[Ips-dsgr] ASWFC Daily Report - 04 October 24 issued 2331 UT on 04 Oct 2024 [SEC=OFFICIAL]

Australian Space Weather Forecasting Centre aswfc at bom.gov.au
Sat Oct 5 09:31:12 AEST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/04 OCTOBER 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 04 OCTOBER AND FORECAST FOR 05 OCTOBER - 07 OCTOBER
STATUS INDICATORS SOL:** RED **   MAG:** RED **     ION: ** YELLOW **
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 04 Oct:  R1

Flares    Max     Fadeout    Freq.  Sectors
  M1.1 03/2328UT  possible   lower  West Pacific
  M4.0    0455UT  possible   lower  E. Asia/Aust.
  M1.1    0521UT  possible   lower  E. Asia/Aust.
  M1.2    1103UT  possible   lower  European
  M1.2    2105UT  possible   lower  East Pacific/
                                    North American
  M1.2    2211UT  possible   lower  East Pacific/
                                    North American

Observed 10.7 cm flux/Equivalent Sunspot Number for 04 Oct: 291/247


1B. SOLAR FORECAST
             05 Oct             06 Oct             07 Oct
Activity     Moderate to high   Moderate to high   Moderate to high
Fadeouts     Probable           Probable           Probable
10.7cm/SSN   290/246            280/233            280/233

COMMENT: Solar activity on UT day 04-Oct was R1, with the strongest 
flare being M4 from AR3842. There are currently eight numbered 
sunspots on the disk. AR3842 (S15W19, beta-gamma) continues to 
grow and dominate as the largest and most complex sunspot. ARs 
3841 (N13W34, beta), 3843 (S07W51, beta) and 3844 (S16W41, beta-gamma) 
have also grown in the past day. All other sunspots are stable. 
Solar activity is expected to be R-R3, with a very slight chance 
of R4 over 5-7 Oct.

 A CME was associated with the M4 flare from AR3843 and can be seen from
 0448 UT; however, this region appeared to have a constant flow of material 
for most of the day. This CME may arrive from 07/1000 UT but
may be earlier due to the solar wind preconditioning from earlier
 CMEs. A CME to the northeast can be seen from 04/2048 UT but 
this has been analysed as a a farside event. 

S0 solar radiation storm conditions were observed on 4-Oct.
 S0-S1 solar radiation storm conditions are expected over 5-7 Oct. 

The solar wind environment was generally near background levels 
on 4-Oct, possibly slightly enhanced, however the first of the
 CMEs from AR3842 has not yet arrived. The solar wind speed was 
on a slow incline, beginning near 300 km/s and ending the day near 
400 km/s. The peak total interplanetary field strength (IMF, Bt) 
was 8 nT and the north-south IMF component range (Bz) was +7 to 
-7 nT. The solar wind environment is expected to become disturbed 
from 5-Oct and likely through to 7-Oct due to multiple expected CMEs.
A small coronal hole may also contribute to increased solar wind 
speeds by 6-7 Oct.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 04 Oct: G0

Estimated Indices 04 Oct : A   K           
   Australian Region       5   22110123
      Cocos Island         5   12111113
      Darwin               7   23211113
      Townsville           7   22111133
      Learmonth            7   22221223
      Alice Springs        5   22110123
      Gingin               8   22120224
      Canberra             5   22110123
      Kennaook Cape Grim   6   21110133
      Hobart               5   22110123    

Estimated Antarctic Regional K Indices 04 Oct :
      Macquarie Island     2   11000112
      Casey               19   44531233
      Mawson              19   33221336

Observed Regional daily pc3 Indices 04 Oct : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               4   (Quiet)
      Canberra             2   (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 04 Oct : A 
           Fredericksburg        12
           Planetary             20                         

Observed AFr/Ap Indices 03 Oct :  A   K
           Fredericksburg         8
           Planetary              7   1111 3222     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
05 Oct    50    G3, chance of G4
06 Oct    60    G2-G3, chance of G4
07 Oct    30    G1-G2, chance G3

COMMENT: ASWFC Geomagnetic Warning 59 was issued on 4 October 
and is current for 4-6 Oct. G0 geomagnetic conditions were observed 
in the Australian and Antarctic regions on UT day 4-Oct, with 
an isolated period of G1 at Casey.

 Sunspot region AR3842 has produced 
several CMEs recently; one from 1-Oct and another from 4-Oct 
have failed to arrive by their predicted time, however are still 
expected on 5-Oct. AR3842 has produced several more CMEs with 
Earth-directed components since, but due to the large number 
of eruptions exact arrival times cannot be calculated with confidence 
as they may or may not interact in space. The result is that 
G3-G4 geomagnetic conditions are possible over 5-6 Oct, beginning 
to taper off by 7-Oct.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
04 Oct      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
05 Oct      Fair           Fair-poor      Fair-poor
06 Oct      Fair           Fair-poor      Poor
07 Oct      Fair           Fair-poor      Fair-poor

COMMENT: HF radio communication conditions on UT day 4-Oct were 
normal. HF radio communication conditions are expected to become 
degraded at all latitudes on 5-Oct due to an anticipated CME 
arrival, followed by several other CMEs. Due to this, a prolonged 
geomagnetic storm is expected over 5-7 Oct, such that HF radio 
conditions are expected to be degraded for this whole period.

-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
04 Oct   156

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day.
      Enhanced by 15% during local night.
   Niue Island Region:
      Enhanced by 20% during local day.
      Near predicted monthly values during local night.
   Northern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 30% during local night.
   Southern Australian Region:
      Enhanced by 15% during local day.
      Enhanced by 25% during local night.
   Antarctic Region (Casey/Davis/Mawson):
      Near predicted monthly values over the UT day.

Monthly T index:
Month  T index
Sep      147
Oct      116
Nov      115

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
05 Oct   120    Near predicted monthly values/depressed 5 to 
                15%
06 Oct   100    Near predicted monthly values/depressed 10 to 
                25%
07 Oct    90    Near predicted monthly values/depressed 10 to 
                35%

COMMENT: ASWFC SWF HF Communications Warning 111 was issued on 
4 October and is current for 4-6 Oct. ASWFC Preliminary HF Communications 
Warning 112 was issued on 4 October and is current for 4-6 Oct. 
Maximum usable frequencies (MUFs) in the Australian region on 
UT day 4-Oct were near predicted values to 30% enhanced. Range 
spread was observed in Cocos Islands during local night hours. 
MUFs are expected to be near predicted values in the beginning 
of UT day 5-Oct, however are expected to become depressed by 
up to 15% upon the commencement of an expected geomagnetic storm. 
MUFs are likely to become progressively worse over 6-7 Oct due 
to expected prolonged geomagnetic storm conditions.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 03 Oct
       Daily Proton Fluence >1 MeV:   2.7E+05
       Daily Proton Fluence >10 MeV:  1.5E+04
       Daily Electron Fluence >2 MeV: 5.40E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C6.1

DSCOVR Satellite Solar Wind Day Averaged Data for 03 Oct
Speed: 332 km/sec  Density:    0.5 p/cc  Temp:    49100 K  Bz:   0 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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