SIDC ursigram

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

Latest issue

:Issued: 2024 May 13 1258 UTC
:Product: documentation at http://www.sidc.be/products/uge
#--------------------------------------------------------------------#
# DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC     #
#--------------------------------------------------------------------#
SIDC URSIGRAM 40513
GEOALERT BRU134
UGEOA 30512 40513 1258/ 9930/ 
12132 21132 30132 
99999
PLAIN

Solar Active Regions and flaring: Solar flaring activity was high during
the last 24 hours with almost all registered activity emitted from NOAA
Active Region (AR) 3664 (magnetic configuration Beta-Gamma-Delta, Catania
sunspot group 86). The most notable activity was an X1.0 flare detected
yesterday at 16:26 UTC, an M6 flare today at 09:44 UTC and an M4 yesterday
at 20:32 UTC. NOAA AR 3676 (magnetic configuration Beta-Gamma) and 3679
(magnetic configuration Alpha) became active during the past 24 hours,
producing an M1 flare each. Further M-class flaring activity is expected
from NOAA AR 3664 and probably from NOAA AR 3676 and 3679. X-class flaring
activity form NOAA AR 3664 is also possible in the next 24 hours.

Coronal mass ejections: No Earth-directed Coronal Mass Ejections (CME) were
observed in the last 24 hours.
Two CME observed yesterday at 02:00 UTC and 03:48 UTC are not likely to be
Earth-directed.

Solar wind: During the last 24 hours the Solar Wind (SW) speed remained
high, however, the magnetic conditions have returned to undisturbed levels.
The SW speed dropped from 980 to 620 km/s, while the total interplanetary
magnetic field (Bt) varied between 3 to 11 nT. The North-South magnetic
component (Bz) ranged between -9 and 9 nT, while the interplanetary
magnetic field phi angle was predominantly directed away from the Sun. In
the next 24 hours the SW speed is expected to drop gradually and the
geomagnetic conditions to remain mild. One or two glancing blows from
passing Coronal Mass Ejections (CME) are expected in the next 24 hours, but
they will most likely have a very minor effect.

Geomagnetism: The global geomagnetic conditions reached moderate storm
levels (NOAA Kp 6- to 6+) during the period from 12 May 21:00 UTC to 13 May
06:00 UTC but they have since dropped to unsettled levels (NOAA Kp 3-). The
local geomagnetic conditions reached minor storm levels (K BEL 5) yesterday
at 21:00-24:00 UTC but they also now dropped to unsettled (K BEL 3) levels.
In the next 24 hours, they are likely to remain at the same levels and
possibly increase to active levels (K=4) for short periods of time, both
globally and locally.

Proton flux levels: The greater than 10 MeV proton flux, as measured by the
GOES-18 satellite, continue its drop and was below the 10 pfu threshold
level during the last 24 hours. It is likely that it will continue its
gradual drop in the next 24 hours, however, there is a chance of a new
proton event and an increase in flux above the alert level.

Electron fluxes at GEO: The greater than 2 MeV electron flux, as measured
by the GOES-18 satellite, was below the 1000 pfu alert level during the
last 24 hours and is expected to remain below this threshold during the
next 24 hours. The 24h electron fluence was at low levels during the past
24 hours and is expected to remain at these levels for the following 24
hours.




TODAY'S ESTIMATED ISN  : 227, BASED ON 18 STATIONS.
UGEOI 30512 40513 1258/ 12/// 
1//// 2222/ 3046/ 4//// 8//// 9//// 
99999
UGEOR 30512 40513 1258/ ///// ///// 
99999
USSPS 31405 13070 25242 01003 30808 11307 02012 20621 24418 03005 25013
21306 04002 16008 12302 05002 17417 13402 06004 27418 24404 07003 18014
2/801 86065 37719 59613 92007 43427 2/803 93004 41120 21307 94005 41423
25407 95006 11419 22305 96002 23809 2/801 97008 34614 25413 98001 34203
0/101 99001 41326 01202
UMAGF 30503 40513 1004/ 12062 1/044 23322 34545
UMAGF 31523 40513 0000/ 12003 1/046 26644 33356
BT
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Details

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