  We present a comprehensive characterization of 26 CME-driven compressive
waves known as Coronal Bright Fronts (CBFs) observed in the low solar corona
between 2010 and 2017. These CBFs have been found to be associated with SEP
events near Earth, indicating their importance in understanding space weather
phenomena. The aim of this study is to analyze and describe the early dynamics
of CBFs using a physics-based heliospheric SEP forecasting system known as the
SPREAdFAST framework. This framework utilizes a chain of data-driven analytic
and numerical models to predict SEP fluxes at multiple locations in the inner
heliosphere by considering their acceleration at CMEs near the Sun and
subsequent interplanetary transport. To estimate the time-dependent plasma and
compression parameters of the CBFs, we utilized sequences of base-difference
images obtained from the AIA instrument on board the SDO satellite, and
measurements of the height-time profiles of the CMEs obtained from the LASCO
instrument on board the SOHO satellite. We employed kinematic measurements and
plasma model results to derive these parameters. The SPREAdFAST framework
facilitated the analysis and correlation of these observations with SEP events
near Earth. Our analysis yielded statistical relations and distributions for
both the shocks and plasma parameters associated with the 26 CBFs investigated.
By combining the observations from the AIA and LASCO instruments, as well as
the data products from the SPREAdFAST framework, we obtained a comprehensive
understanding of the early dynamics of CBFs, including their temporal
evolution, plasma properties, and compressional characteristics. These findings
contribute to the growing body of knowledge in the field and have implications
for space weather forecasting and the study of SEP events.
