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We present a polarization analysis of PSR J0941$-$39 and PSR J1107$-$5907,which exhibit transitions between being pulsars and rotating radio transients(RRATs), using the ultra-wide bandwidth low-frequency (UWL) receiver onMurriyang, the Parkes 64\,m radio telescope. The spectral index of each pulsarwas measured, revealing distinct variations among different states. By usingthe rotating vector model (RVM), we determined that the magnetosphere geometryremains consistent between the RRAT state and the pulsar state for PSRJ0941$-$39, with emissions originating from the same height in themagnetosphere. The occurrence of the RRAT state could be attributed tovariations in currents within the pulsar's magnetosphere. Our results suggestthat the emission mechanism of RRAT may share similarities with that of atypical pulsar.

Wide Bandwidth Observations of PSR J0941$-$39 and PSR J1107$-$5907