TOTAL ECLIPSE OF THE SUN, JANUAEY 22, 1898. 
225 
Table I.— continued. 
Chemical origin. 
Wave-lengths. 
i 
1 
Probable. 
Possil>le. 
Remarks. 
1 
1 
Comparison. 
S 
4-:> 
Origin. 
AA. 
Origin. 
AA. 
5383-6 
1-2 
Fe 
5383-58 
91-7 
2 
— 
— 
Fe 
/ 5391-66 
15391-82 
97-3 + 
3 
Fe 
5397-34 
5401-41 
A 
Fe 
/ 5404-36 \ 
/ 
Chromospheric line covers posi- 
06-0/ 
15405-99/ 
L 
tion occupied by Fe double. 
10-0 
2 
Cr 
5410-00 
15-4 
2 
Fe 
5415-42 
19-0 
1 
22-0 
1 
25-5 
2 
29-9 
3 
Fe 
5429-91 
.32-9 
2-3 
34-7'| 
— 
Fe 
5434-74 
— 
- 1 
to 1' 
2 
— 
— 
Ni 
5436-07 1 
Diffuse line covering Fraun- 
Fe 
/5436-51 f 
hofer group. 
36-8 J 
154.36-80 J 
47-1 
5-6 
Fe 
5447-13 
53-0 
1 
55-8 
5 
Fe 
5455-83 
- 
59-5 
1 
63-5 
4 
Fe 
5463-49 
66-6 
1-2 
— 
Fe 
5466-61 
70-5 
2 
74-1 
3 
Fe 
5474-11 
i 
76-8/ 
4-5 
— 
Fe 
/ 5476-50 
15470-78 
83-3 
1-2 
— 
— 
Fe 
5483-31 
90-4 
1-2 
__ 
_ 
Ti 
5490-37 
94-0 
1-2 
97-7 
2 
Fe 
5497-74 
5501-7 
2-3 
Fe 
5.501-68 
07-0 
2-3 
Fe 
5507-00 
11-6 
2-3 
14-5 
2 
— 
— 
Ti 
/5514-56 
1.5514-75 
18-0 
1-2 
27-6 
6 
— 
— 
— - 
— 
Rather broad and j^robaldy 
1 
1 
double. The strong Mg 
spark line at A 5528-64 
falls on the less refrangible 
portion of the eclipse line. 
35-6 
5 
Ba 
5535-69 
Fe 
5535-64 
40-0 
1 
43-41 
Fe 
/.5543-41 
44-2 J 
15544-10 
46-71 
Fe 
/5540 - 73 
47-2 J 
15517 - 22 
55-1 
1-2 
— 
— 
Fe 
5555 -12 
58-2 
2 
— 
— 
Fe 
5558-21 
—A. 2 G 
VOL. CXCVII. 
