rOTAl. KCLTPSE OF THE SEX, JANHAEV 22 , 1898. 
223 
Table 1.— coatinaad. 
Chemical origin. 
Comparison. 
Probable. 
Origin. 
XA. 
Possible. 
Remarks. 
Origin. 
AA. 
5052 • 8 
56-0 
60 
66 
68 
72 
73 
79' 
79' 
85' 
88 ' 
97- 2 
98- 8 
5105 • 7 
07-6 
07-8 
10-6 
15-5 
21-8 
23-9 
25 • 3 
30-5 
37-4 
43-5 
48-2 
51- 0 
52- 0 
54 • 2 
56 ‘0 
62-4 
67 ■ 6 
69 • 1 
72 A) 
78-0 
83-8 
88-9 
91- 6 
92- 5 
5202-5 
Mg 
Fe 
jj Fc 
Mg 
/'Ti 
Fe 
Fe 
5167-50 
5167-68 
5169-07 
5169-22 
5172-86 
5183-79 
5188-87 
5191- 631 
5192- 52 / 
5202 - 52 
Ca 
2 
_ 
Id 
1 
Fe 
5068-94 
1 
/' Ti 
5072-50 
1 
3 
/Fe 
5079-41 / 
/Fe 
5079-92/ 
1-2 
1-2 
3 
/Ni 
/Fe 
2 
— 
-- 
Fe 
2 
Fe 
5105-72 
.) 
JFe 
5107-62/ 
/Fe 
5107-82/ 
1 
Fe 
5110-57 
1 
2-3 
— 
— 
Ni 
•) 
Fe 
/5123-90/ 
15125-30/ 
2-3 
») 
/Ni , 
/Fe I 
1 
1 
-- 
— 
Fe 
1 
— 
— 
Fe 
2-3 
1-2 
1 
!> Ti 
5154-24 
Vi' 
Fe 
5162-45 
TV J 
5066 -174 
5097-04 
5097- 18 
5098- 75 
5098 - 89 
5115-57 
5137 - 25 
5137-56 
5148-22 
5148-41 
5151- 02 
5152- 09 
5155-94 
5189-02 
{ 
Chromospheric line covers the 
group of Fraunhofer lines 
in solar spectrum. 
Bi'oad line central with nar¬ 
row Fe double. 
Chromosjjheric line covers the 
position occujhed Ity Fe 
lines at given AA. 
F,. 
Ih. * 
h... 
Chromospheric line covers posi¬ 
tion occupied by Fe double. 
This is one of the most enhanced Fc lines, but which of the two are lines at the given AA is the real 
enhanced line it is impossible to say without using much lai'ger dis])ersion. 
