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Prediction for CME (2014-04-01T17:00:00-CME-001)CME Observed Time: 2014-04-01T17:00ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/5077/-1 CME Shock Arrival Time: 2014-04-05T09:40Z Observed Geomagnetic Storm Parameters due to CME: Max Kp: 4.0 Predicted Arrival Time: 2014-04-05T03:00Z Predicted geomagnetic storm max Kp range due to CME: 4.0 - 5.0 Prediction Method: WSA-ENLIL + Cone (NOAA/SWPC) Prediction Method Note: (Arrival Prediction by NOAA/SWPC submitted to this system by M. Leila Mays) (Submitted CME shock arrival time taken from the excerpted Forecast Discussion below). (Submitted Kp estimate is from the excerpted Forecast Discussion and 3-Day Forecast below). -- Product: Forecast Discussion Issued: 2014 Apr 02 1230 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center Solar Activity .24 hr Summary... Solar activity was low. Frequent low-level C-class flares occurred, most of which were from Region 2026 (S11E44, Dai/beta-gamma). Minor spot and penumbra development was noted in Region 2026 along with a mix of polarities in the leading half of the region. A filament, centered near N02E20, erupted from the northeast quadrant at around 01/1439 UTC and was associated with an Earth-directed, asymmetric full-halo coronal mass ejection (CME). The CME was first visible in LASCO images at around 01/1648 UTC and had a speed of around 858 km/s. .Forecast... Solar activity is expected to be low during the period (02-04 Apr) with a chance for an M-class flare (R1-R2, Minor-Moderate). Energetic Particle .24 hr Summary... The greater than 2 MeV electron flux at geosynchronous orbit was at normal levels. The greater than 10 MeV proton flux at geosynchronous orbit was at background levels. .Forecast... The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at normal levels during the period (02-04 Apr). The greater than 10 MeV proton flux at geosynchronous orbit is expected to remain at background levels during the period. Solar Wind .24 hr Summary... Solar wind was slightly enhanced. However, no evident CME signatures were observed from the expected arrival of the first of a series of CMEs that occurred between 28 and 30 Mar. Solar wind speed ranged from 362 to 502 km/s. Total field was relatively steady between 4 nT and 7 nT, while the Bz component was variable at +/- 5 nT. Phi data indicated a positive-polarity (away) solar sector during the period. .Forecast... No significant changes are expected in the solar wind flow until around midday on 04 Apr. A CME is expected to arrive around midday on 04 Apr with enhancements in wind speed, density, and total field expected during the remainder of 04 Apr. Geospace .24 hr Summary... The geomagnetic field was at quiet to (briefly) unsettled levels. .Forecast... Geomagnetic field activity is expected to be at mostly quiet levels until around midday on 04 Apr. Field activity is expected to increase to unsettled to active levels (below G1-Minor) during the latter half of 04 Apr due to a CME passage from the 01 Apr filament eruption mentioned above. -- Product: 3-Day Forecast Issued: 2014 Apr 02 1230 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center A. NOAA Geomagnetic Activity Observation and Forecast The greatest observed 3 hr Kp over the past 24 hours was 2 (below NOAA Scale levels). The greatest expected 3 hr Kp for Apr 02-Apr 04 2014 is 4 (below NOAA Scale levels). NOAA Kp index breakdown Apr 02-Apr 04 2014 Apr 02 Apr 03 Apr 04 00-03UT 1 3 2 03-06UT 1 2 1 06-09UT 1 2 1 09-12UT 1 2 3 12-15UT 1 2 3 15-18UT 1 2 4 18-21UT 1 2 4 21-00UT 2 2 4 Rationale: No G1 (Minor) or greater geomagnetic storms are expected. No significant transient or recurrent solar wind features are forecast. Product: Forecast Discussion Issued: 2014 Apr 03 0030 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center ... Geospace .24 hr Summary... The geomagnetic field was quiet. .Forecast... The geomagnetic field is expected to be mostly quiet for days 1-2 (03-04 Apr). By early on day 3 (05 Apr), the 01 Apr CME associated with a filament eruption is expected to impact the geomagnetic field causing quiet to active conditions with a slight chance for minor (G1-Minor) storm conditions. -- Product: 3-Day Forecast Issued: 2014 Apr 03 0030 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center A. NOAA Geomagnetic Activity Observation and Forecast The greatest observed 3 hr Kp over the past 24 hours was 2 (below NOAA Scale levels). The greatest expected 3 hr Kp for Apr 03-Apr 05 2014 is 4 (below NOAA Scale levels). NOAA Kp index breakdown Apr 03-Apr 05 2014 Apr 03 Apr 04 Apr 05 00-03UT 2 2 2 03-06UT 2 1 4 06-09UT 1 1 4 09-12UT 1 1 3 12-15UT 1 1 3 15-18UT 1 1 3 18-21UT 2 2 3 21-00UT 1 2 3 -- Product: Forecast Discussion Issued: 2014 Apr 03 1230 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center Geospace .24 hr Summary... The geomagnetic field was quiet. .Forecast... Geomagnetic field activity is expected to be at quiet levels during 03 -04 Apr with a slight chance for unsettled levels. Activity is expected to increase to unsettled to minor storm (G1-Minor) levels, with a slight chance for major storm levels (G2-Moderate), beginning early on 05 April due to the arrival of the CME from the filament eruption on 01 April. -- Product: 3-Day Forecast Issued: 2014 Apr 03 1230 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center A. NOAA Geomagnetic Activity Observation and Forecast The greatest observed 3 hr Kp over the past 24 hours was 2 (below NOAA Scale levels). The greatest expected 3 hr Kp for Apr 03-Apr 05 2014 is 5 (NOAA Scale G1). NOAA Kp index breakdown Apr 03-Apr 05 2014 Apr 03 Apr 04 Apr 05 00-03UT 1 2 2 03-06UT 2 1 4 06-09UT 1 1 5 (G1) 09-12UT 2 1 4 12-15UT 2 1 3 15-18UT 1 1 3 18-21UT 1 2 3 21-00UT 1 2 3Lead Time: 57.17 hour(s) Difference: 6.67 hour(s) Prediction submitted by Leila Mays (GSFC) on 2014-04-03T00:30Z |
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