GEOALERT SIDC

3-day-forecast of solar and geomagnetic activity.
Source SIDC (RWC-Belgium)
Frequency Daily
Format Encoded data (ISES)
Mail header GEOALERT SIDC
SIDC code xut

Latest issue

:Issued: 2024 May 18 1231 UTC
:Product: documentation at http://www.sidc.be/products/xut
#--------------------------------------------------------------------#
# GEOALERT message from the SIDC (RWC-Belgium)                       #
#--------------------------------------------------------------------#
GEOALERT BRU139
UGEOA 30512 40518 1231/ 9930/ 
12182 21182 30182 
99999
PLAIN
PREDICTIONS FOR 18 May 2024  10CM FLUX: 215 / AP: 013
PREDICTIONS FOR 19 May 2024  10CM FLUX: 210 / AP: 009
PREDICTIONS FOR 20 May 2024  10CM FLUX: 208 / AP: 006

Solar Active Regions and flaring: Solar flaring activity was high during
the last 24 hours, with an M7 flare emitted from NOAA Active Region (AR)
3685 (magnetic configuration Beta-Gamma, Catania sunspot group 9) yesterday
at 21:08 UTC. The second brightest X-ray flare of the past 24 hours was a
C7 from NOAA AR 3679 (magnetic configuration Beta-Gamma, Catania sunspot
group 6). NOAA AR 3671 (magnetic configuration Beta, Catania sunspot group
93) and NOAA AR 3686 (magnetic configuration Alpha, Catania sunspot group
11) produced the remaining of the C-class flaring activity. For the next 24
hours, the pair of NOAA AR 3685 and 3686 is expected to continue producing
M-class flares with a chance of an X-class flare.

Coronal mass ejections: No Earth directed Coronal Mass Ejections (CME) have
been observed in the available coronagraph data.
A partial halo CME seen in SOHO/LASCO-C2 images as launched yesterday at
12:48 UT is judged to be a back-sided event.

Solar wind: The Solar Wind (SW) conditions were disturbed by a Coronal Mass
Ejection (CME)-induced shock yesterday at 12:40 UTC. The CME itself
followed a few minutes later. This is most likely the CME expected to
arrive as glancing blow yesterday evening. The SW speed peaked to 520 km/s
because of the arrival of the disturbance. The total interplanetary
magnetic field (Bt) increased to 17 nT but has decline significantly now.
The North-South magnetic component (Bz) fluctuated between -15 and 13 nT
during the CME disturbance. The interplanetary magnetic field phi angle
turned to the direction of the Sun as a result of the CME arrival and
stayed predominantly to this direction. The effects of the CME are expected
to diminish in the next 24 hours.

Geomagnetism: The global geomagnetic conditions reached storm levels
yesterday (NOAA Kp: 5 15:00-18:00 UTC, 6 18:00-21:00 UTC, 5+ 21:00-24:00
UTC) and now fluctuate between quiet and unsettled levels. Locally the
conditions also increased to the minor storm level (K BEL 5) yesterday at
18:00-21:00 UTC and now fluctuate between quiet and unsettled levels. For
the next 24 hours the geomagnetic conditions are expected to vary between
active and quiet levels both globally and locally.

Proton flux levels: The greater than 10 MeV proton flux, as measured by the
GOES-18 satellite, continued its drop during the past 24 hours and is now
in low levels. It is likely that it will remain at low levels in the next
24 hours, however, there is a small chance of a new proton event and an
increase in flux above the 10 pfu alert level.

Electron fluxes at GEO: The greater than 2 MeV electron flux, as measured
by the GOES-18 satellite, increased during the past 24 hours and reached
the 1000 pfu alert threshold momentarily. This was most likely a localised
event as it lasted for a very short time and was not observed by GOES-16.
Hence, the electron flux is expected to remain at low levels in the next 24
hours.
The 24h electron fluence increased but remained at normal levels during the
past 24 hours. It is expected to decrease further in the next 24 hours.


TODAY'S ESTIMATED ISN  : 167, BASED ON 12 STATIONS.
99999
UGEOI 30512 40518 1231/ 17/// 
10193 22041 3031/ 4//// 80412 90920 
99999

NOTICEABLE EVENTS SUMMARY
DAY BEGIN MAX  END  LOC    XRAY OP  10CM Catania/NOAA RADIO_BURST_TYPES 
17  2033  2108 2126 S12E62 M7.2 2B       09/3685      II/2IV/2 
END

UGEOR 30512 40518 1231/ ///// ///// 
99999
USSPS 32404 16108 16922 62003 47828 2/801 63002 45221 21302 64002 42719
21304 65000 45223 01204 66001 30408 2/801 67006 20712 31306 69004 33819
21304 71012 22808 24511 72000 13018 0/101 74001 13714 2/802 75002 31323
11307 76018 27513 21406
USSPS 21305 16172 23732 87006 47728 3/801 89012 45720 21406 90007 43318
31306 92002 30808 3/802 93019 20113 21331 95013 33921 31306 96033 22312
51516 99002 12418 0/103 01008 13918 31313 02007 31223 31310 04004 25506
01204 03057 26614 21408 05006 28505 3/801
UMAGF 30503 40518 1004/ 17063 1/037 22234 35433
UMAGF 31523 40518 0000/ 17001 1/031 22323 34565
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Details

The Geoalert message starts with the code GEOALERT BRUXXX, where xxx is the day-of-the-year number.
Besides the ISES codes like UGEOA, UGEOI, UGEOR and USSPS, this message contains the following information:
PLAIN
PREDICTIONS FOR "today" : 10CM FLUX: xxx / AP: xxx
PREDICTIONS FOR "today+1": 10CM FLUX: xxx / AP: xxx
PREDICTIONS FOR "today+2": 10CM FLUX: xxx / AP: xxx
99999
This gives the predicted 10.7 cm radioflux and the predicted Ap index for 3 days starting on the date of the message
NOTICEABLE EVENTS SUMMARY
DAY BEGIN MAX END LOC XRAY OP 10CM TYPE Catania NOAA NOTE

This is the header of a table that lists all major events.
DAY gives the day-of-the-month.
BEGIN, MAX and END give the UT time of the different phases of the X-ray output of the event.
LOC gives the location of the event in heliographic coordinates.
XRAY gives the GOES X-ray class of the event.
OP lists the optical flare class.
10cm gives the 10.7 cm radioflux output of the event.
TYPE specifies the type of radiobursts observed.
Catania gives the Catania sunspot group number where the event happened.
NOAA is the corresponding NOAA active region number.
NOTE is the header of any other type of information, e.g. if a CME was observed associated with the event.


Check the ISES code book for information on ISES codes.