[Ips-dsgr] IPS Daily Report - 28 April 06

rwc rwc at ips.gov.au
Sat Apr 29 09:49:15 EST 2006


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 28/2330Z APRIL 2006 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 28 APRIL AND FORECAST FOR 29 APRIL - 01 MAY
STATUS INDICATORS SOL:** YELLOW **   MAG:GREEN     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 28 Apr:  Low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 28 Apr: 100/48


1B. SOLAR FORECAST
             29 Apr             30 Apr             01 May
Activity     Low to moderate    Low                Low
Fadeouts     Possible           Possible           None expected
10.7cm/SSN   100/48             100/48             100/48

COMMENT: Solar activity was low over the UT day. The most significant 
X-ray flare of the period was a C1.9 at 0826UT from region 0875 
(S12E10). This region is now classified as a DAC beta-gamma spot 
group and although it appears to be declining, remains active 
and is likely to produce further C-class flares over the next 
two days. There is also a chance of an isolated M-class flare 
from this region. Trailing region 0876 (S16E35) has increased 
slightly in size over the period but remains otherwise largely 
stable. A discontinuity occurred in the solar wind at ~00UT, 
associated with some large IMF Bz fluctuations, after which solar 
wind speed increased steadily to ~440km/s. The discontinuity 
was likely a glancing blow from the eastward directed CME which 
occurred on 25 April. 

IPS/USAF Learmonth Observatory reports good flare potential
 from solar region(s):number 875.
-----------------------------------------------------------
2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 28 Apr: Quiet to Active 

Estimated Indices 28 Apr :  A   K           
   Australian Region      10   32432111
      Darwin              10   32432112
      Learmonth           10   32432111
      Culgoora             9   32432001
      Camden               5   21------
      Canberra             9   32432011
      Hobart               6   23321001
      Casey(Ant)          10   33431111
    
Observed Regional daily pc3 Indices 28 Apr : 
      Canberra            16   (Quiet)
      Learmonth            2   (Quiet)
      Culgoora             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. 


Estimated AFr/Ap Indices 28 Apr : A 
           Fredericksburg        14
           Planetary             15                         

Observed AFr/Ap Indices 27 Apr :  A   K
           Fredericksburg         3
           Planetary              5   2211 1212     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
29 Apr     8    Quiet to Unsettled 
30 Apr     5    Quiet 
01 May     5    Quiet 

COMMENT: Geomagnetic activity was generally unsettled over the 
UT day, particularly in the first half of the day with a period 
of active conditions 06-09UT. The activity was due to a solar 
wind discontinuity and large interplanetary magnetic field (IMF) 
fluctuations associated with a glancing blow from a CME. The 
magnetic field activity returned to quiet levels in the latter 
half of the day which is expected to continue. The outlook is 
for generally quiet conditions next 3 days unless an extended 
period of IMF Bz southwards (>12hrs) occurs. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
29 Apr      Normal         Normal         Normal        
30 Apr      Normal         Normal         Normal        
01 May      Normal         Normal         Normal        

COMMENT: Mostly normal HF conditions observed at low and mid 
latitudes. High latitudes showed some depressions and minor disturbances 
during the day, likely associated with the solar wind activity. 
These conditions are expected to continue in the absence of major 
M class flaring activity from AR875. 

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


Date   T index
28 Apr    39

Observed Australian Regional MUFs
   Equatorial PNG/Niue Region:
      Near predicted monthly values.
   Northern Australian Region:
      Near predicted monthly values during local day,
      Enhanced by 25% during local night.
   Southern Australian and New Zealand Region:
      Near predicted monthly values during local day,
      Enhanced by 30% during local night.
      Enhanced by 20% after local dawn.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Depressed by 10% during local day 
      Enhanced by 15% during local night.

Predicted Monthly T index for April:  16

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
29 Apr    40    10 to 25% above predicted monthly values 
30 Apr    41    10 to 25% above predicted monthly values 
01 May    42    10 to 25% above predicted monthly values 

COMMENT: Mostly normal HF conditions observed over the UT day. 
MUFs generally well above predicted monthly values. Some high 
latitude stations observed daytime depressions depending on location, 
likely related to solar wind activity. Mostly normal HF conditions 
expected for the next three days with a continued strengthening 
of the ionosphere due to extra ionising solar radiation from 
active regions 875 and 876. MUFs generally above predicted monthly 
values by 10-25%. 

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

GOES satellite data for 27 Apr
       Daily Proton Fluence >1 MeV:   2.6E+05
       Daily Proton Fluence >10 MeV:  1.7E+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: B1.3

ACE Satellite Solar Wind Day Averaged Data for 27 Apr
Speed: 324 km/sec  Density:    3.5 p/cc  Temp:    43600 K  Bz:  -1 nT

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


IPS Radio and Space Services        email: asfc at ips.gov.au
PO Box 1386                         WWW: http://www.ips.gov.au
Haymarket NSW 1240  AUSTRALIA       FTP: ftp://ftp.ips.gov.au 
tel: +61 2 9213 8010                fax: +61 2 9213 8060 

IMPORTANT: This e-mail, including any attachments, may contain,confidential
or copyright information.  The views expressed in this message are those of
the individual sender, unless specifically stated to be the views of IPS.
If you are not the intended recipient, please contact the sender immediately
and delete all copies of this e-mail and attachments. Occasionally IPS sends 
email promoting IPS products and services to its mailing list customers. 
If you do not wish to receive this promotional material please email 
no-spam at ips.gov.au with the subject header:UNSUBSCRIBE"





More information about the ips-dsgr mailing list