  We present a polarization analysis of PSR J0941$-$39 and PSR J1107$-$5907,
which exhibit transitions between being pulsars and rotating radio transients
(RRATs), using the ultra-wide bandwidth low-frequency (UWL) receiver on
Murriyang, the Parkes 64\,m radio telescope. The spectral index of each pulsar
was measured, revealing distinct variations among different states. By using
the rotating vector model (RVM), we determined that the magnetosphere geometry
remains consistent between the RRAT state and the pulsar state for PSR
J0941$-$39, with emissions originating from the same height in the
magnetosphere. The occurrence of the RRAT state could be attributed to
variations in currents within the pulsar's magnetosphere. Our results suggest
that the emission mechanism of RRAT may share similarities with that of a
typical pulsar.
