[Ips-dsgr] IPS Daily Report - 17 May 07

rwc rwc at ips.gov.au
Fri May 18 09:26:49 EST 2007


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 17/2330Z MAY 2007 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 17 MAY AND FORECAST FOR 18 MAY - 20 MAY
STATUS INDICATORS SOL:** YELLOW **   MAG:** YELLOW **     ION: GREEN
-----------------------------------------------------------
1A. SOLAR SUMMARY
Activity 17 May:  Very low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 17 May:  77/16


1B. SOLAR FORECAST
             18 May             19 May             20 May
Activity     Low to moderate    Low                Low
Fadeouts     Possible           None expected      None expected
10.7cm/SSN    75/13              75/13              75/13

COMMENT: Solar activity was very low over the past 24 hours with 
the only flares being two B-class from spot region 956 (N03E24). 
This region remains large and magnetically complex and has the 
potential to produce C-class or isolated M-class flares over 
the next 24 hours. Flaring from the other two spot groups on 
the visibile disk (AR955, AR957) is unlikely. A small equatorial 
coronal hole is currently located west of central meridian the 
effects of which are expected to arrive on May 19. 

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

Geomagnetic field for Australian Region 17 May: Quiet 

Estimated Indices 17 May :  A   K           
   Australian Region       3   11111112
      Darwin               4   21111112
      Townsville           6   12212222
      Learmonth            4   11112112
      Camden               1   00001011
      Canberra             0   00001001
      Hobart               1   00101111
      Casey(Ant)           5   12212122
    
Observed Regional daily pc3 Indices 17 May : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            0   (Quiet)
      Camden              15   (Quiet)
      Canberra             0   (Quiet)
      Hobart               3   (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 17 May : A 
           Fredericksburg         5
           Planetary              5                         

Observed AFr/Ap Indices 16 May :  A   K
           Fredericksburg         3
           Planetary              4   1111 1112     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
18 May     3    Quiet 
19 May    10    Quiet to unsettled 
20 May    16    Unsettled 

COMMENT: Geomagnetic activity was very quiet over the UT day 
and is expected to be quiet for the next 24 hours (18 May), however 
there is a small chance that a CME observed on 15 May had an 
Earthward-directed component which could produce an isolated 
period of Unsettled-Active conditions early on 18 May. A widespread 
increase in geomagnetic activity is likely on 19 May, continuing 
into 20 May due to the arrival of a high speed coronal hole wind 
stream. 

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

3B. GLOBAL HF PROPAGATION FORECAST
	            Latitude Band
Date        Low            Middle         High 
18 May      Normal         Normal         Normal        
19 May      Normal         Normal         Normal        
20 May      Normal         Normal-fair    Normal-fair   

COMMENT: Frequencies should be near predicted monthly values 
18 May and enhanced 19 May, particularly in the N.Aus/PNG/Niue 
regions. Minor depressions expected 20 May in response to enhanced 
geomagnetic activity, particularly in the S.Aus/NZ/ Antarctic 
regions. SWFs possible 18 May in the sunlit hemisphere. 

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


Date   T index
17 May    15

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

Predicted Monthly T index for May:   9

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
18 May    14    near predicted monthly values 
19 May    24    about 10% above predicted monthly values 
20 May    10    near predicted monthly values 

COMMENT: HF conditions are expected to be normal 18 May. MUF 
enhancements possible 19 May particularly at equatorial and low 
latitudes. Minor MUF depressions may occur 20 May in response 
to enhanced geomagnetic activity, particularly at mid-high  
latitudes. SWFs possible 18 May in the sunlit hemisphere. 

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

GOES satellite data for 16 May
       Daily Proton Fluence >1 MeV:   5.4E+05
       Daily Proton Fluence >10 MeV:  1.8E+04
       Daily Electron Fluence >2 MeV: 7.80E+06   (normal fluence)   
Electron Fluence Daily Deep Dielectric Discharge Probability: 1%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: A3.0

ACE Satellite Solar Wind Day Averaged Data for 16 May
Speed: 336 km/sec  Density:    1.9 p/cc  Temp:    60100 K  Bz:   0 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