[Ips-dsgr] ASWFC Daily Report - 08 April 26 issued 2330 UT on 08 Apr 2026 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Thu Apr 9 09:30:38 AEST 2026


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/08 APRIL 2026
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 08 APRIL AND FORECAST FOR 09 APRIL - 11 APRIL
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 08 Apr:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 08 Apr: 108/58


1B. SOLAR FORECAST
             09 Apr             10 Apr             11 Apr
Activity     R0, chance of R1   R0, chance of R1   R0, chance of R1   
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   105/54             100/48              95/41

COMMENT: Solar flare activity was at the R0 level on UT day 08-Apr, 
with a C8.7 flare at 08/1543 from Active Region (AR) 4414 (N12E65, 
beta), the largest observed over the UT day. This region is one 
of five numbered regions on the solar disk, and has shown some 
growth as it continues to rotate onto the front side of the solar 
disk. AR 4409 (N05W67) remains the most magnetically complex 
region, and will likely rotate off the western limb in the next 
24 hours. Region 4415 (S19E71) has recently shown growth as it 
rotated over the eastern edge of the Sun, and currently exhibits 
an alpha magnetic classification. A small unnumbered region appeared 
at S06W29 and is currently magnetically simple. All other regions 
are either stable or in decay. Solar flare activity is forecast 
to be at the R0 level, with a chance of R1 over 09-11 Apr, due 
to the newly emerged regions on the visible disk. S0 solar proton 
conditions were observed throughout 08-Apr, with solar proton 
flux consistent with background levels across the UT day. S0 
solar proton conditions are forecast for 09-11 Apr. No Earth-directed 
coronal mass ejections (CMEs) were observed over the last UT 
day. Two solar eruptions on the eastern limb were observed in 
SDO/AIA 304A imaging over the last UT day, including one at 07/2317UT, 
and another at 08/0809UT. These produced a combined low velocity 
east-directed CME, which has been modelled to miss the Earth. 
The solar wind was moderate and stable over the last 24 hours, 
with speeds ranging between 380-430 km/s throughout the UT day. 
The interplanetary magnetic field strength (IMF, Bt) peaked at 
6 nT during 08-Apr, with the north-south component (Bz) ranging 
between -5 and +4 nT during this time. The solar wind speed is 
forecast to remain stable over most of 09-Apr, before rising 
late in the UT day as the Earth connects with an equatorial coronal 
hole high-speed wind stream. The solar wind is expected to remain 
elevated over 10-11 Apr.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 08 Apr: G0

Estimated Indices 08 Apr : A   K           
   Australian Region       6   12132122
      Cocos Island         3   11111121
      Darwin               7   22132122
      Townsville           7   22232122
      Learmonth            -   --------
      Alice Springs        6   11132122
      Gingin               6   11032132
      Canberra             4   01132111
      Kennaook Cape Grim   7   12133221
      Hobart               7   12133121    

Estimated Antarctic Regional K Indices 08 Apr :
      Macquarie Island    11   11054211
      Casey               12   34331222
      Mawson              24   33222365

Observed Regional daily pc3 Indices 08 Apr : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth           NA
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             2   (Quiet)
      Hobart               3   (Quiet)

Pc3 pulsations are high frequency (10-45 second period) variations 
of the Earths magnetic field. Daily pc3-indices are the daily sum 
of 20 minute pc3-indices for that station and have been shown to be
well correlated with rejection of high resolution aeromagnetic
survey flight-line data. 

NOTE: Indices may have been generated from data obtained in 
cooperation with the following organisations: Geoscience Australia, 
University of Newcastle Space Physics Group, Australian Government 
Antarctic Division and International Center for Space Weather 
Science and Education, Japan.


Estimated AFr/Ap Indices 08 Apr : A 
           Fredericksburg         6
           Planetary              8                         

Observed AFr/Ap Indices 07 Apr :  A   K
           Fredericksburg         7
           Planetary              9   3221 2223     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
09 Apr    14    G0-G1
10 Apr    20    G0-G1
11 Apr    18    G0, chance of G1

COMMENT: ASWFC Geomagnetic Warning 26 was issued on 7 April and 
is current for 9-10 Apr. Geomagnetic conditions in the Australian 
region were at the G0 level on UT day 08-Apr, with G0 conditions 
also reported at the planetary level. Periods of G1-G2 geomagnetic 
conditions were recorded in the Antarctic region. G0-G1 conditions 
are forecast for 09-Apr, with two equatorial coronal holes likely 
to move into a geoeffective position late in the UT day. G0-G1 
conditions are forecast for 10-Apr due to the high-speed wind 
stream effects of these coronal holes. This will decrease to 
G0, with a chance of G1 on 11-Apr.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
08 Apr      Normal-fair    Normal         Normal-fair    

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
09 Apr      Normal         Normal         Fair-normal
10 Apr      Normal         Normal-fair    Fair-normal
11 Apr      Normal         Normal-fair    Fair-normal

COMMENT: Global ionospheric conditions were mostly normal-fair 
across UT day 08-Apr, with some degradations in the equatorial 
South American and South African regions during local night hours. 
Mostly normal conditions are expected on 09-11 Apr, with some 
degradations possible over this period, particularly in high 
latitude regions, due to upcoming geomagnetic activity. Minor 
shortwave fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
08 Apr    93

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 20% during local day.
      Near predicted monthly values during local night.
   Niue Island Region:
      Enhanced by 25% during local day.
      Near predicted monthly values during local night.
   Northern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 20% during local night.
   Southern Australian Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Davis/Mawson):
      Near predicted monthly values over the UT day.

Monthly T index:
Month  T index
Mar      92
Apr      83
May      81

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
09 Apr    90    Near predicted monthly values
10 Apr    85    Near predicted monthly values
11 Apr    80    5 to 10% below predicted monthly values

COMMENT: Maximum Usable Frequencies (MUFs) in the Australian 
region on UT day 08-Apr were near predicted values, with enhancements 
of 20-25% observed in the Northern Australian region and at Cocos 
Island and Niue Island during local daylight hours. Sporadic-E 
was also observed in Norfolk Island during local night hours. 
Scintillation was observed at Darwin during the interval 08/1324-1340UT. 
MUFs are expected to be near predicted monthly values to around 
10% enhanced over 09-Apr. MUFs may become mildly depressed during 
10-11 Apr, especially in the Southern Australian region, due 
to upcoming coronal hole high-speed wind stream effects. Minor 
shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 07 Apr
       Daily Proton Fluence >1 MeV:   1.2E+06
       Daily Proton Fluence >10 MeV:  2.1E+04
       Daily Electron Fluence >2 MeV: 2.80E+08   (moderate fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability:18%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B4.8

DSCOVR Satellite Solar Wind Day Averaged Data for 07 Apr
Speed: 448 km/sec  Density:    2.0 p/cc  Temp:    64600 K  Bz:  -1 nT

(Courtesy Space Weather Prediction Center, Boulder USA)
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Australian Space Weather Forecasting Centre
Bureau of Meteorology
ASWFC at bom.gov.au
www.bom.gov.au | www.sws.bom.gov.au



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