WA8LMF Mirror of WB4APR Website - 21 July 2008 FIXING DIGIPEATERS

Fixing the 144.39 APRS Network

The New n-N Paradigm

We must get all digipeaters to these new settings! Its been 4 years! If you know of an obsolete digi, contact the owner and assist in getting it updated. This page has been re-organized on 15 June 2008 to put the New-N DIGI settings up front. Then the explanation and other info follows. Here are the new settings for each digi type:

  • KPC-3+ Vers 8.3 to 9.1
  • KPC-3 Vers 8.2
  • UIDIGI-ROMs.
  • DIGI_NED
  • PacComm TNCs.
  • Fill-in WIDE1-1 digis

    RECENT UPDATED CONCEPTS FOR IMPROVING APRS OPERATIONS: As a result of the new streamlined New-N network, these additional concepts have added a rich layer of operational utility to the local RF network.

  • Misconceptions about APRS as only a vehicle tracking system instead of a local INFO channel.
  • European Map of New-N Implementation. . See also map of digi implementation
  • APRS Section Coordinators to help coordinate the New-N Paradigm and Local Info Initiative
  • Displaying local repeater frequency info on mobile radio front panels
  • Proportional Pathing for trackers
  • Very high density APRS planning example
  • the European New-EU Paradigm

    Fixing the APRS Network with the New-N Paradigm:

    Tragedy of the Commons: . APRS suffers the classic fate of all limited resources (as well documented since the 1830's See Tragedy). Whenever there is a balance between individual interests and the common good, human nature guarantees the overloading and ultimate demise of the common resource. In this case, APRS throughput. . This is easy to understand since the benefit of adding one more packet to the network always immediately benefits the SENDER, but the negative "cost" is spread over everyone else, and NOT the sender. . There is no natural solution, other than the establishment of "Golden Rules" to live by for all concerned.

    The APRS Golden Rule - The New-N Paradigm:

    By 2002, the APRS network in the USA was an inefficient conglomeration of legacy systems that were still evolving. see 2002 summary. . The New-N Paradigm began in Nov 2004 to streamline APRS for much better efficiency and much simpler settings for users. . The result has been exciting improvements everywhere it has been implemented. . The APRS network evolved over 13 years and by Nov 2004, it was time to abandon the obsolete settings causing tremendous RELAY-DUPE problems in the USA. . The fix was easy, all we needed were a few changed remote-sysop parameters at the digipeaters without even a trip to the site.

    Use WIDEn-N where N is appropriate for your area. We called this initiative the New-N Paradigm. . The changes simply boil down to one universal path recommendation for all users. . Use WIDEn-N everywhere and N should be 2 in most major APRS areas of the country shown below and 3 only in flat rural desolate areas. . That's about all there is to it. . But read on...


    See also Europe
    See also Australia/New Zealand


    New-N Paradigm SIMPLIFICATIONS:

    SUCCESSFUL APRS: The success of your local APRS is not how many stations you see on your maps, nor how far away, but how reliably your mobile or handheld or portable station can communicate with others in the local area. . There is a big difference and they are mutually exclusive. . This fundamental principal should drive everything we do with APRS in our local areas.

    RELIABLE APRS: Said another way, the more stations you see above about 60 to 100 or so in typical areas, the more packets you don't see due to collisions and the less reliable your network is for local real-time APRS use.

    FIXING THE 144.39 NETWORK: The New-N Paradigm not only changes some DIGIpeater parameters but also stresses USER EDUCATION that a local 1200 baud APRS network capacity is greatly reduced by each additional digipeater used. . The area covered goes up, but the capacity is reduced by half. . Typical areas where people use 2 hops with four or more digis, can only support about 60 to 100 or so users in its RF domain. . Conversly, if no digipeaters were used and eveyone could hear each other direct, APRS could theoreticlly support about 360 users on a simplex channel direct (with time slotting). . But because of many people using too many hops and bad paths that cause too many dupes for surrounding areas, some areas of the country are totally saturated with 10 times the amount of attempted packets with only the strongest and most abusive getting through. . Net reliability is miserable for those locals whose packets cannot even get into the local digi due to out of area congestion. . This is self defeating. There are many things wrong:

  • Lack of user understanding of fundamentals and severe limitations of such a small channel
  • Too many legacy path options due to obsolete paths making it hard to educate users
  • Too many collisions and lost packets due to too many Hops and too many duplicate packets
  • Software that does not place the health of the Network foremost in the eye of the user
  • Poor Digipeater settings (HID not off, UIDWAIT not 0, and bad packet timing, excessive paths)
  • Improperly formatted packets See live error list as captured on FINDU.COM.
  • Unrealistic user Expectations (expecting to see hundreds of stations for hundreds of miles. Can't happen on RF)
  • Failure to properly set up old PacComm "T" digs (see map) for WIDE2-2 support
  • Continued use of obsolete RELAY and WIDE paths that multiply the number of dupes. see how bad
  • DIGI ROMware that cannot be updated. See my wish list for future digi implementations.
  • Fractionalizing and network disentigration due to local sysop (well intended but inconsistent) hacks.

    FIX #1: Phase out RELAY and WIDE Paths (also eliminate TRACE, TRACEn-N):

    The single biggest improvement in the USA was simply getting users to stop using the obsolete RELAY and WIDE paths. (see why). . The obsolete RELAY and WIDE paths generated multiple dupes in the KPC-3 and PacComm and some other implementations because there is no dupe elimination for dupes heard from other digis. . These obsolete paths generated 3 to 5 times more load on the system than the comparable WIDEn-N path which has perfect dupe elimination algorithms. The fix was easy. Use WIDE1-1 in place of RELAY. (see The RELAY fix!) and WIDEn-N in place of WIDE.

    FIX #2: Make WIDEn-N Traceable:

    The original WIDEn-N system was not traceable, making it impossible to do any network assessment or management. . The New-N Paradigm made WIDEn-N traceable!. . (By eliminating TRACEn-N, Sysops can now move WIDEn-N support from the UIFLOOD parameter to the UITRACE parameter.)

    FIX #3: Use WIDEn-N everywhere. The New n-N Paradigm Solution:

    WIDEn-N is the most efficient APRS path, but it is vulnerable to out-of area QRM from user settings of large values of N. . Fortunately, under the New n-N Paradigm, existing digis now trap large-N abuse and greatly simplify user recommendations to simply one WIDEn-N path. . The New n-N Paradigm simplifies the APRS network to a few distinct digipeater types:

  • WIDEn-N ..- The basis of the New n-N Paradigm. They also support SSn-N for state nets (S overlay).
  • WIDE1-1 ...- Fill-In digis (where required only). Set these fill-in digis MYALIAS to WIDE1-1.
  • One-Hop .. - These digis force big-N packets to 1 hop in extreme density areas. (LA or Dayton for example)
  • PacComm . - These old "T" digi ROMS can still be used locally for up to WIDE2-2 support (with P overlay)

    Fix #4: THE NEW STATE SSn-N PATH FOR STATE OR SECTIONS:

    The New n-N Paradigm simplified to a traceable WIDEn-N as the most efficient APRS path. . This works well for small values of N in high density areas. . But sometimes fringe stations in the corner of a state, may need to participate in a state-wide net and need more hops, but do not want to QRM adjacent 2 or 3 neighboring states. For this reason, the New-N Paradigm also includes the SSn-N system. . SSn-N solves this problem for each state (or ARRL section in big states).

    With WIDEn-N support moved to the UITRACE parameter, this left the UIFLOOD process available to support SSn-N, where larger values of N's can be tolerated and can get to the far reaches of a state, but not QRM other states or users in other directions. . For example, a user in central Maryland can hit everyone in the state with WIDE3-3. . But those users in the panhandle and south, need maybe 6 hops to participate in the state wide net. . Using the path of MD6-6 will hit all the way to the ends of the state (about 10 main digis) but there will be no QRM to surrounding states. Conversly, if he had used WIDE6-6 instead, then those packers would QRM almost a DOZEN SURROUNDING STATES and over 140 digis in all directions! . Actually, the size of SSn-N doesnt really matter since it will hit every digi once in a limited area, and no more. See the example:

    UPDATE: The above left photo was typical of what we used to see on RF in the Baltimore area prior 2004 and the New-N paradigm. . To see how this mess has been reduced under 2 years of progress under the New-N Paradigm, see the Jan 2007 map.

    PATH TRACING USING THE SSn-N PATH: SSn-N (using the old UIFLOOD paramter at the DIGI sites), would not normally be traceable. . But if users use the path of WIDE1-1,SSn-N, then the path does become traceable at least with regard to the first and last digi used. . If DIGI Sysops enable SSn-N support using the command: UIFLOOD SS,30,ID, then these paths will be always traced with the FIRST and LAST digi in the path, no matter how many hops are taken. . This is a tremendous benefit for network management. . This packet arrives as DIGI1,WIDE1,DIGIn,SSn* showing the first and last digi used.

    UHF across SSn-N State Lines: if you live on a border town and want to always be able to see the other state's SSn packets, simply put up a cross band digipeater that hears the 144.39 SSn packets from the other state, but digipeates those to a local UHF frequency. . To see the other state's SSn packets, just tune to that UHF channel without any QRM to your local 144.39 operations.

    DIGIPEATER TNC Settings for the New n-N Paradigm:

  • KPC-3+ (plus) Version 8.3 and 9.1 Settings for WIDEn-N
  • KPC-3 Version 8.2 Settings for WIDEn-N
  • UIDIGI-ROM settings.
  • DIGI_NED PC-based software
  • PacComm TNC Settings . See a map of the Remaining Trace-only digis
  • Settings for a WIDE1-1 FILL-IN digi

    Fix #5, Labeling the New n-N Paradigm digis:

    The New-N paradigm also includes educating users. . THe biggest step is to be sure that every digipeater announces its capabilities to users. . Most importantly are the new S, L, 1 and P overlays for the new settings on the digipeaters. . The "S" fully support WIDEn-N and SSn-N for State or section routing. . The "L" digis are the same but are limited and do not support SSn routing, and the "P" digis are old Paccomm Trace digis that have been configured to support WIDEn-N. . One-hop digis in extremely high density areas (like in LA) and fill-in WIDE1-1-only digis will show a "1" to indicate they are an enforced 1-hop digis.

    SECONDLY, as part of user education, ALL digipeaters should show their New-N settings in the position comment text of the DIGI's beacon. . See the Details on Overlays and the proper form for the Position Comment Text.

    Fix #6, Proportional Pathing for Trackers:

    The original APRS design uses a Decaying Algorithm to send new data more frequently than old data, and make each later copy less and less often if the packet is unchanging. Most follow-on APRSclones, and trackers ignored this fundamental principal and transmit far too much duplicate unchanging info. . We need trackers to use direct and local 1 hop paths more often than 2 or 3-hop paths. . I call this Proportional Pathing. . It means that trackers will send at a ONE minute rate, but every other packet is sent LOCAL-DIRECT. . Every 2 minutes it goes via WIDE1-1. . Every 4 miuntes it goes via WIDE1-1,WIDE2-1. And if Proportional-Pathing is set to 3, then once every 8 minutes it will go via 3 hops using WIDE1-1,WIDE2-2. . This technique cuts the load on the network by a HUGE factor since high-rate mobiles with long paths is one of our biggest problems. . Also, this solves the problem of adjustments between areas. A setting of Proportional Pathing = 3 should be OK just about anywhere. . Fortunately, Kenwood included Proportional Pathing in the new D710 radio. See Proportional Pathing.

    TEMPn-N DIGIS for Emergencies and Field Day:

    APRS consists of over 1000 permanent digis across the USA. But there is a vast un-tapped resource of thousands of more digis that can be used in emergencies if needed. . These are the D-700 mobiles that can act as digis. . Normally we want all these mobile digis OFF to avoid added QRM on the network. But we need a way to use them if needed. . The Solution is to set these radios' UITRACE parameter to TEMPn-N permanently. . Because they are not WIDEn-N they normally will not digipeat anything. . But anyone, at any time, needing a path out of an area without digi coverage, can attempt a TEMPn-N packet to use any nearby D700 as an automatic digi. See the TEMPn-N page.

    TEMPn-N FOR FIELD DAY: Another advantage to the TEMPn-N system is the current ARRL Field Day rules which prohibit APRS unless a temporary digi is used for FD. . Instead of trying to re-configure all the digis for FD, we can now just use TEMPn-N because this temporary path could always be there!

    Finally a PICTURE of APRS User Density! :

    Look again at the map of user density below. Imagine concentric rings around the HIGH density areas. . To limit to only 2 hops in the RED areas, then digis in those areas must not support anything above WIDE2-2. . The next tier of digis out from these areas need to trap 3-3 and above packets. The next tier of digis out, has to trap 4-4 and above, etc. . And almost everywhere we need to trap 5-5 through 7-7. . Any area that needs big N's should solve the problem with more IGates, not longer paths.


    See also Europe
    See also Australia/New Zealand

    Remember, for each N that you drop, you improve the network efficiency by a FACTOR of THREE or more. So just getting trackers to cut from 5-5 to 3-3 will reduce their QRM by a factor of 9!. . Cutting from 3-3 to 2-2 will improve efficiency by THREE or more everywhere! Click to see statistics on above map.


    The remainder of this page is all the background that supports the recommendations above


    APRS FUNDAMENTALS: APRS can ONLY work at the local level on RF. It is only a 1200 baud channel shared by your nearest neighbors. . It can only work if you and your neighbors understand how it works and its limitations and you are not QRM'ed to death from packets from out-of-area. . The following table shows the BASIC ASSUMPTIONS about the goals of an APRS network:

    THE ALOHA CONCEPT: The 1200 baud 144.39 channel can only support an average user load of about 60 to 100 or so APRS stations or objects in an RF domain based on the typical transmission rates and number of digipeaters and number of hops. . See the breakdown and analysis. . This is because any greater load than 100% channel capacity guarantees lost packets due to collisions. . The size of your area that holds the number of users capable of generating 100% channel capacity we call your ALOHA circle. You are responsbile to make sure that your packets get to your surrounding ALOHA network but no further so you do not add QRM to other networks. ALOHA Circle concept.

    FIX #7: The ALOHA Circle:

    Every APRS software should calculate and display the ALOHA circle for its user. . It should be overlayed on every map so that it is never out of mind. . But even without the ALOHA calculator built-in, users can still get a good estimate from FINDU.COM. . Simply EDIT-COPY this URL into your browser with YOUR APRS station callsign on the end:

    http://map.findu.com/WB4APR-9 <= your call here

    That FINDU page sorts your 60 nearest APRS stations by range and so the range to the last person on that list is the radius (or range) of your ALOHA circle. . This list of stations is your APRS ALOHA Neighborhood. It also includes which digipeaters you may need to hit, to be able to communicate with them. . More importantly, your packets should not go beyond this circle routinely. . In Southern California, your ALOHA circle may only be 15 miles and you may only need ONE hop to hit everyone. . In WYOMING, you may need more hops....

    The ALOHA circle is automatic now in all copies of APRSdos (APRSmax after APRS871.zip). . See Map plot above. . There is also an add-on for UIview, and the next release of WinAPRS should have it too. . It computes and maintains a plot of the yellow ALOHA range circle on all map zooms. Around Baltimore it is about 45 to 55 miles depending on the number of mobiles at any time. . Also displayed below is the MAP-PLOT-HOPS command that shows a plot of the number of hops it took for surrounding digis to reach me. MAPS-PLOTS-USERS shows the same plot of user hops. . Notice that 2 hops will get one EVERYWHERE within this Aloha Circle even though there are 13 digis in that area!

    Note, that these PHG circles are the new half-size APRS standard which more closely represent a MOBILE's range. . The actual RF range of these digis to fixed stations and other digis is TWICE that shown above.)

    Fix #8: Alt-Input Channel on 144.99:

    Currently what your digi hears on its input is 98% from out of area, thus, you only get in when you overpower the distant QRM. . But this does not work for low-power devices. . The simplest local way to improve local reliability in the presence of QRM at the digi is to move local users to their own input channel such as 144.99 (+600 from .39) if available in your area which simply then cross digipeats back to 144.39 where everyone listens. This simple SYSOP solution can drastically improve local channel reliability! See how to Double local reliability with an ALT-channel input on your digi.

    Fix #9: TURN HID OFF IN THE DIGIs:

    HID OFF: . First turn HID OFF. . This ID packet is not an APRS format and uses the same path as the UNPROTO and goes out every 10 minutes if on. . This, plus a bad UNPROTO path of 3 hops generates almost 100 packets per hour per digi in the area. . But turning HID off and using the 4 LT PATHS and 4 BLT timings can reduce this kind of QRM by a factor of 4! . See digi-rates.txt. . The APRSdos heard display below shows the large number of dupes from digipeaters that have HID on, and that also are using the poor dupe-generating WIDE paths and not using the 4 BLT/LTP/LT settings for best digi efficiency.

    Fix #10: Properly set the Digi Beacon Rate:

    Please set the DIGI beacon rate as shown in digi-rates.txt file. . This results in a local packet every 10 minutes, but only one every 30 minutes at one hop and only one every hour at 2 hops. . This cuts DIGI beacon traffic load by half! . The HEARD display above shows how failure to use the smart beaconing method on the digis and using the old WIDE paths really generate lots of dupes.

    Fix #11: Update the PacComm "T" digis to support WIDE2-2 and change them to "P" digis:

    Please revise these PacComm Settings . The original PacComm TNC's back in 1996 gave us the first callsign-substitution capability in APRS. . We called these digipeaters "TRACE" digis and use an overlay T to designate them. But they do not support the much more efficient WIDEn-N type of routing and were holding back the ultimate improvement of our network in in some areas. . In all these areas, paths using RELAY and WIDE were still being used. . These cause from 3 to 5 times as many duplicate packets. . To prove this to yourself, capture an hour of packets from your TNC and then run the program download APRSTEST.EXE to analyze the results. Below is the result for the Baltimore area:

    Notice how 45% of all packets come from only 25% of the users using W,W,W paths. . Also notice how simply switching to WIDE2-2 is more than 5 times more efficient than W,W,W and twice as efficient as W,W! . But this can be fixed, by encouraging the new WIDE2-2 universal recommendation. . And the old PacComm digis can support this New n-N Paradigm and become a P digi by simply supporting WIDE1-1,WIDE2-2,WIDE2-1 and WIDE3-3 as ALIASES. (see the settings link above for more options).

    Fix #12: Update the very-high-hear-too-much digis:

    To make APRS grow, cell size must get smaller to keep within the ALOHA limits in any one RF area. . High digis can be good if the number of hops of all users is restricted. . But, in generally flat land, more users may require more, but lower digis, and restricting the number of hops. . If you can reduce what the tall-hear-too-much-mountain-top sites hear to only DIRECT packets (and no surrounding QRM) they can support over 100 users... See the very-tall digi problem in the LA basin in Southern California. . There are several options for the tall-super-site digis depending on your area:

  • Option 1: Simply trap all paths to 1 hop. (It can still be used for directed paths beyond 1 hop.) See the fix for Los Angeles
  • Option 1+ You should also reduce what all surrounding digis are re-transmitting as well.
  • Option 2: Move its RX to 144.99 (if avail) so that it has a clear input channel for low-power trackers
  • Option 3: Move its TX to UHF so it can still hear everything but wont QRM anything
    ........ Users can still listen to it on UHF or an IGate on UHF will still get everything

    WE MUST KEEP N SMALL: See how WIDE3-3 can hit most of VA, MD, DE and SE-PA in the above map. . These days, high density areas areas can only support WIDE2-2 and no more. . See the chart:


    click to see 3 digis.
    click to see 2 digis.

    We must cut the number of hops and simplify settings so that the APRS network works everywhere for everyone using consistent settings.

    We can fix it OVERNIGHT: by simply adjusting three of the remote sysop parameters for the ALIAS list and the two n-N distribution mechanisms in most digis. . UIFLOOD floods without being able to trace the path and UITRACE traces but with more overhead. . Choosing the optimum uses of these besides the original WIDEn-N and TRACEn-N and using the ALIAS list as a trap for large N paths, can drastically reduce out of area QRM overnight. . Here is what we can accomplish:

  • Eliminate the multiple dupes of the old RELAY and WIDE (and TRACE and SS) systems.
  • Encourage the use of WIDEn-N
  • Encourage lower values of N to reduce flooding QRM from out of area.
  • Change UIFLOOD from WIDEn-N flooding to the local State SSn-N or section communications
  • Move WIDEn-N to the UITRACE parameter so that all paths are traceable.
  • Use the UIDIGI ALIAS list to Trap WIDEX-X paths for large values of X but allow at least one hop.
  • Both of these put sysops in control of their networks and drastically reduce DX QRM independently of user settings!.
  • Capture and terminate any WIDE5-5 or greater paths everywhere or less, depending on local capacity.

    The User density map displayed earlier shows a first cut estimate of those areas that may want to restrict WIDEn-N to the number of hops shown. . See also the Maryland/VA New n-N plan and map.

    UNIVERSAL MOBILE PATH OF WIDE2-2: Although the path of RELAY,WIDE used to work everywhere, it generated from 3 to 5 times the number of extra dupes. . The better universal path now is WIDEn-N with N limited to 2 or 3 depending on area. . For areas with many fill-in digis, the path of WIDE1-1,WIDE2-1 can be used. Even the old Trace-Only (PacComm) digis can support this as shown above. Most Trace-only digi's are in the east See map of Trace-only digis

    WIDEn-N TRAPING OF LARGE N's: A key to the success of the New-N Paradigm was the realization that we can use existing digis to TRAP large values of N. . This is easily done by putting WIDE4-4, WIDE5-5, WIDE6-6 and WIDE7-7 in the digipeater's alias list. . These packets will be digipeated once, but will not be further propogated. . Users will learn that N's above 3 in most areas will not be digipeated further than one hop.

    ELIMINATE RELAY and WIDE: The old dupe-generating paths of RELAY, WIDE, TRACE and SS are being dropped beacuse of their poor dupe-elimination. . Dropping these cold-turkey is the best way to just get the job done. . The sooner the better.

    USER EDUCATION: The most important value of the New-N Paradigm is the great simplification of paths making universal APRS User education practical. . All the legacy paths before were just making it too dificult for the users. . Now it is simply WIDEn-N with small N. Done. The New n-N Paradigm tools are very powerful, but it still boils down to fundamentals. . Use only what will get you to your nearest 60 to 100 users. . Anything else is QRM.

    BENEFITS of the new n-N paradigm:

    WHAT THE USER SEES:
    The bottom line is what does the user see. . And this is the crux of the whole idea. In the past, we could not train the users because there was no single set of instructions that worked everywhere. . Every area was disintigrating APRS with local hacks that make it impossible to tell users what to use. . So my NEW n-N paradigm has as its whole obejctive to get APRS back to a single set of user parameters that will work everwyhere locally, yet still provide all the power of APRS for other applications:

  • GENERAL MOBILES:........ WIDE2-2
  • LOCAL MOBILES:............. WIDE1-1,WIDE2-1 (if there are FILL-IN digis in the area)
  • HOME STATIONS:............ WIDE2-2 (or 3-3 in eastern USA distant rural areas)
  • STATE OPERATIONS:...... WIDE1-1, SS3-3 as needed

    OFF-LOADING WIDEn-N TRAFFIC:

    For areas that still want to see distant traffic into other SSn-N's or larger DX N's of traffic from all over, it is easy to terminate adjacent OTHERn-N traffic from outside your area into UHF where it enters your area. . Then, anyone who is interested, or IGates or other processes can tune in the OTHERn-N traffic as needed as shown in the sketch below. All it takes is a typical TNC set to digipeat the OTHERn-N traffic it hears on 144.39 and transmit it to a local UHF freq. Done.

    The 2004 image below shows how 50% of the digis in the mid-atlantic area were NOT WIDEn-N and so in general, we were suffering from the severe DUPE problem of using the old RELAY and WIDE paths. . But this is rapidly changing as eveyrone endorses the New n-N Paradigm.

    Collisions and Lost Packets: There is no way to know the reliablity of your network from general statistics of packets heard, because you cannot tell what you DON'T HEAR! . A channel that is 800% overloaded and only passing 1 out of every 8 possible packets can sound identical to one that is 50% loaded and passing 100% of every packet for everyone... SO, one the only way to really measure actual performance by using "probes". . Probes are simply known packets at known rates from "intended user stations" in the "intended areas of coverage" that tell you exactly the performance of your network. . See PROBES or PHGR. To implement this, we simply add one byte to the existing PHG construct. We call the result PHGR.

    THE ID/NOID ISSUE: Another thing that was quite broken in the old APRS network was the inconsistent setting of the ID/NOID parameter. . This determined how a WIDEn-N packet appeard on receipt and whether or not the INITIAL or LAST digi was identified. . Just seeing a digi listed it was imnpossible for anyone but the digi owner to know which it meant because only he knew the setting of the ID/NOID parameter. . For years we tried to get it set to NOID so that the FIRST digi could be identified by using the path of WIDE,WIDEn-N. . But this causes dupes. . Now, we solved this problem by moving WIDEn-N support to the TRACE parameter so all WIDEn-N paths are now traced.

    Further UIFLOOD is now used for SSn-N and we can enforce tracing bby setting ID to ON so that the 1st and last digi are indentified if users use the path of WIDE1-1, SSn-N. . This packet arrives as DIGI1,DIGIn,SSn*. For a historical persepctive you may read about the ID/NOID problem.

    NEW ##LNKn-N INTERSTATE BACKBONES: (OBSOLETE) This was a great idea to limit damage done by large values of WIDEn-N but still allow long-haul linear paths, but as a 3rd n-N system, it cannot be supported in most TNC's and is there fore generally OBSOLETE. . Also it would have taken considerable coordination which is not likely... . This system used the UIFLOOD parameter for creating linear strings of digis along a long-haul interstates using the path name of ##LNKn-N. . This could eliminate abuse since a packet can only go one direction. A 90LNK7-7 packet for interstate 90 only generates 7 copies of the packet along Interstate 90 compared to almost 200 packets for WIDE7-7. . THus it reduces QRM by an order of magnitude and the NETWORK limits the damage instead of being dependent on user education. . See A graphic example of possible LINKn-N systems through Virginia and a suggested (obsolete) list of all ##LNKn-N chains.

    THE APRS-INTERNET SYSTEM: The original (and present) purpose of APRS is to be a tactical real-time local digital communications system for reliable, quick exchange of important local information. . Although in 1997, Steve Dimse and Sproul Brothers began the APRS-IS (Internet System) to glue it all together, nothing in the APRS-IS detracts from that local definition. . The Internet simply allows distant stations to observe such local activity, yet provides connectivity to the global reach of APRS messages. . Thus, to some people, just making the nearest IGate is sufficient for the majority of their conectivity needs.

    So, how far is any station from the nearest Igate?

    The image below shows the number of hops to an Igate for all of California. . Notice that MOST stations are only ONE HOP or less from an IGate and almost everyone is within 2 hops!

    Click here for statewide map

    ALOHA NETWORKS: APRS is a random network based on random transmissions of data among many users trying to share a channel. . This technique was well studied back in the 60's and is called an ALOHA network for where it was first developed at the University of Hawaii. It is the basis for most data networks which evolved into what we know of as the ARPANET and now the INTERNET and other protocols. . Click for the original definition of an ALOHA system.

    Basically the channel must be quiet most of the time, so that a sender will have a good chance of a successful transmission. . You can add more and more users, but eventually you get to the point that adding more users only adds more collisions, and the net reliability goes down drastically. . If you add up the statistical load of about 60 or so APRS users, their packets equal a 100% busy channel. . Any more and the network suffers. So, how many users are there in range of your digi?

    If your digi hears too much then its reliability for local users is poor!
    In this context, LOWER is BETTER (just like CELL phones have grown, by going to smaller and smaller cells!).

    CHECK YOUR DIGI: Here is a list of all digis in the world heard by FINDU in Dec 2004. . It is surprising how some of these digis appear to hear so many stations direct. If your digi and its neighbors actually does hear over 150 DIRECT, then the best way to prevent channel saturation is to implement the New-N Paradigm and have surrounding digis limit the number of hops and by all means to eliminate the obsolete RELAY and WIDE paths. . Not limiting the QRM by these techniques is a good indication that reliability of low power and distant users will suffer badly. . The RANGE shown here is computed from your PHG values. . If they are unrealistic, consider reducing the PHG numbers to better match reality. . Remember to use Height-Above-Average-Terrain and not just the "altitude" of the digi:

  • The Dec 2004 Digis List sorted by Number of Users
  • ALL digis as of Dec 2004 sorted by PHG range.
  • sorted alphabetically.
  • The Jan 2003 BIG Digis List

    Of course, these numbers are inflated due to a number of non-RF stations that also get counted but it is representative. . Best to look at exactly what is in the footprint by going to map.findu.com and looking at the nearby stations to see what exactly is there. . If there are that many RF users in range, then the APRS community in that area must add limits to n-N traffic to reduce the hearing range of these big digipeaters to better serve their local users. . Here are a number of things you can do:

  • First get everyone to use WIDE2-2 or less
  • If there are nearly a hundred users in range of one digi, consider enforcing only 1 hop through that digi
  • Consider switching the input of the BIG DIGI over to 144.99 (if available in your area) to hear low power trackers.
  • Or switch the output over to UHF so that its capacity can double. . (Users monitor the UHF output)
  • Measure your own reliable local network range using his own ALOHA-Circle and reduce his path to match it.
  • Add more LOW-LEVEL local digis, or digipeat across town through a neighbor (who doesnt hear the QRM the digi hears)
  • Ignore big N WIDEn-N QRM at your digi with the new State SSn-N and large N ALIAS TRAPS of the New n-N paradigm.
  • Convert high-site digis (that hear too much) to UHF backbone operations. (See below)
  • Make sure there is an IGate within the footprint of most high density digis
  • for the UHF outputting high-site digis, add a UHF receiver at the local IGate
  • Mark all PERMANENT Igates with the "GATE" with an "I" overlay so everyone can see which Igates are permanent

    APRS Channel Throughput:

    The above screen capture of the APRSdos program called SIMULATE.BAS shows how this program can be used to simulate the throughput on any kind of ALOHA channel. . In this example it shows how 85% of the 40 stations all with a brand-new packet of information will be successful in getting at least one successful digipeat of that new information in the first 8 minutes. . This example caused about 280 packets to be generated using the APRSdos decaying algorithm to decay the retry-time after each attempt so that new data is transmitted more often, and old data decays down to much lower rates to preserve channel capacity.

    Many popular APRS systems, unfortunately, use a constant transmission rate of X packets every Y period of time which results in a DOUBLING of QRM (over 480 packets) being generated for only a 2% improvement in throughput over the same 8 minutes.

    UHF BACKBONE SOLUTION!:

    See the all-new SUPER-LAN CONECPT that has evolved into its own WEB page due to recent discussions and development on the APRSSIG. . The rest of this page was incorporated into this new page...

    In areas where High-Site digis are hearing far too many packets, is to convert those digis to output only on a dedicated UHF frequency. . This instantly doubles throughput by going duplex, but even more importantly it can gain up to an order of magnitude improvement through how it listens to 144.39. . See the original BACKBONE plan. . But remember that we think it is now easier to start not with a BACKBONE, but with a centrally located 9600 BAUD SUPER-LAN CONECPT since it only takes one person to do it, instead of a lot of multi-site coordination..

    The following sketch suggests how such a high digi can be converted to UHF in one major metropolitan area and can still communicate to another adjacent Metro area, but without burdening 144.39 and without any new logic other than the same kind of processing already standard in any IGate:

    The above backbone assumes that a single central site can hear all the smaller-lower digis in a mstropolitan area. . But this concept can be extended to numerous such high site digis as in the following diagram. . Here, three high-site digis can all hear over a dozen lower-local digis, yet they can still share all packets on the backbone using a single 9600 baud data stream:


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    The Naval Academy is a registered user of APRS and WinAPRS. . The purpose of this web page is to show several applications currently in use at this site and should not be considered as an advertisement or an endorsement of any commercial product. WA8LMF Mirror of WB4APR Website - 21 July 2008