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M Oi 05
00 05 CO
B *
a §
T
6700°
6600°
6500°
6400°
6300°
6200°
6100°
6000°
5900°
5800°
A = 0
20 ft
0
779
0
662
0
559
0
470
0
393
0
326
0
270
0
222
0
181
0
146
25
2
209
1
938
1
694
1
474
1
277
1
101
0
945
0
807
0
685
0
579
30
3
743
3
357
2
999
2
671
2
370
2
095
1
844
1
616
1
411
1
226
35
4
844
4
411
4
006
3
626
3
273
2
944
2
639
2
358
2
098
1
859
40
5
382
4
958
4
555
4
177
3
817
3
478
3
160
2
862
2
584
2
322
45
5
458
5
073
4
705
4
353
4
017
3
698
3
395
3
108
2
838
2
583
50
5
232
4
896
4
574
4
264
3
965
3
681
3
408
3
147
2
898
2
661
55
4
841
4
557
4
280
4
014
3
757
3
509
3
270
3
041
2
821
2
610
60
4
378
4
140
3
909
3
683
3
465
3
253
3
049
2
851
2
660
2
477
70
3
451
3
287
3
125
2
968
2
815
2
664
2
517
2
375
2
236
2
101
80
2
662
2
548
2
436
2
326
2
218
2
112
2
009
1
907
1
807
1
710
90
2
046
1
965
1
886
1
808
1
732
1
657
1
583
1
509
1
438
1
367
1
00
1
577
1
521
1
464
1
409
1
353
1
298
1
245
1
191
1
139
1
089
1
10
1
226
1
185
1
144
1
103
1
063
1
f 23
0
983
0
944
0
906
0
869
1
20
0
963
0
932
0
901
0
871
0
840
0
811
782
752
724
695
1
30
763
740
717
694
672
649
626
604
582
560
1
40
611
593
576
558
541
523
506
489
472
455
1
50
495
481
467
453
439
426
413
399
386
372
1
60
403
392
381
371
360
349
338
328
318
307
1
70
332
323
315
306
297
289
280
272
263
255
1
80
276
268
262
255
248
241
234
227
220
214
1
90
231
225
219
214
207
202
197
191
185
180
2
00
196
189
185
180
176
171
166
162
157
152
2
10
165
161
157
153
149
145
141
138
134
130
2
20
140
137
134
131
127
124
121
118
114
111
2
30
121
118
115
113
109
107
104
101
099
096
2
40
104
102
099
097
095
092
090
088
085
083
2
50
090
088
086
084
082
080
078
076
074
072
Sums.
52
718
49
247
45
950
42
826
39
857
37
038
34
392
31
873
29
515
27
281
Max.
5
474
5
077
4
704
4
354
4
024
3
714
3
424
3
153
2
899
2
661
A max.
0
432
0
438
0
445
0
452
0
459
0
466
0
474
0
482
0
490
0
498
Fig. 54 contains the diagrams of the energy curves for 7,700°,
6,900°, 5,800°, and Abbot’s observed ordinates, which closely
agree with the 6,900° curve from wave-length X = 0.50 ¡J- to
X = 1.00 jtt. It is seen that there is a heavy depletion from
X = 0.00 to 0.30 fi or 0.35 {i, a slight excess from X = 0.50 to
0.70 /i, a slight deficiency from X = 0.70 /* to 1.00 /*, and a rapid
increase in the ordinates to agree with those of the 7,700° curve
for X = 1.50 p to 2.50 fi. Whether the matching of the observed
with the computed ordinates is made for the curves 6,500°,
6,600°, 6,700°, 6,800°, 6,900°, 7,000°, the preceding description of
results holds true, but the best coincidence seems to be for 6,900°.
