SPACE WEATHER INFORMATION AND FORECAST SERVICESS

Center for Space Research
The National Research and Innovation Agency
BRIN - Indonesia

2026 Feb 13

Geomagnet

Quiet

Ionosphere

Quiet

Forecast

Geomagnet

Quiet

Ionosphere

Quiet

Issued : 2026 February 14 0800 UTC
Forecast Valid For 24 Hours

ESSENTIAL INFORMATION FOR SPACE WEATHER COMMUNITIES

HF Radio Communication

MUF Depression

Shortwave Fadeout / Radio Blackout

Application

NAVIGATION

Error Positioning

SATELLITES

High Energy Proton

High Energy Electron

Detailed Information

Solar Activity

Solar activity was eruptive in the last 24 hours. 
 
There were 3 flares with all of them are C-class flares in the last 24 hours. The maximum flare class was C1.1 from NOAA4366 peaked at 7:40UT. There were 2 solar radioburst all of which are type-III occurred in the last 24 hours. There was 4 CME event in the last 24 hours. The east-directed CME has the highest median velocity of 272 km/s with an angular width of 20 degrees and the west-directed CME has the highest median velocity of 428 km/s with an angular width of 30 degrees. The latest SDO/HMI Intensitygram data shows 7 active regions (NOAA4367,4368,4369,4371,4373,4374,4375) and the latest BBSO H-Alpha data shows 1 H-Alpha plages (NOAA4370). Based on farside data shows 2 Regions Due to Return 13 Feb to 15 Feb from the east limb of the Solar disk.

Based on today's condition, solar activity for 
February 13th, 2026 04:00 UT - February 14th, 2026 03:59 UT is predicted to be eruptive.
February 14th, 2026 04:00 UT - February 15th, 2026 03:59 UT is predicted to be eruptive.
February 15th, 2026 04:00 UT - February 16th, 2026 03:59 UT is predicted to be eruptive.
February 16th, 2026 04:00 UT - February 17th, 2026 03:59 UT is predicted to be eruptive.

Geomagnetic Activity

The geomagnetic activity was on quiet level for the last 24 hours.

The solar wind speed decrease from 363 km/s to 537 km/s, north-south component of interplanetary magnetic field fluctuate between -6.8 nT and 6.5 nT. There was geoeffective coronal hole at central equator, while the others at eastern equator, north-west and south-west were not geoeffective. CME on 12 February 2026 13:36 UT was mainly errupted toward south-west with speed of 428 km/s and angular width of 30°. The CME was geoeffective and is likely to have impact on 20 February 2026.

Quiet level geomagnetic activity is expected for 13 February 2026 04:00UT - 14 February 2026 03:59UT.
Quiet level geomagnetic activity is expected for 14 February 2026 04:00UT - 15 February 2026 03:59UT.
Quiet level geomagnetic activity is expected for 15 February 2026 04:00UT - 16 February 2026 03:59UT.
Quiet level geomagnetic activity is expected for 16 February 2026 04:00UT - 17 February 2026 03:59UT.

Ionospheric Activity

Evaluation of the ionospheric activity, foF2 value, the increase in the fmin value, Spread-F, and the Sporadic E-Layer cannot be reported due to problems at the CADI station. However the S4 index values (condition of ionospheric scintillation) was on quiet level (S4<0.5) for the last 24 hours over Pontianak. TEC index was on quiet level (VTEC<125) for the last 24 hours over Pontianak.

The ionosphere activity on 13 February 2026, 04:00 UT - 14 February 2026, 03:59 UT is predicted to be quiet.

The ionosphere activity on 14 February 2026, 04:00 UT - 15 February 2026, 03:59 UT is predicted to be quiet.

The ionosphere activity on 15 February 2026, 04:00 UT - 16 February 2026, 03:59 UT is predicted to be quiet.

The ionosphere activity on 16 February 2026, 04:00 UT - 17 February 2026, 03:59 UT is predicted to be quiet.

Navigation

Based on TEC and scintilation , the error of the single frequency GPS positioning for  the last 24 hours was in normal level.

Based on ionospheric scintilation and TEC variation, the probability of error positioning on 13 February 2026, 04:00 UT - 14 February 2026, 03:59 UT is predicted at a normal level.

Based on ionospheric scintilation and TEC variation, the probability of error positioning on 14 February 2026, 04:00 UT – 15 February 2026, 03:59 UT is predicted at a normal level.

Based on ionospheric scintilation and TEC variation, the probability of error positioning on 15 February 2026, 04:00 UT - 16 February 2026, 03:59 UT is predicted at a normal level.

Based on ionospheric scintilation and TEC variation, the probability of error positioning on 16 February 2026, 04:00 UT - 17 February 2026, 03:59 UT is predicted at a normal level.

HF Radio Communication

The evaluation of MUF depression and Short Wave Fadeout (SWF) data can not be reported due to problems at the CADI station.

The MUF depression on 13 February 2026, 04:00 UT - 14 February 2026, 03:59 UT is predicted at quiet level due to previous of geomagnetic activity.

The MUF depression on 14 February 2026, 04:00 UT - 15 February 2026, 03:59 UT is predicted at quiet level due to previous of geomagnetic activity.

The MUF depression on 15 February 2026, 04:00 UT - 16 February 2026, 03:59 UT is predicted at quiet level due to previous of geomagnetic activity.

The MUF depression on 16 February 2026, 04:00 UT - 17 February 2026, 03:59 UT is predicted at quiet level due to previous of geomagnetic activity.

The SWF on 13 February 2026, 04:00 UT – 14 February 2026, 03:59 UT is predicted at quiet level due to the prediction of solar flare.

The SWF on 14 February 2026, 04:00 UT - 15 February 2026, 03:59 UT is predicted at quiet level due to the prediction of solar flare.

The SWF on 15 February 2026, 04:00 UT - 16 February 2026, 03:59 UT is predicted at quiet level due to the prediction of solar flare.

The SWF on 16 February 2026, 04:00 UT - 17 February 2026, 03:59 UT is predicted at quiet level due to the prediction of solar flare.

Satellites

The electron flux was on high level for the last 24 hours.

High level of electron flux is expected for 13 February 2026 04:00UT - 14 February 2026 03:59UT.
Low level of electron flux is expected for 14 February 2026 04:00UT - 15 February 2026 03:59UT.
Low level of electron flux is expected for 15 February 2026 04:00UT - 16 February 2026 03:59UT.
Low level of electron flux is expected for 16 February 2026 04:00UT - 17 February 2026 03:59UT.

The flux of high-energy protons was quiet for the last 24 hours.

Based on today's conditions, the flux of high-energy protons for 
February 13th, 2026 04:00 UT - February 14th, 2026 03:59 UT is predicted to be quiet.
February 14th, 2026 04:00 UT - February 15th, 2026 03:59 UT is predicted to be quiet.
February 15th, 2026 04:00 UT - February 16th, 2026 03:59 UT is predicted to be quiet.
February 16th, 2026 04:00 UT - February 17th, 2026 03:59 UT is predicted to be quiet.