[Ips-dsgr] SWS Daily Report - 03 February 22 issued 2336 UT on 03 Feb 2022

rwc rwc at ips.gov.au
Fri Feb 4 10:36:59 EST 2022


SUBJ: SWS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/03 FEBRUARY 2022 BY Space Weather Services
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 03 FEBRUARY AND FORECAST FOR 04 FEBRUARY - 06 FEBRUARY
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: ** YELLOW **
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1A. SOLAR SUMMARY
Activity 03 Feb:  Low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 03 Feb: 127/80


1B. SOLAR FORECAST
             04 Feb             05 Feb             06 Feb
Activity     Low to moderate    Low to moderate    Low to moderate
Fadeouts     Possible           Possible           Possible
10.7cm/SSN   128/81             130/84             125/78

COMMENT: Solar activity was low on UT day 03 February, due to 
low level C class flaring. Solar region AR2936 (N16W54) and solar 
region AR2940 (N18E26) have been reported to have shown slight 
decay. Current M-class flare probability is 50%. A small coronal 
hole is visible near and just west of solar central meridian. 
Possibly two coronal mass ejections have been recently observed, 
the first around 0238UT appears to be from solar activity from 
the far south-west limb and is not considered geoeffective. The 
second at around 0348UT, appears to be possibly associated with 
activity from region AR2936. The CMEs may have overlapped making 
individual event analysis more difficult. Preliminary analysis 
shows that the larger CME from LASCO imager was probably from 
the far southwest limb event, and unlikely to reach the Earth. 
The solar wind parameters were expected to continue to show the 
declining effects of a recent coronal mass ejection, surprisingly 
the north-south component (Bz) of the interplanetary magnetic 
field (IMF) began to gradually drift increasingly southward from 
around 03UT to reach -18nT at around 07UT, then return to mildly 
northward orientation. The cause of this is unclear, it may be 
a rotating magnetic structure in the solar wind that occurred 
on 19 Dec, and 14 Jan, but if so it has occurred earlier than 
27 day patterns would suggest, or perhaps from a recent minor 
southwest directed coronal mass ejection, but no clear discontinuity 
in solar wind parameters is evident.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 03 Feb: Quiet to Minor 
Storm

Estimated Indices 03 Feb : A   K           
   Australian Region      20   23355322
      Darwin              20   23355322
      Townsville          25   23365332
      Learmonth           26   33365332
      Alice Springs       20   23355322
      Gingin              21   32355422
      Canberra            13   12353221
      Hobart              19   23454322    

Estimated Antarctic Regional K Indices 03 Feb :
      Macquarie Island    28   12565422
      Casey               27   46453222
      Mawson              42   45555364

Observed Regional daily pc3 Indices 03 Feb : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               4   (Quiet)
      Canberra             6   (Quiet)
      Hobart              16   (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 03 Feb : A 
           Fredericksburg        26
           Planetary             34                         

Observed AFr/Ap Indices 02 Feb :  A   K
           Fredericksburg         9
           Planetary              9   3200 2411     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
04 Feb    10    Quiet to Unsettled
05 Feb    12    Unsettled
06 Feb    13    Unsettled to Active

COMMENT: Geomagnetic conditions in the Australian region were 
quiet to minor storm levels on UT day 03 February. An isolated 
major storm period was briefly observed in Antarctica. The geomagnetic 
field was expected to slowly decline from mild activity induced 
by a recent CME. However, the geomagnetic field reached minor 
storm levels overnight due to unexpected strongly southward interplanetary 
magnetic field conditions. A mild increase in geomagnetic activity 
may be observed 05-06 February due to a small coronal hole.

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

PCA Event : No event.

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

COMMENT: HF conditions became unexpectedly degraded on 03 February 
due to unexpected geomagnetic storm activity. Initially poor 
HF conditions expected for 04 February for middle to high latitudes, 
recovering to fair as the day progresses. Also, a mild degradation 
may be experienced 06 February. Shortwave fadeouts are possible 
on daylight HF circuits over the next few days.

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
03 Feb    70

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values.
   Niue Island Region:
      Near predicted monthly values during local day.
      Enhanced by 30% during local night.
      Depressed by 20% after local dawn.
   Northern Australian Region:
      Enhanced by 20% during local day.
      Enhanced by 70% during local night.
   Southern Australian Region:
      Near predicted monthly values during local day.
      Enhanced by 25% during local night.
      Depressed 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      46
Feb      38
Mar      41

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
04 Feb     0    Depressed 15 to 25%/near predicted monthly values
05 Feb    65    Near to 15% above predicted monthly values
06 Feb    65    Near to 15% above predicted monthly values

COMMENT: Australian regional maximum usable frequencies (MUFs) 
were near to 70% above predicted monthly values on 3 February. 
The ionosphere for southern region Australia was expected to 
remain depressed during the local day yesterday, but recovered 
more quickly then became enhanced. Degraded HF conditions were 
observed for the southern region Australia during local night 
hours due to unexpected overnight geomagnetic storm activity. 
As a result of this overnight geomagnetic activity the regional 
ionosphere is depressed about 20-30% in the southern Australian 
region this morning. Isolated shortwave fadeouts are possible 
on daylight HF circuits over the next few days.

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 02 Feb
       Daily Proton Fluence >1 MeV:   3.3E+05
       Daily Proton Fluence >10 MeV:  4.1E+04
       Daily Electron Fluence >2 MeV: 1.10E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 2%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B7.9

DSCOVR Satellite Solar Wind Day Averaged Data for 02 Feb
Speed: 458 km/sec  Density:   11.2 p/cc  Temp:   149000 K  Bz:   4 nT

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

Space Weather Services              email: asfc at bom.gov.au
Bureau of Meteorology
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Haymarket NSW 1240  AUSTRALIA       FTP: ftp://ftp-out.sws.bom.gov.au
tel: +61 2 9213 8010                fax: +61 2 9213 8060 

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