[Ips-dsgr] IPS Daily Report - 19 May 10

rwc rwc at ips.gov.au
Thu May 20 09:44:47 EST 2010


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 19/2330Z MAY 2010 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 19 MAY AND FORECAST FOR 20 MAY - 22 MAY
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 19 May:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 19 May:  69/3

1B. SOLAR FORECAST
             20 May             21 May             22 May
Activity     Very low           Very low           Very low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN    70/5               70/5               72/8

COMMENT: Solar activity was Very Low during the last 24 hours. 
Solar wind speed increased from 350 to 500 km/s at approximately 
1300UT/19 due to recurrent coronal hole. Expect the solar wind 
speed to remain around 500 km/s today, 20 May, and and gradually 
return to pre-coronal hole levels on 21 May. The Bz component 
of the interplanetary magnetic field ranged between +/-10 nT, 
however was mostly positive. Noted a coronal mass ejection on 
the northwest quadrant of the solar disc, first appearing on 
SOHO C3 imagery at 1218UT/19. It is not expected to be geo-effective. 
Solar activity is expected to remain at Very Low levels for the 
next three days. 

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 19 May: Quiet to Unsettled 

Estimated Indices 19 May :  A   K           
   Australian Region       8   22223222
      Darwin               7   12223222
      Townsville          15   33333333
      Learmonth            7   21223221
      Canberra             2   01112200
      Hobart               5   11112311
      Casey(Ant)           7   22222222
    
Observed Regional daily pc3 Indices 19 May : 
      Darwin               4   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Alice_Springs        0   (Quiet)
      Gnangara             2   (Quiet)
      Canberra             6   (Quiet)
      Hobart              19   (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 19 May : A 
           Fredericksburg         6
           Planetary             10                         

Observed AFr/Ap Indices 18 May :  A   K
           Fredericksburg         4
           Planetary              6   2222 2111     

2B. MAGNETIC FORECAST 
Date      Ap    Conditions
20 May    12    Unsettled 
21 May    10    Quiet to Unsettled 
22 May     6    Quiet 

COMMENT: IPS Geomagnetic Warning 5 was issued on 18 May and is 
current for interval 19-21 May. Geomagnetic field went from Quiet 
to Unsettled conditions due to an increase in the solar wind 
speed. Expect Unsettled conditions to prevail over the UT day, 
20 May and gradually return to Quiet levels on 21 May. Isolated 
cases of Active levels possible while solar wind is elevated, 
particularly if the Bz component of the IMF has a prolong negative 
direction. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
20 May      Normal         Normal         Normal-Fair
21 May      Normal         Normal         Normal-Fair
22 May      Normal         Normal         Normal

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4A. AUSTRALIAN REGION IONOSPHERIC SUMMARY

Date   T index
19 May     6

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

Predicted Monthly T index for May:  24

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
20 May     5    depressed 10 to 20%/near predicted monthly values 
21 May     5    depressed 10 to 20%/near predicted monthly values 
22 May    15    Near predicted monthly values 

COMMENT: Mild MUF depressions were observed in the Australian 
region due to the lower EUV levels emitted from the sun, resulting 
from the lack of sunspots on the visible solar disc. Expect this 
trend to continue until sunspot numbers return to predicted levels. 
The Unsettled Geomagnetic activity over the next two days is 
not expected to have a significant effect on the HF conditions 
in the Australian Region. Note, sunspot region 1069 is due to 
rotate onto the visible solar disc on 22 May. 

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5. SPACE ENVIRONMENT SUMMARY

GOES satellite data for 18 May
       Daily Proton Fluence >1 MeV:   1.0E+05
       Daily Proton Fluence >10 MeV:  1.9E+04
       Daily Electron Fluence >2 MeV: 3.70E+06   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A1.5

ACE Satellite Solar Wind Day Averaged Data for 18 May
Speed: 358 km/sec  Density:    1.2 p/cc  Temp:    49400 K  Bz:  -1 nT

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