// CESSI SPACE WEATHER BULLETIN // 14 JULY 2025 // NOMINAL SPACE WEATHER CONDITIONS // Multiple active regions (ARs) on the visible solar disk—namely AR 14136, 14138, 14139, and 14140—have been flagged as flare-productive by the CESSI flare prediction algorithm. As a result, there is a possibility of M- or X-class flares and associated ionospheric perturbations during the week. No Earth-directed coronal mass ejections (CMEs) have been observed recently. However, a few moderately sized filaments are present on the Earth-facing side of the Sun and will be monitored for potential eruption. The solar wind speed remains elevated at over 500 km/s, slightly above quiet levels. This enhanced solar wind condition is expected to persist for the next 3–4 days due to the influence of a large coronal hole located in the southern hemisphere, currently positioned near the central meridian.