|
|
Prediction for CME (2022-03-07T00:12:00-CME-001)CME Observed Time: 2022-03-07T00:12ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/19367/-1 CME Note: This CME is first seen as a faint partial halo to the NW in SOHO LASCO C2 (later in C3) and followed by a more bright and slightly more narrow shape to the W/NW in STEREO A COR2. The source of this CME is an eruption to the E/SE of AR12958 (N17W28) stretching across multiple longitudes from ~W20 to ~W45 based off of the dimming signature seen in SDO/AIA 193. The eruption is best seen in the SDO/AIA 193, 211, 94, 335, and STEREO A EUVI 195 wavelengths. From STEREO A's point of view, the eruption appears as opening field lines along the Eastern limb, while in SDO/AIA's point of view, the eruption is more clear with dimming, a post-eruptive arcade, and a brief EUV wave (seen best in SDO/AIA 211). UPDATE (2022-03-11T14:50Z): Arrival Field indicated by enhancement exceeding 10 nT, accompanied by field component rotation. Preceded by pileup, followed by slight speed increase. Temperature data inconclusive. CME Shock Arrival Time: 2022-03-10T18:37Z Observed Geomagnetic Storm Parameters due to CME: Max Kp: 4.0 Predicted Arrival Time: 2022-03-10T15:00Z (-6.0h, +6.0h) Confidence that the CME will arrive: 60.0% Predicted geomagnetic storm max Kp range due to CME: 4.0 - 5.0 Predicted Dst min. in nT: -30 Prediction Method: WSA-ENLIL + Cone (BoM) Prediction Method Note: A slow coronal mass ejection associated with a filament eruption NW solar quadrant. Enlil model run indicates CME speed is just above background wind speed and a possible glancing blow, uncertain of degree of geoeffectiveness, solar longitude location is quite good, perhaps a bit high in latitude, but the slow speed of the CME and limited visibility in C3 difference images using CAT somewhat reduces confidence, along with a north-east direction evident in C2 imagery. The CME was quite visible in STEREO A difference imagery though perhaps expansion appeared to be only moderate.Lead Time: 66.18 hour(s) Difference: 3.62 hour(s) Prediction submitted by Duty Forecaster (ASWFC) on 2022-03-08T00:26Z |
|
CCMC
Rules of the Road: CCMC requests that users notify the CCMC, CME
model/technique developers and submitting forecasters/researchers before
performing event and validation studies with data from the CME Arrival
Time Scoreboard. It is recommended that such studies be performed with
the knowledge and collaboration of developers and submitting
forecasters/researchers. Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Policy |