Space Weather Events

Space Weather Events

Last checked 9 minutes ago.

Research information from NASA DONKI, not an operational space weather warning service.

Showing 1–20 of 116 records

116 records
Name, sortable; sort Name, A to ZEvent type, sortable; sort Event type, A to ZDate, sortable; sort Date, earliest firstFlare class, sortable; sort Flare class, A to ZCME speed, sortable; sort CME speed (most accurate analysis), lowest firstCME analyses, sortable; sort CME analyses, lowest firstLinked events, sortable; sort Linked events, A to ZInstruments, sortable; sort Instruments, A to ZSummary, sortable; sort Summary, A to Z
Solar flare — 2026-09-19 17:57 UTC (C3.3)Solar flareC3.3——2026-09-19T18:48:00-CME-001GOES-P: EXIS 1.0-8.0The flare was produce by the unnumbered Active Region just behind the limb. This is likely the Active Region that would be numbered AR 14535.
Solar flare — 2026-09-30 02:30 UTC (C8.6)Solar flareC8.6——2026-09-30T03:12:00-CME-001GOES-P: EXIS 1.0-8.0—
Solar flare — 2026-10-04 06:13 UTC (B3.2)Solar flareB3.2——2026-10-04T07:24:00-CME-001GOES-P: EXIS 1.0-8.0First in pair of eruptive flares from AR 14546, followed immediately by a B9.3 class flare peaking at 2026-10-04T06:30Z. These two flares are in close succession, but visually separable in SDO AIA 131 and in their respective field line movements in SDO AIA 171.
Solar flare — 2026-10-04 06:21 UTC (B9.3)Solar flareB9.3——2026-10-04T07:36:00-CME-001GOES-P: EXIS 1.0-8.0Second in pair of eruptive flares from AR 14546, directly preceeded by a B3.2 class flare peaking at 2026-10-04T06:19Z. These two flares are in close succession, but visually separable in SDO AIA 131 and in their respective field line movements in SDO AIA 171.
Solar flare — 2026-10-05 18:36 UTC (M1.0)Solar flareM1.0———GOES-P: EXIS 1.0-8.0—
Solar flare — 2026-10-06 05:38 UTC (M1.4)Solar flareM1.4——2026-10-06T06:23:00-CME-001GOES-P: EXIS 1.0-8.0—
Solar flare — 2026-10-06 07:47 UTC (M1.8)Solar flareM1.8——2026-10-06T09:53:00-CME-001GOES-P: EXIS 1.0-8.0—
Solar flare — 2026-10-07 12:49 UTC (C7.9)Solar flareC7.9———GOES-P: EXIS 1.0-8.0—
Solar flare — 2026-10-08 15:29 UTC (M6.7)Solar flareM6.7——2026-10-08T16:53:00-CME-001GOES-P: EXIS 1.0-8.0—
Solar flare — 2026-10-09 13:55 UTC (M1.3)Solar flareM1.3——2026-10-09T14:36:00-CME-001GOES-P: EXIS 1.0-8.0Region 14547 decayed to a plage on 2026-10-08 and rotated off of the Earth-facing disk early on 2026-10-09. This flare may be occulted due to its location near the west limb.
Solar flare — 2026-10-10 13:56 UTC (M1.2)Solar flareM1.2———GOES-P: EXIS 1.0-8.0—
Solar flare — 2026-10-10 14:58 UTC (M6.4)Solar flareM6.4——2026-10-10T16:15:00-CME-001GOES-P: EXIS 1.0-8.0—
Coronal mass ejection — 2026-09-14 11:08 UTCCoronal mass ejection—897 km/s22026-09-17T01:24:00-IPS-001, 2026-09-17T15:10:00-IPS-001STEREO A: SECCHI/COR2, GOES: CCOR-1CME first seen to the E in STEREO A COR2 starting at 2026-09-14T11:08Z. It is also seen to the W in GOES CCOR-1. This CME is covered by a data gap in SOHO LASCO C2/C3 in real time. The source of this CME is an eruption centered around AR 14528 (S11W38) best seen in GOES SUVI 284 beginning around 2026-09-14T10:00Z. Field line movement can be seen accompanied by brightening and ejecta. Post-eruptive arcades can also be seen in SDO AIA 193. There seems to be a northwestward deflection from the location of the source. There are two large coronal holes (a northern and a southern one) nearby, possibly responsible for this deflection.
Coronal mass ejection — 2026-09-14 17:24 UTCCoronal mass ejection—461 km/s1—SOHO: LASCO/C2, SOHO: LASCO/C3, GOES: CCOR-1CME observed to the NW in SOHO LASCO C2/C3 and GOES CCOR-1, likely not observed in STEREO A COR2 either due to faintness or a data gap starting at 2026-09-14T18:53Z before it becomes visible. The source is far-sided over the NW limb, observed in SDO AIA 171/193 starting around 2026-09-17T15:48Z as slow, wide field line movement. More directly observed in STEREO A EUVI 195/304 starting as early as 2026-09-14T14:55Z, as brightening and dimming centered around an estimated N30W115 in the NW disk near former Active Regions 14523 and 14521.
Coronal mass ejection — 2026-09-15 08:36 UTCCoronal mass ejection—395 km/s1—SOHO: LASCO/C2Very faint CME with an unclear front seen to the NE in early images of SOHO LASCO C2 only. It is not seen in SOHO LASCO C3, STEREO A COR2 and GOES CCOR-1, likely because of its faintness. No source for this feature has been found in EUV imagery.
Coronal mass ejection — 2026-09-18 03:24 UTCCoronal mass ejection—371 km/s1—SOHO: LASCO/C2, SOHO: LASCO/C3, GOES: CCOR-1CME visible to the NE in SOHO LASCO C2/C3. The CME is also faintly visible to the NE in GOES CCOR-1 following a data gap due to Earthshine from 2026-09-18T03:45Z to 2026-09-18T06:10Z. The CME is not visible in STEREO A COR2 imagery. The source is beyond the NE limb and is seen as moving field lines starting at 2026-09-18T02:35Z in GOES SUVI 284 and SDO AIA 171/193 imagery.
Coronal mass ejection — 2026-09-19 16:38 UTCCoronal mass ejection—729 km/s1—SOHO: LASCO/C2, STEREO A: SECCHI/COR2, GOES: CCOR-1Faint, narrow CME seen to the SW in SOHO LASCO C2 and STEREO A COR2 and very faintly seen in a couple of frames of GOES CCOR-1 coronagraph imagery. The CME is not seen in SOHO LASCO C3. Its source is likely seen in STEREO A EUV 304 imagery as a large ejecta off the W limb after 2026-09-19T15Z and not seen in any other EUV imagery. The ejecta is not clearly visible, and it's exact location/longitude is unclear, but it seems to be close to the limb (which would be ~159 deg).
Coronal mass ejection — 2026-09-19 18:48 UTCCoronal mass ejection—321 km/s12026-09-19T17:57:00-FLR-001SOHO: LASCO/C2Faint, minor CME with an unclear front seen to the E-NE in SOHO LASCO C2. Not seen in other coronagraphs. Its source is the long duration C3.3 class flare from unnumbered AR rotating onto disk (N14E90) peaking at 2026-09-19T18:17Z. There is also an associated opening of field lines on/behind the E limb seen in SDO AIA 193 and a minor prominence/ejecta seen in SDO AIA 304/171 starting after 2026-09-19T18:10Z. The initial front is followed by a series of outflows.
Coronal mass ejection — 2026-09-19 22:12 UTCCoronal mass ejection—331 km/s1—SOHO: LASCO/C2, SOHO: LASCO/C3, STEREO A: SECCHI/COR2, GOES: CCOR-1CME observed to the NW in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2. The source is a far-sided filament eruption over the NW limb, observed best in GOES 284/304 starting around 2026-09-19T21:22Z. When STEREO A EUVI 304/195 return from a data gap at 2026-09-20T00:15Z and 2026-09-20T00:25 respectively, dimming and post eruptive brightening can be seen in the NW disk, likely left behind by this filament eruption.
Coronal mass ejection — 2026-09-19 22:24 UTCCoronal mass ejection—341 km/s1—SOHO: LASCO/C2, SOHO: LASCO/C3, STEREO A: SECCHI/COR2, GOES: CCOR-1CME observed brightly to the SW in STEREO A COR2, and very faintly to the SE in SOHO LASCO C2/C3 and GOES CCOR-1. No source is seen in on-disk EUV imagery for this event, and is likely far-sided.

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  • NASA DONKI — Space Weather Events: DONKI events in the look-back window (30 days by default), re-read every hour; older entries remain from earlier refreshes or an optional backfill.

NASA DONKI — Space Weather Events

Source: Data: NASA Community Coordinated Modeling Center (CCMC), DONKI; analyses by the Moon to Mars Space Weather Analysis Office. Last successful refresh: 14 Oct 2026, 18:02 EDT.

  • DONKI information is supplied for research and analysis. It is not an operational emergency-warning service: NOAA's Space Weather Prediction Center (swpc.noaa.gov) is the official US source of space weather forecasts and warnings.
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