All quiet on the space-weather front

416 km/s, direct hit — arrival in ~100 h, expected Kp ≈ 2.4 (none).

Narrow CME seen to the southeast in STEREO A COR2A and very dimly to the due south in SOHO LASCO C2 which is likely associated with an eruption in AR 14464 near S12W20 around 2026-06-12T13:50Z seen best in SDO AIA composite imagery using the sum of 211/193/171 Angstrom imagers.

977 km/s, direct hit — arrival in ~48 h, expected Kp ≈ 4.7 (moderate).

Faint partial halo CME seen in SOHO LASCO C2/C3 and GOES CCOR-1 with preference to the east and seen more narrow with a brighter bulk and disconnected bulk/shock in STEREO Ahead COR2A with brighter bulk to the east-northeast and shock extending from the southeast to the north in association with a filament eruption near N00E35 erupting near 2026-06-12T16:15Z, best seen in SDO AIA composite imagery using the sum of 211/193/171 Angstroms and as well in GOES SUVI/SDO AIA 304 Angstroms. This CME, seen due east and northeast in COR2A, is seen overlapping the previous CME: 2026-06-12T15:38Z which is seen to the southeast and which is a separate eruption.

885 km/s, near-direct hit — arrival in ~52 h, expected Kp ≈ 3.9 (glancing).

Bright loop CME and shock first seen to the Northeast by SOHO LASCO C2 beginning at 2026-06-11T00:36Z, as well as by SOHO LASCO C3, STEREO A COR2 and GOES CCOR-1 in later frames. The source of this CME is a long duration C6.7 class flare from Active Region 14465 (N09E39) seen peaking at 2026-06-11T00:02Z. This flare can be seen in SDO AIA 131 along with a wide region of dimming, field line opening and an EUV wave seen in SDO AIA 171, 193, 211 and GOES SUVI 284.

348 km/s, near-direct hit — arrival in ~119 h, expected Kp ≈ 1.7 (none).

CME first seen to the SW in SOHO LASCO C2 starting at 2026-06-09T21:36Z. It is also seen to the SW in SOHO LASCO C3 and GOES CCOR-1 but is covered by a real-time data gap in STEREO A COR2. The is most likely an eruption from AR 14461 (S21W19) that appears to be heavily deflected southward likely due its proximity to a coronal hole that was centered around N00W05. The eruption is best seen in SDO AIA 193 as moving field lines and a large area of dimming directed toward the south. The eruption is also accompanied by C2.3 class flare from AR 14461 that peaked at 2026-06-09T19:18Z best seen in SDO AIA 131. In coronagraphs, this CME partially overlaps with far-sided CME: 2026-06-09T21:12Z.

293 km/s, glancing blow (10° outside cone) — arrival in ~142 h, expected Kp ≈ 1.3 (none).

Faint CME observed to the E only in STEREO A COR2. The source is likely dimming in SDO AIA 193 starting around 2026-06-11T08:48Z centered around S25W32.

649 km/s, glancing blow (32° outside cone) — arrival in ~68 h, expected Kp ≈ 2.0 (none).

CME first seen to the SW in SOHO LASCO C2 stating at 2026-06-13T13:26Z. It is also seen to the SW in SOHO LASCO C3 and GOES CCOR-1 and to the S in STEREO A COR2. The majority of this CME was missed by SOHO LASCO C2/C3 in real time due to a data gap between downlink periods. The source of this CME is a large eruption in across the far SE portion of the Earth-facing disk centered around AR 14461 (S21W68). The eruption is best seen in SDO AIA 193 as wide opening field lines accompanied by dimming and an EUVI wave beginning around 2026-06-13T12:36Z. This CME is also associated with a C2.5 class flare from AR 14461 which peaked at 2026-06-13T13:09Z. The flare is best seen in SDO AIA 131.