Astronomy. 141 
a ee 
Now Date of Obs. Hour. | Mag. jist alt.)2d alt.fist alt./2d alt. Authority. 
hea Aug. 10, ; ag a © erschel, Proc. Br. Met. Soc., 
: 7, 22 2 2 . ue 9 a2 
oa “/ 10 7 2 73 72 “ “ Lii, 
10g. “| 10.8 74 " - 
310. “ec 9 g 66 Hi “ “ 
311. sl) at.1| 1 54 * - 
312. isi 2 7 56 “ “ 
: by . Co Be: Heis, Ibid., p. 21 
| 315. «f y 31 “ “ 
: 316. “ 72 48 “ “ 
A 317. “ 74 |} 68 “ “ 
‘ 318. “& 64 22 “ “ 
; 319. « 55 | 20 - a 
‘ 320. « 60 | 45 “ “ 
: vb “ 88 | 36 “ “ 
t 322. “ “ “ 
303, e Sage d ‘ 
324. & 541 497 “ Pr 
325. “ png oy “ “ 
326. “ 49 38 “ “ 
327. = | 28 | 20 = - 
“se “ 43 | 30 ~ “ 
90. & “ “ 
eS ey | ‘oe 
331. ss 86 | 5o at - 
332, “ 64 | 48 . es 
333. “ | 156 | 55 é # 
7 334. “ 84 “ « 
33 sé “ ac 
4 5. 40 | 20 
tH ; 336. ‘bz 42 30 “ “ 
337. PY 70 38 “ “ 
338. as 102 | 37 = a 
339. ‘“ 61 | 48 “ C3 
340. ‘“ | 40 36 “ “ 
341. Nov, 13,, 9.5 1 49 | 42 Amer. Jour. [2], xxvii, 143. 
342, ‘ | 9-7, 1 56 26 | “ec &< 
The altitudes Nos, 231-239 were computed from the observations. 
A part of those from No. 25 to No. 87, are taken from Feldt’s article, 
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Tha error in the two processes, of engraving, and of measuring from the 
lagram, 
_ 2. On Sun-Spots and their Connexion with Planetary Configurations ; 
by Baurour Stewart, Esq., Observatory, Kew. (Proceedings of Royal 
Society.) The author was led to investigate the solar autographs taken 
at Kew and Cranford, under the an gereypcrwd of Mr. 
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= fn sen to planetary configuration. The following law was found 
to ho :—If the sun’s disc be full of spots at any time, and if one of 
stom begins to wane as it comes up by means of the sun’s rotation to a 
