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Prediction for CME (2024-08-08T20:00:00-CME-001)CME Observed Time: 2024-08-08T20:00ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/32639/-1 CME Note: Halo CME first seen by SOHO LASCO C2 beginning at 2024-08-08T20:00Z, as well as in later frames by C3 and STEREO A COR2. The beginning of this event is not seen in STEREO A COR2 due to a data gap from 2024-08-08T19:38Z to 2024-08-08T22:53Z. The source of this CME is an X1.3 class flare from AR 3777 (S05W25) that peaked at 2024-08-08T19:36Z. This flare can be seen clearly in SDO AIA 94 and 131, along with an EUV wave seen in SDO AIA 193 and 211. Resulting field line opening is also visible in SDO AIA 171 and GOES SUVI 284. The arrival of this CME (or the combined front of this CME and 2024-08-08T05:30Z CME) is possibly seen around 2024-08-11T12:00Z. This weak arrival signature is characterized by a gradual increase of solar wind speed to around 510 km/s and rotation of magnetic field components, with Bz eventually reaching -18 nT. ~2024-08-11T12:00Z is likely the start of an interaction region or the sheath between the previous ICME arriving on 2024-08-10 and this CME. 2024-08-12T07:44Z is likely to be the arrival of the flux rope of this CME. Note that there is no shock in this arrival due to the interaction with the previous CME (courtesy of Carlos Peres Alanis, LASSOS team). CME Shock Arrival Time: 2024-08-11T12:00Z Observed Geomagnetic Storm Parameters due to CME: ---- Predicted Arrival Time: 2024-08-11T21:11Z (-10.0h, +10.0h) Confidence that the CME will arrive: 100.0% Predicted geomagnetic storm max Kp range due to CME: 3.0 - 5.0 Prediction Method: Ensemble WSA-ENLIL + Cone (NASA M2M) Prediction Method Note: Ensemble modeling estimates the spread/uncertainty in CME arrival time predictions using the WSA-ENLIL+Cone model due to uncertainties in CME input parameters. This is achieved by measuring N CME input parameters, then performing an ensemble of N runs of WSA-ENLIL cone model. This gives an ensemble of N CME arrival times and impact estimates. NASA GSFC SWRC ENLIL settings: ENLIL version: 2.7 Resolution: low2 (256x30x90) Ambient settings: a3b1f WSA version: 2.2 (Enlil 2.7 w/res:low2 ambient:a3b1f, WSA2.2) Please enter a copy of the entire notification here: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI ) ## Message Type: Space Weather Notification - CME update (ensemble) (STEREO A, Missions Near Earth) ## ## Message Issue Date: 2024-08-10T00:52:00Z ## Message ID: 20240810-AL-001 ## ## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This "Experimental Research Information" consists of preliminary NASA research products and should be interpreted and used accordingly. ## Summary: BETA PRODUCT. ENSEMBLE PRODUCT IS STILL IN DEVELOPMENT MODE. PLEASE LET US KNOW IF YOU HAVE ANY SUGGESTIONS FOR MODIFICATIONS. Ensemble modeling update on CME with ID 2024-08-08T20:00:00-CME-001 (see previous notification 20240809-AL-001). Based on analysis by the Moon to Mars Space Weather Analysis Office and heliospheric ensemble modeling carried out at the Community Coordinated Modeling Center, it is estimated that the CME may impact STEREO A. For 24 ensemble members (see notes section), simulations indicate that the leading edge of the CME will reach: - STEREO A between about 2024-08-11T03:05Z and 2024-08-11T16:45Z (average arrival 2024-08-11T09:22Z) for 87% of simulations. Additionally the CME is estimated to reach NASA missions near Earth between about 2024-08-11T11:28Z and 2024-08-12T07:12Z (average arrival 2024-08-11T21:11Z) for 100% of simulations. The ensemble-based forecast indicates that there is a 64% chance for the maximum Kp index to be in the 3-5 range (below minor to minor). Links to the ensemble details of the modeled event: https://iswa.gsfc.nasa.gov/ENSEMBLE/2024-08-09_ncmes1_sims24_LAHAINA063/20240808_200000_ncmes1_sims24_LAHAINA063_anim_tim-den.gif https://iswa.gsfc.nasa.gov/ENSEMBLE/2024-08-09_ncmes1_sims24_LAHAINA063/20240808_200000_ncmes1_sims24_LAHAINA063_arrival_Earth.gif https://iswa.gsfc.nasa.gov/ENSEMBLE/2024-08-09_ncmes1_sims24_LAHAINA063/20240808_200000_ncmes1_sims24_LAHAINA063_Earth_stack.gif https://iswa.gsfc.nasa.gov/ENSEMBLE/2024-08-09_ncmes1_sims24_LAHAINA063/20240808_200000_ncmes1_sims24_LAHAINA063_arrival_STA.gif https://iswa.gsfc.nasa.gov/ENSEMBLE/2024-08-09_ncmes1_sims24_LAHAINA063/20240808_200000_ncmes1_sims24_LAHAINA063_STA_stack.gif ## Notes: This CME event (2024-08-08T20:00:00-CME-001) is also predicted to impact Parker Solar Probe at 2024-08-11T00:53Z and Lucy at 2024-08-12T09:00Z (plus minus 7 hours) based on previous heliospheric modeling (see notification 20240809-AL-001). This CME event (2024-08-08T20:00:00-CME-001) is associated with X1.3 flare from AR 3777 (S04W23) with ID 2024-08-08T19:01:00-FLR-001 which peaked at 2024-08-08T19:35Z (see notifications 20240808-AL-002, 20240808-AL-003). Ensemble CME modeling at M2M is performed by building sets of initial CME parameters and carrying out separate simulations for each set. This approach allows a mapping of initial CME parameter uncertainties into a statistical characterization of CME arrival times and impact at locations of interest. Description of links: For each location, the first link shows the WSA-ENLIL+Cone model animation for the median CME input parameters, the second link shows the probabilistic distribution of predicted arrival times histogram, and the third link shows a stack plot of the WSA-ENLIL+Cone modeled magnetic field, velocity, density, and temperature for all ensemble members. For missions near Earth, a histogram of the probabilistic Kp forecast is also provided. For the full details of the modeled event, please go here: https://iswa.gsfc.nasa.gov/ENSEMBLE/2024-08-09_ncmes1_sims24_LAHAINA063/Detailed_results_20240808_200000_ncmes1_sims24_LAHAINA063.txt Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information (CCMC DONKI) Disclaimer Data and/or information stored within the CCMC DONKI is provided "as is" without any warranty of any kind, either expressed, implied, or statutory, including, but not limited to, any warranty that the data and/or information will conform to specifications, any implied warranties of merchantability, fitness for a particular purpose, or freedom from infringement, any warranty that the information will be error free, or any warranty that documentation, if provided, will conform to the data and/or information. In no event shall the United States Government, or its contractors or subcontractors, be liable for any damages, including, but not limited to, direct, indirect, special or consequential damages, arising out of, resulting from, or in any way connected with this information, whether or not based upon warranty, contract, tort, or otherwise, whether or not injury was sustained by persons or property or otherwise, and whether or not loss was sustained from, or arose out of the results of, or use of, the data and/or information. The United States Government disclaims all warranties and liabilities regarding third party data and/or information, if present in the data and/or information generated and/or compiled by CCMC DONKI, and distributes it "as is". Use of data and/or information stored within the CCMC DONKI does not, in any manner, constitute an endorsement by NASA of any test results, resulting designs, hardware, or other matters. Use of data and/or information stored within the CCMC DONKI does not, in any manner, constitute the grant of a license to RECIPIENT under any NASA copyright, patent, patent application or other intellectual property. The terms of this disclaimer shall be construed, and the legal relations between the parties hereto shall be determined, in accordance with United States federal law. NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This "Experimental Research Information" consists of preliminary NASA research products and should be interpreted and used accordingly.Lead Time: 38.50 hour(s) Difference: -9.18 hour(s) Prediction submitted by Mary Aronne (M2M Office) on 2024-08-09T21:30Z |
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