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 | meu |
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Latest issue
:Issued: 2026 Jul 14 1231 UTC :Product: documentation at http://www.sidc.be/products/meu #--------------------------------------------------------------------# # DAILY BULLETIN ON SOLAR AND GEOMAGNETIC ACTIVITY from the SIDC # # (RWC Belgium) # #--------------------------------------------------------------------# SIDC URSIGRAM 60714 SIDC SOLAR BULLETIN 14 Jul 2026, 1230UT SIDC FORECAST SOLAR FLARES : C-class flares expected, (probability >=50%) GEOMAGNETISM : Active conditions expected (A>=20 or K=4) SOLAR PROTONS : Quiet PREDICTIONS FOR 14 Jul 2026 10CM FLUX: 100 / AP: 010 PREDICTIONS FOR 15 Jul 2026 10CM FLUX: 099 / AP: 020 PREDICTIONS FOR 16 Jul 2026 10CM FLUX: 098 / AP: 008 Solar Active Regions and flaring: Solar flaring activity has been low over the past 24 hours, with few C-class flares. The strongest flare was a C1.5 flare (SIDC Flare 8200) peaking at 09:56 UTC on July 14, associated with SIDC Sunspot Group 910 (NOAA Active Region 4482, magnetic type alpha). There are currently three numbered active regions on the solar disk, all with alpha magnetic configuration. SIDC Sunspot Group 909 (NOAA Active Region 4485) has rotated behind the west limb. SIDC Sunspot Group 914 and SIDC Sunspot Group 915 (NOAA Active Region 4448) have decayed into plage. The solar flaring activity is expected to be low over the next 24 hours, with C-class flares very likely and a small chance for M-class flares. Coronal mass ejections: A Coronal Mass Ejection (SIDC CME 687) was observed in LASCO/C2 coronagraph imagery, lifting off from the southeast limb starting from 19:36 UTC on July 13. It is likely a backsided event that is not expected to impact Earth. No other Earth-directed CMEs were observed in the available coronagraph imagery during the last 24 hours. Solar wind: Over the last 24 hours, the solar wind parameters (SOLAR-1 and ACE) reflected mostly slow solar wind conditions. The solar wind speed decreased from 430 km/s to around 360 km/s. The interplanetary magnetic field was between 5 nT and 10 nT. The Bz component varied between -6 nT and 5 nT. The interplanetary magnetic field angle phi was predominantly in the negative sector. Mostly slow solar wind conditions are expected over the next 24 hours. There is a chance for enhanced conditions in case of high- speed stream arrivals from the southern, positive polarity coronal holes (SIDC Coronal Holes 172 and 173) and a late glancing blow arrival associated with SIDC CME 686. Geomagnetism: Geomagnetic conditions globally were mostly quiet (NOAA Kp 2- to 2), with an interval of active conditions (NOAA Kp 4- ) between 21:00 UTC on July 13 and 00:00 UTC on July 14. Geomagnetic conditions locally were mostly at unsettled levels (K Bel 3) until 01:00 UTC on July 14, decreasing then to quiet (K Bel 1 to 2). Mostly quiet to unsettled conditions (NOAA Kp 2 to 3) are expected over the next 24 hours. There is with a chance of isolated active or minor storm intervals (NOAA Kp 4 to 5), in case of high-speed stream arrivals from the southern, positive polarity coronal holes (SIDC Coronal Holes 172 and 173) and a late glancing blow arrival associated with SIDC CME 686. Proton flux levels: The greater than 10 MeV proton flux was below the 10 pfu threshold during the past 24 hours. It is expected to remain below the threshold level over the next 24 hours. Electron fluxes at GEO: The greater than 2 MeV electron flux measured by GOES 18 was above the 1000 pfu threshold between 15:00 UTC and 23:10 UTC on July 13. The greater than 2 MeV electron flux measured by GOES 19 was above the 1000 pfu threshold between 13:00 UTC and 18:45 UTC on July 13. The greater than 2 MeV electron flux is expected to remain below the 1000 pfu threshold over the next 24 hours. The 24-hour electron fluence was at normal levels and it is expected to remain so over the next 24 hours. TODAY'S ESTIMATED ISN : 037, BASED ON 23 STATIONS. SOLAR INDICES FOR 13 Jul 2026 WOLF NUMBER CATANIA : 059 10CM SOLAR FLUX : 103 AK CHAMBON LA FORET : 015 AK WINGST : 010 ESTIMATED AP : 011 ESTIMATED ISN : 044, BASED ON 33 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 # # # # Website http://www.sidc.be. # # E-mail sidc-support@oma.be # # To unsubscribe http://www.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 # #--------------------------------------------------------------------#
Details
The SIDC ursigram starts with the code SIDC URSIGRAM YMMDD, whereY is the last digit of the year number,
MM is the number of the month,
DD is the day of the month.
A forecast is given on:
the global flare probability,
geomagnetic disturbances,
solar proton events.
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
COMMENT
ESTIMATED ISN : xxx, based on xx stations.
where ISN stands for International Sunspot Number.
OBSERVED SOLAR INDICES FOR THE DAY BEFORE
SUNSPOT INDEX : xxx, the Wolf number observed by Catania
10CM SOLAR FLUX : xxx,
AK CHAMBON LA FORET : xxx,
AK WINGST : xxx,
ESTIMATED AP : xxx,
ESTIMATED ISN : xxx, based on xx stations.
NOTICEABLE EVENTS SUMMARY
DAY BEGIN MAX END LOC XRAY OP 10CM TYPE Catania NOAA NOTE
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.
