// CESSI SPACE WEATHER BULLETIN // 11 JULY 2025 // NOMINAL SPACE WEATHER CONDITIONS // A new active region, AR14136, has produced two low M-class flares and is drawing attention as it rotates further into view. The CESSI flare forecasting algorithm flags this region as flare-productive. Increased M-class or even X-class flare activity from this region is likely in the coming days. At present, there are no Earth-directed coronal mass ejections (CMEs). Several small-scale filaments are visible across the solar disk. Although currently stable, their potential eruption could trigger CME activity. The solar wind speed is currently around 350 km/s. A large trans-equatorial coronal hole is located near the central meridian. This structure may drive a high-speed solar wind stream, likely causing an increase in solar wind speed over the next 3–4 days.