[Ips-dsgr] IPS Daily Report - 12 April 10

rwc rwc at ips.gov.au
Tue Apr 13 09:51:04 EST 2010


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 12/2330Z APRIL 2010 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 12 APRIL AND FORECAST FOR 13 APRIL - 15 APRIL
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 12 Apr:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 12 Apr:  75/13

1B. SOLAR FORECAST
             13 Apr             14 Apr             15 Apr
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    75/13              75/13              75/13
COMMENT: Solar activity was very low over the UT day. Solar 
activity is expected to remain at very low levels for the 
next three days. During the last 24 hours the solar wind 
speed gradually decreased from around 420 km/s to 380 km/s. 
The Bz component of the IMF remained negative upto -10 nT 
until 0200UT and then stayed between +/-4 nT for most part 
of the remaining day. 
-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 12 Apr: Mostly unsettled to
active. Periods of minor and major storms 
reported by some stations. 

Estimated Indices 12 Apr :  A   K           
   Australian Region      14   43333321
      Darwin              11   33322331
      Townsville          14   43333321
      Learmonth           15   43333331
      Canberra             7   33222210
      Hobart              11   42223321
      Casey(Ant)          13   44-32221
    
Observed Regional daily pc3 Indices 12 Apr : 
      Darwin               2   (Quiet)
      Townsville           2   (Quiet)
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Gnangara             6   (Quiet)
      Canberra             0   (Quiet)
      Hobart               6   (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 Space Environment Research Center, Japan.


Estimated AFr/Ap Indices 12 Apr : A 
           Fredericksburg        18
           Planetary             22                         

Observed AFr/Ap Indices 11 Apr :  A   K
           Fredericksburg         8
           Planetary              8   1010 3333     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
13 Apr     8    Quiet to Unsettled 
14 Apr     5    Quiet 
15 Apr     4    Quiet 
COMMENT: Geomagnectic activity was high mainly during the 
early hours of the day due to strong solar wind stream and 
negative Bz. Mostly unsettled to active periods were recorded 
through the day with some reports of periods of minor and major 
storm conditions during the early hours of the day. Geomagnetic 
conditions are expected to stay mostly at quiet to unsettled 
levels on 13 April and then gradually decline to quiet levels 
for the following two days. 

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
12 Apr      Normal         Normal-fair    Normal-fair    
PCA Event : No event.

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
13 Apr      Normal         Normal         Normal-Fair
14 Apr      Normal         Normal         Normal
15 Apr      Normal         Normal         Normal
COMMENT: HF conditions were mostly at normal to fair levels 
for most locations on 12 April. Mostly normal conditions may 
be expected for the next three days on most locations with 
the possibility of minor to mild degradations on high latitude 
locations on 13 April due to some possibility of continued 
enhancement in geomagnetic activity levels on this day. 
-----------------------------------------------------------
4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY
12 Apr    29

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

Predicted Monthly T index for April:  20

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
13 Apr    30    near predicted monthly values 
14 Apr    32    near predicted monthly values 
15 Apr    32    near predicted monthly values 
COMMENT: HF conditions in Aus/NZ regions are expected to 
remain mostly normal for next three days as the geomagnetic 
activity is expected to decline to lower levels on 13 April 
and then expected to stay low for the following two days. 
-----------------------------------------------------------
5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 11 Apr
       Daily Proton Fluence >1 MeV:   3.6E+06
       Daily Proton Fluence >10 MeV:  1.7E+04
       Daily Electron Fluence >2 MeV: 2.80E+09   (very high fluence)  

Electron Fluence Daily Deep Dielectric Discharge Probability:41%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A2.7

ACE Satellite Solar Wind Day Averaged Data for 11 Apr
Speed: 380 km/sec  Density:    4.0 p/cc  Temp:    33200 K  Bz:  -1 nT

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


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