If you are looking for the observed sunspot number derived from optical
observations of the sun, you've been miss-routed.
This link provides a comparison of the effective SSN shown on this page to the observed solar sunspot number.
These plots provide a look at the global behavior of the ionospheric F2 layer over the past week as measured by the NWRA effective sunspot number (SSNe) calculated from current observations. The upper panel shows the SSNe variation, the third panel provides a goodness-of-fit metric (described below), and the lower panel gives the total number of foF2 observations in each SSNe calculation. In all three panels the two black curves use data from observatories between -50 and +50 degrees geomagnetic latitude (heavy curve uses data collected from the previous 24 hours; light curve the previous 6 hours). The heavy green and red curves use data from observatories between -50 and -15, and +15 and +50 degrees geomagnetic latitude, respectively, collected during the previous 24 hours. (Note that the quasi- diurnal variation in the 6 hour SSNe values is primarily due to unequal longitude spacing of the foF2 stations from which the SSNe are being calculated.)
The second panel shows the provisional (quicklook) Kp index from GFZ Potsdam. This is provided to assess the impact of geomagnetic activity on SSNe.
Also shown on the upper panel is the long-term predicted smoothed sunspot number as provided by the NOAA Space Weather Prediction Center. The heavy dash line is the expected value from the prediction, and the two light dashed lines are the upper- and lower-bounds on the expected value.
The goodness-of-fit metric shown in the middle panel is the RMS percent difference between the foF2 observations used in the SSNe calculations and the model foF2 values generated using the SSNe in the URSI-88 foF2 model. It generally runs around 15%, with the largest departures occurring during major geomagnetic disturbancesThe following table summarizes the observations used in calculating the most recent SSNe value. The X entry for a particular station/time indicates there was an foF2 value available and it was used in the SSNe calculation. A - entry indicates that an foF2 value was available, but it was excluded from the SSNe calculation (it was identified as an outlier point). The bar (|) symbol along the time axis of the table indicates the latest-data time (i.e., data to the right of this column are from the previous day). The SH and NH tags on the far right of each line indicates which stations were included in the southern- and northern-hemisphere SSNe calculations, respectively.
Date: 20190120 000000000011111111112222 GMLAT Station Used Rej 012345678901234567890123 ----- ------------------- ---- ---- +-----------------|------+ 49.7 Boulder 24 00 |XXXXXXXXXXXXXXXXXXXXXXXX| NH 49.4 Fairford 20 00 |XXXXX XX XXXXXXXXXXXXX| NH 49.0 Wallops Island 21 00 |XX XXXXXXXXXXXXXXXXXXX | NH 46.8 Dourbes 22 00 |XXXXX XXXXXXXXXXXXXXXXX| NH 46.3 Pruhonice 18 00 |XXXX XXXXXXXXX | XXXXX| NH 42.1 Eglin AFB 20 00 | XXX XXXXXXX XXXXXXXXXX | NH 41.6 Khabasrovsk 01 00 | X | | NH 38.7 Wakkanai 15 00 |XXXXXX X XX X XX | XXX| NH 36.8 Rome 19 00 |XXX XXXXXXXXXX|XXXXXX| NH 34.1 Gibilmanna 09 00 |X XXX X XX | XX| NH 34.1 Beijing 01 03 | |-- - X| NH 33.2 I-Cheon 05 00 | X XX|X X | NH 30.3 Ramey 01 00 | X | | NH 29.4 Jeju 16 00 |XXXXXXXXXX X X XXX X | NH 28.7 Kokubunji 13 00 |XXXXXX XXX X | XXX| NH 24.0 Yamagawa 16 00 |XXXXXXXXXXXX X | XXX| NH 0.9 Jicamarca 16 00 |XXX XX X XX XXX| XXXXX| -22.3 Darwin 21 00 |XXXXXXXXXXXXXXX X|XX XXX| SH -28.9 Townsville 13 01 | XX- XXXXXXXX XX X | SH -32.9 Learmonth 16 00 |X XXXXXXX XXX X XXX X| SH -36.9 Brisbane 16 00 |X XX X XXXXX XXXX| XX X | SH -45.6 Perth 17 00 | XX X XX XXX XXX|XXXXXX| SH -46.0 Canberra 20 00 |XXXXXXXXXX XXXXX |XXXX X| SH ------------------- ----- ---- ---- +-----------------|------+ NH : # Expected / # Received / Percent: 768 / 224 / 29.2 ALL : # Expected / # Received / Percent: 1248 / 344 / 27.6 SH : # Expected / # Received / Percent: 408 / 104 / 25.5
If you would like to get a feel for how effective these effective-SSN indices are, foF2 plots comparing the observations with model foF2 values calculated using the NWRA SSNe and the SWS T indexes are available. There is a one-day delay between the latest SSNe values available and these plots to permit more data to arrive at the NOAA SWPC for comparison.
The foF2 data used in these calculations were obtained from the NOAA SWPC.
[ Space Weather Home Page | Scintillation Home Page ]
[ Home | About NWRA | Staff | Research Areas | Products ]
How to contact NWRA
Copyright © 1996-2017 NorthWest Research Associates, Inc. All rights reserved.