<html><head><meta http-equiv="content-type" content="text/html; charset=utf-8"></head><body dir="auto"><div>Hear hear.<br><br>Sent from my iPhone</div><div><br>On 21 Feb 2016, at 18:19, Scott Evans <<a href="mailto:vk7hse@gmail.com">vk7hse@gmail.com</a>> wrote:<br><br></div><blockquote type="cite"><div><p dir="ltr">Storm in a teacup guys! The impact would be low to negligible and well let's face it, it's a short term project with the sole purpose of APRS! </p>
<p dir="ltr">How many people will track it's progress and get some level of enjoyment and even possibly assisting with getting the balloons data back into the APRSIS 😉</p>
<p dir="ltr">Just my deprecated thoughts and please enjoy the rest of your day! </p>
<br><div class="gmail_quote"><div dir="ltr">On Sun, 21 Feb 2016, 16:27 A Nguyen <<a href="mailto:an@comms.net.au">an@comms.net.au</a>> wrote:<br></div><blockquote class="gmail_quote" style="margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex"><div style="word-wrap:break-word">Hi Ian,<div><br></div><div>WIDE2-1 is a globally acceptable path for balloons, recommended by Bob Bruninga WB4APR, the founder of APRS.<br><div><br></div><div>Int the early days of APRS pico balloon flights over the eastern states, some effort was made to check for impact to the network from a high altitude balloon using WIDE2-1, and no issues were observed with a 5 minute TX interval.</div><div><br></div><div>PS-61 transmits one compressed APRS packet every 5 minutes in full sun, and every 10 minute at night.</div><div><br></div><div>Regards,</div><div>Andy VK3YT</div><div><br></div><div><br></div><div><div><br><div></div></div></div></div></div><div style="word-wrap:break-word"><div><div><div><div><div>On 21 Feb 2016, at 1:40 pm, Ian Bennett <<a href="mailto:ibennett@tpg.com.au" target="_blank">ibennett@tpg.com.au</a>> wrote:</div><br></div></div></div></div></div><div style="word-wrap:break-word"><div><div><div><div><blockquote type="cite">
<div bgcolor="#FFFFFF" text="#000000">
<tt>Reported from <a href="http://aprs.fi" target="_blank">aprs.fi</a>:<br>
<br>
</tt><br>
Last path: <span style="vertical-align:middle">VK3YT-12>APZ269
via WIDE2-1,qAS,<a href="http://aprs.fi/info/VK3VHF-1" target="_blank">VK3VHF-1</a></span>
<span><path-seriously-bad.png></span></div></blockquote></div></div></div></div></div><div style="word-wrap:break-word"><div><div><div><div><blockquote type="cite"><div bgcolor="#FFFFFF" text="#000000"><br>
This station appears to be flying at high altitude and using
digipeaters, which causes serious congestion in the APRS network.
The tracker should be configured to only use digipeaters when at low
altitude.<br>
<br>
<tt>You might want to revisit your path settings ???<br>
<br>
Ian<br>
VK1IAN<br>
<br>
<br>
</tt>
<div>On 21/02/16 10:44, A Nguyen wrote:<br>
</div>
<blockquote type="cite">
Hi all,
<div><br>
<div>FYI,</div>
<div><br>
</div>
<div>PS-61 APRS PICO balloon is heading north from Melbourne</div>
<div><br>
</div>
<div>Solar powered party balloon, 10mW TX</div>
<div>APRS on 145.175Mh, call sign VK3YT-12</div>
<div><a href="http://aprs.fi/#%21mt=roadmap&z=7&call=a/VK3YT-12&timerange=86400&tail=86400" target="_blank">http://aprs.fi/#!mt=roadmap&z=7&call=a%2FVK3YT-12&timerange=86400&tail=86400</a></div>
<div><br>
</div>
<div>Olivia 8/250 on 434.650Mhz (Dial frequency 434.649Mhz,
starting tone at 1kHz) RSID enabled.</div>
<div>Tracked on SNUS as PS-61 </div>
<div><a href="http://tracker.habhub.org/#%21mt=roadmap&mz=6&qm=1_day&f=PS-61" target="_blank">http://tracker.habhub.org/#!mt=roadmap&mz=6&qm=1_day&f=PS-61</a></div>
<div><br>
</div>
<div>Tracking info <a href="http://picospace.net/?p=736" target="_blank">http://picospace.net/?p=736</a></div>
<div><br>
</div>
<div>Currently at 9400m alt east of Melbourne.</div>
<div><br>
</div>
<div>Prediction: <a href="http://picospace.net/wp-content/uploads/2016/02/NewImage3.png" target="_blank">http://picospace.net/wp-content/uploads/2016/02/NewImage3.png</a></div>
<div><br>
</div>
<div>Regards,</div>
<div>Andy VK3YT</div>
</div>
<div><br>
</div>
<br>
<fieldset></fieldset>
<br>
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