CME ScoreBoard Header

CME Scoreboard

CME Scoreboard: Prediction Detail

Prediction for CME (2016-05-15T15:36:00-CME-001)

CME Observed Time: 2016-05-15T15:36Z
iSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/10657/-1
CME was not detected at Earth.
Observed Geomagnetic Storm Parameters due to CME:
----

Predicted Arrival Time: 2016-05-18T11:30Z (-12.0h, +12.0h)
Confidence that the CME will arrive: 30.0%
Predicted geomagnetic storm max Kp range due to CME: 4.0 - 7.0
Prediction Method: Other (SIDC)
Prediction Method Note:
:Issued: 2016 May 16 1250 UTC
:Product: documentation at http://www.sidc.be/products/meu
#--------------------------------------------------------------------#
# DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC     #
# (RWC Belgium)                                                      #
#--------------------------------------------------------------------#
SIDC URSIGRAM 60516
SIDC SOLAR BULLETIN 16 May 2016, 1249UT
SIDC FORECAST (valid from 1230UT, 16 May 2016 until 18 May 2016)
SOLAR FLARES  : C-class flares expected, (probability >=50%)
GEOMAGNETISM  : Active conditions expected (A>=20 or K=4)
SOLAR PROTONS : Quiet
PREDICTIONS FOR 16 May 2016  10CM FLUX: 104 / AP: 012
PREDICTIONS FOR 17 May 2016  10CM FLUX: 100 / AP: 012
PREDICTIONS FOR 18 May 2016  10CM FLUX: 100 / AP: 016
COMMENT: Over the past 24 hours solar activity has been moderate. The
largest flare was a C3.2 class flare. Active Region (AR) 2542 (Macintosh
class:Cai; Mag. type:Beta) produced the largest flare, the C3.2 class
flare, peaking at 16:03 UT yesterday. ARs 2544 (Dai; Beta-gamma) and 2545
(Cao; Beta) also produced a couple of B and C class flares. AR 2544 has
exhibited significant flux emergence and cancellation in HMI observations,
which may lead to further flares. A partial halo CME with angular width of
158 degrees and a speed 538 km/s (as measured by the CACTUS automated CME
detection algorithm) was observed at 15:24 UT yesterday. The CME was
produced from a filament eruption that occurred in the Western hemisphere
(N10W62), near the solar limb. The eruption was associated with the above-
mentioned C3.2 flare. The CME is largely orientated to the West, however,
an Earth directed component may be expected to interact with the Earth
system on 18-May-2016 at 16:30 UT +/- 12 hours. Solar protons have remained
at background levels over the past 24 hours, with a small peak at 21:00 UT
yesterday evening, which may have been related to the above mentioned CME.
Solar activity is expected to remain moderate over the next 24 hours with a
high probability of C-class flares and a medium probability of M-class
flares.
The solar wind speed has increased from around 400 to 550 km/s over the
past 24 hours. The total magnetic field strength has remained around 9 nT.
The Bz component fluctuated between -9 and +9 nT. The fluctuating magnetic
field may lead to increased geo-activity over the coming day. Geomagnetic
conditions ranged between Kp index 2-4 (NOAA) and local K index 1-4
(Dourbes) over the past 24 hours. A positive polar coronal hole is
currently positioned in the Western hemisphere of the Sun and the resulting
high-speed stream (HSS) may enhance solar wind speeds later today and as a
consequence may increase geo-activity levels. The CME produced at 15:24 UT
on 15-May-2016 may also increase geo-activity at the Earth around 16:30 UT
(+/- 12 hours) on 18-May-2016.
TODAY'S ESTIMATED ISN  : 064, BASED ON 19 STATIONS.

SOLAR INDICES FOR 15 May 2016
WOLF NUMBER CATANIA    : ///
10CM SOLAR FLUX        : 108
AK CHAMBON LA FORET    : 021
AK WINGST              : 016
ESTIMATED AP           : 016
ESTIMATED ISN          : 085, BASED ON 31 STATIONS.

NOTICEABLE EVENTS SUMMARY
DAY BEGIN MAX  END  LOC    XRAY OP  10CM Catania/NOAA RADIO_BURST_TYPES 
NONE
END

BT

#--------------------------------------------------------------------#
# Solar Influences Data analysis Center - RWC Belgium                #
# Royal Observatory of Belgium                                       #
# Fax : 32 (0) 2 373 0 224                                           #
# Tel.: 32 (0) 2 373 0 491                                           #
#                                                                    #
# For more information, see http://www.sidc.be.  Please do not reply #
# directly to this message, but send comments and suggestions to     #
# 'sidctech@oma.be'. If you are unable to use that address, use      #
# 'rvdlinden@spd.aas.org' instead.                                   #
# To unsubscribe, visit http://sidc.be/registration/unsub.php        #
#                                                                    #
# Legal notices:                                                     #
# - Intellectual Property Rights:                                    #
#   http://www.astro.oma.be/common/internet/en/data-policy-en.pdf    #
# - Liability Disclaimer:                                            #
#   http://www.astro.oma.be/common/internet/en/disclaimer-en.pdf     #
# - Use and processing of your personal information:                 #
#   http://www.astro.oma.be/common/internet/en/privacy-policy-en.pdf #
#--------------------------------------------------------------------#
Lead Time: 25.23 hour(s)
Difference: -----
Prediction submitted by Leila Mays (GSFC) on 2016-05-17T10:16Z
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