[Ips-dsgr] IPS Daily Report - 17 April 15 issued 2341 UT on 17 Apr 2015

rwc rwc at ips.gov.au
Sat Apr 18 09:41:58 EST 2015


SUBJ: IPS DAILY SOLAR AND GEOPHYSICAL REPORT
ISSUED AT 2330UT/17 APRIL 2015 BY IPS RADIO AND SPACE SERVICES
FROM THE AUSTRALIAN SPACE FORECAST CENTRE
SUMMARY FOR 17 APRIL AND FORECAST FOR 18 APRIL - 20 APRIL
STATUS INDICATORS SOL:GREEN   MAG:GREEN     ION: GREEN
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1A. SOLAR SUMMARY
Activity 17 Apr:  Low

Flares: none.

Observed 10.7 cm flux/Equivalent Sunspot Number for 17 Apr: 150/105


1B. SOLAR FORECAST
             18 Apr             19 Apr             20 Apr
Activity     Low                Low                Low
Fadeouts     None expected      None expected      None expected
10.7cm/SSN   155/109            155/109            155/109

COMMENT: There were a number of C-class flares during 17 April 
from regions 2324 and 2325 located in the NE quadrant. Solar 
activity is expected to be predominantly low with the chance 
of moderate activity. No Earth directed CMEs were observed during 
17 April. Solar wind speeds have declined slowly during 17 April 
as a coronal hole wind stream gradually subsides and are presently 
around 600 km/s. Solar wind conditions are expected to continue 
to decline slowly over the next two days.

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2A. MAGNETIC SUMMARY

Geomagnetic field for Australian Region 17 Apr: Quiet to Active

Estimated Indices 17 Apr : A   K           
   Australian Region      12   43332222
      Cocos Island         8   33222221
      Darwin               9   33322122
      Townsville          11   43322222
      Learmonth           11   33333221
      Alice Springs       11   43322221
      Norfolk Island      10   33332121
      Culgoora            12   43332222
      Gingin              11   42323222
      Camden              12   43332222
      Canberra            11   33332222
      Launceston          19   44443232
      Hobart              14   43432222    

Estimated Antarctic Regional K Indices 17 Apr :
      Macquarie Island    27   44555321
      Casey               16   44333232
      Mawson              46   57544353
      Davis                7   2-------

Observed Regional daily pc3 Indices 17 Apr : 
      Darwin               0   (Quiet)
      Townsville           0   (Quiet)
      Learmonth            4   (Quiet)
      Alice Springs        2   (Quiet)
      Gingin              61   (Active)
      Canberra            65   (Active)
      Melbourne          148   (Severe storm)

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 International Center for Space Weather 
Science and Education, Japan.


Estimated AFr/Ap Indices 17 Apr : A 
           Fredericksburg        25
           Planetary             28                         

Observed AFr/Ap Indices 16 Apr :  A   K
           Fredericksburg        28
           Planetary             38   5544 4455     


2B. MAGNETIC FORECAST 
Date      Ap    Conditions
18 Apr    10    Quiet to Unsettled
19 Apr     8    Quiet to Unsettled
20 Apr    15    Unsettled to Active

COMMENT: Unsettled to active levels were observed during 17 April 
over the Australian region with storm periods at high latitudes 
under the influence of a coronal hole wind stream. Storm levels 
were observed at high latitudes. Mostly quiet to unsettled levels 
are expected for 18 April with isolated active levels possible 
as the coronal hole effects subside.

-----------------------------------------------------------
3A. GLOBAL HF PROPAGATION SUMMARY
	            Latitude Band
Date        Low            Middle         High 
17 Apr      Normal         Normal         Normal         

PCA Event : No event.

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

COMMENT: Mostly normal conditions are expected for the next few 
days with the small chance of SWFs. Slightly degraded conditions 
may be observed at high latitude regions.

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


Date   T index
17 Apr    97

Observed Australian Regional MUFs
   Cocos Island Region:
      Enhanced by 30% during local day.
      Depressed by 20% during local night.
   Niue Island Region:
      Mostly near predicted monthly values.
   Northern Australian Region:
      Mostly near predicted monthly values.
      Enhanced by 20% after local dawn.
   Southern Australian and New Zealand Region:
      Near predicted monthly values.
   Antarctic Region (Casey/Scott Base/Davis/Mawson):
      Depressed by 15% over the UT day.

Monthly T index:
Month  T index
Mar      99
Apr      90
May      89

4B. AUSTRALIAN REGION IONOSPHERIC FORECAST
Date   T index  MUFs
18 Apr   110    Near predicted monthly values
19 Apr   110    Near predicted monthly values
20 Apr   110    Near predicted monthly values

COMMENT: Mostly normal conditions are expected for the next few 
days with the small chance of SWFs.

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

GOES satellite data for 16 Apr
       Daily Proton Fluence >1 MeV:   1.3E+06
       Daily Proton Fluence >10 MeV:  1.0E+04
       Daily Electron Fluence >2 MeV: 2.70E+07   (normal fluence)
Electron Fluence Daily Deep Dielectric Discharge Probability: 4%
Fluence (flux accumulation over 24hrs)/ cm2-ster-day.
       X-ray background: B7.5

ACE Satellite Solar Wind Day Averaged Data for 16 Apr
Speed: 605 km/sec  Density:    3.8 p/cc  Temp:   298000 K  Bz:  -3 nT

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