SOHO/LASCO Halo CME  20251111

COMMENTS:  Asymmetric HALO CME resulting from a X5.1 class X-ray flare of AR 14274
                          centered at location [N23, W27]. 
                          LASCO velocity:  1671.4 km/sec at PA 324 degrees.  Acceleration: 209.76 m/sec^2.
                  
                   A Solar Energetic Particle (SEP) event is detected by GOES with Flux > 100MeV proton particles.
                         

Halo Alert: halo-message.20251111



UCMEO 93001 51111 1915/
51111 71024 81442 3341/ 333// 333// 41671
51111 60951 81021 42423 14274 1112/
99999

PLAIN


SOHO/LASCO   HALO CME NOVEMBER 11, 2025

C2 Start Time:      10:24 UT

C3 Start Time:      10:30 - 14:42 UT 

Type of CME:
FULL  HALO CME — FRONTSIDE
pa1:  334      pa2:  333       Total Width:  360 degrees

Velocity Measurements:

C2    1 points     Could not measure C2
C3    6 points     1671.4 km/sec @ PA 324
          Only C3 FOV:      1671.4 km/sec  Acceleration: 209.76 m/sec^2. 

COMMENT:  SDO AIA 193 shows a flare from AR 14274 09:51 - 10:21 UT at location
             [N23, W24].  The flare produces an amazing global EUV wave
                        and a dimming that spans ~80% of the Northern Hemisphere
            along with a post loop arcade.
       
        Increased proton particles seen in the LASCO C2 and C3 fields of view.
           
        A Solar energetic particle (SEP) event detected by GOES.
         Flux of > 100MeV proton exceeds 1 pfu beginning 2025-11-11 10:20 UT         
 
            STEREO Beacon Data
            COR2 A, 10:23 - 11:38 UT; shows an asymetric HALO CME over the Northeast.
            Preliminary time/height measure gives 1852.0 km/sec @ 060 degrees.
                              

NOAA/GOES reports a X5.1 class X-ray flare from AR 14274 09:49/10:04/10:17 UT
          
Preliminary UCMEO velocity and position measurements are delivered first.
Images, movies, and time/height information for this event will soon be available at:

https://umbra.nascom.nasa.gov/lasco/observations/halo/2025/251111a/


Best Regards,

--Kevin Schenk

BT


[Images from the original alert message are omitted here]



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SOHO/LASCO C2 Diff
SOHO/LASCO C3 Diff
SDO AIA 195 angstrom
20251111_102420_c2rdiff.gif
20251111_110611_c3rdiff.gif 20251111_100607_aia_193.gif
GOES-19 CCOR1 SDO AIA  195 angstrom  Diff STEREO/COR2 AHEAD Diff
20251111_0000_goes-19_CCOR1.jpeg 20251111_100304_aia_193_rdiff.gif 20251111_112354_scc_cor2_ahead_rdiff.gif
SOHO/LASCO C2 SOHO/LASCO C3 GOES-19 SUVI 195A
20251111_1124_c2.png 20251111_1130_c3.png 20251111_or_suvi-l2-ci195_g19_s20251111T101200Z_e20251111T101600Z_v1-0-2.png


SOHO/LASCO C2
20251111_1100_D2_combo.gif
SOHO/LASCO C3
20251111_1218_D3_combo.gif
SDO AIA TRI-211 / 193 / 171 Angstrom
20251111_sdo_aia_tri_1.png



Time/Height Velocities and Plots

C2/C3
20250830_c2c3_ht.png

Click on Links below for additional information.
     

ENUL Forecast Model(TO DO)

Courtesy of Community Coordianted Modeling Center (CCMC) and the Space Weather Research Center (SWRC)

ENUL-2.7 20251111 Time/Density
ENUL Time Density Plot



MPEG Movies



Additional Information

LASCO Software IDL Save Files (.mvi)






  • Please, send questions and comments to Kevin Schenk