CME ScoreBoard Header

CME Scoreboard

CME Scoreboard: Prediction Detail

Prediction for CME (2016-11-05T04:48:00-CME-001)

CME Observed Time: 2016-11-05T04:48Z
iSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/11494/-1
CME Note: Filament Eruption off the northern Hemisphere giving a very wide-angle partial halo. Another CME came off the farside and eastern limb at a similar time. Evident in SOHO and STEREO imagery after 05/0200UTC.
CME Shock Arrival Time: 2016-11-09T05:28Z
Observed Geomagnetic Storm Parameters due to CME:
Max Kp: 5.0

Predicted Arrival Time: 2016-11-08T10:00Z
Predicted geomagnetic storm max Kp range due to CME: 5.0 - 5.0
Prediction Method: WSA-ENLIL + Cone (NOAA/SWPC)
Prediction Method Note:
Product: Forecast Discussion
Issued: 2016 Nov 06 0030 UTC
Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction
Center

Solar Activity

.24 hr Summary...
Solar activity was very low and Regions 2605 (N08W48, Bxo/beta) and 2606
(N11E36, Axx/alpha) were stable throughout the period.  A filament
eruption centered near N24W15 was observed in SDO 193 imagery between
05/0200-0500 UTC and an associated CME was observed in C2 coronagraph
imagery beginning at 05/0424 UTC.  Forecaster analysis and ENLIL model
output suggest CME arrival early on day three (08 Nov); see geomagnetic
forecast for additional details.

.Forecast...
Solar activity is expected to continue at very low levels over the next
three days (06-08 Nov).

Energetic Particle

.24 hr Summary...
The greater than 2 MeV electron flux reached high levels this period
with a peak flux of 3,750 pfu observed at 05/1615 UTC.  The greater than
10 MeV proton flux was steady at background levels.

.Forecast...
The greater than 2 MeV electron flux is expected to reach high levels on
day one and two (06-07 Nov) but is expected to decrease to normal levels
on day three (08 Nov) in response to elevated geomagnetic field
activity.

Solar Wind

.24 hr Summary...
Solar wind parameters were at background levels this period.  Total
field strength values varied between 2-5 nT and the Bz component was
generally northward.  Solar wind speeds were steady between 320-375 km/s
and the phi angle was in a positive (away) solar sector orientation.

.Forecast...
Solar wind parameters are expected to continue at background levels on
days one and two (06-07 Nov).  The onset of a positive polarity CH HSS
combined with the anticipated arrival of the 05 Nov CME on day three (08
Nov) is expected to enhance the near-Earth solar wind environment.

Geospace

.24 hr Summary...
The geomagnetic field was quiet under a background solar wind
environment.

.Forecast...
The geomagnetic field is expected to be quiet on days one and two (06-07
Nov) under a nominal solar wind regime.  The weak influence of a
positive polarity CH HSS combined with the anticipated arrival of the 05
Nov CME is expected to cause periods of active field conditions, with a
chance for G1 (Minor) geomagnetic storms, on day three (08 Nov).

Thank you for using the Product Subscription Service. If you would like to remove a product subscription or update the personal information in your account, go to the Product Subscription Site. Please do not use the from address for correspondence, as it is not monitored. For comments or help, please contact SWPC Help.
Lead Time: 76.97 hour(s)
Difference: 19.47 hour(s)
Prediction submitted by Barbara Thompson (GSFC) on 2016-11-06T00:30Z
CME Scoreboard Footer

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.

If you are looking for the official U.S. Government forecast for space weather, please go to NOAA's Space Weather Prediction Center (https://swpc.noaa.gov). This "Experimental Research Information" consists of preliminary NASA research products and should be interpreted and used accordingly.

Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Collection Consent Agreement