[Ips-dsgr] ASWFC Daily Report - 27 February 23 issued 2331 UT on 27 Feb 2023 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Tue Feb 28 10:31:07 EST 2023


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/27 FEBRUARY 2023
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 27 FEBRUARY AND FORECAST FOR 28 FEBRUARY - 02 MARCH
STATUS INDICATORS SOL:** YELLOW **   MAG:** RED **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 27 Feb:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 27 Feb: 161/115


1B. SOLAR FORECAST
             28 Feb             01 Mar             02 Mar
Activity     R0-R1              R0-R1              R0-R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   160/114            158/112            154/109

COMMENT: Solar activity on UT day 27-Feb was at the R0 level, 
with multiple C-class flares. The largest was a C4.5 flare at 
27/1022UT, produced by AR3234 (N24W21, beta-delta). There are 
currently 7 numbered sunspot regions on the solar disk and 1 
unnumbered region. AR3234 showed sunspot development over the 
UT day and is the largest and most magnetically complex region 
on the solar disk, although it has not produced an M-class flare 
since 23-Feb. AR3229 (N26W73, alpha), which produced the major 
flaring on 24-25 Feb, showed decay over the UT day and is soon 
to rotate off the solar disk. All other numbered sunspot regions 
are stable or in decay. An unnumbered region is present at S04W10 
with beta magnetic characteristics, this region developed over 
the UT day. Solar activity is expected to be at R0-R1 levels 
over 28-Feb to 2-Mar, with a chance of R2. Several CMEs were 
observed over the UT day, but none are considered to be geoeffective. 
The solar wind speed on UT day 27-Feb increased, ranging between 
523 and 883 km/s, and is currently near 700 km/s. A moderate 
shock was observed in the solar wind at 27/1018UT, likely due 
to an anticipated impact from a CME first observed on 25-Feb. 
The peak interplanetary field strength (IMF, Bt) reached 20 nT 
and the north-south IMF component (Bz) range was +13 to -19 nT. 
Bz was predominately southward over 27-Feb, with the longest 
period of sustained Bz at -5 nT or lower occurring from 27/0518UT 
to 27/1141UT. The solar wind speed is expected to decline over 
28-Feb to 2-Mar as coronal hole and CME induced high speed wind 
stream effects wane. The shock in the solar wind on 27-Feb is 
likely due to an impact from the CME forecast to arrive on 28-Feb, 
however there is a slight chance that further CME-caused enhancements 
may occur on 28-Feb. In the absence of further CME activity, 
the solar wind speed is expected to return to background levels 
on 2-Mar. The solar energetic proton flux (>10 MeV) remains enhanced, 
but below the S1 threshold. Further S1 conditions are unlikely.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 27 Feb: G2

Estimated Indices 27 Feb : A   K           
   Australian Region      46   44565555
      Cocos Island        33   33354555
      Darwin              41   44465455
      Townsville          46   44565555
      Learmonth           60   55566556
      Alice Springs       49   54565555
      Gingin              54   54466556
      Canberra            44   44565554
      Hobart              75   44677664    

Estimated Antarctic Regional K Indices 27 Feb :
      Macquarie Island    95   45776775
      Casey               44   56545445
      Mawson              83   65666676

Observed Regional daily pc3 Indices 27 Feb : 
      Darwin               2   (Quiet)
      Townsville           4   (Quiet)
      Learmonth           35   (Quiet to unsettled)
      Alice Springs       16   (Quiet)
      Gingin              95   (Minor storm)
      Canberra           105   (Major storm)
      Hobart              NA

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 27 Feb : A 
           Fredericksburg        60
           Planetary            102                         

Observed AFr/Ap Indices 26 Feb :  A   K
           Fredericksburg        18
           Planetary             22   3234 2155     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
28 Feb    32    G1-G2, chance of G3
01 Mar    18    G0-G1
02 Mar    12    G0, chance of G1

COMMENT: ASWFC Geomagnetic Warning 8 was issued on 26 February 
and is current for 26-28 Feb. G3 geomagnetic conditions were 
observed at the planetary level on UT day 27-Feb. Mostly G1 geomagnetic 
conditions were observed in the Australian region on 27-Feb, 
with one period of G2. Two periods of G3 conditions were observed 
at Hobart. G3 geomagnetic conditions were observed at Macquarie 
Island, G1 conditions with a period of G2, were observed at Casey 
and G2 conditions with a period of G3 were observed at Mawson. 
A very weak (6 nT) shock was observed at 27/1017UT, likely indicating 
the arrival of a CME first observed on 25-Feb however there is 
a slight chance that this CME is yet to arrive. G1-G2 geomagnetic 
conditions, with a chance of an isolated period of G3, are expected 
on 28-Feb due to ongoing geomagnetic activity. G0-G1 geomagnetic 
conditions are expected on 1-Mar and G0 conditions with a chance 
of G1 are expected on 2-Mar as coronal hole and CME effects wane.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
27 Feb      Normal-fair    Fair           Fair-poor      

PCA Event : 10MeV Proton/PCA Event Began at 2100UT 25/02, Ended at 1830UT 26/02
 and, 10MeV Proton/PCA Event Began at 1935UT 26/02, Ended at 2005UT 26/02
 and, 10MeV Proton/PCA Event Began at 2035UT 26/02, Ended at 2245UT 26/02

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
28 Feb      Fair           Fair           Fair-poor
01 Mar      Normal         Normal-fair    Fair
02 Mar      Normal         Normal         Normal-fair

COMMENT: Degraded HF conditions are expected on 28-Feb particularly 
at high latitudes, due to ongoing geomagnetic activity. HF conditions 
are expected to recover over 1-2 Mar, with a chance of degraded 
conditions on 1-Mar, particularly at high latitudes. Shortwave 
fadeouts are possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
27 Feb    90

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 15% during local day.
      Near predicted monthly values during local night.
      Enhanced by 20% after local dawn.
   Niue Island Region:
      Enhanced by 35% during local day.
      Enhanced by 50% during local night.
      Enhanced by 45% after local dawn.
   Northern Australian Region:
      Depressed by 15% during local day.
      Enhanced by 15% during local night.
   Southern Australian Region:
      Mostly near predicted monthly values.
      Depressed by 35% 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
28 Feb    80    Near predicted monthly values
01 Mar    95    Near to 15% above predicted monthly values
02 Mar    95    Near to 15% above predicted monthly values

COMMENT: ASWFC HF Communications Warning 23 was issued on 26 
February and is current for 27-28 Feb. Maximum usable frequencies 
(MUFs) in the Northern Australian region on UT day 27-Feb were 
between 15% depressed and 15% enhanced. MUFs in the southern 
Australian region were near monthly predicted values to 35% depressed, 
with the strongest depressions occurring at Hobart during local 
night. The depressed HF conditions are due to ongoing geomagnetic 
activity due to a combination of coronal hole high speed wind 
stream effects and two CME impacts on 27-Feb and 28-Feb. Significant 
sporadic-E was observed at Norfolk Island and Niue during local 
night and Brisbane during local dawn. Spread F was observed at 
Hobart during local night. MUFs are expected to be near predicted 
monthly values to 20% depressed over 28-Feb, due to ongoing geomagnetic 
activity. The strongest depressions are expected at higher latitudes. 
MUFs are expected to recover to near predicted monthly values 
to 15% enhanced over 1-2 Mar as geomagnetic activity wanes, with 
mild depressions possible on 1-Mar in the southern Australian 
region. Shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 26 Feb
       Daily Proton Fluence >1 MeV:   1.7E+08
       Daily Proton Fluence >10 MeV:  2.8E+06
       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: C1.6

DSCOVR Satellite Solar Wind Day Averaged Data for 26 Feb
Speed: 474 km/sec  Density:   18.3 p/cc  Temp:   181000 K  Bz:   2 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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