[Ips-dsgr] ASWFC Daily Report - 13 September 23 issued 2330 UT on 13 Sep 2023 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Thu Sep 14 09:30:42 EST 2023


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/13 SEPTEMBER 2023
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 13 SEPTEMBER AND FORECAST FOR 14 SEPTEMBER - 16 SEPTEMBER
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 13 Sep:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 13 Sep: 143/97


1B. SOLAR FORECAST
             14 Sep             15 Sep             16 Sep
Activity     R0-R1              R0-R1              R0-R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   145/99             145/99             148/102

COMMENT: Solar activity on UT day 13-Sep was at the R0 level, 
with a C5.5 flare produced by AR3423 (N17W61, beta) the largest 
flare of the day. 

There are currently six numbered sunspot regions 
visible on the solar disk and three unnumbered regions. Both 
AR3429 (N11E20, beta-gamma) and AR3430 (S16W31, beta) displayed 
spot development over the UT day. AR3429 is the most magnetically 
complex region on the solar disk, but it is small and has so 
far only produced one M-class flare on 11-Sep. AR3423 is the 
largest and most significant sunspot region on the solar disk. 
It appears stable and is expected to rotate off the western limb 
in the second half of 16-Sep. There are three unnumbered sunspot 
regions visible on the solar disk, one at N16E29 with alpha magnetic 
characteristics, one at S15E20 with beta-gamma characteristics 
and one at N15W17 with beta characteristics. 

Solar activity is expected to be at R0-R1 levels, over 14-16 Sep. 

The >10MeV proton flux was slightly enhanced over 13-Sep but S0 
conditions are expected over 14-16 Sep. 

No Earth directed CMEs were observed on 13-Sep. A filament lift 
off is visible in SDO, GOES SUVI and H-Alpha imagery from 13/0959UT 
at around S35W450. An associated, narrow southeast directed CME is 
visible in SOHO and STEREO-A imagery from 13/1100UT. This CME is not 
considered geoeffective. 

The solar wind speed increased at the start of 13-Sep, before 
decreasing by the end of the day. The wind speed ranged from 
446 to 371 km/s and is currently near 395 km/s. The peak total 
interplanetary field strength (IMF, Bt) was 13 nT and the north-south 
IMF component (Bz) range was +5 to -9 nT. The day began with 
a sustained period of -Bz until around 13/0100UT. 

The solar wind speed is expected to remain low over 14-16 Sep, with 
the possibility of mild enhancements on 14-15 Sep due to a pair of 
small coronal holes in geoeffective positions.

-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 13 Sep: G0 Australian 
region, G1 planetary

Estimated Indices 13 Sep : A   K           
   Australian Region       9   32223312
      Cocos Island         9   32223312
      Darwin               9   32223312
      Townsville          11   33223322
      Learmonth           13   422-----
      Alice Springs       10   33223312
      Gingin              10   32223313
      Canberra            11   22234312
      Hobart              12   32234312    

Estimated Antarctic Regional K Indices 13 Sep :
      Macquarie Island    15   33244411
      Casey               13   33422313
      Mawson              35   43323656

Observed Regional daily pc3 Indices 13 Sep : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               7   (Quiet)
      Canberra             0   (Quiet)
      Hobart               6   (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 13 Sep : A 
           Fredericksburg        15
           Planetary             18                         

Observed AFr/Ap Indices 12 Sep :  A   K
           Fredericksburg        17
           Planetary             25   2123 5634     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
14 Sep    10    G0
15 Sep     7    G0
16 Sep     5    G0

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on 13-Sep. G0 conditions were mostly observed in the Antarctic 
region with periods of G1-G2 observed at Mawson. Planetary geomagnetic 
conditions reached G1 for the first period of 13-Sep. G0 geomagnetic 
conditions are expected over 14-16 Sep.

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
13 Sep      Fair           Fair-poor      Poor           

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
14 Sep      Normal         Normal         Normal-fair
15 Sep      Normal         Normal         Normal
16 Sep      Normal         Normal         Normal

COMMENT: HF radio propagation conditions on UT day 13-Sep were 
degraded at middle to high latitudes. Mostly normal HF conditions 
are expected over 14-16 Sep. Isolated minor shortwave fadeouts 
are possible.

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


Date   T index
13 Sep    86

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 40% during local day.
      Enhanced by 30% during local night.
      Enhanced by 25% after local dawn.
   Niue Island Region:
      Enhanced by 20% during local day.
      Depressed by 15% during local night.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian Region:
      Depressed by 20% during local day.
      Depressed by 25% during local night.
      Depressed by 25% after local dawn.
   Antarctic Region (Casey/Davis/Mawson):
      Depressed by 15% over the UT day.

Monthly T index:
Month  T index
Aug      115
Sep      96
Oct      93

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
14 Sep   100    Near predicted monthly values
15 Sep   110    Near predicted monthly values
16 Sep   110    Near predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) on UT day 13-Sep were 
depressed by up to 25% in the southern Australian region and 
near predicted monthly values in the northern Australian region. 
Significant spread F was observed at Brisbane, Canberra and Hobart 
and Sporadic E was observed at Hobart, degrading local HF conditions. 
MUFs are generally expected to be near predicted monthly values 
over 14-16 Sep. Isolated minor shortwave fadeouts are possible.

-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 12 Sep
       Daily Proton Fluence >1 MeV:   6.0E+05
       Daily Proton Fluence >10 MeV:  1.8E+04
       Daily Electron Fluence >2 MeV: 2.80E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: C1.4

DSCOVR Satellite Solar Wind Day Averaged Data for 12 Sep
Speed: 368 km/sec  Density:   10.3 p/cc  Temp:    21300 K  Bz:  -1 nT

(Courtesy Space Weather Prediction Center, Boulder USA)
-----------------------------------------------------------

Australian Space Weather Forecasting Centre
Bureau of Meteorology
ASWFC at bom.gov.au
www.bom.gov.au | www.sws.bom.gov.au



More information about the ips-dsgr mailing list