The Most Intense Solar Fraunhofer Lines
9006-025
9006-025a
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
333.6689 |
0.0416 |
112.1 |
Mg I |
341.4779 |
0.0816 |
209.9 |
Ni I |
343.3579 |
0.0492 |
125.2 |
Ni I2 |
344.0626 |
0.1243 |
315.0 |
Fe I |
344.1019 |
0.0634 |
160.6 |
Fe I |
344.3884 |
0.0655 |
165.7 |
Fe I |
344.6271 |
0.0470 |
118.7 |
Ni I |
345.8467 |
0.0656 |
164.5 |
Ni I |
346.1667 |
0.0758 |
189.8 |
Ni I |
347.5457 |
0.0622 |
154.5 |
Fe I |
1After MOORE, MINNAERT, and HOUTGAST.
2Blended line.
3Magnetic sensitive line.
9006-025b
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
347.6712 |
0.0465 |
115.4 |
Fe I2 |
349.0594 |
0.0830 |
204.4 |
Fe I |
349.2975 |
0.0826 |
203.1 |
Ni I |
349.7843 |
0.0726 |
178.0 |
Fe I |
351.0327 |
0.0489 |
119.1 |
Ni I |
351.5066 |
0.0718 |
174.3 |
Ni I |
352.1270 |
0.0381 |
92.2 |
Fe I |
352.4536 |
0.1271 |
306.9 |
Ni I |
355.4937 |
0.0404 |
95.9 |
Fe I |
355.8532 |
0.0485 |
114.9 |
Fe I2 |
9006-025c
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
356.5396 |
0.0990 |
233.6 |
Fe I |
356.6383 |
0.0458 |
108.0 |
Ni I |
357.0134 |
0.1380 |
324.8 |
Fe I |
357.8693 |
0.0488 |
114.3 |
Cr I |
358.1209 |
0.2144 |
501.5 |
Fe I |
358.6990 |
0.0532 |
124.0 |
Fe I |
359.3495 |
0.0436 |
101.3 |
Cr I |
360.8869 |
0.1046 |
240.9 |
Fe I |
361.8777 |
0.1410 |
323.0 |
Fe I |
361.9400 |
0.0568 |
130.1 |
Ni I |
9006-025d
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
363.1475 |
0.1364 |
310.3 |
Fe I2 |
364.7851 |
0.0970 |
218.7 |
Fe I2 |
367.9923 |
0.0448 |
99.2 |
Fe I2 |
368.5196 |
0.0275 |
60.7 |
Ti II |
370.5577 |
0.0562 |
122.8 |
Fe I |
370.9256 |
0.0573 |
124.9 |
Fe I2 |
371.9947 |
0.1664 |
360.7 |
Fe I |
373.4874 |
0.3027 |
651.0 |
Fe I |
373.7141 |
0.1071 |
230.1 |
Fe I |
374.5574 |
0.1202 |
257.0 |
Fe I2 |
9006-025e
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
374.8271 |
0.0497 |
106.1 |
Fe I |
374.9495 |
0.1907 |
406.9 |
Fe I |
375.8245 |
0.1647 |
349.8 |
Fe I |
375.9299 |
0.0334 |
70.9 |
Ti II |
376.3803 |
0.0829 |
175.6 |
Fe I |
376.7204 |
0.0820 |
173.3 |
Fe I |
378.7891 |
0.0512 |
107.1 |
Fe I |
379.5012 |
0.0547 |
113.9 |
Fe I2 |
380.6718 |
0.0209 |
43.3 |
Fe I2 |
381.5851 |
0.1272 |
262.1 |
Fe I |
9006-025f
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
382.0436 |
0.1712 |
351.9 |
Fe I |
382.5891 |
0.1519 |
311.3 |
Fe I |
382.7832 |
0.0897 |
183.7 |
Fe I |
382.9365 |
0.0874 |
178.8 |
Mg I |
383.2310 |
0.1685 |
344.2 |
Mg I |
383.4233 |
0.0624 |
127.3 |
Fe I |
383.8302 |
0.1920 |
391.0 |
Mg I |
384.0447 |
0.0567 |
115.3 |
Fe I |
384.1058 |
0.0517 |
105.1 |
Fe I2 |
384.9977 |
0.0608 |
123.1 |
Fe I |
9006-025g
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
385.6381 |
0.0648 |
130.7 |
Fe I |
385.9922 |
0.1554 |
312.9 |
Fe I |
387.8027 |
0.0555 |
110.7 |
Fe I |
388.6294 |
0.0920 |
182.7 |
Fe I |
389.9719 |
0.0436 |
86.0 |
Fe I |
390.2956 |
0.0530 |
104.4 |
Fe I2 |
390.5532 |
0.0816 |
160.5 |
Si I |
392.0269 |
0.0341 |
66.6 |
Fe I |
392.2923 |
0.0414 |
80.7 |
Fe I2 |
392.7933 |
0.0187 |
36.4 |
Fe I |
9006-025h
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
393.0308 |
0.0108 |
21.0 |
Fe I |
393.3682 |
2.0253 |
3926.6 |
Ca II2 |
394.4016 |
0.0488 |
94.1 |
Al I |
396.1535 |
0.0621 |
118.7 |
Al I |
396.8492 |
1.5467 |
2946.3 |
Ca II |
404.5825 |
0.1174 |
215.2 |
Fe I |
406.3605 |
0.0787 |
143.0 |
Fe I2 |
407.1749 |
0.0723 |
130.8 |
Fe I |
407.7724 |
0.0428 |
77.2 |
Sr II2 |
410.1748 |
0.3133 |
558.7 |
H |
9006-025i
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
413.2067 |
0.0404 |
71.0 |
Fe I2 |
414.3878 |
0.0466 |
81.4 |
Fe I |
416.7277 |
0.0200 |
34.5 |
Mg I |
420.2040 |
0.0326 |
55.4 |
Fe I |
422.6740 |
0.1476 |
247.9 |
Ca I |
423.5949 |
0.0385 |
64.4 |
Fe I2 |
425.0130 |
0.0342 |
56.8 |
Fe I2 |
425.0797 |
0.0400 |
66.4 |
Fe I2 |
425.4346 |
0.0393 |
65.1 |
Cr I2 |
426.0486 |
0.0595 |
98.3 |
Fe I |
9006-025j
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
427.1774 |
0.0756 |
124.3 |
Fe I |
432.5775 |
0.0793 |
127.1 |
Fe I2 |
434.0475 |
0.2855 |
454.6 |
H |
438.3557 |
0.1008 |
157.4 |
Fe I |
440.4761 |
0.0898 |
138.9 |
Fe I |
441.5135 |
0.0417 |
64.2 |
Fe I2 |
452.8627 |
0.0275 |
40.2 |
Fe I2 |
455.4036 |
0.0159 |
23.0 |
Ba II |
470.3003 |
0.0326 |
44.2 |
Mg I |
486.1342 |
0.3680 |
467.2 |
H |
9006-025k
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
489.1502 |
0.0312 |
39.1 |
Fe I |
492.0514 |
0.0471 |
58.4 |
Fe I2 |
495.7613 |
0.0696 |
85.0 |
Fe I2 |
516.7327 |
0.0935 |
105.1 |
Mg I2 |
517.2698 |
0.1259 |
141.2 |
Mg I |
518.3619 |
0.1584 |
176.9 |
Mg I |
525.0216 |
0.0062 |
6.7 |
Fe I3 |
526.9550 |
0.0478 |
51.6 |
Fe I2 |
532.8051 |
0.0375 |
39.6 |
Fe I |
552.8418 |
0.0293 |
28.8 |
Mg I |
9006-025l
Wavelength, nm |
Bandwidth, nm |
Bandwidth, GHz |
Element |
588.9973 |
0.0752 |
65.0 |
Na I(D2)2 |
589.5940 |
0.0564 |
48.7 |
Na I(D1) |
610.2727 |
0.0135 |
10.9 |
Ca I |
612.2226 |
0.0222 |
17.8 |
Ca I |
616.2180 |
0.0222 |
17.5 |
Ca I |
630.2499 |
0.0083 |
6.3 |
Fe I3 |
656.2808 |
0.4020 |
280.0 |
H |
849.8062 |
0.1470 |
61.1 |
Ca II |
854.2144 |
0.3670 |
150.9 |
Ca II |
866.2170 |
0.2600 |
104.0 |
Ca II |
Table reproduced from "Astrophysical Formulae", edited by K.R. Lang, Springer
Verlag, 1978, p175.
Related material:
Solar-Type Spectra
The Columbus Optical SETI Observatory
Copyright (c), 1990
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