[Ips-dsgr] ASWFC Daily Report - 12 March 24 issued 2330 UT on 12 Mar 2024 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Wed Mar 13 10:30:57 EST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/12 MARCH 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 12 MARCH AND FORECAST FOR 13 MARCH - 15 MARCH
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 12 Mar:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 12 Mar: 131/85


1B. SOLAR FORECAST
             13 Mar             14 Mar             15 Mar
Activity     R0-R1              R0-R1              R0-R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   130/84             130/84             135/89

COMMENT: Solar activity on UT day 12-Mar was at the R0 level. 
Solar region AR3599(S13W67, beta-gamma-delta), currently the 
largest and most complex region on the solar disk produced only 
low level C class flare activity in the past 24 hours. Penumbral 
area of the leader spots of AR3599 has increased, with the trailer 
spots showing decline, as the region approaches the southwest 
solar limb. Solar regions AR3606(N09E32, beta) and AR3607(S17E47, 
beta) are showing growth. There are currently five numbered regions 
on the solar disk. All other active regions are either stable 
or in decay. A 10 degree long solar filament located at S25W45 
erupted during 12/1747-1838UT in GONG H-alpha imagery. Solar 
activity is expected to be at the R0-R1 level over 13-15 Mar. 
Several CMEs were observed but none are considered to be Earth 
directed. A faint westward CME was observed from 12/1016UT in 
LASCO C2 imagery but could not be correlated with on disk activity. 
The erupting filament did not as yet appear to have an associated 
CME (available images up to 12/1848UT). The solar wind speed 
on UT day 12-Mar was steady, ranging from 410 to 420 km/s and 
is currently near 375 km/s. The peak total interplanetary field 
strength (IMF, Bt) was 6 nT and the north south IMF component 
(Bz) range was +5 to -5 nT. An isolated equatorial coronal hole 
located west of the solar central meridian and a possible weak 
CME graze are expected to cause a mild increase in wind speed 
during 14-15 Mar.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 12 Mar: G0

Estimated Indices 12 Mar : A   K           
   Australian Region       4   21121201
      Cocos Island         -   --------
      Darwin               3   21111102
      Townsville           3   11121201
      Learmonth            -   --------
      Alice Springs        4   21121201
      Gingin               5   31121201
      Canberra             3   21121101    

Estimated Antarctic Regional K Indices 12 Mar :
      Macquarie Island     6   11042300
      Casey                9   34321111
      Mawson               9   42322210

Observed Regional daily pc3 Indices 12 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth           NA
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra            14   (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 12 Mar : A 
           Fredericksburg         7
           Planetary              7                         

Observed AFr/Ap Indices 11 Mar :  A   K
           Fredericksburg         4
           Planetary              5   1122 1221     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
13 Mar     8    G0
14 Mar    16    G0, slight chance G1
15 Mar    10    G0

COMMENT: G0 geomagnetic conditions were observed in the Australian 
and Antarctic region on UT day 12-Mar. Generally G0 geomagnetic 
conditions are expected over 13-15 Mar, with a coronal hole wind 
stream together with a chance of a weak CME graze expected to 
produce a mild increase in geomagnetic activity for 14-15 Mar.

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3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
12 Mar      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
13 Mar      Normal         Normal         Normal-fair
14 Mar      Normal         Normal-fair    Fair
15 Mar      Normal         Normal         Normal-fair

COMMENT: HF radio communication conditions on UT day 12-Mar were 
normal. HF radio communication conditions are expected to be 
mostly normal over 13-15 Mar, with a chance of fair conditions 
at high latitudes on 14-Mar. Isolated shortwave fadeouts are 
possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
12 Mar   121

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 30% during local day.
      Enhanced by 15% during local night.
   Niue Island Region:
      Near predicted monthly values during local day.
      Depressed by 15% during local night.
   Northern Australian Region:
      Near predicted monthly values to 50% enhanced.
   Southern Australian Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Davis/Mawson):
      Enhanced by 25% over the UT day.

Monthly T index:
Month  T index
Feb      138
Mar      111
Apr      112

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
13 Mar   110    Near predicted monthly values
14 Mar   110    Near predicted monthly values
15 Mar   110    Near predicted monthly values

COMMENT: ASWFC SWF HF Communications Warning 26 was issued on 
11 March and is current for 11-13 Mar. Maximum usable frequencies 
(MUFs) in the Australian region on UT day 12-Mar were generally 
near predicted monthly values. Enhancements of 50% were observed 
at Darwin late in the local day and during local night hours. 
Minor scintillation was observed at Darwin and Weipa 12/12-15UT. 
Minor spread F was observed at Perth during local night hours. 
MUFs are expected to be near predicted monthly values over 13-15 
Mar. Isolated shortwave fadeouts are possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 11 Mar
       Daily Proton Fluence >1 MeV:   1.4E+06
       Daily Proton Fluence >10 MeV:  2.0E+04
       Daily Electron Fluence >2 MeV: 5.00E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 7%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B4.4

DSCOVR Satellite Solar Wind Day Averaged Data for 11 Mar
Speed: 378 km/sec  Density:    2.8 p/cc  Temp:    40100 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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