Alerts:
none
Solar-terrestrial indices for 30 December follow.
Solar flux 182 and estimated planetary A-index 8.
The estimated planetary K-index at 0300 UTC on 31 December was 1.67.
No space weather storms were observed for the past 24 hours.
Space weather for the next 24 hours is predicted to be moderate.
Radio blackouts reaching the R2 level are likely.
Geo Magnetic Forecast:
NOAA Ap Index Forecast
Observed Ap 29 Dec 009
Estimated Ap 30 Dec 009
Predicted Ap 31 Dec-02 Jan 012-029-018
NOAA Geomagnetic Activity Probabilities 31 Dec-02 Jan
Active 30/35/40
Minor storm 15/40/20
Moderate storm 05/15/05
Strong-Extreme storm 01/01/01
NOAA Kp index forecast 31 Dec - 02 Jan
Dec 31 Jan 01 Jan 02
00-03UT 1.67 5.00 3.67
03-06UT 1.67 5.00 3.67
06-09UT 2.00 3.67 3.33
09-12UT 2.00 3.33 3.33
12-15UT 2.33 3.33 3.00
15-18UT 2.67 4.33 3.00
18-21UT 3.33 4.00 3.00
21-00UT 4.33 3.33 3.00
Extended Three Day Forecast:
A. NOAA Geomagnetic Activity Observation and Forecast
The greatest observed 3 hr Kp over the past 24 hours was 3 (below NOAA
Scale levels).
The greatest expected 3 hr Kp for Dec 31-Jan 02 2026 is 5.00 (NOAA Scale
G1).
NOAA Kp index breakdown Dec 31-Jan 02 2026
Dec 31 Jan 01 Jan 02
00-03UT 1.67 5.00 (G1) 3.67
03-06UT 1.67 5.00 (G1) 3.67
06-09UT 2.00 3.67 3.33
09-12UT 2.00 3.33 3.33
12-15UT 2.33 3.33 3.00
15-18UT 2.67 4.33 3.00
18-21UT 3.33 4.00 3.00
21-00UT 4.33 3.33 3.00
Rationale: G1 (Minor) or greater geomagnetic storms are possible on 01
Jan.
B. NOAA Solar Radiation Activity Observation and Forecast
Solar radiation, as observed by NOAA GOES-18 over the past 24 hours, was
below S-scale storm level thresholds.
Solar Radiation Storm Forecast for Dec 31-Jan 02 2026
Dec 31 Jan 01 Jan 02
S1 or greater 15% 15% 15%
Rationale: No S1 (Minor) or greater solar radiation storms are expected.
No significant active region activity favorable for radiation storm
production is forecast.
C. NOAA Radio Blackout Activity and Forecast
No radio blackouts were observed over the past 24 hours.
Radio Blackout Forecast for Dec 31-Jan 02 2026
Dec 31 Jan 01 Jan 02
R1-R2 60% 60% 60%
R3 or greater 25% 25% 25%
Rationale: R1-R2 (Minor-Moderate) radio blackouts are likely, with a
chance for R3 (Strong) or greater events, on 31 Dec-02 Jan.
Extended Space Weather Discussion:
Solar Activity
.24 hr Summary...
Solar activity has been at low levels for the past 24 hours, with few
C-class flares mostly coming from Region 4325 (S08E17, Eki/beta-gamma).
The largest flare of the period was a C5.0/Sf, peaked at 30/0645 UTC,
from Region 4324 (N24E25, Dao/beta-gamma).
Region 4330 (S16E41, Axx/alpha) was responsible for two eruptions seen
in SUVI imagery. The first eruption was associated with a CME, first
observed at coronagraph imagery at 30/0700 UTC and closely followed by a
second CME from the northeast quadrant (potentially from near Region
4324). But none of their modeled trajectory indicated direct impact
near-Earth.
Further coronagraph images are necessary to evaluate if the second
eruption from Region 4330 will result in a visible CME. No other
Earth-directed CME was observed during the period.
.Forecast...
Solar activity is likely to be moderate with a chance for X-class flares
through 02 Jan due to the current magnetic complexity and development of
the active regions on the visible solar disk.
Energetic Particle
.24 hr Summary...
The greater than 2 MeV electron flux, measured at geostationary orbit by
GOES-19, reached a peak level of 5,612 pfu at 30/1545 UTC and decreased
to moderate levels after 30/1915 UTC. The greater than 10 MeV proton
flux remained at background levels during the period.
.Forecast...
The greater than 2 MeV electron flux is expected to reach high levels
again on 31 Dec and 01-02 Jan. The greater than 10 MeV proton flux has a
slight chance of crossing threshold on days 31 Dec, 01-02 Jan.
Solar Wind
.24 hr Summary...
Solar wind parameters remained at background conditions during most of
the day. Solar wind speed oscillated around 400 km/s, but reached a peak
of 563 km/s at 30/1514 UTC during a brief disturbance. Total IMF
oscillated around 5 nT most of the period, and reached 9 nT at 30/2323
UTC. The maximum southward component of Bz reached -6 nT at 30/1515 UTC,
during a brief disturbance that was likely anticipating a sector
crossing observed as the phi angle change (from mostly positive to
mostly negative after that), likely associated with a negative CH HSS.
.Forecast...
Solar wind parameters are expected to increasingly respond to the
influence of a negative CH/HSS located at the northwest solar quadrant
in the next days: higher speeds, lower densities and negative phi angle.
By late 31 Dec / early 01 Jan, a glancing blow of CME that left the Sun
on 28 Dec is anticipated to disturb the solar wind near Earth. Later on
01 Jan, an extra disturbance caused by the multiple CMEs from 29 Dec is
also possible.
Geospace
.24 hr Summary...
The geomagnetic activity has been at quiet to unsettled levels for the
past 24 hours.
.Forecast...
The geomagnetic activity is expected to be at quiet to active levels on
31 Dec, unsettled to minor storm levels on 01 Jan and unsettled to
active levels on 02 Jan.
27 Day Forecast:
Date | Radio Flux | Planetary A Index | Largest Kp Index
2025 Dec 29 185 5 2
2025 Dec 30 175 5 2
2025 Dec 31 170 8 3
2026 Jan 01 165 15 4
2026 Jan 02 160 18 4
2026 Jan 03 160 15 4
2026 Jan 04 155 12 4
2026 Jan 05 150 5 2
2026 Jan 06 155 5 2
2026 Jan 07 140 5 2
2026 Jan 08 130 5 2
2026 Jan 09 125 15 4
2026 Jan 10 120 10 4
2026 Jan 11 120 5 2
2026 Jan 12 120 10 4
2026 Jan 13 120 15 4
2026 Jan 14 115 15 4
2026 Jan 15 120 5 2
2026 Jan 16 120 5 2
2026 Jan 17 125 20 5
2026 Jan 18 135 20 5
2026 Jan 19 145 18 4
2026 Jan 20 155 18 4
2026 Jan 21 165 8 3
2026 Jan 22 165 8 3
2026 Jan 23 175 5 2
2026 Jan 24 175 5 2
v4.16b
v4.X Release 17th Dec 2020)
Fixed New GOES and HPI inputs from noaa for Json (17/12/20).
Addded the ability to add 2 custom Magnetometers in settings (comming soon) (18/10/19).
Improved Hobart Magnetometer code. (18/18/19)
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Added GeoSpace Kp Model Prediction. (3/7/18)
Added SWPC Kp Forecast + Observation. (2/7/18)
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> v1.0 (Started 20/10/2014)
Mawson and Macquarie Island data is copyright Commonwealth of Australia (Geoscience Australia), and redistributed under Creative Commons v4.
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