[Ips-dsgr] SWS Daily Report - 11 April 22 issued 2331 UT on 11 Apr 2022 [SEC=OFFICIAL]

Regional Warning Centre rwc at ips.gov.au
Tue Apr 12 09:31:19 EST 2022


SUBJ: SWS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/11 APRIL 2022 BY Space Weather Services
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 11 APRIL AND FORECAST FOR 12 APRIL - 14 APRIL
STATUS INDICATORS SOL:GREEN   MAG:** RED **     ION: GREEN
ASWAS SCALE DESCRIPTION: https://sws.bom.gov.au/
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1A. SOLAR SUMMARY
Activity 11 Apr:  R0 - None

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 11 Apr:  99/46


1B. SOLAR FORECAST
             12 Apr             13 Apr             14 Apr
Activity     R0 - None		R0 - None	   R0 - None
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    98/45              95/41              95/41

COMMENT: On UT day 11 Apr, solar activity was at R0 level, with
no major sunspot groups observed on the solar disk. A single C1.6
flare was observed with an associated filament eruption from
AR2987. The filament eruption was observed at ~05UT on 11 Apr,
located at S15E05, with a filament length of ~10 degrees; an
associated halo CME was observed in both LASCO C2/C3 and STEREO A
imagery. Event analysis and modelling indicates an Earth-directed
CME, with impact on UT Day 13 Apr at ~16UT. An isolated equatorial
coronal hole is visible in the eastern solar hemisphere, which is
expected to increase the solar wind speed in the coming week.
Solar activity is expected to be at R0 level on 12-14 Apr. On UT
day 11 Apr, the solar wind parameters were slightly enhanced due
to weak coronal hole effects, with a min/max of 443/546 km/s.
There is a declining trend in the solar wind speed as the coronal
hole effects abate with solar rotation. The total interplanetary
magnetic field (IMF; Bt) peaked at 9 nT and the IMF north-south
component (Bz) varied between +/-6 nT. Solar wind conditions are
expected to be enhanced on 13-14 Apr due to CME impacts from
filament eruption observed on 11 Apr.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 11 Apr: G0 - None

Estimated Indices 11 Apr : A   K           
   Australian Region       7   32231120
      Darwin               7   32231111
      Townsville           9   33232121
      Learmonth            7   32231220
      Alice Springs        8   33231120
      Gingin               9   32232230
      Canberra             7   32231120
      Hobart              10   33242120    

Estimated Antarctic Regional K Indices 11 Apr :
      Macquarie Island    12   33252120
      Casey               20   55342222
      Mawson              25   44333255

Observed Regional daily pc3 Indices 11 Apr : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice Springs        0   (Quiet)
      Gingin               9   (Quiet)
      Canberra            15   (Quiet)
      Hobart              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 11 Apr : A 
           Fredericksburg        14
           Planetary             15                         

Observed AFr/Ap Indices 10 Apr :  A   K
           Fredericksburg        18
           Planetary             29   2753 3322     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
12 Apr    12    G0 - None
13 Apr    30    G0-G1 - Minor
14 Apr    20    G1-G0 - Minor

COMMENT: G0 geomagnetic conditions were observed in the Australian 
region on UT day 11 Apr. G1 levels were observed in Antarctica. 
G0 tending towards G1 conditions expected on 13-14 Apr due to 
halo CME impacts associated with filament eruption observed on 
11 Apr. Chance of isolated G2 period on 13 Apr.

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
11 Apr      Normal         Normal         Normal-fair    

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
12 Apr      Normal         Normal         Normal-fair
13 Apr      Normal         Normal-fair    Normal-poor
14 Apr      Normal         Fair-normal    Fair-normal

COMMENT: Mild to moderate MUF degradations may be observed on 
13-14 Apr due to anticipated arrival of coronal mass ejection 
observed on 11 Apr.

-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY


Date   T index
11 Apr    63

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 50% during local day.
      Near predicted monthly values during local night.
      Enhanced by 25% after local dawn.
   Niue Island Region:
      Enhanced by 20% during local day.
      Near predicted monthly values during local night.
      Enhanced by 20% after local dawn.
   Northern Australian Region:
      Enhanced by 15% during local day.
      Enhanced by 15% during local night.
   Southern Australian Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Near predicted monthly values over the UT day.

Monthly T index:
Month  T index
Mar      64
Apr      46
May      49

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
12 Apr    60    Near predicted monthly values
13 Apr    50    Near predicted monthly values/depressed 10 to 
                20%
14 Apr    35    Depressed 10 to 20%/near predicted monthly values

COMMENT: Maximum usable frequencies (MUFs) on UT day 11 Apr were 
near monthly predicted values to slightly enhanced. Mild to moderate 
MUF degradations may be observed at high to mid latitude regions 
on 13-14 Apr due to anticipated arrival of coronal mass ejection 
observed on 11 Apr.

-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 10 Apr
       Daily Proton Fluence >1 MeV:   6.2E+05
       Daily Proton Fluence >10 MeV:  3.9E+04
       Daily Electron Fluence >2 MeV: 4.00E+06   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B2.6

DSCOVR Satellite Solar Wind Day Averaged Data for 10 Apr
Speed: 482 km/sec  Density:    6.8 p/cc  Temp:   206000 K  Bz:  -1 nT

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

Space Weather Services              email: asfc at bom.gov.au
Bureau of Meteorology
PO Box 1386                         WWW: http://www.sws.bom.gov.au
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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