412 
xMR J. EVEIiSHED ON WAVE-LENGTH DETEEMINATIONS, ETC., 
Table II.— continued .. 
Wave-length 
No. 4 
Remarks. 
WaA’e-length, 
solar 
’Sc 
5 
•spectmin. 
o 
spectrum. 
liOAA'LAXD. 
o 
3 
3745-98 
1 
r3745-717 
8 
6 
Fe 
Fe 
3748-47 
0 
3748-408 
10 
Fe 
3750-21 
2 
— 
— 
Hk 
3759-53 
0 
Well-defiued and A^ery small dots. 
3759-447 
12 
Ti 
3761-40 
3761-464 
7 
Ti 
3770-80 
'"1 
— 
— 
PL 
3798-12 
3 
— 
— 
R9 ' 
3820-09 
3825-77 
1 ' 
0 
> 
Not AA'ell defined. 
7 3820-586 
25 
20 
Fe 1 
Fe 
3829-39 
0 ^ 
3829-501 
10 
Mg 
3832-56 
1 
3832-450 
15 
Mg 
38.35-63 
3 
— 
— 
H,, 
3838-56 
2 
Well-defined nearly circular dots. 
3838-435 
25 
Mg 
3860-14 
1 
Slightly Avinged. 
3860-055 
20 
Fe 
3889-09 
4 
— 
HC ^ 
3900-5 
0 
3900-681 
5 
Ti(S) 
3913-2 
0 
3913-609 
5 
Ti(Fe) 
3933-8 
10 
K, triangular l>lack spot. 
3933-825 
rooo 
Ca 
(3944-0) 
0 
Not measured Avave-length in No. 3 spectrum 
3944-160 
15 
A1 
3968-6 
10 
H, triangular 1)lack spot. 
3968-625 
700 
Ca 1 
4026-3 
4077-8 
5 } 
r 
Fairly good definition.. < 
(4026-342) 
4077-885 
8 
He i 
Sr 
4102-2 
5 
Circular lilack spot Avith Avings due to motion 
4102-000 
40 
m : 
in line of sight 
1 
4215-7 
2 
4215-703 
5 
Sr 
4340-6 
5 
Same as HS. 
4340-634 
20 
Hy ’ 
4471-8 
3 
Well-defined spot. 
(4471-646) 
— 
He 
4713-1 
1 
(4713-252) 
— 
He 
4861-5 
5 
Circular spot slightly Avinged. 
4861-527 
30 
H/3 
