  Discovery of nine populations in a set of 193 select SOHO Kreutz sungrazers
(Sekanina 2021) is confirmed for the first time via a histogram of the true
longitudes of the ascending node, constructed for a revised set of 220 select
sungrazers imaged exclusively by the SOHO's C2 coronagraph. Marsden's orbits
are approximately corrected for effects of the out-of-plane nongravitational
force. Population I displays two peaks in the histogram, one presumably
belonging to a side branch alike to Population Pe, but with no related
naked-eye sungrazer known. Swarms/clusters of objects are commonplace,
providing evidence on cascading fragmentation proceeding throughout the orbit.
Augmentation to all C2-only SOHO Kreutz comets, aimed at removing deliberate
bias against Populations I and Pe, reduces the appearance of Populations Ia and
Pre-I to bulges along the slope of the histogram because of the swollen wings
of Populations I and Pe, respectively. Populations II through IV change very
little or not at all. The high Population I-to-II abundance ratio, of 14:1, may
be a product of temporal limitations in fragment release. A drop in the number
of fragments toward the ends of the nodal-longitude distribution, especially
from Population II to IV, is in line with the contact-binary model.
