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Anemophilous (wind‐driven) pollen is one type of primary biological aerosol particle, which can rupture under high humidity conditions and form smaller sub‐pollen particles (SPPs). Both pollen and SPPs can reach the upper troposphere under convective conditions, acting as cloud condensation nuclei (CCN) and ice nucleating particles (INPs), thus influencing cloud formation and precipitation. However, the impacts of these biological aerosols on cold cloud formation and local climate remain unclear as there are large uncertainties on their emission flux and ice nucleating abilities. Here, we incorporate pollen emission and rupture processes in the Weather Research and Forecasting Model with Chemistry (WRF‐Chem) simulations and update the Morrison microphysics scheme within WRF‐Chem using aerosol‐aware INP parameterizations to account for pollen in addition to other anthropogenic and biogenic aerosol. INP parameterizations for pollen and SPP are derived from laboratory experiments. When including pollen rupture rates as observed in a series of chamber studies, SPP concentrations increase, leading to an increase of cloud ice and water by up to 50% and potentially extending the duration of the convective system. Among all simulated hydrometeors, graupel and raindrops exhibit the largest enhancements from the inclusion of SPPs, with intensifying precipitation at the backside of the convective system and a greater spatial extent. Sensitivity simulations indicate that SPPs have a greater effect on cloud microphysical processes than whole pollen grains, and further observational evidence is needed to constrain these processes. Plain Language Summary: Pollen grains are emitted by vegetation and carry the reproductive material of plants. Under certain conditions (e.g., high humidity, lightning), pollen grains can rupture to form smaller sub‐pollen particles (SPPs). Both intact pollen grain and SPPs have been observed to influence the formation of cloud liquid droplets and ice crystals, potentially impacting cloud properties and precipitation. In this study, we include pollen emission and pollen‐cloud interactions into a meteorology‐chemistry model and investigate the effects of pollen grains and SPPs on a strong thunderstorm event associated with a mesoscale convective system. We find that SPPs have a greater impact than whole pollen grains on the convective system properties by increasing cloud ice and water content, facilitating the transition of cloud droplets and ice into graupel, and ultimately intensifying precipitation. These changes alter the impact of the convective system, leading to an extension of the storm width and lengthening of its duration. Key Points: Sub‐pollen particles (SPPs) enhance cloud microphysical processes more than intact pollen grainsSPPs influence the spatial extent and vertical structure of convective systemsSimulated SPP impacts are intensified when incorporating laboratory measured pollen rupture rates [ABSTRACT FROM AUTHOR]

W-Re alloys are one of the most important refractory materials with excellent high-temperature performance that were developed to improve the brittleness of tungsten. In the present work, we firstly summarized the research progress on the preparation and strengthening methods of a W-Re alloy. Then, the strengthening mechanisms of the W-Re alloy were discussed, including the influence of Re, solid solution strengthening, second-phase reinforcement and fine-grain strengthening. The results showed that the softening effect of Re was mainly related to the transformation of the preferred slip plane and the introduction of additional d-valence electrons. Some transition elements and refractory metal elements effectively strengthened the W-Re alloy. Carbides can significantly enhance the high-temperature mechanical properties of W-Re alloys, and the reasons are twofold: one is the interaction between carbides and dislocations, and the other is the synergistic strengthening effect between carbides and Re. The objective of this work was to enhance the comprehension on W-Re alloys and provide future research directions for W-Re alloys. [ABSTRACT FROM AUTHOR]