OBTAINED AT THE TOTAL SOLAR ECLIPSES OF 1900, 1901 AND 1905 
423 
Spectrum 
of 
chromosphere. 
1 
Wave- No. of Inten- 
length. photos.; sity. 
Element. 
Probabl 
Wave¬ 
length. 
e identifies 
Spark. 
tion. 
Intensity. 
Arc. 
Sun. 
f Cr 
3984-06 
7 
5 
3 
3984*13 
3 
1 
J 
J* Probably Fe. 
1 Fe 
3984-11 
3 
0 
4 
J 
3988 *67 
8 
2 
La 
3988 -66 
30 
5 
0 
3990*11 
6 
2 
f Ti 
l - 
3989 -91 
3990-13 
20 
8 
4 
1 
1 Not entirely due to Ti. The line 3990*13 identified as 
J Mn-Cr in the sun. 
3990 *42 
1 
1 
— 
— 
— 
— 
— 
f Cr 1 
f 9 
4 
i 
3991*43 
5 
2 
3991-33 
r 3 
l Zr J 
l. 15 
8 
J 
f Co 1 
f 8 
2 
1 
3991*85 
2 
1 
3991 -87 
\ 
l 2 
1 Cr j 
l 2 
3 
i 
3992 -50 
2 
1 
— 
— 
— 
— 
— 
r Cr i 
f 5 
3 
3993*03 
2 
0 
3992 -97 
) 
I 3(1 ? 
l v J 
l 12 
<5 
J 
3994 *14 
1 
0 
— 
— 
— 
— 
— 
3994*87 
3 
2 
N<1 
3994-83 
5 
— 
2 
3995*90 
6 
2 
La 
3995 -90 
5 
5 
1N<1 
3996 *48 
1 
1 
— 
— 
— 
— 
— 
3997 '09 
3 
1 
— 
— 
— 
— 
— 
3997 *95 
2 
1 
•Co 
3998-05 
10 
9 
4d ? 
f Zr 
3999-12 
15 
0 
1 
Identified in sun as Zr, Fe. 
3999-28 
9 
0 
l v 
3999*37 
6 
0 
0 
4000 *51 
5 
1 
— 
— 
— 
— 
— 
4002 *75 
1 
1 
Fe 
4002 *65 
i 
1 
Od 
Identified in sun as Fe, Ti. 
4003*62 
1 
0 
Cr 
(4003-48) 
5 
0 
— 
4004-13 
2 
1 
— 
— 
— 
— 
— 
4004-84 
2 
0 
— 
— 
— 
— 
— 
4005*44 
1 
2 
Fe 
4005-41 
8 
8 
7 
4005*86 
2 
1 
V 
4005-86 
20 
0 
3 
4006 *70 
1 
0 
— 
— 
— ' 
— 
— 
4007 -51 
2 
0 
Fe 
4007-43 
2 
4 
5 
4008 *16 
1 
0 
1 
— 
— 
— 
— 
4008-92 
3 
1 
— 
— 
— 
— 
— 
4009 *85 
1 
0 
Fe 
4009-86 
3 
6 
3 
4010*47 
1 
1 
— 
— 
— 
— 
— 
4011-41 
1 
0 
— 
— 
— 
— 
— 
4012-50 
9 
10 
Ti 
4012-54 
7 
2 
4 
4013-77 
1 
1 
*> 
— 
— 
— 
— 
f Sc 1 
r 8 
_ 
1 
4014-77 
4 
1 
4014*68 
\ 
I 5d ? 
l Fe J 
l 2 
2 
J 
4015*71 
3 
1 
— 
4015-76 
— 
— 
3 
4017*72 
2 
1 
— 
— 
— 
— 
— 
4019 *24 
2 
1 
— 
— 
— 
— 
— 
4020*50 
5 
2 
Sc 
4020 *55 
8 
4 
1 
4021-92 
6 
2 
Ti 
4022 *02 
4 + 
6 
4 
Identified In sun as Ti-Fe-V. 
4023*55 
6 
2 
V 
4023*53 
10 
1 
3 
Identified in sun as V Co. 
