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Page 450
The Balmer line Ha at 6562.808 A dominates the solar Generally speaking , abundance determination respectrum as far as intensity is concerned , in spite of solves itself into three steps . First , the solar lines must the fact that the ...
The Balmer line Ha at 6562.808 A dominates the solar Generally speaking , abundance determination respectrum as far as intensity is concerned , in spite of solves itself into three steps . First , the solar lines must the fact that the ...
Page 451
Two Zn i identification of the leading low - level lines of Tc i in es having an E P of 4 ev give rise to solar lines of S - stars , as reported by P. W. Merrill ( 17 ) . ensity 3 on the Rowland scale . The entire multiplet In spite of ...
Two Zn i identification of the leading low - level lines of Tc i in es having an E P of 4 ev give rise to solar lines of S - stars , as reported by P. W. Merrill ( 17 ) . ensity 3 on the Rowland scale . The entire multiplet In spite of ...
Page 453
Thus , the leading line is observed about 28 percent of the predicted lines in each of two at 8047.60 A , has the wave number 12,422.65 K , and regions , 6600 A to 8680 A and 3600 A to 4300 A. The represents the transition a 5F5 - 27D ...
Thus , the leading line is observed about 28 percent of the predicted lines in each of two at 8047.60 A , has the wave number 12,422.65 K , and regions , 6600 A to 8680 A and 3600 A to 4300 A. The represents the transition a 5F5 - 27D ...
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