[Ips-dsgr] ASWFC Daily Report - 07 March 24 issued 2330 UT on 07 Mar 2024 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Fri Mar 8 10:30:08 EST 2024


SUBJ: ASWFC DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/07 MARCH 2024
FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE
SUMMARY FOR 07 MARCH AND FORECAST FOR 08 MARCH - 10 MARCH
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://bit.ly/3lmaMBx
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1A. SOLAR SUMMARY
Activity 07 Mar:  R0

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 07 Mar: 137/91


1B. SOLAR FORECAST
             08 Mar             09 Mar             10 Mar
Activity     R0-R1              R0-R1              R0-R1
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   140/94             140/94             145/99

COMMENT: Solar activity on UT day 07-Mar was at the R0 level, 
with no significant flares observed. There are currently seven 
numbered regions on the solar disk. Solar regions currently on 
the visible solar disk are relatively small. Solar region AR3599(S12E02, 
beta) continues to develop with spot redistribution evident and 
produced several C class flares with the largest a C8.3 at 07/0618UT. 
Earlier in the UT day this region exhibited a more complex though 
weak beta-gamma magnetic configuration. A new small region is 
emerging at S17E34. Other regions are either stable or in decay. 
Solar filament motion was observed in the southeast solar quadrant 
07/0600-0700UT in SDO304 imagery. Learmonth GONG imagery showed 
a small northward section of filament possibly erupting at 07/0847UT 
located at S17E15. However no CME appeared associated with these 
events. Small localised coronal diming was observed to the southwest 
of solar region AR3602(N18W09, beta) at 07/1236UT in SDO193 imagery. 
Solar activity is expected to be at the R0-R1 over 08-10 Mar, 
with low level R class flare activity becoming more likely from 
AR3599. S0 conditions were observed on 07-Mar and are expected 
over 08-10 Mar. No new Earth directed CMEs have been observed. 
A narrow CME was observed to the north-northwest from 07/1336UT. 
Later a more north westward and presumed far side event was observed 
from 07/1624UT. A model run was conducted assuming with low confidence 
that the minor on disk diming and the steep and narrow north-northwest 
CME are associated. The model run showed an Earth miss with the 
CME passing above the Earth. The solar wind speed was steady 
on 07-Mar, ranging from 366 to 466 km/s and is currently near 
435 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 near 
background levels over 08-Mar. A mild increase in wind speed 
may be observed from mid 09-Mar/early 10-Mar due to the filament 
eruption on 05-Mar. A very small isolated equatorial coronal 
hole now in the western solar hemisphere may slightly increase 
wind speed 09-10 Mar.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 07 Mar: G0

Estimated Indices 07 Mar : A   K           
   Australian Region      12   32332332
      Cocos Island         9   31222332
      Darwin              11   32332322
      Townsville          12   32332332
      Learmonth           13   42332332
      Alice Springs       12   32332332
      Gingin              13   31332342
      Canberra             8   21322322    

Estimated Antarctic Regional K Indices 07 Mar :
      Macquarie Island    10   21223422
      Casey               18   43532233
      Mawson              22   33343354

Observed Regional daily pc3 Indices 07 Mar : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               0   (Quiet)
      Canberra             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 07 Mar : A 
           Fredericksburg        11
           Planetary             14                         

Observed AFr/Ap Indices 06 Mar :  A   K
           Fredericksburg         5
           Planetary              5   1312 2101     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
08 Mar     8    G0
09 Mar    16    G0, chance G1
10 Mar    16    G0, chance G1

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 07-Mar. Mostly G0 conditions were observed in 
the Antarctic region, with one isolated period of G1 conditions 
observed at Casey. G0 geomagnetic conditions are generally expected 
over 08-10 Mar. A mild increase in geomagnetic activity may be 
experienced from mid 09-Mar to first half of 10-Mar due to possible 
graze from a recent solar filament eruption/CME and possible 
minor influence from a small coronal hole wind stream.

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

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
08 Mar      Normal         Normal         Normal-fair
09 Mar      Normal         Normal-fair    Fair
10 Mar      Normal         Fair-normal    Fair

COMMENT: HF radio communication conditions on UT day 07-Mar were 
normal. HF radio communication conditions are generally expected 
to be mostly normal over 08-10 Mar. Mild degradation possible 
for high latitudes 09-10 Mar. Isolated minor HF fadeouts possible.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
07 Mar   119

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 15-30%.
   Niue Island Region:
      Near predicted monthly values.
   Northern Australian Region:
      Near predicted monthly values.
   Southern Australian Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Davis/Mawson):
      Near predicted monthly values 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
08 Mar   110    Near predicted monthly values
09 Mar   110    Near predicted monthly values
10 Mar   110    Near predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) in the Australian 
region on UT day 07-Mar were near predicted monthly values. MUFs 
are expected to be near predicted monthly values over 08-10 Mar. 
Isolated minor HF fadeouts possible.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 06 Mar
       Daily Proton Fluence >1 MeV:   3.4E+04
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 1.40E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B5.9

DSCOVR Satellite Solar Wind Day Averaged Data for 06 Mar
Speed: 405 km/sec  Density:    2.4 p/cc  Temp:    59200 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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