Report on the Radiolaria Collected by H.M.S. Challenger During the Years 1873-1876, Second Part: Subclass Osculosa; Index: Report on the Scientific Results of the Voyage of H.M.S. Challenger During the Years 1873-76, Vol. XVIIIHaeckel, Ernst
Science
Report on the Radiolaria Collected by H.M.S. Challenger During the Years 1873-1876, Second Part: Subclass Osculosa; Index: Report on the Scientific Results of the Voyage of H.M.S. Challenger During the Years 1873-76, Vol. XVIII
Haeckel, Ernst
Radiolaria
The sagittal ring (or the primary vertical ring) inherited from the
Stephanida and Semantida, shows in the #Spyroidea# great variety in its
form and in its relation to the cephalis. These variations are far greater
than Bütschli (1882, _loc. cit._) supposed. We may distinguish the
following six principal cases:--A. The ring lies completely in the wall of
the cephalis, and causes a deep sagittal constriction in it. In this case
the lower part or basal segment of the ring separates the basal pores into
pairs; its anterior part or ventral rod the facial pores; its upper part or
coryphal rod the apical pores; and its posterior part or dorsal rod the
occipital pores. No part of the ring is free in the shell-cavity. B. The
greater part of the ring lies enclosed in the shell-wall; only its dorsal
rod arises free in the shell-cavity and ascends vertically or obliquely to
the apex, where it is usually prolonged into the apical horn. This seems to
be the most common case. C. The coryphal and the basal part of the ring lie
enclosed in the shell-wall, with its dorsal and ventral rod free in the
shell-cavity; the dorsal rod ascends vertically to the apex, the ventral
rod obliquely upwards to the upper part of the facial plate (the nasal or
orbital region). This case, regarded by Bütschli as the usual one, is far
less common than he supposed. D. The greater part of the ring lies free in
the shell-cavity, its basal rod only is enclosed in the shell-wall, and
separates the right from the left group of the cortinar pores. This case
seems to be rarer than the preceding. E. The whole ring lies free in the
shell-cavity, and is connected with the sagittal constriction of the
shell-wall by numerous short radial beams. The distance of the shell-wall
from the enclosed ring is usually least on the basal rod, and greatest on
the dorsal rod. F. The whole ring lies free in the shell-cavity (as in the
preceding case), and is connected by numerous short radial beams with a
secondary larger, concentric sagittal ring, which is developed in the
longitudinal constriction of the shell-wall.
{1020}Comparing these six principal cases, in respect of the relation of
the primary sagittal ring to the cephalis of the #Spyroidea#, we may
suppose that they represent together a continuous phylogenetical series of
which the first (A) is the original, and the last (F) the latest case; and
that the true cause of the various changes is a successive separation of
the ring, which becomes more and more free and independent from the
lattice-plate of the cephalis. Since the intimate study of the structure of
the cephalis in many #Spyroidea# is very difficult, it requires further
accurate observations (from all six sides of the shell). There are also
some other more difficult complications of its structure, which cannot be
solved without exact study and extended comparison.
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