[Ips-dsgr] IPS Daily Report - 25 June 12 issued 2330 UT on 25 Jun 2012

rwc rwc at ips.gov.au
Tue Jun 26 09:30:52 EST 2012


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/25 JUNE 2012 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 25 JUNE AND FORECAST FOR 26 JUNE - 28 JUNE
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: ** YELLOW **
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 25 Jun:  Low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 25 Jun:  89/33


1B. SOLAR FORECAST
             26 Jun             27 Jun             28 Jun
Activity     Low                Low                Low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    90/34              95/41             100/48

COMMENT: Solar activity was low over the last 24 hours with a 
single C1 flare from region 1512 (S16E39). This region emerged 
over the last 24 hours and continues to grow. No active regions 
with significant flare potential are currently on the visible 
Sun. A small CME was observed late in the UT day directed to 
the south eastern limb. It is not expected to be geoeffective. 
Solar wind conditions are ambient. Low flare activity and ambient 
solar wind conditions are expected for the next 3 days.

-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 25 Jun: Quiet to Unsettled

Estimated Indices 25 Jun : A   K           
   Australian Region       7   11223231
      Darwin               7   21213231
      Townsville          11   32323232
      Learmonth            8   22223231
      Norfolk Island       4   11212121
      Camden               5   11223120
      Canberra             4   11212120
      Hobart               4   01222---    

Estimated Antarctic Regional K Indices 25 Jun :
      Macquarie Island     7   00324210
      Casey                8   22322231
      Mawson              14   43333231

Observed Regional daily pc3 Indices 25 Jun : 
      Darwin               0   (Quiet)
      Townsville          34   (Quiet to unsettled)
      Learmonth           NA
      Alice Springs        0   (Quiet)
      Gnangara             0   (Quiet)
      Canberra             0   (Quiet)
      Hobart              57   (Unsettled)

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 Space Environment Research Center, Japan.


Estimated AFr/Ap Indices 25 Jun : A 
           Fredericksburg         8
           Planetary              8                         

Observed AFr/Ap Indices 24 Jun :  A   K
           Fredericksburg         5
           Planetary              4   2111 1221     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
26 Jun     5    Quiet
27 Jun     5    Quiet
28 Jun     5    Quiet

COMMENT: Geomagnetic conditions have been mostly Quiet over the 
past 24 hours with isolated Unsettled periods. Conditions are 
expected to be mostly quiet for the next 3 days.

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
25 Jun      Normal         Normal         Normal         

PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
26 Jun      Normal         Normal         Normal
27 Jun      Normal         Normal         Normal
28 Jun      Normal         Normal         Normal

COMMENT: HF propagation conditions are good however the maximum 
useable frequencies are depressed due to low levels of ionising 
EUV flux and are expected to remain depressed for the next 3 
days.

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


Date   T index
25 Jun    51

Observed Australian Regional MUFs
   Cocos Island Region:
      Near predicted monthly values during local day.
      Depressed by 30% during local night.
   Niue Island Region:
      Depressed by 20% during local day.
      Depressed by 20% during local night.
   Northern Australian Region:
      Depressed by 30% during local day.
      Depressed by 30% during local night.
   Southern Australian and New Zealand Region:
      Depressed by 20% during local day.
      Near predicted monthly values during local night.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Depressed by 20% over the UT day.

Predicted Monthly T index for June:  78

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
26 Jun    50    Depressed by up to 30%
27 Jun    50    Depressed by up to 30%
28 Jun    50    Depressed by up to 30%

COMMENT: IPS HF Communications Warning 23 was issued on 24 June 
and is current for 25-26 Jun. IPS HF Communications Warning 23 
was issued on 24 June and is current for 25-26 Jun. MUF depressions 
were observed over most of the Australian region during the last 
24 hours. MUFs are expected to be depressed by up to 30% in the 
Australian region over the next 2-3 days.

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

GOES satellite data for 24 Jun
       Daily Proton Fluence >1 MeV:   1.1E+06
       Daily Proton Fluence >10 MeV:  1.2E+04
       Daily Electron Fluence >2 MeV: 1.20E+08   (moderate fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability:12%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A6.8

ACE Satellite Solar Wind Day Averaged Data for 24 Jun
Speed: 365 km/sec  Density:    5.7 p/cc  Temp:    26500 K  Bz:   2 nT

(Courtesy Space Weather Prediction Center, Boulder USA)
ACE data can be incorrect during strong proton events.
-----------------------------------------------------------

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