//CESSI SPACE WEATHER BULLETIN//27 MAY 2025// MODERATE SPACE WEATHER CONDITIONS// Active Region (AR) 14098, after producing multiple M-class flares and one X1.1-class flare, is now showing a decline in flaring activity. Although several active regions are currently present on the solar disk, most exhibit low potential for significant flare production. Among them, AR 14100 and AR 14099, located in the eastern hemisphere, have drawn attention based on the CESSI flare forecasting algorithm. There remains a possibility of M-class or even X-class flares from these regions in the coming days. No Earth-directed coronal mass ejections (CMEs) have been observed over the past 4–5 days, making CME-driven geomagnetic disturbances unlikely unless new eruptive events occur near the solar disk center. A few small to medium-length filaments are present across the visible disk, which could become CME sources if they erupt. Near-Earth solar wind speeds are currently around 400 km/s, indicating nominal space weather conditions. However, an increase in solar wind speed is expected over the next 2–3 days due to the influence of a long trans-equatorial coronal hole positioned near the central meridian.