milky way galaxy mysteries probed by u.c. laboratory at hat creek

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An experimental infrared video transmitter, capable of sending 20 simultaneous televi- sion ciiannels or 20,000 voice channels over line-of-sight distances on a single beam of intense infrared light. Heart of device is a tiny crystal of gallium arsenide, size of a pin- head mounted near bottom end of black rod seen through circular window, that gen- erates a modulated infrared light beam with an intensity up to 2,500 watts per square centimeter this gallium arsenide diode should be able to penetrate the ionized plasma sheath that builds up around a space capsule during re-entry in the atmos- phere. This new optical communication technique, if it can be suitably em- ployed, might make it possible to avoid the blackout that occurs during re-fentry when radio frequencies are used for communication. Gallium arsenide diodes which have thus far been operated have an active area only as big as the head of a com- mon pin and produce a peak light power output of 3 watts. Since these diodes radiate up to 2,500 watts per square cen- timeter, it is quite reasonable to expect th^t large diodes can be made with peak outputs of 15,000 watts or more. The high-quality video transmissions in May were made on the roof of Lin- coln Laboratory (a distance of about 275 feet). With a more refined but still relatively simple system for focussing and pointing the light beam, the present generator should produce a beam that can be received clearly and distinctly at a distance of 30 miles or more. Optical filters will permit operation in daylight. These gallium arsenide diodes are small and simple in appearance. They consist of a thin wafer of single-crystal gallium arsenide with a tiny spot of zinc difi'used into one surface, and two wires to which the electric input is connected. The input current supplies the operating power and also carries the signal to be transmitted. The modulated input cur- rent is converted directly into modulated infrared light output, by a process called "band-to-band recombination radiation." The diodes generate light at wave- lengths in the near infrared region of the optical spectrum, just beyond the red region of the visible light spectrum. The light is confined to a narrow band of wavelengths, only a few hundred ang- stroms wide, depending on the tempera- ture at which the diode is operated. (The lower the temperature, the narrower the spectrum, and the better the efficiency and power output.) To obtain optimum efficiency the present diodes are operated at a tem- perature of 77 Κ (about 370 degrees be- low zero Fahrenheit), which is the tem- perature of liquid nitrogen that is used to cool the container in which the diode operates. Milky Way Galaxy mysteries probed by U.C. Laboratory at Hat Creek The quietest (in terms of radio interfer- ence) accessible valley in Northern Cali- fornia, was chosen in 1959 for the Uni- versity of California's new Radio Astronomy Laboratory, which formally went into service in Hat Creek Valley, 20 miles north of Lassen Volcanic Na- tional Park in June of this year, and is now in full operation. With a pair of "ears" aimed at outer space, the laboratory is performing signi- ficiently in a broad program supported in large part by the Office of Naval Re- search. The program will seek answers to questions that have puzzled man for centuries: How are the stars formed? What "shape" is the universe? Is there life on other planets? In keeping with the University's educational role, the new facility will serve both instruction and re- search: graduate students in astronomy are at work on a research project along with U.C. faculty members and visiting scientists. The $1.2 million facility includes 33- foot and 85-foot telescope "dishes" cap- able of detecting radio waves from far beyond the limits of visual astronomy. They were designed, developed and built in Palo Alto by the Philco Corp., a sub- sidiary of the Ford Motor Co. The two sky-searching dishes—futuristic land- marks in the wilderness—are located 400 feet apart on an east-west base line; the two massive instruments are made up of thin aluminum reflectors mounted in aluminum and steel frames and sup- ported on steel towers. The large telescope weighs about 200 tons, stands 110 feet above the ground, and is built to withstand winds of up to 100 miles per hour. By means of re- motely controlled electric motor arives and large gears, the telescopes can be pointed at any spot in the sky and can track a radio source as the earth rotates. Adjacent to each telescope is a labora- tory building containing control instru- ments and sensitive, specially designed radio receivers. The receivers are con- nected to recording devices where the in- coming radio signals are traced as wavy lines on a moving paper strip. During the Laboratory's tuning-up period, the smaller telescope soon after it was erected mapped a portion of the northern Milky Way. This observation revealed new de- tails about the star-studded spiral arms of the whirling galaxy in which the sun is a minor star. In its initial tests, the 85-foot telescope recorded radio signals from deep within the galactic center—the hub of our island universe that is completely hidden from visual observation. The distribution ot Atop a portable elevator, technician makes adjustments on antenna horn at focus of U.C.'s new 85-foot steerahle radio telescope. Radio waves from space, reflected into the coaxial horn, travel to receivers in a nearby laboratory where they are recorc 756 ELECTRICAL ENGINEERING SEPTEMBER 1962

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Page 1: Milky way galaxy mysteries probed by U.C. Laboratory at Hat Creek

An experimental infrared video transmitter, capable of sending 20 simultaneous televi­sion ciiannels or 20,000 voice channels over line-of-sight distances on a single beam of intense infrared light. Heart of device is a tiny crystal of gallium arsenide, size of a pin-head mounted near bottom end of black rod seen through circular window, that gen­erates a modulated infrared light beam with an intensity up to 2,500 watts per square

centimeter

this ga l l i um a r sen ide d iode shou ld be ab le t o p e n e t r a t e the ionized p l a s m a shea th t h a t bui lds u p a r o u n d a space capsu le d u r i n g re -en t ry in the a t m o s ­p h e r e . T h i s n e w opt ical c o m m u n i c a t i o n t e chn ique , if it can be su i t ab ly e m ­p loyed , migh t m a k e it possible to avoid t he b l a c k o u t t h a t occur s d u r i n g re-fentry

w h e n r a d i o f requenc ies a r e used for c o m m u n i c a t i o n .

G a l l i u m a r sen ide d iodes w h i c h h a v e t hus far been o p e r a t e d h a v e an ac t ive a r ea on ly as big as t he h e a d of a c o m ­m o n pin a n d p r o d u c e a p e a k light p o w e r o u t p u t of 3 wa t t s . S ince these d iodes r a d i a t e u p to 2 ,500 wa t t s p e r s q u a r e cen­

t ime te r , it is qu i t e r e a s o n a b l e t o expec t th^ t l a r g e d iodes can be m a d e wi th p e a k o u t p u t s of 15,000 w a t t s o r m o r e .

T h e h igh -qua l i t y v ideo t r ansmi s s ions in M a y w e r e m a d e o n the roof of L in ­co ln L a b o r a t o r y ( a d i s t ance of a b o u t 275 feet). W i t h a m o r e refined bu t still re la t ive ly s imple sys tem for focuss ing a n d p o i n t i n g t h e l ight b e a m , the p r e sen t g e n e r a t o r shou ld p r o d u c e a b e a m tha t c a n be rece ived c lea r ly a n d dis t inct ly at a d i s t ance of 30 mi les o r m o r e . Opt ica l filters will p e r m i t o p e r a t i o n in day l igh t .

T h e s e ga l l i um a r sen ide d iodes a re smal l a n d s imple in a p p e a r a n c e . T h e y cons is t of a th in wafe r of s ingle-crys ta l ga l l i um a r sen ide wi th a t iny spot of z inc difi'used in to o n e su r face , and t w o wires to wh ich the e lec t r ic inpu t is c o n n e c t e d . T h e input c u r r e n t suppl ies the o p e r a t i n g p o w e r a n d a l so ca r r i e s t he signal t o be t r a n s m i t t e d . T h e m o d u l a t e d inpu t cur ­r en t is c o n v e r t e d d i rec t ly in to m o d u l a t e d inf ra red l ight o u t p u t , by a p rocess cal led " b a n d - t o - b a n d r e c o m b i n a t i o n r a d i a t i o n . "

T h e d iodes g e n e r a t e l ight at w a v e ­l eng ths in the n e a r in f ra red reg ion of t he op t ica l s p e c t r u m , just b e y o n d the red r eg ion of t he vis ible l ight s p e c t r u m . T h e l ight is conf ined to a n a r r o w b a n d of w a v e l e n g t h s , on ly a few h u n d r e d ang­s t r o m s wide , d e p e n d i n g o n the t e m p e r a ­t u r e at wh ich the d i o d e is o p e r a t e d . ( T h e lower the t e m p e r a t u r e , t he n a r r o w e r the s p e c t r u m , a n d the be t t e r the efficiency a n d p o w e r ou tpu t . )

T o o b t a i n o p t i m u m efficiency the p r e sen t d iodes a r e o p e r a t e d at a t e m ­p e r a t u r e of 77 Κ ( a b o u t 370 degrees be­low z e r o F a h r e n h e i t ) , w h i c h is t he t em­p e r a t u r e of l iquid n i t r ogen t h a t is used t o cool the c o n t a i n e r in w h i c h the d iode o p e r a t e s .

Milky W a y G a l a x y mysteries probed by U.C. Laboratory at Hat Creek

T h e quie tes t ( in t e r m s of r a d i o in ter fer ­e n c e ) access ib le val ley in N o r t h e r n C a l i ­forn ia , was chosen in 1959 for the U n i ­versi ty of Ca l i fo rn i a ' s new R a d i o A s t r o n o m y L a b o r a t o r y , wh ich f o r m a l l y wen t in to service in H a t C r e e k Va l l ey , 20 mi les n o r t h of Lassen V o l c a n i c N a ­t iona l P a r k in J u n e of this year , a n d is n o w in full o p e r a t i o n .

Wi th a pa i r of " e a r s " a i m e d at o u t e r space , the l a b o r a t o r y is p e r f o r m i n g signi-ficiently in a b r o a d p r o g r a m s u p p o r t e d in la rge p a r t by the Office of N a v a l R e ­search . T h e p r o g r a m will seek answer s to ques t ions tha t h a v e puzz led m a n for cen tu r i e s : H o w a re the s tars f o r m e d ? W h a t " s h a p e " is the un ive r se? Is t h e r e life on o t h e r p l ane t s? In keep ing wi th the Univers i ty ' s educa t i ona l ro le , the new facility will serve b o t h ins t ruc t ion and re ­s e a r c h : g r a d u a t e s tuden t s in a s t r o n o m y a re at w o r k on a r e sea rch projec t a long wi th U . C . facul ty m e m b e r s a n d visi t ing scient is ts .

T h e $1.2 mi l l ion facili ty inc ludes 3 3 -foot a n d 85-foot t e lescope " d i s h e s " c a p ­ab le of de tec t ing r a d i o waves f r o m far b e y o n d the l imits of visual a s t r o n o m y . T h e y w e r e des igned , deve loped and bui l t in P a l o A l t o by the P h i l c o C o r p . , a sub ­

s id iary of t h e F o r d M o t o r C o . T h e t w o sky - sea rch ing d i shes—fu tu r i s t i c l and ­m a r k s in the w i l d e r n e s s — a r e loca ted 400 feet a p a r t on an eas t -wes t base l ine ; t he t w o mass ive i n s t r u m e n t s a r e m a d e u p of th in a l u m i n u m reflectors m o u n t e d in a l u m i n u m a n d steel f r ames a n d sup­p o r t e d o n steel t ower s .

T h e la rge te lescope we ighs a b o u t 2 0 0 tons , s t a n d s 110 feet a b o v e the g r o u n d , and is bui l t to w i t h s t a n d w i n d s of u p to 100 mi les p e r h o u r . By m e a n s of r e ­m o t e l y con t ro l l ed e lec t r ic m o t o r a r ives and la rge gea r s , the te lescopes c a n be po in t ed at any spot in the sky a n d c a n t r ack a r a d i o sou rce as the e a r t h ro t a t e s .

Ad jacen t to each te lescope is a l a b o r a ­to ry bu i ld ing c o n t a i n i n g con t ro l ins t ru­m e n t s a n d sensi t ive , specia l ly des igned r a d i o rece ivers . T h e rece ivers a re con ­nec ted to r e c o r d i n g devices w h e r e the in­c o m i n g r a d i o s ignals a r e t r a c e d as w a v y l ines on a m o v i n g p a p e r s t r ip . D u r i n g the L a b o r a t o r y ' s t u n i n g - u p pe r iod , t h e sma l l e r t e lescope soon af ter it was e rec ted m a p p e d a p o r t i o n of the n o r t h e r n Mi lky W a y . T h i s o b s e r v a t i o n r evea l ed n e w de ­tai ls a b o u t t he s t a r - s tudded spira l a r m s of t he wh i r l i ng g a l a x y in w h i c h t h e sun is a m i n o r s tar .

In its init ial tes ts , the 85-foot t e l escope r e c o r d e d r a d i o s ignals f r o m d e e p wi th in t he ga lac t ic c e n t e r — t h e h u b of o u r i s land un ive r se t ha t is c o m p l e t e l y h i d d e n f rom visua l o b s e r v a t i o n . T h e d i s t r i bu t ion o t

Atop a portable elevator, technician makes adjustments on antenna horn at focus of U.C.'s new 85-foot steerahle radio telescope. Radio waves from space, reflected into the coaxial horn, travel to receivers in a nearby laboratory where

they are recorc

756 E L E C T R I C A L E N G I N E E R I N G S E P T E M B E R 1962

Page 2: Milky way galaxy mysteries probed by U.C. Laboratory at Hat Creek

Construction scene: workmen place the 4-legged ''feed" into the 6,000-square-foot re­flector dish for radio telescope, now in operation at Hat Creek, Calif. Earlier, the re­

flector itself was hoisted onto its tower the same way

gaseous m a t e r i a l in t h e g a l a x y a n d t h e m o t i o n s of th is m a t e r i a l will be of g rea t in teres t to scient is ts e n g a g e d in t he s t udy . " F r o m the s tudy of these aspec t s of t h e gas we h o p e t o l e a r n m o r e a b o u t t h e s t n i c t o e a n d d y n a m i c s of the ga l axy , a n d a b o u t t he w a y it c h a n g e s wi th t i m e , " D r . H a r o l d W e a v e r , a Berke ley a s t r o n o ­m e r , says .

T h e first o b s e r v i n g p r o g r a m wi th t he 33 - foo l t e l e scope h a s a l r e a d y p r o d u c e d a sky m a p of t he n o r t h e r n M i l k y W a y s b o w i ^ . the p a t t e r n of t h e r m a l r a d i a t i o n arisfrig f r o m h y d r o g e n gas . F r o m th is m a p t h e a s t r o n o m e r s will d e d u c e t h e d i s ­t r i bu t i on of ion ized h y d r o g e n — k n o w n to

be a s soc ia t ed wi th ho t , b r i g h t s t a r s — a n d will t r a c e t h e p a t t e r n of t hese s t a r s in t h e spi ra l a r m s of the ga l axy .

S tud ies of the ga l ac t i c c e n t e r s a r e be ­ing m a d e a t t w o r a d i o f r e q u e n c i e s : a t 8 ,000 m c the t e l e scope p r o v i d e s a c l ea r ly defined p i c tu r e of t he gas in the n u c l e u s as seen p r o j e c t e d aga ins t t he sky ; a n d at 1,420 m c it r evea l s i n f o r m a t i o n o n t h e m o t i o n s of t he gas .

R a d i o a s t r o n o m y , a y o u n g a n d p r e ­coc ious sc ience , h a s b e g u n t o ske t ch t h e first a c c u r a t e p i c t u r e of t h e M i l k y W a y : it h a s focused o n severa l s u p e r n o v a e , t h e g i an t r e m n a n t s of e x p l o d i n g s t a r s , a n d e x p l a i n e d the i r i n t ense r a d i a t i o n in t e r m s

of a n e l e c t r o n - a c c e l e r a t i n g " c y c l o t r o n " effect; it h a s p e e r e d in to t h e cen t e r of t he ga l axy , t he r e g i o n h i d d e n t o op t i ca l t e l escopes , a n d has b e g u n t o d e v e l o p in­f o r m a t i o n o n the ga lac t i c c i r c u l a t i o n of m a t t e r ; it ha s d e t e c t e d a pa i r of ga laxies in co l l i s ion ; a n d has l i s t e n e d — s o far w i t h o u t s u c c e s s — f o r messages f r o m u n ­k n o w n c iv i l i za t ion o n s o m e d i s t an t p l ane t .

C l o s e r to h o m e , it has inc reased m a n ' s k n o w l e d g e of t h e sun , t he m o o n , a n d n e i g h b o r i n g p l a n e t s in the so la r sys tem, i n c l u d i n g a n e w e s t i m a t e of t h e sur face t e m p e r a t u r e of V e n u s w h i c h is expec t ed t o be of g r ea t v a l u e in fu tu re space ex­p l o r a t i o n . It ha s a l so p i o n e e r e d a n e w s y s t e m of ce les t ia l n a v i g a t i o n ( t h e r a d i o s e x t a n t ) t h a t c a n be used t o guide m a r i n e r s a n d i n t e r c o n t i n e n t a l rocke t s .

E l e c t r o m a g n e t i c w a v e s of every l eng th a r e p r o b a b l y t r a v e l i n g t h r o u g h o u t e r s p a c e ; t h o s e t h a t r e a c h the e a r t h en te r t h r o u g h t w o " w i n d o w s " ; t he n a r r o w o p ­t ical w i n d o w t h a t a l lows us t o see t h e l ight of ce les t ia l ob jec ts , a n d the m u c h b r o a d e r r a d i o w i n d o w o p e n to waves in t h e t e lev i s ion a n d p a r t s of t he m i c r o w a v e a n d s h o r t - w a v e r a d i o f r equenc ies ( f r o m a b o u t Vi i nch t o 100 feet l o n g ) . In s im­plified o u t l i n e , r a d i o a s t r o n o m y can be c o m p a r e d t o a c o m b i n a t i o n of opt ica l a s t r o n o m y a n d t h e n o w fami l i a r h o m e r e c e p t i o n of r a d i o o r te lev is ion s ignals . T h e p a r a b o l i c d i sh , o r o t h e r type of re ­flector, se rves t o focus t he waves f rom a p rec i se spo t in the sky o n t o the a n t e n n a , in t h e s a m e w a y t h a t op t i ca l t e l e scope re ­flectors focus r a y s of l ight .

B o r n of e l ec t ron i c s a n d b r ing ing a f resh a p p r o a c h t o a n o ld sc ience , r a d i o a s t r o n o m y h a s o n l y b e g u n to s h o w its full a p p r o a c h t o capab i l i t i e s in e x p a n d ­ing m a n ' s k n o w l e d g e of the un ive r se .

O t h e r O N R - s p o n s o r e d pro jec t s inc lude a n 85- foot r a d i o t e l e scope o p e r a t e d by t h e U n i v e r s i t y of M i c h i g a n ; o n e at O w e n s Va l l ey , Calif . , o p e r a t e d by t h e C a l i f o r n i a In s t i t u t e of T e c h n o l o g y ; a n d o n e n e a r D a n v i l l e , 111. T h e H a t C r e e k p ro j ec t is o n e of o u r l a rges t .

Lasers advance in accuracy of detecting motion: improve in power A grea t a d v a n c e in t h e a c c u r a c y of d e ­tec t ing a n d m e a s u r i n g m o t i o n h a s b e e n m a d e by a laser d o p p l e r r a d a r m o d e l , a n d a t e c h n i q u e is n o w used for mu l t i ­p ly ing the p o w e r of a laser , a c c o r d i n g t o r ecen t a n n o u n c e m e n t s .

LASER D O P P L E R R A D A R

Feas ib i l i ty of a laser d o p p l e r r a d a r t h a t can de tec t a n d m e a s u r e m o t i o n 10 ,000 t imes m o r e a c c u r a t e l y t h a n the bes t m i ­c r o w a v e sys tems k n o w n has been d e m o n ­s t ra ted by the S p e r r y G y r o s c o p e C o m ­p a n y .

A w o r k i n g l a b o r a t o r y m o d e l e m p l o y ­ing a m o v a b l e m i r r o r as a t a r g e t h a s s h o w n t h a t a r a d a r c a n m e a s u r e ve loc i ty wi th equa l a n d a b s o l u t e p rec i s ion f r o m orb i t a l inject ion speeds of 5 mi l e s p e r second all t h e w a y d o w n to a v i r t ua l s t o p — l e s s t h a n o n e t e n - t h o u s a n d t h of an inch p e r second . Such a r a d a r s h o w s p r o m i s e for b r o a d use as a space veh ic l e

r e n d e z v o u s a id a n d for t r a c k i n g miss i les a n d sa te l l i tes .

M i c r o w a v e d o p p l e r e c h o e s a r e a c c u ­r a t e o n l y at h igh r a d a r - t o - t a r g e t ve loc i ­t ies . B u t a l a se r d o p p l e r r a d a r o p e r a t i n g at a f r e q u e n c y of h u n d r e d s of t r i l l ions of cycles p e r s e c o n d c a n eas i ly d e t e c t a n d m e a s u r e t he d o p p l e r shift p r o d u c e d by a veh ic le edg ing u p to a s p a c e s t a t ion even at a smal l f r ac t ion of a n inch p e r s econd . A c o n t r o l s y s t e m e m p l o y i n g a s ignal o u t p u t of th is p r ec i s ion w o u l d a l l ow a sh ip to d o c k as l ight ly as a f ea the r . It is sa id t o b e t he first dev ice of its k ind .

A l s o , t h e phys ica l d i v e r g e n c e of a l aser b e a m , m u c h n a r r o w e r t h a n t h e s p r e a d of m i c r o w a v e e n e r g y , w o u l d p u t a g r e a t e r p r o p o r t i o n of t h e t r a n s m i t t e d e n e r g y d i rec t ly o n the t a r g e t s t a t i on as the space sh ip e n t e r e d its l a n d i n g p a t t e r n t h o u s a n d s of mi les f r o m t o u c h d o w n .

S p e r r y ' s m o d e l uses a n e w h e l i u m -

n e o n c o n t i n u o u s w a v e gas laser . A m o d i ­fied M i c h e l s o n i n t e r f e r o m e t e r spli ts t he l a s e r o u t p u t in t w o . ha l f def lect ing 9 0 d e g r e e s t o b o u n c e off a s t a t i o n a r y m i r r o r a n d the o t h e r ha l f pa s s ing s t r a igh t t h r o u g h t o reflect off a m o v a b l e t a r g e t m i r r o r . T h e l ight f r o m the s t a t i o n a r y m i r r o r c o m e s b a c k t h r o u g h the b e a m sp l i t t e r a n d is de t ec t ed by a p h o t o m u l t i -p l ie r t u b e . T h e b e a m f rom t h e t a r g e t m i r r o r is deflected b a c k off the b e a m sp l i t t e r a t 9 0 d e g r e e s a n d a l so h i t s t h e p h o t o t u b e .

W i t h t h e t a r g e t m o t i o n l e s s , t h e t w o b e a m s s t r ike t he p h o t o m u l t i p l i e r at t he s a m e f r e q u e n c y . But m o v e m e n t of t h e t a r g e t p r o d u c e s a d o p p l e r shift b e t w e e n t h e d e t e c t e d b e a m s — a f r e q u e n c y shift s o m e 10 ,000 t imes s h a r p e r in r e s o l u t i o n t h a n a m i c r o w a v e shift .

E N E R G Y C O N C E N T R A T I O N

A n e w t e c h n i q u e for c o n c e n t r a t i n g t he e n e r g y of a l a se r t o m u l t i p l y its ins tan­t a n e o u s p o w e r as m u c h as 1,000 t imes h a s been d e v e l o p e d by G e n e r a l D y n a m i c s C o r p . By the s a m e m o d u l a t i o n m e t h o d , a l a se r b e a m h a s a l so b e e n swi tched

S E P T E M B E R 1962 · E L E C T R I C A L E N G I N E E R I N G 757