ARNewsline Young Ham of the Year – Erin King AK4JG

Erin King, AK4JG, a 17-year-old from Columbus, Georgia, who re-founded her high school’s radio club and then lofted a ham radio-carrying balloon to over 90,000 feet, recovered the flight data and used it to produce a truly striking video of that flight, has been named as recipient of the 2012 Amateur Radio Newsline Young Ham of the Year Award.

Watch MIT’16 EA Tube goes to Near Space!

Ever wondered how to execute a high altitude balloon mission? Erin King, AK4JG, talks about the process, planning and options in a presentation at Dayton in 2012.

Watch Launching Radios and Other Cool Stuff into the Stratosphere AK4JG.wmv

Erin is the daughter of Paul, K4ETY, and Patricia King.  She has two siblings:  Brandon, age 16 and Rachel, age 15.  Erin became a licensed radio amateur in 2009 and now holds an Extra Class license.  She is a member of the ARRL, the Columbus Amateur Radio Club, and the Russell County Radio Club.  She enjoys operating on local VHF and UHF repeaters as well as phone and digital modes on the High Frequency amateur radio bands. She is looking forward to mastering Morse Code as her next amateur radio challenge.

Erin King AK4JG

Erin King AK4JG

Erin became interested in amateur radio after joining a club at her high school dealing with robotics and then ham radio-equipped high-altitude balloon launches.  This school group has participated in FIRST Robotics competitions, and Erin has twice been Team Lead for Programming. The club also launches several high-altitude balloon missions each year, in a program called DREAMS.  They have flown various scientific experiments as part of these missions, in addition to planning, building, and integrating radios, Global Positioning System (GPS) units and TNCs to track and recover the balloons.  To facilitate these activities, the group’s sponsor, Luther Richardson, KI4AOJ, has encouraged the students to obtain their amateur radio licenses.

A subset of this group,including Erin, has participated in the Massachusetts Institute of Technology’s (MIT’s) “InvenTeam” competition, designing and building a portable lightning detector and early warning system. In addition, Erin re-started the Columbus High School Radio Club and served as its president for the past two years.  The club was active in the 1950s and ’60s, and Erin’s great-grandfather (the original K4ETY) was one of its mentors at that time. The new club obtained the callsign W4CHS (Columbus High School) and has been active on the air.

Erin King AK4JG working 6m for Field Day 2011 - Image Credit Columbus Amateur Radio Club W4CVY

Erin King AK4JG working 6m for Field Day 2011 – Image Credit Columbus Amateur Radio Club W4CVY

Erin’s involvement with amateur radio and FIRST Robotics has helped fuel her interest in science and engineering. Last year, she applied for early admission to both Georgia Tech and MIT; she was accepted to both and will be attending MIT this fall.

Inside the shiny tube which contained Erin’s MIT acceptance letter was a note suggesting that the students “hack” their tubes, meaning to do something cool with them, in along-standing tradition of MIT hacks or stunts. Erin chose to send her tube to near-space.

Drawing on her ballooning experience,Erin planned, built, integrated, and tested a complete new tracking setup to fit into the very small shipping tube.  The payload consisted of two GPS units, two custom-made antennas, one Argent Data OpenTracker+ kit (which Erin built), one handheld radio, and a fellow ham’s Byonics Pocket Tracker, a self-contained 100-milliwatt tracker/radio combination in an Altoids® tin.  Erin also talked her mother into letting her use mom’s brand new GoPro Hero HD video camera.

With the assistance of a group of hams from the Columbus Amateur Radio club, Erin launched her balloon from Lumpkin, GA.  A couple of hours later, she and the tracking team successfully recovered it, along with the complete HD video record of the flight. Erin took this video, as well as other photos and videos taken of the launch activities, and compiled it into an 8-minute presentation,complete with background music.  She posted it to YouTube, and put a link to it on the MIT hack-the-tube site (see<http://tinyurl.com/ak4jg-space-video>). According to YouTube statistics, Erin’s video has been viewed thus far in excess of 82,500times.

This past May, Erin was invited to participate in no less than three forums and sessions at the 2012Dayton Hamvention®.  These included the 25thanniversary “Youth Forum,” the “Ham Radio Town Meeting” and an “ARRL Expo”presentation where her video was screened.

Award Ceremony

The 2012 Amateur Radio Newsline™ “Young Ham ofthe Year Award” will be presented on Saturday, August 18th at the Huntsville Hamfest in Huntsville, Alabama.  As the 2012″Young Ham of the Year,” Erin will receive –courtesy of Yaesu USA — an expense-paid trip to the Huntsville Hamfest, along with a gift of Yaesu brand ham radio equipment.  CQ magazine will treat her to an expense-paid week at Spacecamp Huntsville,and will present Erin with a variety of CQ products.  Amateur Radio Newsline™ will provide Erin with a commemorative plaque at the award ceremony.  Once again, the cost of year’s plaque has been underwritten by Dave Bell (W6AQ), President of DBA Entertainment Inc., Hollywood, California.  Heil Sound Ltd. will also be presenting Erin with a ham radio-related gift.

The presentation of the Young Ham of the Year Award has been a regular feature of the Huntsville Hamfest since 1993.  This has been made possible through the generosity and kindness of the event’s Planning Committee and the good offices of Huntsville Hamfest Association Vice President Charlie Emerson, N4OKL. (See http://www.hamfest.org)

This year’s award ceremony will be hosted by Bill Pasternak, WA6ITF, and Don Wilbanks, AE5DW, of Amateur Radio Newsline™, Rich Moseson, W2VU, of CQ Communications, and representatives of Yaesu USA and Heil Sound.

Award Program Background

The Amateur Radio Newsline™ “Young Ham of the Year” award (formerly the Westlink Report Young Ham of the Year Award) has been presented annually since 1986 to a licensed radio amateur (ham) who is 18years of age or younger and who has provided outstanding service to the nation,his/her community or the betterment of the state of the art in communications through the amateur radio hobby/service. A website with full information on the award program and background material is located at http://www.arnewsline.org/YHOTY.

Award Sponsors

The award program is sponsored by the Los Angeles, California-based Amateur Radio Newsline™ with corporate support from Yaesu USA Corporation of Cypress, California, CQ Magazine of Hicksville, New York, and Heil Sound of Fairview Heights, Illinois.

Since 1976, Amateur Radio Newsline™ and its predecessor, the Westlink Radio Network, have been providing radio amateurs around the world with up-to-the-minute news at no cost to them. (See http://www.arnewsline.org)

The award’s three major corporate underwriters are world leaders in their respective areas of Amateur Radio product support.

Yaesu USA, which has been a corporate underwriter since the inception of the award program in 1986, is considered the trailblazer in the design, manufacture and distribution of high quality amateur gear as well as commercial two-way,  monitoring, marine and air-band communications equipment (See http://www.yaesu.com).

CQ magazine and its sister publications, CQ VHF,Popular Communications and World Radio Online, are publishedby CQ Communications, Inc., and are considered the trend-setting publications serving today’s modern radio amateur.  (See http://www.cq-amateur-radio.com)

Heil Sound Ltd. Is considered as a world leader in the development and manufacture of new technology microphones and related audio products for professional sound reinforcement and amateur radio communications.  (See http://www.heilsound.com)

Watch Venus Transit Online June 5-6

At 22:09 UT on June 5, 2012 the planet Venus will appear as a small, dark disk moving across the face of the Sun. The transit will finish at 04:49 UTC on June 6 (exact time depends on location of observer).

Clouds permiting, it may be visible to observers in the UK from dawn (about 03:46 UT in London).

This will be the last time the planet Venus will make the trek across the face of the sun as seen from Earth until the year 2117.

Note: Observing the Sun directly without appropriate protection can damage or destroy retinal cells, causing temporary or permanent blindness.

Clint Bradford K6LCS has posted a collection of URL’s where you should be able to watch the Venus transit online from sites around the world.

NASA (USA) http://venustransit.nasa.gov/2012/transit/

NASA Edge http://www.nasa.gov/multimedia/podcasting/nasaedge/index.html

University of Barcelona  (from a telescope in Norway) https://gaia.am.ub.es/serviastro/www/html/venus2012/live/index.html

National Solar Observatory http://venustransit.nso.edu/live.html

Exploratorium  (via the Mauna Loa Observatory) http://www.exploratorium.edu/venus/

NASA TV http://www.nasa.gov/ntv

Coca Cola Space Science Center (from Australia) http://www.ccssc.org/transit2012.html

Bareket observatory (Israel)
http://www.bareket-astro.com/live-astronomical-web-cast/live-free-venus-transit-webcast-6-june-2012.html

Mt. Lemmon Sky Center http://skycenter.arizona.edu/annoucement/live

Astronomers Without Borders (from Mt. Wilson, California)
http://www.astronomerswithoutborders.org/projects/transit-of-venus/live-webcast.html

The 2012 Transit of Venus using HAM Radio http://aprs.org/VenusTransit2012.html

Transit of Venus Special Event June 6, 2012
http://www.southgatearc.org/news/may2012/transit_of_venus_special_event.htm

Ultra-high Definition video recording of 2012 Venus Transit
http://www.nasa.gov/multimedia/videogallery/index.html?media_id=145648241

AMSAT-LU Balloon Launch May 19

LU7AA brings news that on Saturday May 19 from 11hs-LU on (GMT-3), a free Balloon UV Repeater will fly from the city of General Pico (Airport), Province of La Pampa, Argentina, 571 Km west of Buenos Aires City. See details and photos http://www.amsat.org.ar/globo19.htm

Given administrations requests by Amsat Argentina, launch is authorized and appropiate NOTAM (NOTification to AirMen) had been issued and granted by National Civil Aviation Administration.

Contest & Prices: first 10 station making the most distance & contacts will receive special certificate, top winner will receive a UHF/VHF handy.

Payload will operate as an UHF to VHF crossband repeater, with CW tlm, APRS location and SSTV emissions in local and space frequencies.

According estimates Balloon could reach 100,000 feet height, traveling from 50 to 100 miles towards east.

Thus allowing contacts between stations located in provinces of Buenos Aires, Santa Fe, Entre Rios, Cordoba, Catamarca, Santiago del Estero, La Pampa, San Luis, Mendoza, San Juan, Rio Negro, Neuquen, Uruguay & Chile. (Launch is from Argentina Geo-Center to permit higher participation). See coverage map on
http://www.amsat.org.ar/picocubr.jpg and estimated trajectory in
http://www.amsat.org.ar/pico120519.jpg .

For these experiences, Amsat-LU works with and it is thankful to hams of Radio Clubs of Gral.Pico, QRM Belgrano, APRS Group and amsat-LU members development team as well as those who have actively participated and sent their reports in previous events.

More information at
http://www.amsat.org.ar/lu4aao/experimento_globo_y_parapente.htm.

Several flown experiments have been successfully operated during 2011/12 in manned-gliders, airplanes, captive and free Balloons allowing operational & practice for hams contributing to platform validaton of LUSEX satellite (LU Satellite EXperiment) on development by Amsat Argentina. More on http://lusex.org.ar

In order to monitor the payload (if you are within 400 miles of launch area) you need just an FM receiver either handy or base, in 145.950 for repeater and/or 144.930 for APRS. The repeater, that is activated via 123 Hertz subtone, operates receiving voice FM in 435.950 kHz (-112dbm, 0,56 uV) and emits with 2W the received audio live on 145.950 kHz.

Simultaneously APRS data will be sent in Packet at 1200 bauds in 144.930, and also in 145.950.

The DTI APRS symbol would change from a Balloon (/O) during the ascent to a glider (/g) during parachute descent.

Payload would operate as voice repeater activated by 123 Hz subtone during 1 minute, a warning bip at 40 seconds will indicate telemetry is coming, which is emitted if the repeater is not in use, if in 20 seconds more voice repeater still in use a two bips will be heard signaling that short APRS packages will begin in the different frequencies, also every 5 minutes CW (telegraphy with tones of audio) with CQ + callsign (LU7AA), sequence#, ext. and int. centigrade temperatures and voltage of batteries, after which the cycle will repeat.

Experiment will also emit SSTV pictures in ROBOT-36 (36 seconds) in real time, showing what glider/Balloon sees. Every 5 minutes during ascent/descent and more spaced at high altitudes. (It can be received among others with MIXW, MMSTV & RX-SSTV ).

To study propagation and allow DX station to listen, balloon will also carry a 150 mW CW 7021 Khz transmitter, emiting callsign, sequence, external and internal temperatures and battery voltage.

Payload would also carry on board two TV cameras (one towards earth and another towards horizon) recording video and sound during the flight. These captured videos could be recovered when payload is recovered.

APRS trajectory could be seen every minute, including speed, height, external and internal temperatures and 7.2v battery voltage using UI-View (download from the UI-View official site on http://www.ui-view.org/) and/or to see/follow from Internet connecting to http://aprs.fi/?call=lu7aa-11 or locally via Packet at specified frequencies.

There are georeferenced Maps for UI-View in
http://www.amsat.org.ar/pico.jpg, http://www.amsat.org.ar/pico.txt.
Download and place them in directory Program Files/Peak Systems/UI-View32/MAPS and rename .txt file to .inf.

The experiment in 435.950 KHz besides voice, receives and accepts DTMF sequences commands on demand, I.E. sending B* (DTMF with handy keyboard on UHF) will return S5 … ….. in 145,950 VHF CW, reporting in CW signal strength received from your station, if S9+10 will returns P10.

There are also DTMF commands qualifying emission of CW tlm or APRS beacon or SSTV emission, commands that allows remote release of payload, mode changes, timers control, energy, power, etc.

Frequencies for previous coordination, announcements and flights will be 7090 Khz LSB +/-10 Khz and local repeaters.

During the flights will remain active wide coverage AMSAT-LU APRS Igate LU7AA-10 on 144.930 and 430.930 KHz, operating from the Constituyentes Investigation Center transferring whatever is received towards Internet.

For being an experiment oriented to a next satellite, the contacts made between stations via this payload will be considered valid for the recently announced permanent, gratuitous and applicable Satellite Certificate that AMSAT-LU and RClub QRM Belgrano grants, more info on http://www.amsat.org.ar/certsat.html.

During the Balloon flight, amateur groups will chase the payload, aiming to locate and recover. Trapping ventures holds on this activity, as in the case of the Pampero 15 Balloon sent from San Miguel del Monte which landed in the middle of the Magdalena’s state prison … See http://www.lu5egy.com/Proyecto_pampero/vuelo_15/n_1esk.htm

All reports welcome. If you wish or can organize or want be part of control, or like to pursuit and recovery, or like operating and capturing data as an independent station, and/or wishes to join us personally in this adventure from the launching places email us to parapente at amsat.org.ar.

We appreciate reading of this information and thankful if distribution possible.

73, LU7AA, Amsat-LU, aiming at the future by making the present funny.
Web: http://www.amsat.org.ar/
Email: info at amsat.org.ar

Amateur Radio Party Balloon Success!

One of the 5 party balloons

Bob Bruninga WB4APR reports on the 2nd Party Balloon mission, carrying APRS and a 2.4 GHz wireless camera, that took place Friday, April 27.

Everything possible went wrong! A disaster of monstrous proportions.  But finally got it all working and just wanted it gone!  We released it about 1545 which means we missed getting off the academy before the afternoon’s formal parade and lost 30 minutes going out gate 1 and 3/4 of the way around the yard through Annapolis traffic.  But everything worked perfectly after release.  The balloon was just about making land over Kent Island 8 miles away before we even got onto Rt 50.

With Friday afternoon beach traffic we were chasing the whole time.  Thomasson was bragging about his altitude prediction when it reached his 6500′ altitude as we crossed the Bay bridge.  We were still 16 miles behind it at Easton with
Fick making time in all the traffic as the driver.   Several minutes later Thomasson ate crow as it passed through 8000′ and was speeding up to 45 MPH.

Headed south on 50 towards Easton we were still 16 miles behind it as it overflew Easton.  Then we noticed the altitude descending.  It was down to 6500 feet…

Since we were beyond the Choptank (last water body) and descending slowly we decided not to send the cut-loose command and ride it down.  When we got in about 4 miles range we began to see the wireless camera again and could see chicken coops below.  At 2000′ we turned on a farm road and told the other car to go to the next road and turn.  It passed over us and we got a solid visual.

Radioed to Mids in other car and they got a visual.  Ballester and Garcia got to within 100 yards at touchtown.

We did send the cut command at about 1000 feet just to see if it worked, and it was acknowledged but the payload remained attached.  It landed in a field and the bright red balloons flopping about 10 feet high in the breeze made it a walk in the park to get to.  The release had worked, but the parachute had gotten entangled in the one balloon that had burst and so they came down together.

Clearly one of the 5 balloons had burst at 8000′ and started the descent. With the balloon chards hanging down where the parachute was also hanging down, it is clear that entanglement was certain (bad planning).  Next time, we will
widely separate the balloons from the payload and chute to avoid this.

But all systems worked well and gave great proof of concept for the next one.  The payload was about 320 grams (0.6 lb)consisting of two Lithium 9v batteries a complete APRS digipeater and command/control/telemetry plus a 2.4 GHz wireless camera.  Mission duration was under 2 hours, distance about 50 miles just slightly within the attention span of a student 😉

You can see the track on the web page http://aprs.fi and enter the callsign W3ADO-11 and then ask for the appropriate number of hours of history.  The balloon landed at 2123z or 1723 EDT after a 98 minute flight.

Our joy and enthusiasm were destroyed, however, after a parking lot formed on the bay bridge returning.  All lanes were blocked for several hours.. doubling the time of the entire mission.  Yuk!

LESSONS LEARNED:

Having now flown two party-balloon missions, I am happy with the results compared to Latex balloons.  The missions are very different profiles, but they meet our educational goals quite well.  Here are some thoughts.  I am not a balloon expert (only my 3rd attempt in 20 years) so take these opinions with your own grains of salt.

1) 3′ dia party balloon (unfilled.  On line) cost under $2 each.  Making a 5 balloon launch about $10 for the balloons.

2) Mylar Balloons have a high mass to lift ratio so these are all LOW ALTITUDE missions.  Even with zero payload, the MAX altitude is around 25,000′ where the full balloon can only support its own weight no matter how many balloons.

3) OUr first mission was an extremely small 50 gram payload with HF oscillator and some CW telemetry, attemting a 10 day around the world flight.  Since it went over the atlantic toward africa, who knows what happened to it.  You could only year the milliwatt XMTR within line-of sight (about 100 miles)…

4) Helium loss through Mylar appeared to be around 1% per day compared to higher rates through latex.

5) Mylar balloons are an order of magnitude less vulnerable to UV rays which will almost always burst laytex after several hours exposure at high altitude.

6) Mylar are fixed volume.  THey get to a fixed height, where they are over-pressure and remain there (unless they burst).

7) Below 10,000′ temperatures are not an issue with electronics compared to the -60C temps for the typical high altitude flights.

8) I use clear plastc bottles for the enclosure and the temp inside remains high (solar heating).   Even at 8000′ the temp never got below about 40C.  We must use water proof containers because of all the bay and waters around.

9) This second mission used a full APRS system, wtih GPS and 2.4 GHz wireless camera using the Byonics MT-TT4 all-in-one APRS circuit board all in under 0.6 lbs including waterproof botttle container and chute.

10) WIth these mylar constant-pressure designs, extreme care must be used in underfilling each balloon exactly the same.  Any balloon that is slightly higher than the others will rise to a HIGHER Pressure and will be the first to burst.

The jury is still out as to whether a long duration mission is possile.  Ours will always go immediately to the Atlantic and at the low altitude, will take days to reach anyone in Europe (Our last went headed for africa where no one was listening).

** A ballast release mechanism is reuired for long duration.  We attempted a clever block of Ice (sublimation mass loss), but dont know if it worked, because no one reported hearing it in Africa?)

11) The amount of over pressure at equilibrium altitude is equal to the amount of excess lift.  So it is a difficult balance.  Too little lift and you need an extremely large launch area.  Too much and you are sure to burst.

12)  IN fact, with a modest excess-lift on our intentional shout duration mission, maybe there will always be a FIRST TO POP as in our case.  This was perfect though.  The loss of one balloon gave an almost balanced up and down profile .  No need for a chute.

13) The bright red multiple balloons (all full, except the one shreaded one) make for a highly visible descent and recovery.  If we had cut the payload loose, the chances of finding a clear plastic bottle with nothing around it but a tiny chute woiuld have been 1% of the success of finding 4 waving balloons!

14) Observing this, we thought about maybe using multiple string cutters for our next mission to control descent by cutting loose balloons.  But cutting loose only eliminates about half the mass as letting one burst. When it bursts, it loses lift, but the mass (nearly half the total lift) remains with the payload making descent better.

SO, maybe the plan next time will be to slightly overfill one balloon to assure a first-to-pop, and therefore have an automatic descent!  Still we will have a payload cutter just to make sure we can release before the Atlantic!

FINALLY, The abuse these party balloons can tolerate are an order of magnitude greater than Latex.  We launched in a 20 MPH wind!  After walking all 5 balloons from the classroom, across a road and through a narrow chain-link fence gate in that 20 MPH wind (3 times!) they survived.  Just prior to release, I noticed it was still transmitting all 3 packets at a 10 second rate!  We had to bring it all back indoors, cut loose the payload, go reprogram it, and then re-assemble  and go do it all again!

With multiple balloons, we fill a spare, so that if we busrt one, we can quickly tie in a replacemet in the field.  If they all survive getting to the launch point, then we release the spare to see exatly where the winds are going, so we can find the best spot to clear the 100′ high light posts surrounding the field.

Photos of this last mission will eventually make it to the http://aprs.org/balloons.html page.

But right now, I’m burned out.

Bob, WB4APR

March 2012 – First Party Balloon Launch http://www.uk.amsat.org/6163

DQ0STRATEX VHF & UHF Balloon Mission March 10

DL, GERMANY
DQ0STRATEX is a special event call on the occasion of the stratospheric balloon project (StratexB) planned for March 2012 by the local DARC clubs Duelmen (N28) and Luedinghausen (N29). They plan to send an amateur radio load, consisting of an APRS and a speech beacon, to the stratosphere with this balloon project. Another payload will be added by the HAMs of the German Aerospace Center (DLR) in Bremen (I04) with an experimental ADS-B receiver. The special event station DQ0STRATEX is active in all modes on all bands between Jan 13,2012, and Jan 31, 2013, handing out the special DOK STRATEXB.

They have two balloon missions planned, on Mar 10 around 0930 UTC and on Mar 24 around 1600 UTC, both starting on the airport at Borkenberge near Luedinghausen.

The APRS beacon is transmitting on 144.800 MHz and the speech beacon in FM on 430.375 MHz. SWL reports are highly appreciated (also online).

QSL cards via DK4REX. See also: http://www.darc.de/distrikte/n/29

[ANS thanks the DXNL 1770 – Mar 7, 2012 DX Newsletter for the above information]


73 de JoAnne K9JKM
k9jkm@amsat.org
Editor, AMSAT News Service

AMSAT-LU SSTV and Crossband Repeater on Glider and Balloon

AMSAT-LU SSTV and GPS Payload

View of communications experiment: Below is the plate of the repeater. Top left is the SSTV camera and top right is the GPS receiver module. Image credit LU7AA

An SSTV and crossband repeater payload developed by AMSAT-LU will be flown on a Glider and a High Altitude Balloon on March 3 and 17.

AMSAT-LU LU7AA report:

We are pleased to inform next Saturday March-3 2012 (if weather permits) from 12hs (GMT-3), Amsat-LU and friends will be flying from Zarate (Route 193, km 19 from Buenos Aires) an UV repeater including APRS + SSTV + CW + DTMF thru several flights aboard manned glider, as test for LUSEX (LU Satellite Experiment), being developed by AMSAT-LU.

Afterwards on Saturday March-17 from 12hs-LU on (GMT-3), a free Balloon will fly same payload from the city of Junin (Club of Gliders, Lagoon of Gomez), 250Km west of Buenos Aires City.

Payload will operate as an UHF to VHF crossband repeater, with CW tlm, APRS location and SSTV emissions in local and space frequencies.

According to estimates Balloon could reach 100,000 feet (30 km) in height, travelling from 50 to 100 miles towards east.

Thus allowing contacts between stations located in provinces of Buenos Aires, Santa Fe, Entre Rios, Cordoba, La Pampa, San Luis and Uruguay.  See coverage map on http://www.amsat.org.ar/junincubr.jpg and possible trajectory in http://www.amsat.org.ar/junin120215.jpg .

For these experiences, Amsat-LU works with and it is thankful to hams of Radio Clubs of Junin, QRM Belgrano, APRS Group, Don Bosco Ramos Mejia School, gliders Clubs of Zarate, Junin and Cañuelas, and the twelve Amsat-LU members development team as well as those who have actively participated and sent their reports in previous experiences.

More information at http://www.amsat.org.ar/lu4aao/experimento_globo_y_parapente.htm

AMSAT-LU Glider

Glider

Several flown experiments have been successfully operated during 2011 in manned-gliders, airplanes, captive and free Balloons allowing operational & practice for hams contributing to platform validaton of LUSEX satellite (LU Satellite EXperiment) on development by Amsat Argentina. More on http://lusex.org.ar

In order to monitor the payload (if you are within 400 miles of launch area) you need just an FM receiver either handy or base, in 145.950 for repeater and/or 144.930 for APRS. The repeater, that is activated via 123 Hertz subtone, operates receiving voice FM in 435.950 Khz (-112dbm, 0,56 uV) and emits with 2W the received audio live on 145.950 Khz.

Simultaneously APRS data will be sent in Packet at 1200 bauds in 144.930, and also in 145.950.

The DTI APRS symbol would change from a Balloon (/O) during the ascent to a glider (/g) during parachute descent.

Payload would operate as voice repeater activated by 123 Hz subtone during 1 minute, a warning bip at 40 seconds will indicate telemetry is coming, which is emitted if the repeater is not in use, if in 20 seconds more voice repeater still in use a two bips will be heard signaling that short APRS packages will begin in the different frequencies, also every 5 minutes CW (telegraphy with tones of audio) with CQ + callsign (LU7AA), sequence#, ext. and int. centigrade temperatures and voltage of batteries, after which the cycle will repeat.

AMSAT-LU RF Module

The system board containing RF transmitter module, receiver module, level adjustments, duplexer and antenna connector. Image credit LU7AA

Experiment for the first time in these flights will emit SSTV pictures in ROBOT-36 (36 seconds) in real time, showing what glider/Balloon sees. Every 5 minutes during ascent/descent and more spaced at high altitudes. (It can be received among others with MIXW, MMSTV & RX-SSTV ).

Payload would also carry on board two TV cameras (one towards earth and another towards horizon) recording video and sound during the flight. These captured videos could be recovered when payload is recovered.

APRS trajectory could be seen every minute, including speed, height, external and internal temperatures and 7.2v battery voltage using UI-View ( download from the UI-View official site on http://www.ui-view.org/ ) and/or to see/follow from Internet connecting to http://aprs.fi/?call=lu7aa-11 or locally via Packet at specified frequencies.

There are georeferenced Maps for UI-View in http://www.amsat.org.ar/junin.jpg, http://www.amsat.org.ar/junin.txt, http://www.amsat.org.ar/zarate.jpg, http://www.amsat.org.ar/zarate.txt, http://www.amsat.org.ar/lachoza.jpg and http://www.amsat.org.ar/lachoza.txt . Download and place them in directory Program Files/Peak Systems/UI-View32/MAPS and rename files .txt to .inf.

The experiment in 435.950 KHz besides voice, receives and accepts DTMF sequences commands on demand, I.E. sending B* (DTMF with handy keyboard on UHF) will return S5 … ….. in 145,950 VHF CW, reporting in CW signal strength received from your station, if S9+10 will returns P10.

There are also DTMF commands qualifying emission of CW tlm or APRS beacon or SSTV emission, commands that allows remote release of payload, mode changes, timers control, energy, power, etc.

Frequencies for previous coordination, announcements and flights will be 7090 Khz LSB +/-10 Khz and local repeaters.

During the flights will remain active wide coverage AMSAT-LU APRS Igate LU7AA-10 on 144.930 and 430.930 KHz, operating from the Constituyentes Investigation Center transferring whatever is received towards Internet.

For being an experiment oriented to a next satellite, the contacts made between stations via this payload will be considered valid for the recently announced permanent, gratuitous and applicable Satellite Certificate that AMSAT-LU and RClub QRM Belgrano grants, more info on http://www.amsat.org.ar/certsat.html

During the Balloon flight, amateur groups will chase the payload, aiming to locate and recover. Trapping ventures holds on this activity, as in the case of the Pampero 15 Balloon sent from San Miguel del Monte which landed in the middle of the Magdalena’s state prison … See http://www.lu5egy.com/Proyecto_pampero/vuelo_15/n_1esk.htm

All reports welcome. If you wish or can organize or want be part of control, or like to pursuit and recovery, or like operating and capturing data as an independent station, and/or wishes to join us personally in this adventure from the launching places email us to parapente at amsat.org.ar.

We appreciate reading of this information and thankful if distribution possible.

73, LU7AA, Amsat-LU, aiming at the future by making the present funny.
http://www.amsat.org.ar/
info at amsat.org.ar