Stellar atmospheres : $b A contribution to the observational study of high temperature in the reversing layers of stars — John Shaqi
Stellar atmospheres : $b A contribution to the observational study of high temperature in the reversing layers of starsPayne-Gaposchkin, Cecilia
Science
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.)
The unionized (or neutral) atom in the unexcited state absorbs the
ultimate lines by the removal of one electron from its normal
stationary state to some other which can be reached from that state,
and re-emits them by the return of the electron to that state. The
electron may, of course, leave the state to which it was carried by
the ultimate absorption and pass to some state other than the normal
one. If this final state is a state of higher energy than the previous
state, the line produced by the process will be an absorption line; if
[Pg 12]
it is of lower energy the result will be the production of an emission
line. In either case the line produced by the transfer of an electron
from a stationary state other than the normal state is known as a
subordinate line. The distinction between series of ultimate
and subordinate lines is of great importance in the astrophysical
applications of the theory of ionization.
Figure 2
The hydrogen atom. The ten innermost orbits possible for the single
electron of the atom of hydrogen are diagrammatically represented.
All possible quantum transitions between the orbits are indicated as
follows:—short dashes, Lyman series, terminating at a 1-quantum orbit;
full lines, Balmer series, terminating at a 2-quantum orbit; long
dashes, Paschen series, terminating at a 3-quantum orbit. Transfers are
only possible between orbits with azimuthal quantum numbers differing
by ±1.
When the energy supply from the environment is great enough,
the “outermost” (or most easily detachable) valency electron is
entirely removed by the energy absorbed. In consequence the atom is
superficially transformed, giving rise to a totally new spectrum,
which strongly resembles the spectrum of the atom next preceding in
the periodic system. Bohr’s table embodies the interpretation of
[Pg 13]
this resemblance—the so-called Displacement Rule of Kossell and
Sommerfeld[7]—which has recently been strikingly confirmed by a very
complete investigation of the arc and spark (neutral and ionized)
spectra of the atoms in the first long period.[8] It may be seen at
once, for instance, that the removal of the outermost (or )
electron from the atom of aluminum () produces an arrangement
of external electrons identical with that for magnesium (). The
ionized atom produced by the complete removal of one electron gives,
like the neutral atom, two kinds of line spectrum—the ultimate lines
and the subordinate lines.
[Pg 14]
Figure 3
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