[Ips-dsgr] ASWFC Daily Report - 04 February 23 issued 2331 UT on 04 Feb 2023 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Sun Feb 5 10:31:04 EST 2023


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/04 FEBRUARY 2023
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 04 FEBRUARY AND FORECAST FOR 05 FEBRUARY - 07 FEBRUARY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 04 Feb:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 04 Feb: 139/93


1B. SOLAR FORECAST
             05 Feb             06 Feb             07 Feb
Activity     R0                 R0                 R0
Fadeouts     None expected      None expected      None expected
10.7cm/SSN   140/94             145/99             150/105

COMMENT: Solar activity on UT day 4-Feb was at the R0 level, 
with several low level C-class flares, with a long duration C2.2 
flare at 4/0055UT the most significant of the day. There are 
currently five numbered sunspot regions visible on the solar 
disk. All sunspot regions showed development of their trailer 
spots. AR3211 (S17W28, gamma) showed the most significant development 
over the UT day and is the most magnetically complex area on 
the solar disk. Solar activity is expected to be at the R0 level 
over 5-7 Feb. A filament eruption is visible on the solar disk 
in SDO, H-Alpha and GOES-SUVI imagery from 4/0029UT at around 
S15E50 and is associated with the long duration C2.2 flare at 
4/0055UT. An associated very slow, south east directed CME is 
visible in LASCO and STEREO-A imagery from 4/0125UT. Modelling 
suggests a possible glancing impact with Earth at 8/1700UT ± 
12 hours, although this is low confidence. A slow filament lift 
off is visible on the solar disk at around N40W30 from 3/2301UT 
in GOES SUVI imagery. An associated very slow, north west directed 
CME is visible in LASCO and STEREO-A imagery from 4/0248UT. Modelling 
suggests a possible glancing impact with Earth at 6/1700UT ± 
12 hours. Several other CMEs were observed, but none are considered 
to be geoeffective. The solar wind speed on UT day 4-Feb was 
low. The wind speed ranged from 292 to 371 km/s, and is currently 
near 360 km/s. The peak total interplanetary field strength (IMF, 
Bt) was 8 nT, and the north-south IMF component (Bz) range was 
+6 to -7 nT. The solar wind speed is expected to remain low over 
5-Feb. An increase is expected over 6-7 Feb due to the combined 
effects of possible glancing impacts from CMEs first observed 
on 3-Feb and 4-Feb and high speed wind stream effects from a 
group of small equatorial coronal holes currently rotating towards 
a geoeffective position.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 04 Feb: G0

Estimated Indices 04 Feb : A   K           
   Australian Region       3   22101002
      Cocos Island         2   22110000
      Darwin               2   21100012
      Townsville           4   22101112
      Learmonth            3   22100002
      Alice Springs        3   22100002
      Gingin               2   22101001
      Canberra             2   21101002
      Hobart               3   21111002    

Estimated Antarctic Regional K Indices 04 Feb :
      Macquarie Island    18   11102056
      Casey               10   34322112
      Mawson              13   54222211

Observed Regional daily pc3 Indices 04 Feb : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             0   (Quiet)
      Hobart               0   (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 Feb : A 
           Fredericksburg         7
           Planetary              8                         

Observed AFr/Ap Indices 03 Feb :  A   K
           Fredericksburg         6
           Planetary              7   1100 1332     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
05 Feb     5    G0
06 Feb    15    G0, chance of G1
07 Feb    10    G0, chance of G1

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 4-Feb. G0 geomagnetic conditions were observed 
at Casey, G0 conditions with an isolated period of G1 were observed 
at Mawson, and periods of G1 and G2 geomagnetic conditions were 
observed at Macquarie Island. G0 geomagnetic conditions are expected 
over 5-Feb. G0 geomagnetic conditions with a chance of G1 are 
expected on 6-7 Feb due to the combined effects of possible glancing 
impacts from CMEs first observed on 3-Feb and 4-Feb and high 
speed wind stream effects from a group of small equatorial coronal 
holes currently rotating towards a geoeffective position.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
05 Feb      Normal         Normal         Normal
06 Feb      Normal         Normal         Normal-fair
07 Feb      Normal         Normal         Normal-fair

COMMENT: Normal HF propagation conditions are expected over 5-7 
Feb. Disturbed conditions are possible on 6-7 Feb due to possible 
geomagnetic activity due to a group of equatorial coronal holes 
currently rotating towards a geoeffective position and possible 
glancing impacts from CMEs first observed on 3-Feb and 4-Feb.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
04 Feb   132

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 25% during local day.
      Enhanced by 75% during local night.
      Enhanced by 50% after local dawn.
   Niue Island Region:
      Enhanced by 35% during local day.
      Enhanced by 20% during local night.
   Northern Australian Region:
      Enhanced by 30% during local day.
      Enhanced by 30% during local night.
   Southern Australian Region:
      Enhanced by 20% during local day.
      Enhanced by 20% during local night.
      Enhanced by 20% after local dawn.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Monthly T index:
Month  T index
Jan      119
Feb      75
Mar      76

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
05 Feb   130    Near to 15% above predicted monthly values
06 Feb   125    Near to 15% above predicted monthly values
07 Feb   120    Near to 15% above predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) in the Australian 
region on UT day 4-Feb were 20-30% enhanced. Sporadic E was observed 
throughout the Australian region. Spread F was observed at Hobart 
during local night. MUFs are expected to be near predicted monthly 
values to 15% enhanced over 5-7 Feb, with a chance of depressions 
over 6-7 Feb due to possible geomagnetic activity caused by a 
group of equatorial coronal holes currently rotating towards 
a geoeffective position and possible glancing impacts from CMEs 
first observed on 3-Feb and 4-Feb. Sporadic E is possible during 
local night, affecting lower frequencies.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 03 Feb
       Daily Proton Fluence >1 MeV:   3.2E+05
       Daily Proton Fluence >10 MeV:  2.6E+04
       Daily Electron Fluence >2 MeV: 2.20E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B5.5

DSCOVR Satellite Solar Wind Day Averaged Data for 03 Feb
Speed: 345 km/sec  Density:    7.1 p/cc  Temp:    25500 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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