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I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

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Page 1: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

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Page 2: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

310

APPENDIX A

APERTURE SYNTHESIS

The method of interferometric aperture synthesis is

best understood by first considering the analogy with the

single-dish telescope. The voltage V produced at the horn

of this telescope by an element of .area of the dish dudv

due to radiation at frequency w from an element of sky

dxdy may be written as.

i [t+{-(x,y,t)] i2n[U.(X-x 0 ).+V(Y-y

V(u,v,x,y,t)=V(x,y)W(u,v)e e

where-the telescope is -pointed at (x%0, y ), u and v are

measured in wavelengths, is a random function which

varies rapidly in all coordinates, and W is a weighting

function which accounts for taper introduced by the horn

and which is zero outside the dish area. The total

voltage at the horn is the integral of this voltage over

the dish and the sky. This voltage is then detected by a

system which responds to the time average of the power.

Thus

Page 3: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

311

R(x0 , y0) =

co ' oo • o.002 2r% ~S] dudvJ du'dv' dxdy 'dx'dy' T (x,y)

T(x',y)W(u,v)W (uv)exp[ 2i u(x x)-u'(x'-x0 )+v( y0)

-v (y' -y0) (-exp .il( (x, y 't.) - (x', ty.',t

where we introduce the brightness temperature of the sky

2T(x, y), where T(x, y) is proportional to V2(x, y). Since

i(x,yt)-g(x',y',t)]

2(e )= 6(x-x' y -y)

by our assumption of a random noise signal, the response

simplifies to

R y ) sfoou c -2Ti[(u-u')x +(v-v')y

R (x = 4dud fdu'dv'e 0

0 0• 0

W(u, v) W(u' , v')

.00

x f dxdy T(x,y)ei2n [(u-u' )x+ (v-v' )y]

(A-1)

F.

Page 4: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

312

Transforming coordinates we obtain finally

00 -2ni(ux04yR(x 0 ,y.0 = ) dudV F(u,v)A(u,v)e

-oo

(A-2)unc in-i.*d,.ied a

where the complex fringe visibility function is defined as

2C i2rr (ux,+vy)F(u,v) 2 dxdy T(x,y)ei uv

and the autocorrelation of the weighting function is

co

A(u,v) f du'dv' W(u+u', v+v') W(u',v').

-co

Thus, the single dish responds to the Fourier transform of

the visibility function weighted by a sampling function.

Let us now consider the standard sampling theorem

(Bracewell 1958). We sample the visibility function at

regular intervals in u of 1/2 xc and v of 1/2 yc The

sampled visibility function may be written as

2V' (u,v) = III(2x mAu, 2y nAv) V(u,v)

c c

where the III (sha) function is defined as

S2- 00c co 2iII(xy) = 0 Z 6 (x-p, y-v).

If we Fourier transform the sampled visibility function we

obtain a map given by

- j'!M

Page 5: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

313

2R(x, y) = 2III(x/2x, y/2y) * T(x, y)c c

where.. T(x, y) is the true brightness distribution and *

denotes a convolution. In other words, we now have -the

desired map repeated at intervals of 2x in x and 2y in

y. If

T(x, y) = 0 for jxj > x c or yl >yC ..

then the repetition does not cause the maps to overlap and

hence causes no error. Therefore, we must sample the

visibility function at intervals smaller than the inverse

diameter of the .source be ng observed.

Since this sampling interval is about 400 feet (for

the sources in this program at 21 cm) which is larger than

the diameter of almost all single-dish telescopes, .. ' all

information collected by the elements of a single dish is

redundant for such sources... We may remove this redundancy

or lack of resolution at reasonable cost if we sacrifice

collecting area. We use one small -telescope as the central

surface element of the aperture to be synthesized while

another movable telescope provides other surface elements

of the synthesized aperture (Figure Al). If the voltages

Page 6: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

314

Ni

D

Figure Al. Geometry of two-element interferometer.

P

North South

Figure A2. Celestial sphere with source (Q) and pole ofbaseline (B) .

Page 7: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

.'315

from .the two telescopes are multiplied together and

smoothed the output is2 iT(x, y) ( )

R(x, y) = V e (A-3)0

2nDwhere T(x, y) =-y sino(x,y) and V0 is the voltage pro-

duced by the source at each telescope. As the earth

rotates, sinG varies producing an approximately sinusoidal

output called fringes. The phase T may be expanded about

some angle 9 as0

2nD 2nD

T = sine + cost AG (A-4)

where 'the first term is the "expected fringe" which is

removed during reduction .and the second term is the "fringe

phase". For an extended source, the total response of the

interferometer is just the integral of the separate

responses of equation (A-3) to produce

or i2T (ux+vy)R(u,v) = JJ dxdy T(x,y)e

where the expected fringe has been removed and the phase

s cosO a.g has been expressed in rectangular coordinates.x 0

In other words, the interferometer directly measures the

visibility function.

Page 8: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

316

The formulae for sin9 0 , u, and v may be derived as

follows. The three points indicated on the celestial

sphere in Figure A2 are the north celestial pole P, the

pole of the extended baseline B and the source .Q. The

hour angle and declination of the source are h and 6,..

respectively, while the corresponding quantities for the

baseline are H and A. The angle between Q and B is r/2-.-G

The law of cosines is used on the triangle PQB to give..

sinG = sinbsinA + cosbcosAcos (h-H) .

The projection of the baseline along constant longitude is

D .asinG D

S n cososin--sincosAcos•(h--H)

.and the projection of the baseline alongs constant latitude

u .D_1 D n - cos6sin(h-H).

Xcos6 ,h

The choice of signs for u and v is a matter of convention

while the factor (l/cosb) enters the equation for u so that

x may be expressed in units of angle rather than time. As

the source changes hour angle, the values of u and v describe

an ellipse in the (u, v) plane. To fully sample the visi-

bility function, we observe the source through the

I- -

Page 9: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

317

available range of hour angle at a number of discrete

antenna separations D.

The Hermitian property of the .. visibility function

is quite useful and easily derived. Since the visibility

function and the source brightness are a Fourier-transform

pair we may write

• co. -i2m (ux+vy)

T(x, y) =. dudv V(u,v)e

Writing the visibility function as the sum of a real and

imaginary part we obtain ..the imaginary part of T as

Im(T(x, y)) =

y _.

cooa f dudv[I(uv)cos2n(ux+vy)-R(uiv)sin2n(ux+vy)]

Since this must be zero we may use the symmetry properties

of sines and cosines and the independence of R and I to

show that

1.(u, v) = R(-u, -v)

I(u, v) = - I(-u, -v)or

V(u, v) = V*(-u, -v) .

Therefore we need sample the visibility function over only

one-half of the (u, v) plane. This formalism is only a

more elegant way to express the fact that the only

Page 10: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

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Page 11: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

(a)

(C)

(e)

OUT

Figure A-I. Receiver Logic

A. A-2

2

(a')

(C')

(e1')(e')

Page 12: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

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.. C..442 . .z/~tc44

Page 13: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

3

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C 14C,

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::... ....1_...... --¢ , ,... .... _ _ .0 yC c _(ltr jJ/ ...ZLJZY....A :: _ :__ _... -Z -__t .-/ ....... hF __ ttA+...%/c.. ..t....

Page 14: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

499

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-- - - Ycs~z t~ta( 2 t-~ I~iAz )tt9IF

•T .,t .-.. 1r)% .(r.tc~ (tz'-tr~

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..Z 4 4 . . - .- .~

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. .'. -:b .-- , .~ . Q • . ...r

, .--- - - - - -

Page 15: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

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Page 16: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

6

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Page 17: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

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-_ . _ ,t,

LP L- V ii~, i 1-IL S.~' G LJ~.zsi

-- -- . ,C.trO cx-46r2 7 .

-d_ .t .-9taz9 , ~'ct~ pc) " 7 A-t-t-t&

_.. .. z -/cc -

/ .fl.

-- " ~ -a'a, _

- 7 ~ L; --z; - --

.. .... .. ............- " ., -.. ̂ ..... ~_. ..... .. ..... . .. :. ....-.- . I .-. . _... ..... _._.... . ..-.................. .

- IP . , ".... . * 6 .c ..... .

• - .t ; i... . . .AX/ .3/-- *-I-l •CT _ .-_-- C.- .....I

-... . .~-~ -__ _~. .~;~ ;..._1__ _ _s. , .. ~~J

. ........ :.-- -- 1--- - --- .......... .- ......................... I----.,~-. ~ ,~ -~,,.. __.

_G....2 ... . 'f -...."t l/ __._- -.,---.-~--.Y'" ~ ri C12rZ....... ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ,. "I,.._ . ... . ....-......... ".......... "............. ' ':" ...... L.

...--- -"-- : ." ~~~T~ _~~

S....._~. ...-. ........ _- ................- _ ._...... .._.. . " ~ "., _ ., .. . . . _ . . ., , _ _ . . .. _ , ... .. .. .; .. ..L :... . . ....: : _.:...:. . . ..,... . . .. .... .."... ... ;. _ :.. . . .... .. ....... ;,. ...... ... .:

•.. ,I s . /~ c " .j~R CP "~ ' - " "i . -i " ' ' . .

~ ,..~r-:~ __~_ _~~_--- ------ ------- ~...a.--- _ -~ ~ ;..~~~. ~ .- -- ,-- . - -.---. i.

•s .- , . . . . . . , .- -- - - - -~-.-..-~....~~.... l -- ~-"--~-- - -- - - - ---- -- -

........................--......., p.... -.. f.... , , ... .., ....... ......y' ..........,.«..#.... . -._._... ._....._,. .-....... w._.i.... . : M . • " ..... '.._

• • • ' ,~ - 2-Tu,- "~ r- : "~ iL~~FII~ .""- '- " -~ • '."-- .... -D , .------- ,- .-, .,_ >~ .*- .-, . ../ .^~_.._ ,, -: , .zr .. i . .-l

* , xA/IUCZZ COA' ) " : . .. "...-ro..

j.,..C T CtA. / I . . , • . .. ... . .-

.. - ....... ....P .X A. ~-~pjzrk,4

Z"... ...•~~-~ . - ....

Page 18: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

_.C..>.J J v A.-k,J./t

- • &... . . . .... .

_ _ _ _ I ) -a -.. . . .-__ __ __ _ _ _

.-. ' - '-" -- -.- _ _ _ " _ - " ._ . - . " " . .

-__ ,. _ J.fQ .c&.

"_ ._-- .&.Z/c 1 'cnQa ~2 -- _-

Mm .- 0 .

' . .~' A'.

•- --. -- i.c -..... 9~zu4 . 4.z, t~s~v __S

•el.

- _A.

_ /t ~ w Lt V ..__ ~ &&w . - ~ -.... ir t-. . - /4..>~ L c>c& Zrt

-- ._..__M.._.._,...._.... ......_._._..a_... ...... .. ,... .. _.,... .>. . ... ._....,_.. .w,. .:.:a.....,,.,.._. ,., .ww.W..... .,,.,.._... .... ; ....,...... .y...--,._...:r__. .<..,.._... .. ,.,.,, .. , ,.r_....,...w__._a :,..._._.......;w.r..,_... a,._...._._....v::_., ......:.. ...... ........:....._:r._

.r,....,,.. .a.. .. _...__nM......_.._.,...... ._.._.,..:.r...w...,..._,. .,..,..._..._.._ .. _.._

-_._... .. _..,.._.............._._,_.._.,.._.. .. _.__..rr. __......., .rw....w..,.v...... ....._ ._,..._._._,_ . . ....... Y.._ ._.. ,_ ..... r. ........... wr..,:...a ... M........,....._,.rr...,.,..a_...__..... ... .. ......,a....... :. ... .. ,_.. a.,_.......__..._..._..__

....wiw....a.....a.... r+. ........... e.,..w. .r.......a..w........ ... -. rv ... W...wv..+ver.. -....winrW n,.- .. w.....4. . w...u.,u e.4a s rk .. wrM.w _ w nn.r< ... w..a.....,wai.r axw... .-..s..nwrt"am..v.ros.a ......w.....ra.,.n...e-....rww . .. w ... wrrwn"+. .v+. .. r...w..>.as"w+-w..Fr.........nrw.e.... .........+....r.q. ,. r. .. .n....

Page 19: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

• . .. .

c.. , . st.. I- . .

-'S . . -.

_ . . .- t .1t .-- r i L W 4Cc;rt.*;

,.. .... . .

. A . t,.. 4Zi . - - -...

__ :-i_..., __ <,.. _-:- Ld I. _ _!p J._P _. FL_..• .<.r ". .!2 ,.• - -. . - -...... ': -L ; I ... .. . .. . .7/ .... ... . - " .. 2_ ; : :- . . ... ... ...... i - .. . .: --- . .. . . .... ... ..- - - .... .. ." ..... .. .: --. ...". ... -. .. ..-.7 ::.... . . .. .. ... " -... ..

" - A a At" '>

- "tn £r4t- -i &tt&t r~_._ V~ 6 a) t) c_ ~ r B°ct a__ _____

.... _ ..... " '. . i ' . ': " . , . V . .. . - .• & & t .1 ~td />1v V

-- - - --- -- -

- . -.-... .Z.. . .. : .iL •Z--CC -k c- (c z ,4 xa /r .A. ) §...........•. , .. /. - .C - - ,

/2. cwt " - ILt •w~i tt4L r. . - ' V -~ € . " / . 4 PZ" , ->J

.. _ . , .Z _ ..... ___... _ _ l__.,_ ._._. _ - .... --l-(_ ~ ~--I L. _ - _.. .- _ ...J..~__- .-- - -,..- .,_ .I_t..5 Ci..._..-~--.- , :.-I.__ ;_ _ _ ... V '--.-.-~~ ~ . _ ll. .... . .. 111II-. I .... ..... .. _. :, . •'.I ".~ ~'~. ~ L.--.- ~-- - ------ _-_^---- 1.-I-- I ~--L i- -- ------ --. ---^--iI- C-

+ • • " . . . " " " " • " . ..... . ..... : . . . . .. -i' _:.L _L. . . ...... _ ....... . . .. . . .. .......... .. .. % . . ......... . . ..... . ......... .. .. .. .

......... .- .. . . . ..... . ... .. _ _,.. ..... . ...... ,.- .- ;- -, . .. ... -. r I...

;"~c ......

•C~~ ~ .! , • ~I~Iacf~?.. _c ,~-- -~ . . ' " " :I "

• ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ r •.I . .. .. : i. ' - • " " " . .',,' - ... . " ".................................---. --. -- : ...... '-c -I . .--- ;.-. - --- .- -.... .... ., ...... _... : .... , ... ... .

.. f . . . . ,. " , . . . ...a/ r /, - g .--- • _ (.7/ / ., .r > $. -, , -A). .. . t- . ... L-.. .- w~' o-.--zn• - "&d.~ /I ~ f

S,- ... " . . ' . - ... <- - , ,

I-I- - -I------ - - c%'3.Z t4L4.. Ct~"tt~tuO - -L (trZ - 2 -/9.50 h t$.Zf Y

.-t %c. t..t - -L l , c- J~ ., ,- C t... . ,, tt

.. c. '%&- f .. - ',- " c ..cf. jUI / .-.- .... 4 A". ... A /Q. r -.

Page 20: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

. ... / -.

r•

--.~

. .. . ....

-.- ,---, i

...

_~~~~s~- ---- S4 7 t 717& IJ7- t2L -- -- -

..-_ _,. ,- Z +c- t zZ 2 n C rt 4 .Yc r .t~ s . - . . ,.. ,

__-l ~i- c I- 4cP"L /c&aczAe rcc -IAetLt c~J ,a

.. ,c. ,... .A. (-c .1./Z.. .t & - .

.. . .- , < C. . . 7 / . . - • ,

. - , - --- -.- - .-

---- &rt,-t- v-(4'Q e. /_ ZS,(L-..$r+ A, , X -

It Ii-,r-j rr -

•~~~~~ . </_ ... . .. ...

~Z~y ~-t 4 ~..gt ,C/--

. . .. . .... -L.

. . .,- . ... - r -- , --.- -- ---- .. .

-"_ 7Z 4CAA" 424" y -- . .... " 27t :A.t----- -• . ---------. .~ . ..

. f l- " . .- ,

;.___ _ Q

__ _'~7~'" C~;-I------ A--I _:~c ->_C ZI - - ---

_ _ - -Z±~ ,<.

• .y i t .t t, /•-jI 4 .tr 7/ .ti..

-. ,...I -._, __ ,,I~- .--

~ .

. . .• ,

d . • , , , - .

.ro .t .. - ---- - -I- ---- ---- 1 1-- - - . •L^-l -

... ... . .. . ... . .. ... . ..... .... ... ... ... ... ... . . . ... .. . - . . . .. .. . . . ... . . .. . .. , . _ , .. ... £. .. .. .. ,._ __ .. , '= ";.. . . . . . . . , _.. .

• .-,~~.-- .. ..-_.......-*-L--II

.t~i~- X ;lef~~~q:_r_ _

• -... L.

IW~~I ------,,,,. ----__ ~ -~' ---- lc.~~.,-s ---.,.. *-., ~ - - - - - - - ---- -- --- ------

- -- - ----- ,rJ a

- II

Page 21: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

- at n , ~ 6-iicLcv- •-- -. t.- r .. i - : .- t. . 6 "4 .

- .~ . •-& . i-e -c.c-rt .~

A , . A. .# .,-

) .tt {f '. ) , zs- c Ztn t cc .x'ct /4

C~~ "

-- 7/ -/ _pig

w. .

............. T---].-.. ................... •~~ .al~~e ~ cj~ 1 ~ IZ ~~

S . ,-P . . 2/t4 .....4.t..2

.C' Z L- t.2 r C( IC

.. ~oL C.. . ...

- - - -- . . W v).) m6%•o) .

A - - --- - . . -

-- ~- ..-- -I~ At ft-K CWZ4 A>4A&-~-~ I-Z-Z. t....... ./ ---3 Yj4to . p. . . ". -xi. . -.... .. ... U ; c ,it,, .. ~"---i-.- ",l-'- t"-- ------ , - .--.- Y - - J ._ 1. ..... ..........l---L - " ............. .... ... .... , ......., _ ./ ..:_. .,.+ -, .. ., ..... , ., .__ .... . . ... ...... _ ...... . ... ........ ...... ......, .

... .........- -- --. -.-.... -.. .... --.. . . -. , -n . UI...~. --. ~--.. , ,.--... . ._...- , ., ._ '..-I-.- "- -i.-~ --..1- --I-.-- I ------ ". -- .--....-- , _ .:r----- o-# ., ., •- --^1- ... ... ..

Page 22: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

-1800 -900

+370

X

XX' "

CL

u 0>

0C

I-

2:

124

U - WARVELENGTHSn

t A .I Jt

x # P X

XXX

X XxyX

xCxC

xCxC

xC

x

X

x

xC

xx

x

X

XX

xxx

XXX

'x

x'Cxxi

x xx X

x X

xx

x)x xX

XX

XX X

XXX

Xx

-1800 -900 900 1800U - WAVELENGTHS

Figure 16. 3C461, continuum frequency shift: distri-bution of data points.

Qannf I mnn"

Xx

Sxx

X

xx

X

xX

x

'Cxx

'xxX

x

C)

CCon

0)

tf)

I-

Li~1-~ 1

a:c

SI

C

XX

x'..

kt

1- ---- - - - - .% a -L _~_ I

- L 11_~~_? I -. -- ---

xx

,

\i

1.

T-I -I,

Page 23: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

125

MINUTES OF ARC

U

cc

cC-E3

(-

ZZ

MINUTES OF ARC

Figure 17a. 3C461, continuum frequency shift: dirtybeam pattern, contour interval = 10%, largearea.

U)ccCL

L

H

Page 24: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

-8 -i 0 L 8MINUTES OF ARC

8

4

U

OCcc

LI-

C

LU1--

0

-8

t.

3

.

.

t

Page 25: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

- . .. .) A. . -.. 4t .4

.. _. I . . .. • . .. .. ,. .~. . . ' .. ,. • .

, -. .- .Y .t.. ..Y&..CI

- - I , , . . . . - .,. *.. " . . ._.. 1_.;_... _._.._.__ ~ _. ~ _..- _. . , ... .. .. , . , , .._~

--; .Q). . . -r .t4CdJ_ 4 .ttatztj c .., s . ___

. .,-,. .. ..-- , . . . o . . ..... ... . . . .... .......-- ~1--~ . ... . , . •;~.~

-. c.y LttA.~t D ' Z . ., ,

..- . , U . : ..-

T'4 t') _77 5 (1r.t&t YryiXtIYCL.,.- -- -- CI-L -i -)L-)-- -li -- 7 -- Ls -

,.- - .0T, .4C 4/2.2 A . .z4 ..

aj tt,4 . - _ /4

-- -- - - - kL~wa ~ ... ,../7./.r #_ , ~ < tstt

7/t /~__SL___C z/

- - ___- -- 5' 74 .7? ~ ~

.., . , - - - - 4 /e. - - / - &O.fc - - z - & _c & .- " ' ., ., -/ - - _ rt icv " - 4?/- ....- -, ." .'

t. t. clc A w / .A t . ..r t §2 a /i ', .i-i

__.-•4 A , - z . ~ C . . ,

- /tt.'- ---.. - - - -., - - " ' " -. :." .. -,4 Sy -.4-Lc-"y ./z- . . . .• -- . . .. . •. : . .. .- ~T _ :P ~ ..... ~ -: ............... --. ............ .....

- a . - . .

• - . . . . -.- '. . . . . . . , . . .... " . -__ , . ..... .,,-- .--'* " # ' " " l " ' " """ fZ

o .-. ....." .. ........ ... ... .-.....•. .... ............. ....%. . . . .. ... .... ... .... __._... .. .. .... ..

.. .... ... .. ... .. .. ... . :. .... : .. . . . ..:. . ... . ." -. ..... . . . .. .. . ... ... . . .. .. . . . .- . -...: .. . .. .. .. . ... . ..-. ....------ --------- -- ..

S. - ; /. - ' -A-"A 'P !/ . , x • o. • . , f --..- •- C i .A \ A . .-- Z4. ..,__C-. . .,,g..:. . I /{ .t. . - T . .tt, .vt cr-,.

, Prt. " "- '- >2 " -,, - --- - I - -

(... ±-.,. _ . 779il , t . -" . -t -r'--. •r .. -.. " $4 ct- .

- ' -- . " C «. - i("..g~. J.t ' ->.Z . % /- cUt44"wt. . ...

- - 'u.t/tritt .. Zt</ttt ti - ,4 " .- ." - - -- . - • -- - .- . . -. -

....... ....... ....._. ... ...:< .<_ -'+ ..... -' - " " ": --. .<. .+- ,_.i... ...... ;......, ...... ... ................ = ......... .....-__ ........-__._ ....... .........;.__._.......:.. ....." .... .... ..... ....._ ...

Page 26: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

f r f

8 o-- -( *

0 0-

-. ..

.. .'. . . , :.

" .( I

$1 t N

cc I,/,.

; "

-

- I II I% K.

.t .

. . : . •

\\. ' . .

( .

-a -I 0 41 8MINUlTES O~F RC

'-..'. .

,/, ')" .I .

_.,-8 -11 0 " 4 "8 :J ( /]MINUTES •O" RHO

Page 27: I'-' -4 t6 / -4 . · 316 The formulae for sin9 0, u, and v may be derived as follows. The three points indicated on the celestial sphere in Figure A2 are the north celestial pole

/1; ~Y

4.

r ''

<Jf ,A-t . • , ,- sj

--- - . - CL - -- g-t{4-CC- cgi A> ri-d 4&- - 4.- -et .

- t .- c>:w to /-

-- - -- t&') .zatctc~,L -. ~ -j~ fadC_ _ -e~ ~ ' '--

*~&s .. -tFs.- -- >t- < - an. Az ~

- -""v~ _ t~ r ~ - t -c -c-c-t --- ~ cc ~ r T (n~ -i- 1/a /0z C I- 1-__ --- -I - ----̂ -- --

O*Lue-~~~k. _. . t . F,,z.... P_., -"t " " ..

-- -- ---- -- - ± _ _---

,.-. IV1YVLII1-Q 7t : - . .

I.-..- il..-I-.-..~~~. -..~ -.---~... I .1 . .' .."- =--~-- I , -. -r -. l " ...... ..-- --- - ---- .-- ~ r3 - .~--.~. - - - ---

_ _ I

- - - ----- - ------ --- ---- * *-.~ ~"- - A - - - - -- -

._ _..: _,. . .. _ . ._. _._. _ w .__._ _._..4_ _...__.. ._ _ _ _._ ____. _ _._ __.__._.__ _.1-~-

---r ^--- -. ---I ̂ .- --------~

.. __._ r~ ~----- -- I-- __ ----- .-- --- -

-- ----- -- -- ---~----~ ------- ~- ~- -------~- -~~-~--- ---- ----- -------- ---------- ----- -

-- ---~--

----~--- -~- -~-~~--~- ----- -~- -- ----~- ~--------~--- ----- -------------------~~-~-- -- ~------ ~- -~ -- --~- ----- ------- -~ --------- --~-- ~~----- ~--- --~--- --~ ~--~-~-- -~----~-- ------------ -

II

"~"~' '~~"

~-"-"~~ ~^" 'L-"-~ 'i""~

~....,.~. .. _.~ ., -L __- . -- 1- - -I - . ---- - C.-- I 11-C~ -- - ------

- -- -- -- I- --- - '- - -~ --- --- ' -- ~~ --- '- - '- ' "---- - ---- -- 2-- -- --- ,,.-

- ----- -- ~ I --' *s-

.- ----- --- --.--t l-- L -r - - -- - . -- - - ~-- - - ---~T -C - ---- -- 1 II-

--lr- - - - ~r---- ~ ----r- ~- - ~-~ ----

r-^- u ---r rr- - -- ----- ~~--- - - -- ~ - " '- -- ---- ~ - - -1 ~ ---

--

.-- - r. L ' ~ ' - -- ---- --- -- - ~114 - ----C_

-~------ r - ---+-r---- r

-~- -i- - --- cl_ .i-- - r --r -I- C --~--

*-1,...-,