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Weather: TAS
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Alerts:
Space Weather Message Code: WATA30
Serial Number: 264
Issue Time: 2026 Mar 16 2108 UTC

WATCH: Geomagnetic Storm Category G2 Predicted
Highest Storm Level Predicted by Day:
Mar 17:  None (Below G1)   Mar 18:  None (Below G1)   Mar 19:  G2 (Moderate)
THIS SUPERSEDES ANY/ALL PRIOR WATCHES IN EFFECT

Comment: G2 (Moderate) geomagnetic storming is likely on 19 Mar with the arrival of a CME that left the Sun on 16 Mar. This is a reissue of the previous watch to correct an internal system error.
www.swpc.noaa.gov/noaa-scales-explanation
Potential Impacts: Area of impact primarily poleward of 55 degrees Geomagnetic Latitude.
Induced Currents - Power grid fluctuations can occur. High-latitude power systems may experience voltage alarms.
Spacecraft - Satellite orientation irregularities may occur; increased drag on low Earth-orbit satellites is possible.
Radio - HF (high frequency) radio propagation can fade at higher latitudes.
Aurora - Aurora may be seen as low as New York to Wisconsin to Washington state.

Space Weather Message Code: WATA30
Serial Number: 264
Issue Time: 2026 Mar 16 2025 UTC

WATCH: Geomagnetic Storm Category G2 Predicted
Highest Storm Level Predicted by Day:
Mar 17:  None (Below G1)   Mar 18:  None (Below G1)   Mar 19:  G2 (Moderate)
THIS SUPERSEDES ANY/ALL PRIOR WATCHES IN EFFECT

Comment: G2 (Moderate) geomagnetic storming is likely on 19 Mar with the arrival of the 16 Mar CME event. This event was associated with an M2.7 flare from AR 4392.
www.swpc.noaa.gov/noaa-scales-explanation
Potential Impacts: Area of impact primarily poleward of 55 degrees Geomagnetic Latitude.
Induced Currents - Power grid fluctuations can occur. High-latitude power systems may experience voltage alarms.
Spacecraft - Satellite orientation irregularities may occur; increased drag on low Earth-orbit satellites is possible.
Radio - HF (high frequency) radio propagation can fade at higher latitudes.
Aurora - Aurora may be seen as low as New York to Wisconsin to Washington state.

Space Weather Message Code: ALTEF3
Serial Number: 3648
Issue Time: 2026 Mar 16 1320 UTC

CONTINUED ALERT: Electron 2MeV Integral Flux exceeded 1000pfu
Continuation of Serial Number: 3647
Begin Time: 2026 Mar 15 1630 UTC
Yesterday Maximum 2MeV Flux: 1429 pfu
Potential Impacts: Satellite systems may experience significant charging resulting in increased risk to satellite systems.

Space Weather Message Code: SUM10R
Serial Number: 901
Issue Time: 2026 Mar 16 1229 UTC

SUMMARY: 10cm Radio Burst
Begin Time: 2026 Mar 16 1209 UTC
Maximum Time: 2026 Mar 16 1213 UTC
End Time: 2026 Mar 16 1217 UTC
Duration: 8 minutes
Peak Flux: 380 sfu
Latest Penticton Noon Flux: 109 sfu

Comment: Associated with M2.7 flare from AR 4392.
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.

Space Weather Message Code: ALTTP4
Serial Number: 705
Issue Time: 2026 Mar 16 1226 UTC

ALERT: Type IV Radio Emission
Begin Time: 2026 Mar 16 1212 UTC
Description: Type IV emissions occur in association with major eruptions on the sun and are typically associated with strong coronal mass ejections and solar radiation storms.

Space Weather Message Code: ALTTP2
Serial Number: 1469
Issue Time: 2026 Mar 16 1224 UTC

ALERT: Type II Radio Emission
Begin Time: 2026 Mar 16 1209 UTC
Estimated Velocity: 1227 km/s

Comment: Likely associated with M2.7 flare from AR 4392.
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.


Solar-terrestrial indices for 16 March follow.
Solar flux 111 and estimated planetary A-index 10.
The estimated planetary K-index at 0600 UTC on 17 March was 1.00.

Space weather for the past 24 hours has been minor.
Radio blackouts reaching the R1 level occurred.

No space weather storms are predicted for the next 24 hours.


Geo Magnetic Forecast:

NOAA Ap Index Forecast
Observed Ap 15 Mar 017
Estimated Ap 16 Mar 012
Predicted Ap 17 Mar-19 Mar 010-008-040

NOAA Geomagnetic Activity Probabilities 17 Mar-19 Mar
Active                30/25/15
Minor storm           10/05/20
Moderate storm        01/01/35
Strong-Extreme storm  01/01/25

NOAA Kp index forecast 17 Mar - 19 Mar
             Mar 17    Mar 18    Mar 19
00-03UT        2.67      2.67      1.67
03-06UT        3.00      2.33      5.33
06-09UT        2.33      2.00      6.33
09-12UT        2.00      1.33      5.67
12-15UT        2.00      1.67      4.33
15-18UT        2.00      2.00      3.33
18-21UT        2.33      2.33      3.67
21-00UT        2.67      2.67      4.00


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 Mar 17-Mar 19 2026 is 6.33 (NOAA Scale
G2).

NOAA Kp index breakdown Mar 17-Mar 19 2026

             Mar 17       Mar 18       Mar 19
00-03UT       2.67         2.67         1.67
03-06UT       3.00         2.33         5.33 (G1)
06-09UT       2.33         2.00         6.33 (G2)
09-12UT       2.00         1.33         5.67 (G2)
12-15UT       2.00         1.67         4.33
15-18UT       2.00         2.00         3.33
18-21UT       2.33         2.33         3.67
21-00UT       2.67         2.67         4.00

Rationale: G2 (Moderate) geomagnetic storming is likely, with a chance
for isolated periods of G3 (Strong) geomagnetic storming, on 19 Mar with
the arrival of the 16 Mar CME.

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 Mar 17-Mar 19 2026

              Mar 17  Mar 18  Mar 19
S1 or greater    5%      5%     10%

Rationale: A slight chance for S1 (Minor) levels will exist on 19 Mar
with any shock enhancement with the arrival of the 16 Mar CME.

C. NOAA Radio Blackout Activity and Forecast

Radio blackouts reaching the R1 levels were observed over the past 24
hours. The largest was at Mar 16 2026 1215 UTC.

Radio Blackout Forecast for Mar 17-Mar 19 2026

              Mar 17        Mar 18        Mar 19
R1-R2           30%           30%           30%
R3 or greater    5%            5%            5%

Rationale: Solar activity is expected to be at low levels, with a chance
for M-class (R1-R2/Minor-Moderate) flares through 19 Mar.


Extended Space Weather Discussion:

Solar Activity

.24 hr Summary...
Solar activity has been at moderate levels for the past 24 hours. There
are currently 4 numbered sunspot regions on the disk. Region 4392
(S16E15, Csi/beta-gamma) continued to evolve during the early portions
of the period, developing additional penumbra and spots. AR 4392 was the
culprit of the largest event of the period, which was an M2.7 flare at
16/1215 UTC. This event was associated with a Type II raido sweep with
an estimated speed of 1,227 km/s, a Type IV radio sweep and a tenflare
that peaked at 16/1213 UTC at 380 sfu. The resulting CME was then first
observed in LASCO C2 imagery at approximately 16/1236 UTC as an
asymmetric halo. Modeling of this event determined arrival at Earth on
19 Mar.

.Forecast...
Solar activity is expected to be at low levels, with a chance for
M-class (R1-R2/Minor-Moderate) flares through 19 Mar.

Energetic Particle

.24 hr Summary...
Electrons greater than 2 MeV at geosynchronous orbit reached a peak
level of 2212 pfu at 16/1440 UTC. The greater than 10 MeV proton flux
was at background levels.

.Forecast...
The greater than 2 MeV electron flux is expected to continue to reach
high levels through 19 Mar. The greater than 10 MeV proton flux is
expected to continue at background levels through 18 Mar. A slight
chance for S1 (Minor) levels will exist on 19 Mar with any shock
enhancement with the arrival of the 16 Mar CME.

Solar Wind

.24 hr Summary...
Solar wind parameters reflected the waning influence of a positive
polarity CH HSS. Solar wind speed reached a peak of 637 km/s at
16/0606 UTC. Total IMF reached 6 nT at 16/1233 UTC. The maximum
southward component of Bz reached -4 nT at 16/1133 UTC. Phi was
predominantly in a positive orientation.

.Forecast...
Solar wind parameters are expected to remain elevated, but gradually
decline over the course of 17 and 18 Mar. Moderate enhancements are
expected on 19 Mar with the arrival of the 16 Mar CME.

Geospace

.24 hr Summary...
Geomagnetic field activity reached unsettled levels.

.Forecast...
Geomagnetic field activity is expected to be primarily quiet to
unsettled over 17-18 Mar under a waning positive polarity CH HSS regime.
G2 (Moderate) geomagnetic storming is likely, with a chance for isolated
periods of G3 (Strong) geomagnetic storming, on 19 Mar with the arrival
of the 16 Mar CME.


27 Day Forecast:

Date | Radio Flux | Planetary A Index | Largest Kp Index
2026 Mar 16     108          15          4
2026 Mar 17     108          10          3
2026 Mar 18     105           8          3
2026 Mar 19     105           5          2
2026 Mar 20     105          10          3
2026 Mar 21     100          35          5
2026 Mar 22     102          25          5
2026 Mar 23     105          15          4
2026 Mar 24     110          15          4
2026 Mar 25     100          18          5
2026 Mar 26     110          10          3
2026 Mar 27     120           8          3
2026 Mar 28     125           5          2
2026 Mar 29     125           5          2
2026 Mar 30     125          15          4
2026 Mar 31     125          10          3
2026 Apr 01     130           5          2
2026 Apr 02     135           5          2
2026 Apr 03     140          18          5
2026 Apr 04     135          20          5
2026 Apr 05     135           8          3
2026 Apr 06     130          15          4
2026 Apr 07     135           8          3
2026 Apr 08     130           5          2
2026 Apr 09     125          25          5
2026 Apr 10     120          40          6
2026 Apr 11     115          20          5


  • GRAPH OPTIONS: Learn more
    It is recommended that you start out with the default options. As you get used to AF you can disable additional information and combine data series' together to maxamise the use of screen space.

  • DATA SOURCES: Learn more
    Some data sources can only be enabled or disabled via the tick box. Others are disabled using the slider set to 0, or enabled by setting the slider from 0.5 to 4. This number also represents the thinkness of the line plot onto the graph.

  • 'The' Aurora Forecast Index: Learn more
    These are two good options for predicting Auroras.

    The Aurora Forecast Index takes into account many data sources. As a general rule if it stays high for many hours there is a good possibility of an Aurora present.

    Aurora Forecast website usage is also a good indicator, as visitors to the site come from many traffic sources. General internet and community chatter transplating to visits is a great indicator.

  • Planatary K Index (Kp): Learn more
    The Kp number is a system of measuring aurora strength. The range goes from 0 to 9 (0 being calm, 1 very weak, all the way up to 9, which would represent a major geomagnetic storm with strong auroras visible).

    Kp 5 and above is classified as a geomagnetic storm. Most Aurora Hunters consider prolonged 3+ or higher worth investigation.

  • Ovation (Model) Short Term Forecast (GW):' Learn more
    The Ovation-Prime Model produced by SWPC calculates the energy interacting with the Earths magnetic field. This is a good indicator for Aurora activity.
  • DSCOVR Observatory (L1): Learn more

    The DSCOVR or Deep Space Climate Obervatory sits 1.5 million Kilometers from Earth, between the Earth and the Sun in the L1 orbit point, the neutral gravity point between the Earth and the Sun. DSCOVR provides space weather readings, allowing for up to an hour of warning on weather events. This is why DSCOVR's data appears in the future on the graph.

    Strong negative Bz direction is linked to Aurora's because the solar wind magnetic direction is in direct oposition with the Earths magnetic field.

  • ACE Observatory (L1): Learn more

    ACE or Advanced Composition Explorer sits 1.5 million Kilometers from Earth, between the Earth and the Sun in the L1 orbit point, the neutral gravity point between the Earth and the Sun. ACE has now been replaced by DSCOVR, but the data is still useful for comparing to DSCOVR.
  • GOES Satalites: Learn more

    GOES or Geostationary Operational Environmental Satellites sit 46 Kilometers above the Earth in geostationary orbit. They provide local space weather data and are a good indicator for current geomagnetic conditions.

  • Terrestrial Magnetometer Sources: Learn more
    Terrestrial or surface magnetometers detect fluctuations in the Earths magnetic field from the ground.
    These do not work as well as satalites as the magnetic field obsorbs some of the effects from the solar winds.
    There is a mix of govenment and citizen science stations listed here, including two run by Aurora Forecast in Hobart.
  • User Magnetometer ID's: Learn more
    If you have a TAFS Magnetometer and you want to add it to the graph you can do it here.
    Insent your Mag's Unique ID.

 

v4.16b

Aurora Forecast is free to use, however it takes a lot of time and effort to maintain. If you find it useful and are a regular user then please consider making a donation to keep it running. Feedback is always welcome.


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)
Move all presets into their own pop out side menu. (19/06/19)
Added Composite weather maps (TAS, VIC and SA), thanks to Oz forecast! (19/06/19)
UI Upgrades, Name, Logo and Website Site Changes.
Added custom line widths for most items.
Added GOES Difference (#1 - #2)
Added Ovation-prime model outputs.

v3.8x
Various Updates, New AF Index Algo. (8/12/18)

v3.6x
Added more Presets. Disabled Presets overwriting graph views (6/7/18)
Added GeoSpace Kp Model Prediction. (3/7/18)
Added SWPC Kp Forecast + Observation. (2/7/18)
Removed WingKP and USKp. :( No longer Avaliable. (2/7/18)
Removed feed from www.dunedinaurora.nz (Unreliable). (2/7/18)
Updates to latest JQuery, JQuery Mobile and AmCharts etc. (2/7/18)
Enhanced Pro setting with Dynamic Preasure. (2/7/18)
Added Quickselect preset buttons to main page. (2/7/18)
 
v3.5x
Added Ruru Observatory Magnetometer. (25/4/28)
Added Forecast Sub Tabset. (1/3/18)
Added Extended Discussion Text, 27Day FC (1/3/18)
Removed Dial, and Added Forecast Report. (28/2/18)
Updated A few settings for better visilation. (28/2/18)
Updated Goes-13 is Now Goes-14 (15/2/18)
Improved Commmunity Activity for faster loads.
Consolidated Proton Density / Dynamic Preasure.
Added Additional Balloon Text.
Added TAFS Visual Probability in %.
User Interface Upgrades.
Add 'Dial' for the basics, with default support.
Added one click presets.
 
v2.1 - v2.49
Added 'Automatic Chart Update' option in settings.
Database caching enabled, significant load time improvements.
Extension to max 96 hours of data, up from 24.
Added ACE Bt,Bx and By for comparison.
Added More User Presets.
Fixed Orentation Change Alert.
Small layout changes.
Added Header Image.
Removed Top Header to fee up Space, Refresh added to Chart Tab.
Added Community Activity Indicator
Fixed MAG value issues in graph.
Added Second Hobart MAG Source.
Updated Comment Features (Disable).
 
v2.0
Fixed DSCOVR B? display bug.
Added MAG Stack Feature.
Upgrade to json feeds.
Feeds are timezone and forecast aware, making them super fast.
DB Optimisation, improved DB search times.
Charts are now zoomable, allow selection and export.
Added USAF Kp, Updated Wing Kp.
Added Ovation Aurora Short Term Forecast.
Added Macquarie Island MAG feed.
Added Mawson MAG Feed.
Added Canberra Feed.
Added MAG feed from www.dunedinaurora.nz (Portobello).
Added Brendan's experemental MAG feed (Hobart).
Fixed cookie bug, One Alert is enough for landscape mode.
 
> v1.0 (Started 20/10/2014)

  Mawson and Macquarie Island data is copyright Commonwealth of Australia (Geoscience Australia), and redistributed under Creative Commons v4.
Thanks to INTERMAGNET for promoting high standards of magnetic observatory practice in providing access to these feeds. (www.intermagnet.org).

Local Australian weather composite maps provided by Oz Forecast


Aurora Forecast is free to use, however it takes a lot of time and effort to maintain.
Why not make a donation to keep it running?
Feedback is always welcome. - ©2022 Brendan Davey