... HamCap is an interactive application. When you move the mouse cursor over the chart, the time and all other parameters of the point under the cursor areMessage 1 of 17 , Apr 9, 2005View Source
> While we're on the subject, a question I have wondered about -- why do HamHamCap is an interactive application. When you move the mouse cursor over
> Cap's charts not have a graduated hour scale on the X axis? Have I missed
> an option to turn them on?
the chart, the time and all other parameters of the point under the cursor
are displayed on the status bar.
I tried to make the HamCap window as small as possible so that it could be
used during contesting and DXing when screen space is a valuable resource,
so I removed all unnecessary elements form the user interface, including the
time scale on the chart.
73 Alex VE3NEA
A while ago I did some comparisons of median SNR predictions from VOACAP to the observations of NCSXF beacons. Ingemar SM5AJV developed a program that measuresMessage 1 of 17 , Apr 9, 2005View SourceA while ago I did some comparisons of median SNR predictions from VOACAP to
the observations of NCSXF beacons. Ingemar SM5AJV developed a program that
measures the SNR of beacon signals using a sound card and an FFT
transformation. A correlator is used to compare the received waveform to
that of the beacon's callsign, to make sure that the signal actually comes
from the beacon. Ingemar was kind enough to send me his logs for June 2004,
these logs cover about 24% of the month.
I developed a viewer utility for the logs that converts the observed SNR
into dB-Hz, calculates medians, and plots both predicted and observed median
values along with the observation points for the selected beacon and band.
The program lacks a sophisticated user interface, which I may develop in the
future if there is sufficient interest. A few screenshots of typical plots
are here: http://www.dxatlas.com/Private/SnrPlot.zip .
For those who want to play with the viewer, I uploaded it to
The zip file also includes the observation data, with permission
from Ingemar. Please preserve the directory structure when unzipping.
Though this is just the first alpha version of the program and thus it may
contain errors, the plots it produces are very interesting. The shape of the
VOACAP prediction chart is very close to that of the observation chart,
though the absolute values are way off. On average, VOACAP underestimates
the SNR by 20+ dB.
Also, these charts explain why the median SNR is a bad indicator of
propagation conditions. The median value makes sense only for unimodal
distributions, while the distribution of SNR is bi-modal at best (that is,
has two or more peaks). One peak is formed by the observations that where
performed when the path was open with a good propagation mode, and one or
more peaks come from the days when only very lossy modes were available or
the path was closed.
73 Alex VE3NEA
OK - thanks! Makes sense. 73, PeteMessage 1 of 17 , Apr 9, 2005View SourceOK - thanks! Makes sense.
At 12:56 PM 4/9/2005, Alex, VE3NEA wrote:
> > While we're on the subject, a question I have wondered about -- why do Ham
> > Cap's charts not have a graduated hour scale on the X axis? Have I missed
> > an option to turn them on?
>HamCap is an interactive application. When you move the mouse cursor over
>the chart, the time and all other parameters of the point under the cursor
>are displayed on the status bar.
>I tried to make the HamCap window as small as possible so that it could be
>used during contesting and DXing when screen space is a valuable resource,
>so I removed all unnecessary elements form the user interface, including the
>time scale on the chart.
>73 Alex VE3NEA
>Yahoo! Groups Links
[With apologies to readers of the VOACAP list, who are joining this in mid-thread, I feel that Bill and I are floundering fairly far out of our depth in thisMessage 1 of 17 , Apr 9, 2005View Source[With apologies to readers of the VOACAP list, who are joining this in
mid-thread, I feel that Bill and I are floundering fairly far out of our
depth in this discussion that began on the dxatlas list. The question
began as what SSN to use in Ham Cap, a simplified front end for
VOACAP. HamCAP comes with a table of predicted international SSNs, but can
also link with IonoProbe, which downloads daily SSNs from the SEC. VE3NEA,
the author of Ham Cap, prefers the SEC numbers, but the variance from the
international SSns is considerable, with the SEC number typically running
much higher. Any advice appreciated!]
Bill, there's some apples and oranges, or something going on
here. IonoProbe gets its numbers from the Joint USAF/NOAA Solar and
Geophysical Activity Summary. Here's a sample:
"SGAS Number 099 Issued at 0245Z on 09 Apr 2005
This report is compiled from data received at SWO on 08 Apr
A. Energetic Events
Begin Max End Rgn Loc Xray Op 245MHz 10cm Sweep
B. Proton Events: None
C. Geomagnetic Activity Summary: The geomagnetic field was quiet.
D. Stratwarm: Not Available
E. Daily Indices: (real-time preliminary/estimated values)
10 cm 088 SSN 056 Afr/Ap 005/004 ...."
Ionoprobe's retrospective record of these reports shows March 12 (chosen
randomly) with a SSN of 67, versus 42 on the table you cite. March 18 is
37 versus 25, and so on.
I have no idea what the explanation is, though I do note that there is
another table, ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SUNSPOT_NUMBERS/2005
, which gives the numbers just for this year to date and states that
"Values are preliminary after Dec 2004."
There is an interesting explanation of how various sunspot numbers are
seems clear from this explanation that the international sunspot number is
a highly-massaged, worldwide average number that does not become final for
some months after the date of observation. By contrast, the number cited
in the SGAS is the SEC's every-six-hour figure, and must be based strictly
on its own observations. An interesting graph at
http://www.nwra-az.com/spawx/comp.html speaks to this. To quote from the
" This plot illustrates the differences between the "real" sunspot number
(SSN), which is calculated from optical observations of the sun, a sunspot
number derived from the 10.7cm solar radio flux (SSNf), and a sunspot
number derived from fitting an ionospheric model to ionospheric
measurements. All of these indices are used as inputs to models of the
ionosphere for use in communications-performance predictions - this plot
shows that they don't always agree as to what the SSN should be in that
Note: The F10.7-derived SSN (SSNf) is calculated from the 10.7cm solar
radio flux (the Penticton Radio Observatory noon value) using the following
F10.7 = 63.74 + 0.727*SSNf + 0.000895*SSNf**2
So, where does this leave us? Where it left me, frankly, is wondering why
we use sunspot numbers at all, rather than solar flux and A/K indices, or
at least the SSNf, which would be closer to the values Bill cited than to
the current high value of optically-observed SSN. On the other hand, Alex
argues that results from using the lower SSNs seem to run consistently low
in terms of predicted vs. observed S/R ratio.
It would be interesting to pass this discussion over to the VOACAP list and
see what the gurus there, particularly including Greg Hand and George Lane,
think of it. In fact, I have done that, and it will be interesting to see
what comes of it.
73, Pete N4ZR
At 09:12 AM 4/9/2005, bill_w4zv wrote:
> > Maybe the logic of
> > the calculation has an error somewhere in its data collection.
>Definitely so. The current 90 day average (1 Jan 05 - 31 Mar 05) is
>28.4 using this data:
>I don't have IonoProbe, but it must have a problem if the 47 number
>Pete quoted for the IonoProbe calculation is correct. Anyhow, now I
>know what to use and will probably just go with the NOAA forecast
>which seems to be fairly accurate at this stage of the cycle.
>Yahoo! Groups Links
... wondering why ... I agree. Seems like measured solar flux, which supposedly shows the actual effect of sunspots on the ionosphere, would be better. AfterMessage 1 of 17 , Apr 10, 2005View Source--- In firstname.lastname@example.org, Pete Smith <n4zr@c...> wrote:
> So, where does this leave us? Where it left me, frankly, is
> we use sunspot numbers at all, rather than solar flux and A/K indices,I agree. Seems like measured solar flux, which supposedly shows the
actual effect of sunspots on the ionosphere, would be better. After
all, when there is a large CME, we often can see little effect on the
ionosphere depending on how it's directed toward Earth, which way Bz
points, etc. Of course if VOACAP was originally based on SSN's, then
maybe they should be the input. Hopefully Greg Hand will respond, and
please post anything of interest here since I am not on that list. No
model is any better than its input..."Garbage In Garbage Out" as
I wrote: The current 90 day average (1 Jan 05 - 31 Mar 05) is 28.4 using this data: ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SUNSPOT_NUMBERS/RIDAILY.PLT VE3NEAMessage 1 of 17 , Apr 10, 2005View SourceI wrote: The current 90 day average (1 Jan 05 - 31 Mar 05) is
28.4 using this data:
VE3NEA wrote: These are the RI indices, not daily SSN values.
Alex, the NOAA site below calls these "Provisional International
Sunspot Numbers, so what do you mean they are not daily SSN numbers?
See especially their comments preceded by ***** below:
>The provisional daily Zurich relative sunspot numbers, Rz, were basedupon
observations made at Zurich and its two branch stations in Arosa and
and communicated by M. Waldmeier of the Swiss Federal Observatory.
January 1, 1981, the Zurich relative sunspot number program is
the "Sunspot Index Data Center" (c/o Dr. P. Cugnon, 3 av. Circulaire,
***** The determination of the provisional International Sunspot
Numbers Ri results from a statistical treatment of the data
originating from more than twenty-five observing stations. These
stations constitute an international network, with the Locarno
(Switzerland) station as the reference station, to guarantee
continuity with the past Zurich series of Rz.*****
>The definitive International Sunspot Numbers Ri are evaluated by asimilar method based on a network of observing stations selected for
high number of observations, their continuity during the whole year
existing series of observations during the last years. Also taken into
account is the stability of the K monthly factors with reference to the
*****These relative sunspot numbers are now designated Ri
(International) instead of Rz (Zurich).*****
It seems to me Ri is exactly what should be used, but am really
waiting to see what Greg Hand, etc. of VOACAP have to say.