“…Jiang and Ramirez (2013) found the following necessary conditions for RI in the inner core: total raining area >3,000 km 2 , total volumetric rain >5,000 mm · hr · km 2 , maximum near-surface radar reflectivity >40 dBZ, maximum 20-dBZ (40-dBZ) echo height >8 (4) km, minimum 85-GHz polarization-corrected brightness temperature <235 K, and minimum 10.8-mm brightness temperature <220 K. Using airborne Doppler radar data, Rogers et al (2013) found that intensifying TCs have a larger number of convective bursts located inside the radius of maximum wind. Tao et al (2017) showed that the onset of RI follows a significant increase in the occurrence and azimuthal coverage of stratiform rainfall in all shear-relative quadrants, especially upshear left, which are related to the moistening/humidification of the inner core, particularly in the upshear quadrants. Tao et al (2017) showed that the onset of RI follows a significant increase in the occurrence and azimuthal coverage of stratiform rainfall in all shear-relative quadrants, especially upshear left, which are related to the moistening/humidification of the inner core, particularly in the upshear quadrants.…”