A practical look at the 2026 WIA band plan revision, including the main HF changes, the tradeoffs behind them, and original comparison charts that point back to the official WIA documents.
The Wireless Institute of Australia has published its revised 2026 Australian Amateur Radio Band Plan after the 2025 consultation process. Band plans are voluntary, but they still shape how amateurs find each other, avoid interference, and build shared expectations about where different kinds of activity belong.
This revision is not just a visual refresh. Some HF frequencies that many Australian amateurs will recognise have moved, several digital-heavy areas are now shown more clearly in the published plan, and parts of the VHF, UHF, and microwave sections have been reorganised to match current operating patterns more closely.
Show headline changes
This is a shortlist of the changes most likely to affect day-to-day operating. If you want the full
set of bands, use the band chart and inspector below.
80m
Emergency comms moves to 3610 kHz; AM CoA becomes 3686 kHz.
The old 3600 kHz emergency reference overlaps with the data part of the band.
The 2026 plan names 3686 kHz as the AM centre of activity.
40m
The main references move to 7110 kHz for emergency comms and 7125 kHz for AM; 7074-7080 kHz is now shown as DATA.
The 2026 plan names 7125 kHz as the AM centre of activity.
The 7074-7080 kHz segment is now published as DATA rather than being left as a voice/data overlap area.
30m
Recommended voice operation narrows to 10120-10131 kHz.
The change is small on paper and significant in practice because the band is already tight.
20m
The emergency communications frequency shown in the plan moves from 14125 kHz to 14300 kHz.
The new position aligns with IARU Region 3.
6m
The band plan changes the DATA, beacon, and experimental segments quite heavily.
50.220-50.330 MHz becomes the new DATA segment.
52.000-52.500 MHz is now wideband experimental all-modes.
VHF/UHF/SHF
Repeaters, ATV, and wideband data see some of the largest layout changes in the new plan.
This matters more to coordinators and experimenters than to casual operators.
Why the plan changed
The consultation outcomes point to a few recurring problems.
One was friction between voice activity and parts of the bands that now carry heavy digital use. That
shows up on 80m, 40m, and 30m. Another was that some informal operating habits had drifted away
from what the published plan still showed. The 2026 revision updates the published plan to match that
reality more closely.
That has advantages, but it also has a cost. A more realistic band plan is useful only if people
actually adjust to it, and that means some operators will need to give up habits that have been around
for years. Even where the new plan makes technical sense, not everyone will agree that the new
boundaries are the right ones.
There is also a difference between bands where the changes affect everyday operating and bands where the
changes mostly affect coordinators, repeater groups, ATV users, or microwave experimenters. Some parts
of the revision will feel immediately relevant. Other parts will seem remote unless you already work in
those areas.
What this means in practice
For ordinary operating, the main message is simple: a few familiar frequencies should no longer be treated as the obvious default.
If you operate HF voice, especially on 80m, 40m, 30m, or 20m, it is worth checking the new
plan rather than relying on memory. Several of the updates move voice or emergency activity away from
digital-heavy areas, and several AM centres of activity are now listed by frequency in the plan.
That should reduce avoidable clashes over time. In the short term, though, it may do the opposite.
During any transition, some operators will still be listening on the old frequencies, others will move
to the new ones straight away, and some will not even realise anything has changed.
For POTA and SOTA activators, the main effect is better frequency choice on HF, especially around the
revised voice, data, and emergency communications segments.
Band-by-band changes
Band Inspector
Select a band
Pick a band from the spectrum selector. The terminal below updates with the specific frequencies,
segment changes, and tradeoffs for that band.
LF / HFVHF / UHFSHF
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CWDATAVOICEREPEATERBEACONALL MODESATVSATELLITE
radio://wia-band-inspector
> inspect --band 630m
The 2026 plan splits 630m into specific CW, DATA/CW, and VOICE/CW sections.
630 metres
472 kHz to 479 kHz
Earlier arrangement
Pre-2026 WIA style
CW / DATA
Shared narrowband use
472476479
2026 plan
WIA 2026
CW
DATA / CW
VOICE / CW
LSB voice
472476479
The older arrangement is shown in simplified form here because the 2026 review mainly changed how this small band is divided up.
What changed
The band is now split into separate CW, DATA/CW, and VOICE/CW sections. The 2026 plan specifically lists 478.5 kHz as the LSB voice centre of activity.
Why this was changed
This is more than a small marker change. The WIA has rewritten the way the band is divided up.
What to watch for
The band is still specialised, so a clearer plan does not necessarily mean broader use.
> inspect --band 160m
The main visible change is that 1870 kHz is now listed as the AM centre of activity.
160 metres
1800 kHz to 1875 kHz
Earlier arrangement
Pre-2026
CW / DATA emphasis
VOICE
180018381875
2026 plan
WIA 2026
CW / DATA emphasis
VOICE
AM CoA
180018381875
What changed
1870 kHz is now the nominated AM centre of activity.
Why this was changed
The alternatives raised in consultation sat too close to either CW-priority or data-heavy parts of the band.
What to watch for
Centres of activity can harden into habits more rigidly than the band plan itself requires.
> inspect --band 80m
Emergency comms moves to 3610 kHz and AM activity moves to 3686 kHz.
80 metres
3500 kHz to 3800 kHz
Earlier arrangement
2009 / previous WIA
CW
SSB
DATA
SSB
EmCom
350036503800
DX window 3776-3800 kHz
2026 plan
WIA 2026
CW
VOICE / CW
DATA / CW
VOICE / CW
VK EmCom
AM CoA
350036503800
DX window 3776-3800 kHz
What changed
The Australian emergency communications centre of activity moves from 3600 kHz to 3610 kHz. The AM centre of activity becomes 3686 kHz.
Why this was changed
The older 3600 kHz emergency arrangement sat awkwardly inside the data segment.
What to watch for
The old 3600 kHz habit will probably persist for a while. Operators may need to monitor both old and new references during the transition.
> inspect --band 40m
7110 kHz replaces the older emergency reference, and 7074-7080 kHz is now shown as DATA.
40 metres
7000 kHz to 7300 kHz
Earlier arrangement
2009 / previous WIA
CW
SSB
Old WICEN
IARU R3
700071507300
DATA 7040-7060 kHz
SSB 7060-7074 kHz
Voice overlap 7074-7080 kHz
2026 plan
WIA 2026
CW
VOICE / CW
EmCom
AM CoA
700071507300
DATA / CW 7040-7060 kHz
VOICE / CW 7060-7074 kHz
DATA / CW 7074-7080 kHz
What changed
7110 kHz is now the Australian emergency communications centre of activity shown in the plan. 7125 kHz becomes the AM centre of activity.
7074-7080 kHz is now shown as DATA instead of being left as an area where voice and digital use were colliding.
Why this was changed
The WIA is reflecting the fact that digital activity in the lower part of the old voice area is already well established on air.
What to watch for
Some voice operators will see this as confirmation that the part of the band they used casually is no longer really available in the same way. This is also a band where older habits die slowly.
> inspect --band 30m
The recommended voice window is reduced to 10120-10131 kHz.
30 metres
10100 kHz to 10150 kHz
Earlier arrangement
Pre-2026
CW
VOICE / CW
DATA / CW
101001012510150
2026 plan
WIA 2026
CW
VOICE / CW
DATA / CW
101001012510150
What changed
The recommended voice segment contracts from a broader domestic window down to 10120-10131 kHz.
Why this was changed
The change reflects heavier international data use above 10131 kHz.
What to watch for
30m was already a narrow band, so even a small move here feels consequential.
> inspect --band 20m
The main change is that the emergency communications frequency shown in the plan moves from 14125 kHz to 14300 kHz.
20 metres
14000 kHz to 14350 kHz
Earlier arrangement
2009 / previous WIA
CW
SSB
WICEN
140001417514350
DATA 14070-14100 kHz
IBP / DATA 14100-14112 kHz
2026 plan
WIA 2026
CW
VOICE / CW
EmCom
140001417514350
DATA / CW 14070-14099 kHz
IBP 14099-14101 kHz
DATA / CW 14101-14112 kHz
What changed
The emergency communications frequency shown in the Australian plan moves from 14125 kHz to 14300 kHz.
Why this was changed
That aligns the Australian plan with the IARU Region 3 emergency reference.
What to watch for
14300 kHz is already a well-known frequency, so not everyone will regard it as clear and neutral space.
> inspect --band 12m
24950 kHz remains the emergency communications reference, so 12m changes less than the neighbouring HF bands.
12 metres
24890 kHz to 24990 kHz
Earlier arrangement
Pre-2026
CW
DATA
VOICE
WICEN
248902494024990
2026 plan
WIA 2026
CW
DATA / CW
VOICE / CW
EmCom
248902494024990
IBP 24929-24931 kHz
What changed
24950 kHz remains the Australian emergency communications reference.
Why this was changed
The consultation considered dropping it but retained it because of WICEN interest.
What to watch for
There is less to relearn here, but that also means the panel can feel less relevant unless you actually use 12m.
> inspect --band 6m
The DATA, beacon, and 52 MHz experimental sections are all rearranged in the 2026 plan.
6 metres
50 MHz to 54 MHz
Earlier arrangement
2009 / previous WIA
ALL MODES
Narrowband
Simplex / Repeaters
DX call
WICEN
5052.00054
CW 50-50.1 MHz
CW / SSB 50.1-50.22 MHz
DATA 50.22-50.24 MHz
CW / SSB 50.24-50.32 MHz
DATA 50.32-50.4 MHz
Reserved 50.5-50.7 MHz
2026 plan
WIA 2026
ALL MODES
Wideband experimental
Repeater input
Simplex
Repeater output
FT8
AM CoA
WICEN
5052.00054
IBP 50-50.03 MHz
Beacons 50.03-50.08 MHz
CW 50.08-50.105 MHz
VOICE / CW 50.105-50.22 MHz
DATA 50.22-50.33 MHz
VOICE / CW 50.33-50.4 MHz
Beacons 50.4-50.5 MHz
Simplex 52.5-52.5375 MHz
What changed
The DATA segment is now 50.220-50.330 MHz. The 50.280-50.320 MHz beacon segment is withdrawn in favour of 50.400-50.500 MHz.
52.000-52.500 MHz becomes a wideband experimental all-modes block.
Why this was changed
The updated layout gives more weight to digital weak-signal use and to experimentation above 52 MHz.
What to watch for
The band becomes more structured and less intuitive to remember at a glance.
> inspect --band 2m
The layout is more explicit about digital and repeater use, but the real change is tighter control over the -1.6 MHz repeater pairs.
2 metres
144 MHz to 148 MHz
Earlier arrangement
2009 / previous WIA
Narrowband modes
Mixed simplex / repeater use
Repeater inputs
Outputs / simplex
Repeater inputs
APRS
WICEN
144146.000148
Satellite 144-144.025 MHz
Digital simplex 144.7-144.9 MHz
FM / digital simplex 145.075-145.4 MHz
Satellite 145.8-146 MHz
2026 plan
WIA 2026
Digital / DATA
Analogue simplex / shared inputs
Repeaters
Repeaters / inputs
APRS
WICEN APRS
ARDF
144146.000148
Satellite 144-144.025 MHz
CW 144.025-144.1 MHz
VOICE / DATA / CW 144.1-144.4 MHz
Beacons 144.4-144.6 MHz
ALL MODES 144.6-144.7 MHz
Satellite 145.8-146 MHz
Analogue simplex 147.3875-147.6125 MHz
The main 2026 difference here is not a complete relayout of the band. It is the tighter rule on when the shared -1.6 MHz repeater pairs should be used.
What changed
The 2026 chart spells out where digital voice, digital repeaters, and the shared offset repeater pairs sit. The real policy change is tighter control over when the -1.6 MHz repeater pairs should be used.
Why this was changed
The WIA is trying to stop the exceptional repeater offsets from becoming routine convenience choices.
What to watch for
This is more useful to repeater coordinators than to casual operators.
> inspect --band 70cm
The 2026 plan points 70cm more firmly toward -7 MHz repeater logic, even though legacy arrangements remain on air.
70 centimetres
430 MHz to 450 MHz
Earlier arrangement
2009 / previous WIA
Satellite
ATV
WICEN
FM call
430440.000450
Narrowband modes 431.95-432.7 MHz
Beacons 432.4-432.6 MHz
ALL MODES 433.025-434.775 MHz
FM / digital simplex 438.95-439.775 MHz
ALL MODES 441-441.975 MHz
2026 plan
WIA 2026
Satellite
DVB-T ATV
WICEN
FM call
430440.000450
Links 430-431 MHz
Repeater input A 431-431.9375 MHz
CW 431.9375-432.1 MHz
VOICE / CW 432.1-432.3 MHz
DATA / CW 432.3-432.4 MHz
Beacons 432.4-432.6 MHz
Repeater input B 432.6-433.05 MHz
LIPD overlap / all modes 433.05-434 MHz
Links 434-434.5 MHz
Hotspot input 434.5-434.79 MHz
Repeater input alt 434.79-435 MHz
Digital simplex 438-438.9375 MHz
Outputs / simplex / repeater 438.9375-440 MHz
Links 440-441 MHz
ALL MODES 441-441.5 MHz
Hotspot 441.5-442 MHz
Links 449-450 MHz
What changed
The 2026 chart labels repeater inputs, outputs, hotspot space, and link blocks in a much more literal way than the older layout. The consultation outcomes point toward -7 MHz as the long-term preferred repeater logic.
Why this was changed
The WIA is trying to reduce confusion and reduce interaction with LIPD-heavy parts of the band.
What to watch for
Existing systems and legacy offsets mean the lived band will stay messier than the published plan for some time.
> inspect --band 23cm
ATV is kept lower in the band and new repeater guidance appears at 1257.5 / 1297.5 MHz to reduce interference risk.
23 centimetres
1240 MHz to 1300 MHz
Earlier arrangement
Pre-2026, based on the consultation outcomes
ATV-heavy use
12401270.0001300
Legacy repeater output 1273-1274 MHz
Legacy repeater input 1293-1294 MHz
FM simplex 1294-1295 MHz
Weak signal 1295-1296 MHz
Mixed narrowband / EME 1296-1300 MHz
2026 plan
WIA 2026
ATV
Experimental / satellite
Experimental
FM call
12401270.0001300
Repeater output 1257.5-1258 MHz
Legacy output 1273-1274 MHz
Legacy input 1293-1294 MHz
Experimental 1294-1296 MHz
CW / DATA 1296-1296.1 MHz
Narrowband 1296.1-1296.4 MHz
Beacons 1296.4-1296.6 MHz
FM simplex 1296.6-1297.5 MHz
Repeater input 1297.5-1298 MHz
Simplex 1298-1299 MHz
EME / future narrowband 1299-1300 MHz
What changed
Most ATV use is now kept below 1258 MHz in the published layout. A new repeater pair is shown at 1257.5-1258.0 MHz output and 1297.5-1298.0 MHz input.
FM simplex and narrowband activity are moved into safer positions around 1296.6 MHz and above.
Why this was changed
The post-WRC environment means the band has to be used in a way that reduces the risk of RNSS interference complaints.
What to watch for
The changes are prudent, but they also make the band feel more constrained and less forgiving than before.
> inspect --band 13cm
13cm gains a repeater pair and a more deliberate ATV layout.
13 centimetres
2400 MHz to 2450 MHz
Earlier arrangement
Pre-2026, based on the consultation outcomes
ATV
All modes / wideband data
ATV
24002425.0002450
Satellite 2400-2403 MHz
Narrowband modes 2403-2403.6 MHz
Simplex 2403.6-2405 MHz
All modes 2448-2450 MHz
2026 plan
WIA 2026
ATV
ATV
24002425.0002450
Satellite 2400-2403 MHz
EME / CW / DATA 2403-2403.1 MHz
Narrowband 2403.1-2403.4 MHz
Beacons 2403.4-2403.6 MHz
Simplex 2403.6-2405 MHz
Repeater input 2405-2406 MHz
All modes 2424-2425 MHz
Repeater output 2425-2426 MHz
Wideband data 2426-2430 MHz
All modes 2448-2450 MHz
What changed
A 20 MHz repeater pair is now built into the band plan. ATV channels are now labelled in a way that makes the DVB channel positions easier to see.
Why this was changed
The 2026 plan is trying to support practical repeater development rather than leaving the band purely theoretical.
What to watch for
On a busy ISM-adjacent band, any extra structure can still feel optimistic if local noise is the real limit.
> inspect --band 9cm
9cm keeps much of its earlier layout, but the repeater pair and ATV channel positions move around radio astronomy limits.
9 centimetres
3300 MHz to 3400 MHz
Earlier arrangement
Pre-2026, based on the consultation outcomes
ATV
All modes / wideband
ATV
ATV
33003350.0003400
All modes 3300-3302 MHz
All modes 3394-3398 MHz
Narrowband 3398-3400 MHz
2026 plan
WIA 2026
ATV
Wideband / all modes
ATV
ATV
33003350.0003400
All modes 3300-3302 MHz
RA exclusion overlap 3332-3339 MHz
All modes 3339-3345.8 MHz
RA exclusion overlap 3345.8-3352.5 MHz
All modes 3352.5-3356 MHz
Repeater output 3356-3357 MHz
All modes 3357-3358 MHz
All modes 3394-3396 MHz
Repeater input 3396-3397 MHz
Simplex 3397-3398 MHz
CW 3398-3398.4 MHz
Beacons 3398.4-3398.6 MHz
All modes 3398.6-3400 MHz
What changed
A new repeater pair appears in the 3356-3357 / 3396-3397 MHz area. ATV channels are rearranged around exclusion constraints.
Why this was changed
The final plan is a compromise between introducing new uses and respecting radio astronomy limitations.
What to watch for
This is one of the harder charts to read casually because the restrictions are part of the story.
> inspect --band 6cm
6cm shows the shift from alternating voice/data blocks to wider data channels.
6 centimetres
5650 MHz to 5850 MHz
Earlier arrangement
Pre-2026, based on the consultation outcomes
ATV
20 MHz data
20 MHz voice
ATV
Simplex / narrowband
20 MHz data
20 MHz voice
Satellite
56505750.0005850
Satellite 5650-5660 MHz
All modes 5660-5670 MHz
ATV 5815-5825 MHz
2026 plan
WIA 2026
ATV
40 MHz data
ATV
40 MHz data
Satellite
56505750.0005850
Satellite 5650-5660 MHz
All modes 5660-5670 MHz
Repeater output 5730-5735 MHz
All modes / narrowband 5755-5770 MHz
Repeater input 5770-5775 MHz
ATV 5815-5825 MHz
All modes 5825-5830 MHz
What changed
The former 20 MHz data and voice blocks are merged into broader 40 MHz data channels. A new 40 MHz repeater pair appears at 5730-5735 / 5770-5775 MHz.
Why this was changed
The revision better supports Wi-Fi-aligned networking experiments and newer ATV practice.
What to watch for
Operators who still value the old wide voice concept may see this as a one-way shift toward data.
> inspect --band 3cm
3cm follows the same wideband trend and adds a repeater pair of its own.
3 centimetres
10000 MHz to 10500 MHz
Earlier arrangement
Pre-2026, based on the consultation outcomes
All modes
Simplex / mixed
Satellite
1000010250.00010500
20 MHz data 10160-10180 MHz
20 MHz voice 10180-10200 MHz
ATV 10200-10220 MHz
20 MHz data 10220-10240 MHz
20 MHz voice 10240-10260 MHz
ATV 10260-10280 MHz
20 MHz data 10280-10300 MHz
20 MHz voice 10300-10320 MHz
ATV 10320-10340 MHz
ATV 10420-10440 MHz
2026 plan
WIA 2026
All modes
Wideband data
Wideband data
Satellite
1000010250.00010500
40 MHz data 10160-10200 MHz
ATV 10200-10220 MHz
40 MHz data 10220-10260 MHz
ATV 10260-10280 MHz
ATV 10320-10340 MHz
Simplex 10340-10355 MHz
Repeater input 10355-10360 MHz
Simplex 10360-10368 MHz
EME 10368-10368.1 MHz
Narrowband 10368.1-10368.4 MHz
Beacons 10368.4-10368.6 MHz
ATV 10420-10440 MHz
All modes 10440-10445 MHz
Repeater output 10445-10450 MHz
What changed
Former 20 MHz voice slots are absorbed into larger data sections. A new repeater pair appears around 10355-10360 / 10445-10450 MHz.
Why this was changed
The new layout is aimed more at data networking and modern ATV use than at preserving the older wide voice blocks.
What to watch for
That direction will not appeal equally to every microwave operator.
What the consultation outcomes suggest
Reading the consultation outcomes alongside the final plan gives a better sense of the tradeoffs.
Some of the changes are clearly overdue. A few older arrangements had become awkward enough that leaving
them alone would have been harder to justify than changing them. That is particularly true where voice
and data were sitting on top of each other in ways that no longer reflected actual operating.
At the same time, not every change will feel neutral. Some operators will read the revision as sensible
housekeeping. Others will read parts of it as the WIA publishing changes that confirm older operating
habits no longer fit the band as well as they once did. Both views can be true at once.
The strongest point in the new plan is that it is generally more in touch with current practice. The
weakest point is that current practice is not always universally welcomed. A band plan can reflect
reality, but it cannot make everyone happy about the reality it reflects.
Final thoughts
The 2026 WIA Australian Amateur Radio Band Plan is worth reading even if you normally ignore band-planning documents.
Several of the changes affect frequencies that many Australian amateurs use regularly, especially on
80m, 40m, 30m, and 20m. Others are more relevant to repeater groups, ATV users, and microwave
experimenters, but still show where the WIA thinks structure is needed.
The update should reduce some longstanding friction. It may also create a short-term adjustment period,
especially where familiar frequencies have moved or long-established habits are being pushed aside. That
is probably unavoidable.