MR. J. EYERSHED ON THE SOLAR ECLIPSE OF 1900, MAY 28. 
4r)cS 
Abnormal Ti Lines. 
In sun. 
In flash. 
If 
enhanced. 
1 
Eemarks. 
tVave-length. 
Intensity. 
tVave-length. 
Intensity. 
Ln 
les .stron< 
^ in flash 
1 
3.50.5 • 06 
0 
3505-1 
20 
1 
: 
3510-99 
5 
3511-1 
30 
% 
3520-10 
0 
3520-4 
20 
1 
1 
1 
f Perhaps compounded of Ti and a 
3535-55 
4 
3535 - 75 
50 
1 
< line at 3535-87, intensity 3 ’ 
1 origin. 
3611-47 
4 
3641-48 
40 
1 
1 
4294-20 
2 
4294-35 
12 
Yes 
1 
4395-20 
3 
4395-15 
30 
Yes 
1 
4417-88 
3 
4417-7 
20 
Yes 
1 
4501 - 45 
5 
4501-5 
30 
Yes 
I 
iines weak or absent in flash and exceeding intensity 3 in O. 
365.3-64 
5 
3653-67 
5 
1 
3753-00 
4 
3652-72 
0 
No 
3924-67 
4 
3924-8 
0 
No 
3948-82 
4 
3949-11 
4 
No 
3981-92 
4 
3981-3 d 
3982-2 J 
5 
iNO 
j 
3989-91 
4 
3990-12 
2 
No 
4171-21 
4 
Absent 
.— 
No 
1 
4291-11 4 
3 
Absent 
— 
No 
1 
-28 / 
0 
4306-08 
4 
4306-0 
1 
No 
4533-42 
4 
Al)sent 
— 
No 
1 Perhaps obscured by strong Ti line 
4534 - 95 
4 
Alisent 
— 
No 
J at 4534-14. ' 
4981-91 
4 
Al)se4it 
— 
No 
Spectrum very weak here. 
Chromium Lines in Snn and Flash. 
Including all isolated lines in Rowland’s table assigned to Cr only. 
Rowland’s intensity 
in O. 
Number of lines 
in ©. 
Number of lines 
in flash. 
Percentage of lines 
in flash. 
Average intensity 
in flash. 
0 and 1 
109 
3 
3 
0 
2 
22 
4 
18 
1 
.3 
15 
8 
46 
2 
4 
3 
3 
100 
1 
5 
O 
O 
2 
67 
o 
O 
6 to 8 
3 
3 
100 
13 
j 9 and 10 
2 
2 
100 
25 
