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Saturday, April 25, 2009
On to the Canary Islands
As I've been doing, I decided to see who was at the other end of that line. It was Luis, EA8AY (pictured above). Luis's station picked up my 18 milliwatt signal at 2106 UTC on April 24. The distance was 1871 miles (3011 kilometers). I was 23 db below the noise.
Luis has a very nice web page: http://www.ea8ay.com/index.html (Warning: This site will likely cause feelings of extreme jealousy: Luis is living in a fantastic location, with a beautiful family AND he is the owner of an Argonaut 509!)
On his site, Luis has a nice video that will give you a sense of what WSPR is like:
wspr with 100 mw from luis on Vimeo.
Friday, April 24, 2009
Crossing a small bit of the pond...
(The images above and below are of Jan's locations in the Faroe islands (from his site).
Thursday, April 23, 2009
WSPRing along at 27 db below the noise....
http://wsprnet.org/drupal/wsprnet/spots
Be sure to click on the map display also.
I was intrigued by the Signal to Noise ratio column, and wondered what the reference bandwidth for the noise was. K1JT's pages show the reference bandwidth is 2500 Hz, and that WSPR can decode signals that are as much as 27 db below that noise.
That's great. I guess I don't have to worry about the lower sideband of my 30 mw signal causing anyone any trouble. It will be very far down in the noise.
Wednesday, April 22, 2009
Are Diode Ring Mixers Fundamentally Different?
Here is my latest e-mail to Joop. The RSGB diagram for the ring diode mixer appears above.
Joop: I think the way the diode ring mixer works is very different from the way a two diode singly balanced mixer functions. The effect, of course, is the same. But the polarity reversing element introduced by the ring configuration -- it seems to me -- makes this a very different circuit.
Attached is the RSGB Handbook diagram I mentioned. I like it, because you can really SEE how the actions of the diode ring produce the sum and difference freqs (you have to keep Fourier in mind, and imagine the results of filtering).
The two diode circuit simply "chops" the input signal at the rate of the LO. And it would even work in a non-switching mode -- you could, for example, use FETs instead of the diodes and bias them to operate in the non-linear portion of their curves, right? This makes me think that the diode ring mixer circuits (aka "polarity switching mixers" or "commutating mixers") are very different.
73 Bill
Tuesday, April 21, 2009
Balloon! Project Blue Horizon Reaches Mid-Atlantic
Balloon Launch - Assist in Tracking
The NS3 group of Cornell University engineering graduate students will launch PBH-9 (Project Blue Horizon) from Lockheed Martin in Owego NY on Sunday evening, 19 Apr 09, at approximately 21:00 EDT (Monday, 20 Apr 09, 01:00UT)
This ARHAB flight (Amateur Radio High Altitude Ballooning) will ascend and then float for up to 50-hours while drifting to the east.
The payload will include a KC2TUA-8 144.390 APRS beacon
(track via (http://findu.com/cgi-bin/find.cgi?call=KC2TUA-8)
and HF CW position report and telemetry downlinks on 7.104MHz and 10.148MHz.
The NS3 PBH-9 team requests distant ground stations receive and report HF telemetry via N2XE@arrl.net including reception UT date and time.
Distant receiving stations are welcome to also submit HF
reception reports to W0RPK@amsat.org for the ARHAB <50mhz href="http://showcase.netins.net/web/wallio/ARHABrecords.htm" target="_blank">http://showcase.netins.net/web/wallio/ARHABrecords.htm.
Additional PBH-9 information including HF telemetry transmit schedule and format is available via
http://showcase.netins.net/web/wallio/ARHABlaunchannouncements.htm.
Flight updates are available from the NS3 PBH-9 team
via http://twitter.com/pbh3.
Sunday, April 19, 2009
WSPR Double Sideband Success!
Following guidance from Gene, W3PM (whose FB SSB rig inspired this effort), I set my oscillator at 10138700. That puts the upper sideband in the middle of the WSPR band.
Here's my first set of reports:
Reported | Distance | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
Date | Call | SNR | by | km | mi | ||||||
2009-04-19 18:32 | N2CQR | -18 | DL0TUH | 1353 | 841 | ||||||
2009-04-19 18:32 | N2CQR | -24 | PA1GSJ | 1343 | 835 | ||||||
2009-04-19 18:30 | N2CQR | -19 | DL0TUH | 1353 | 841 | ||||||
2009-04-19 18:26 | N2CQR | -22 | DL0ODX | 977 | 607 | ||||||
2009-04-19 18:26 | N2CQR | -30 | G8BKE | 1519 | 944 | ||||||
2009-04-19 18:26 | N2CQR | -26 | PA1GSJ | 1343 | 835 | ||||||
2009-04-19 18:24 | N2CQR | -23 | PA1GSJ | 1343 | 835 | ||||||
2009-04-19 14:24 | N2CQR | -22 | M0WQR | 1601 | 995 |
Hey, is this a first? Has anyone else run WSPR DSB?
Saturday, April 18, 2009
Sicily, Mt. Etna... and The Godfather
It was COLD up there. We didn't stay long. Within 90 minutes of this picture being taken, the kids were back at sea level, and in the pool at 80F.
Here is a GoogleEarth View. The yellow marker shows the place at which we took the picture of us in the snow. (The Google shots were from May/June 2006).
Those of you who are fans of The Godfather movie will remember this scene:
Well, here we are, in the same place (but without the shotguns):
Francis Ford Coppola filmed most of the Sicilian scenes not in Western Sicily (where the village of Corleone really is) but in the East, near the beach resort of Taormina, in the village of Savoca. The Bar Vitelli is where Michael Corleone met Apollonia's father. Savoca also has the church where Michael and Apollonia began their brief and unfortunately explosive marriage.
We really liked Sicily. It is a beautiful place, rich in history, and with really nice people.