SOHO/LASCO Halo CME  20170910

COMMENTS:  Asymmetric HALO CME resulting from a long duration (LDE) X8.2 class X-ray flare of
                          active region 12673 located [S08, W88] as seen in SDO AIA 193A.
                          LASCO velocity:  3287.6 km/sec at PA 253 degrees.  Acceleration: *****
                          SEP (Solar Energetic Particle) event.  Extreme Increased proton flux seen in the LASCO images.

Halo Alert: halo-message.20170910



UCMEO 93001 70911 1739/
70910 61600 81818 2531/ 252// 333// 33288
70910 61545 81651 38808 12673 1112/
99999

PLAIN


SOHO/LASCO  HALO CME September 10, 2017 

C2 Start Time:   16:00 UT

C3 Start Time: 16:06 - 18:18 UT 

Type of CME:
Asymmetric HALO CME — FRONTSIDE
pa1:  253      pa2:  252       Total Width:  360 degrees

Velocity Measurements:

C2 1 points  ****.* km/sec @ PA 253
C3 5 points  3212.4 km/sec @ PA 253
Average through both fields:   3287.6 km/sec  Acceleration:  

COMMENT:   AIA 193 shows a long duration (LDE) impulsive flare event
              of AR 12673 at location [S08, W88] beginning 15:45 - 16:51 UT.
              The event produces an EUV wave and a dimming across the disk,
              followed by a post loop arcade.
           
            LASCO shows extreme proton flux in the field of view (SEP).

            STEREO Beacon Data
            COR2 A, in progress 16:24 - 16:40 UT; shows an asymmetric HALO CME
            Preliminary time/height measure gives 2630.4 km/sec @ 110 degrees.
                       
NOAA/GOES reports a X8.2 class X-ray flare of AR12673 15:35/16:06/16:31 UT.
NOAA/GOES shows an increase in proton particles with flux >100 MeV
            and surpasses solar storm threshold conditions.
                    
           
Preliminary UCMEO velocity and position measurements will be delivered first.
Images, movies, and time/height information for this event will be available at:

http://umbra.nascom.nasa.gov/lasco/observations/halo/2017/170910/


 Best Regards,

--Nick Padgett


BT


[Images from original message are omitted here]

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SOHO/LASCO C2 Diff
SOHO/LASCO C3 Diff
SOHO/LASCO C2
20170910_162408_c2_rdiff.gif
20170910_165407_c3_rdiff.gif
20170910_1624_c2.png
STEREO/COR2 AHEAD
SDO/AIA 193 Diff
STEREO/COR2 AHEAD
20170910_163924_scc_cor2_ahead_rdiff.gif
20170910_155704_aia_rdiff_512.gif
20170910_162424_scc_cor2_ahead.jpg
SDO/AIA 193

SOHO/LASCO C3
20170910_155704_aia_193.gif
20170910_1654_c3.png


SOHO/LASCO C2
20170910_1736_D2_combo.gif
SOHO/LASCO C3
20170910_1706_D3_combo.gif
SDO/AIA 193
20170910_155704_aia_193_combo.gif



Time/Height Velocities and Plots

C2/C3
20170906_c2c3_ht.png

Click on Links below for additional information.
      

ENUL Forecast Model

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

ENUL-2.7 20170910 Time/Density
ENUL Time Density Plot



MPEG Movies



Additional Information

LASCO Software IDL Save Files (.mvi)






  • Please, send questions and comments to Kevin Schenk