodiment of the telescope 10 shown in Fig 1 is αfocαl (not focused) An imager is used to tocus light to α point or focal plane Thus, the output beam from the telescope 10 has pai allel limit rays as shown in Fig 1 The structure of the semi active locus nd ther mal compensation system 20 eliminates the need foi a mechanical focus system, which is nioi e complex, expensiv e, and less iehable The semi active locus and thermal compensatron system 20 also takes very lillle volume or weight on a gimbαl (not show n) on which the telescope 10 may be disposed The semi-active tocus and thermal compensation system 20 may be used in any tlnee minor anastigmat telescope or in any telescope having a sunilai configuration The semi-active focus and thermal compensation system 20 directly addresses the fundamental problem oi non isothermal optics in the three minor anastigmat telescope 10, rathei than coti ecting the effects ot the problem 1 he simple implementation embodied in the semi active focus and thermal compensation system 20 may be used to provide active boresight and tocus in addition to isothermal contiol The semi active locus and themial compensation s stem 20 uses simply fabricated, low cost parts The semi-active focus and thermal compensation system 20 uses electrical control, and it is much easiei to optimize in-sttu, resulting in lower development cost and risk In high pei formance electro-optical imaging sensors, such s those developed by the assignee of the present invention, foi e xample, a processoi may already exist, which may be programmed to implement the control functions of the temperature compensation controller 21 , thus add g capabilrty without addttronal cost. The components used rn the semr-active focus and thermal compensation system 20 are also r eadily available and ate iehable, which reduces cost and risk The semi-active focus and thennal compensation system 20 is mechanically rigid and piovides an optimal structuie since no sliding mechanisms or linkages are used. There is no loss of stiuctural stiffness of the telescope 10 when using the seπn- acttvc focus and theπnal compensatron system 20 Thus, an unproved centrally-obscured reflective telescope havtng a semi-active focus and thermal compensatron system has been drsclosed It is to be under stood that the desct bed embodiments are merely illustratrve of some of the many specrfrc embodiments which represent applications of the principles of the present mventron Clearly, numerous and other arrangements can be readily devrsed by those sktlled in the art wrthout departing from the scope of the invention

Claims: CLAIMS What is claimed is: 1. A three mirror anastigmat telescope (10) comprising: a pπmary mirror (12), a secondary mirror (13) suspended between the input window and the pπmary mirror by a plurality of support struts (14); a tertiary mirror (16); and a semi-active focus and thermal compensation system (20) compnsing: a heating element (22) disposed on each of the support struts; a first temperature sensor (23) disposed on the secondary mirror; a second temperature sensor (24) that generates a reference temperature; a temperature sensor (25) disposed on each of the support struts; and a temperature compensation controller (21) coupled to the heating elements and the temperature sensors that senses temperatures of the support struts, primary mirror and secondary mirror and controls the heat output of the plurality of heating elements to selectively heat the support struts to control the position of the secondary mirror. 2. The telescope (10) recited in Claim 1 wherein the temperature sensors (23, 24, 25) comprise thermistors 3. The telescope (10) recited in Claim 1 wherein the heating elements (22) are tailored to expected temperature gradients expeπenced by the telescope. 4. The telescope (10) recited in Claim 1 wherein the heating elements (22) are shielded from the optical path of the telescope. 5. The telescope (10) recited in Claim 1 wherein the temperature compensation controller (21) is hardwired to the heating elements (22) and controls the heating elements in an analog fashion. 6. The telescope (10) recited in Claim 1 wherein the temperature compensation controller (21) controls the heating elements using a software algorithm. 7. The telescope (10) recited in Claim 1 wherein the heating elements (22) comprise thermo-foil heating elements 22. 8. The telescope (10) recited in Claim 1 wherein the heating elements (22) comprise embedded heating elements (22). 9. The telescope (10) recited in Claim 1 further comprising an input window (11). 10. The telescope (10) recited in Claim 1 further comprising a fold mirror (15) disposed between the secondary mirror (13) and the tertiary mirror (16). 11. A semi-active focus and thermal compensation system (20) for use with a three mirror anastigmat telescope (10) comprising a primary mirror (12), a secondary mirror (13) suspended between the input window and the primary mirror by a plurality of support struts (14), and a tertiary mirror (15). said system (20) comprising: a heating element (22) disposed on each of the support struts; a first temperature sensor (23) disposed on the secondary mirror; a second temperature sensor (24) that generates a reference temperature; a third temperature sensor (25) disposed on each of the support struts; and a temperature compensation controller (21) coupled to the heating elements and the temperature sensors that senses temperatures of the support struts, primary mirror and secondary mirror and controls the heat output of the plurality of heating elements to selectively heat the support struts to control the position of the secondary mirror. 12. The system (20) recited in Claim 11 wherein the temperature sensors (23, 24, 25) comprise thermistors. 13. The system (20) recited in Claim 11 wherein the heating elements (22) are tailored to expected temperature gradients experienced by the telescope (10). 14. The system (20) recited in Claim 11 wherein the heating elements (22) are shielded from the optical path of the telescope (10). 15. The system (20) recited in Claim 11 wherein the temperature compensation controller (21) is hardwired to the heating elements (22) and controls the heating elements in an analog fashion. 16. The system (20) recited in Claim 11 wherein the temperature compensation controller (21) controls the heating elements using a software algorithm. 17. The system (20) recited in Claim 11 wherein the heating elements (22) comprise thermo-foil heating elements (22). 18. The system (20) recited in Claim 11 wherein the heating elements (22) comprise embedded heating elements (22).

Inventors: HULL DAVID A, HULL, DAVID, A.
Applicants: RAYTHEON CO, RAYTHEON COMPANY
Application year: 2001
Main classification: G02B23
IPC codes: G02B23