Stellar atmospheres : $b A contribution to the observational study of high temperature in the reversing layers of starsPayne-Gaposchkin, Cecilia
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Stellar atmospheres : $b A contribution to the observational study of high temperature in the reversing layers of stars
Payne-Gaposchkin, Cecilia
Astrophysics; Stars -- Spectra; Stars -- Temperature; Thesis (Ph. D.)
Fe+
13
Ibid.
The value of is dependent on the effective level, and hence
upon the excitation potential. Without the introduction of unjustified
assumptions, more than one critical potential cannot be deduced
from observations of intensity maximum. The excitation potential
corresponding to a line could be roughly inferred from the observed
maximum, by observing the shift of predicted maximum produced by the
level effect (discussed in Chapter IX) if the ionization potential were
known. There are, however, no data as yet that could be used in drawing
inferences of this kind.
DURATION OF ATOMIC STATES
The successful application of theory to the astrophysical determination
of the life of an atom requires the fulfilment of special conditions.
The requirements of the idea developed by Milne[434] demand that
the atom shall exist in appreciable quantities in only two states
simultaneously. This condition is fulfilled by the ionized atoms of the
alkaline earth elements, and it is with calcium that the estimates here
discussed are concerned.
[Pg 159]
The investigation relates to the calcium present in the high-level
chromosphere, where, owing to remoteness from the photosphere, thermal
ionization is negligible. Photoelectric ionization may be operative in
removing the first electron from the calcium atom, but the sun is too
deficient in light of wave-length 1040 for second stage photoelectric
ionization to be appreciable. The calcium present in the high-level
chromosphere is probably largely in the once ionized condition, since
an atom once ionized is likely to remain so for a long time, owing to
the scarcity of free electrons in the tenuous outer regions of the sun.
The present investigation neglects altogether the neutral and doubly
ionized calcium atoms, and furthermore assumes that the transfers
corresponding to the and lines of the
series are the only ones that occur in appreciable quantities. The
latter assumption is apparently not accurately fulfilled, as the
lines of Ca+ have recently been detected in the high
level chromosphere.[435]
[Pg 160]
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