  The culmination of solar cycle 24 by the end of 2019 has created the
opportunity to compare the differing properties of coronal mass ejections
(CMEs) between two whole solar cycles: Solar cycle 23 (SC 23) and Solar cycle
24 (SC 24). We report on the width evolution of limb CMEs in SC 23 and 24 in
order to test the suggestion by Gopalswamy et al. (2015a) that CME flux ropes
attain pressure balance at larger heliocentric distances in SC 24. We measure
CME width as a function of heliocentric distance for a significantly large
number of limb CMEs (~1000) and determine the distances where the CMEs reach
constant width in each cycle. We introduced a new parameter: the transition
height (hc) of a CME defined as the critical heliocentric distance beyond which
the CME width stabilizes to a quasi-constant value. Cycle and phase-to-phase
comparisons are based on this new parameter. We find that the average value of
hc in SC 24 is 62% higher than in SC 23. SC 24 CMEs attain their peak width at
larger distances from the Sun as compared to SC 23 CMEs. The enhanced
transition height in SC 24 is new observational ratification of the anomalous
expansion. The anomalous expansion of SC 24 CMEs which is caused by the weak
state of the heliosphere, accounts for the larger heliocentric distance where
the pressure balance between CME flux rope and the ambient medium is attained.
