Satellites and orbital operating
Amateur satellites (and the ISS) reward portable operators: a handheld yagi, a dual-band radio, and a clear horizon. Orbital work is parallel to POTA/SOTA — you can combine a satellite pass with a park activation for grid/rare-DX fun, and the satellite QSO itself can count. POTA's current rules (v1.3, dated Aug 18, 2026; checked 2026-10-08) say "Satellite repeaters are allowed," so a complete satellite contact from inside the park counts toward your 10. Global WWFF rules v5.10 also accept satellite contacts. Details and caveats are under Combining with POTA / SOTA.
Intro: Easy Portable Satellite Operation (PDF) · AMSAT · field tracking deep-dive: N5DUX Satellite Guide — Tracking
FM vs SSB transponders
| Type | Examples (change over time) | Radio needs | Portable antenna |
|---|---|---|---|
| FM repeater birds | SO-50-style V/U or U/V | Dual-band FM HT or mobile | Arrow / Elk handheld yagi |
| Linear SSB/CW | FO-29, RS-44-class | All-mode V/U (IC-705, FT-818, IC-9700) | Same yagis; more Doppler skill |
FM is the on-ramp: one contact through the bird proves your setup. SSB linear transponders behave like a moving passband — tune both uplink and downlink. Start on FM before you graduate to linear birds; you will make fewer mistakes on a crowded SSB passband once your arm (or rotator) already knows how to track.
Minimum portable FM kit
From Ham Sat Tracker equipment guide and common field practice:
- Dual-band HT or dual-VFO mobile (true full-duplex HT like TH-D72/D74 class is ideal; half-duplex works with practice)
- Handheld yagi (Arrow II or Elk log periodic — 2 m + 70 cm on one boom)
- Pass predictor app (Look4Sat, Ham Sat Tracker, SatSat, and others)
- Headphones — satellite downlink in a noisy park is painful without them
Power: 5 W is enough on FM with a good antenna. More power can desense the transponder for everyone (QRP satellite ops).
Tracking — the skill that matters most
If you do not know when and where to point, the pass is over before you find the bird. Lucky listening exists; deliberate tracking is more fun. The notes below paraphrase and update the practical framing from N5DUX’s tracking page for getontheair / POTA parking-lot ops.
Tools (web and phone)
| Tool | Notes |
|---|---|
| N2YO | Long-time web go-to; location from IP is usually close enough for handheld “sloppy” pointing |
| AMSAT Track | Classic lat/lon calculator; less flashy than N2YO, still solid |
| Heavens-Above | Web (and Android app); older standard many ops still know |
| iOS: SatSat, HamSatHD, GoSatWatch | SatSat is a common free choice; others are paid with richer features |
| Android: Heavens-Above, W1ANT apps | Free/ad-supported and paid options |
Most phone apps cache TLEs (two-line elements). When the park has no cell, you can still track if you refreshed data before you left pavement. On a boat or deep-woods hike, that pre-download is the whole plan.
Feature comparison wiki (apps): linked from the N5DUX tracking page resources.
Azimuth (compass heading)
Azimuth is degrees from north: 0° N, 90° E, 180° S, 270° W, then back toward 360°/0°. Cardinal words are fine for hiking; satellite pointing wants numbers. For handheld work you only need to be close enough — a 10° error in arm pointing is normal and usually still works on FM birds. Memorize the four primary points and the midpoints (45° = NE, etc.) so a glance at the app becomes muscle memory.
In a POTA parking lot: stand where you have the clearest horizon toward the predicted AOS azimuth, phone compass calibrated (away from the truck’s steel), and face that heading before the bird rises. Trees, the visitor-center roof, and a motorhome beside you all eat low-elevation passes — walk twenty steps if the lot allows.
Elevation (up from the horizon)
Elevation (altitude) is the angle up from the horizon: 0° on the horizon, 90° straight up, 45° halfway. Tracking apps draw a polar map with concentric rings — commonly 90° at center, then rings for 60° / 30° / 0° (horizon). When the path crosses into the outer usable ring you are near AOS; when it exits the horizon ring you are at LOS.
AOS / LOS and obstacles
AOS = Acquisition of Signal; LOS = Loss of Signal. Those times assume a mathematical horizon at 0° elevation. They do not know about your oak tree, ridge line, or the pavilion roof. Expect real AOS later and real LOS earlier whenever terrain or structures block the path. From a typical park lot, treat published AOS as “start listening and pointing,” not “guaranteed audio.”
Max elevation — don’t worship the overhead pass
Maximum elevation is the highest point of that pass for your location. A near-overhead (~90°) pass feels easy to work; it is not inherently “better.” Low passes stretch the footprint — a bird skimming 15° on your eastern horizon is still high for someone far west of you. Operators chasing Satellite Worked All States and long-haul contacts deliberately work those horizon grazers. For first FM QSOs from a park, pick something with max elevation above ~15–20° and a clear sector; once you are comfortable, chase the low ones for distance.
Pass workflow
- Predict: pick pass with max elevation above ~15–20° for first tries; ISS passes above 60° for SSTV/HT-only attempts.
- Setup early: 5 minutes before AOS, antenna compass direction, radio memories programmed.
- Acquire: listen on published downlink; adjust for Doppler (shift downlink as bird approaches/recedes).
- Call: brief CQ with grid — satellite QSOs are short by physics.
- Log: satellite name, mode, uplink/downlink freqs, grid if exchanged.
Doppler (practical)
Uplink and downlink both shift as the satellite moves. FM ops often pre-load three memories (high → nominal → low). SSB ops continuously tune uplink while keeping downlink stable — skill builds with reps.
Numbers, not vibes: LEO birds at VHF can move several kHz over a pass. Pre-load high / mid / low memories from the current AMSAT / tracker card for that object — published Doppler tables change when the bird is replaced. FM: start a few kHz high at AOS, click toward the mid memory as elevation rises, click low toward LOS. Linear birds: lock the downlink in the ears (or on a second VFO / 9700 full duplex) and walk the uplink so your own signal stays in the passband. If you cannot hear yourself through the bird, you are off frequency or underpowered — stop calling and listen.
Parking-lot habit: phone tracker cached TLEs before you lose cell, compass calibrated away from the truck steel, yagi on the AOS azimuth five minutes early. HF mast stays down until LOS so you do not spear the yagi.
Antenna pointing — you are the rotator (until you aren’t)
Rotate the yagi in azimuth; adjust elevation by tilting the boom. Practice without transmitting first — hearing the bird is half the battle. From a POTA lot, a quick mental map helps:
- Note AOS azimuth and LOS azimuth from the app before the pass.
- Track the path across the sky; elevation rises toward mid-pass, then falls.
- Keep the boom pointed at the bird, not at the truck antenna you meant to use for HF later.
Arm fatigue is real on long linear passes. That is where a portable rotator earns its keep.
Portable rotator: WA4MCM PSR-100 Mk2
WA4MCM (Don Friend) sells the PSR-100 Mk2 — a portable, lightweight satellite antenna rotor kit built for Arrow / Elk-class handheld yagis, not permanent tower installs. It is weather-susceptible by design (portable first); do not leave it bolted outside like a Yaesu G-5500.
What field / rover / park ops care about (from the product page and Mk2 manual):
- Mounts on a camera tripod (¼-20) — easy to stage beside a picnic table or parking-lot pad
- Max antenna weight ~2 lb (900 g) — standard Arrow / Elk class; the heavier Arrow Alaskan is too much
- Removable boom mount sized for Arrow ¾″ square boom or Elk log periodic (choose mount; both available)
- Wi‑Fi to any 2.4 GHz network; control and calibration via a web browser (Mk2 dropped the old Windows-only companion app)
- Talks to tracking software over UDP — protocols include Yaesu GS-232B, EasyComm II, and direct CSN Technologies S.A.T. Box
- Works with SatPC32, SkyRoof, HRDSatTrack, Gpredict, MacDoppler, PstRotator, and similar via the included serial-to-UDP bridge where needed
- Field power: a small ~3 Ah LiFePO4 is a common pairing (battery not in the kit); wall supply included for bench test/calibration
- Flip mode for passes that cross north through the azimuth stop; park position to stow between birds
How rovers use it: assemble the tripod and rotor before AOS, snap on the Arrow/Elk, join the rotor’s Wi‑Fi (or your phone hotspot / local network), open the web UI, run calibration if you moved the mount, then let Gpredict / SatPC32 / the S.A.T. Box drive az/el while you work the radio. You get two free hands for logging, Doppler, and half-duplex juggling — useful in a POTA parking lot where you also need to watch for cars and keep coax out of the lane.
It is not a substitute for learning handheld tracking. Learn with your arm first; add the PSR-100 when pass rate and fatigue justify the kit cost and setup time. Purchase is typically via WA4MCM’s contact/purchase-request flow (hamfest-oriented sales), not a random cart checkout — confirm current price and shipping on wa4mcmkits.com.
Combining with POTA / SOTA
Legal and practical separation:
- POTA credit (rules checked 2026-10-08): POTA's rules (v1.3, Aug 18, 2026) allow satellite repeaters and ban land repeaters. The POTA glossary puts the line at the Kármán line: a repeater on an object above it is a satellite repeater, and one below it (a mountaintop, balloon or drone) is a land repeater. A full satellite exchange from inside the park counts toward the 10. The ISS crossband repeater counts too, because the ISS orbits well above that line. Log the satellite name (ADIF
SAT_NAME, withPROP_MODE=SAT) so the QSO is clear later. Check the rules page again before a big trip, because rules get revised. - WWFF: global rules v5.10 (3 Sept 2025), §3.10, accept satellite contacts such as QO-100. Older KFF FAQ wording treated satellites as repeating devices, so check your national programme's FAQ.
- SOTA: check the current General Rules on sota.org.uk before counting a pass toward the four.
- Grid: satellite grids are valuable for grid chasers; your activator grid still comes from the park pin for
MY_GRIDSQUAREon POTA uploads. - Time budget: a 10-minute FM pass fits before or after a HF activation; do not miss minimum QSOs chasing a low-elevation pass.
- Horizon: pick the side of the lot with the open sky toward AOS; a vertical HF mast on the hitch can wait until after LOS.
SOTA on summits: FM satellite from a peak is classic; watch weight and keep AZ boundaries in mind. A tripod rotator may be overkill on a short summit stay — handheld still wins for grams.
The ISS — voice repeater, APRS, SSTV and school contacts
The International Space Station carries amateur radio stations run by ARISS (Amateur Radio on the International Space Station), an international partnership of space agencies and national amateur radio and AMSAT organizations. Independent guide — not affiliated with ARISS, NASA, ARRL or AMSAT.
What is on right now changes often. Radios are switched modes or turned off for spacewalks, dockings and crew schedules. Always check the ARISS current status page and the ISS lines on the AMSAT satellite status page (live reports from hams) before a pass.
ISS frequencies (as published by ARISS, checked Oct 2026)
| Service | Downlink (you listen) | Uplink (you transmit) | Notes |
|---|---|---|---|
| Crew voice | 145.800 MHz FM (worldwide) | 144.490 MHz (ITU Regions 2 and 3, including the Americas) · 145.200 MHz (Region 1) | Scheduled school contacts and occasional crew general contacts. Never transmit on the downlink. |
| Voice repeater (crossband) | 437.800 MHz FM | 145.990 MHz FM, 67.0 Hz CTCSS tone | When active, it works much like an FM satellite: short exchanges, call sign and grid. |
| Packet / APRS | 145.825 MHz (VHF) or 437.825 MHz (UHF) | Same frequency (simplex digipeater) | Which one is active varies; check status. |
| SSTV events | 437.550 MHz FM, Robot36 mode | Receive only | Images about every two minutes during scheduled events. |
Status example (dated): on Oct 7, 2026 ARISS listed NA1SS (Columbus module) in voice repeater mode (145.990 up / 437.800 down) and RS0ISS (Zvezda) with APRS active on 437.825 MHz. Treat that as a snapshot, not a schedule.
Call signs used aboard include NA1SS (USA), RS0ISS (Russia) and DP0ISS / OR4ISS / IR0ISS (Europe).
Working the ISS voice repeater
- An HT with a handheld yagi (or a good mobile setup) is enough; the ISS radio is relatively strong.
- Program 437.800 receive with Doppler steps (about 437.810 at AOS → 437.790 at LOS) and 145.990 transmit with the 67 Hz tone — see Doppler above.
- Same etiquette as a busy FM bird: listen first, give your call sign and grid, keep it short, one contact per pass when crowded.
APRS through the ISS digipeater
- A 2 m or 70 cm APRS radio or a TNC/sound-card setup can send a position or short message through the ISS digipeater. Use the frequency ARISS lists as active.
- ISS-heard packets show up on the ARISS APRS status page — a quick way to confirm your packet made it. Packets in that list show the path
APRSAT; follow ARISS's current guidance for path settings. - Keep beacons infrequent during a pass; the digipeater is shared by everyone in the footprint.
- New to APRS (SSIDs, paths, aprs.fi)? See APRS for beginners.
SSTV events
- During scheduled events, the ISS transmits slow-scan TV images on 437.550 MHz in Robot36, with roughly two minutes between images. Older guides listing 145.800 MHz for SSTV are out of date for current events.
- Receive with a 70 cm FM radio (or SDR) and a decoder app; correct for Doppler on 70 cm (±10 kHz). Setup: SSTV.
- Dates are announced on Upcoming SSTV events; you can upload received images to the ARISS SSTV gallery and request an award certificate where offered.
- QSL information for ISS contacts and SSTV reception: ARISS QSL cards.
How ARISS school contacts are arranged
A scheduled ARISS contact is a roughly 10-minute voice question-and-answer session between students and an astronaut during one ISS pass.
| Step | What happens (US process as published by ARISS) |
|---|---|
| 1. Pick a type | Direct — a ham station at or near the school talks to the ISS (often set up by a local club). Telebridge — an ARISS ground station elsewhere makes the radio link and the audio is carried to the school by phone/internet. Multipoint telebridge links several sites to one contact. |
| 2. Plan the education | Proposals need a real education plan: space science/exploration topics plus communication, wireless and radio science. Bigger, well-integrated audiences score better. |
| 3. Apply in a window | US proposals are accepted in quarterly windows. Example (dated): the Oct–Dec 2026 window closes Dec 31, 2026, for contacts in July–Dec 2027. Download the planning/proposal guide, attend an online information session, and submit the proposal form. |
| 4. Selection | A committee from NASA, ARRL and AMSAT reviews proposals; results go out about 6–8 weeks after the window closes. |
| 5. Prepare | Selected hosts get an orientation and an ARISS Technical Mentor, submit an equipment plan, and need flexibility — dates can shift with ISS operations. |
Start at Hosting an ARISS contact in the US or, outside the US, Apply to host an ARISS contact. Background: About ARISS contacts. Clubs: a school near you may need a local ham team — see Clubs and Elmers and Parents & youth.
Etiquette
- One contact per pass segment when crowded — do not hog the transponder.
- Identify clearly; satellite pileups are fast.
- If you cannot hear yourself through the bird (half-duplex), listen for others working you before you call again.
- Keep power reasonable; the bird is a shared resource.
Habits / gotchas / checklist (satellites)
Related
- SSTV · Planning (grid pin) · Technician HF & propagation · Glossary
- RV & camping setups (rooftop / lot passes)
- Resources — N5DUX tracking · WA4MCM PSR-100
Notes & edits
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