North American MW Coverage Maps

USA, Canada AM radio antenna patterns

Many MW broadcasters use antennas with directional radiation patterns in order to focus their signal on to a particular geographical area. This serves two purposes. Firstly it avoids radiating an expensive signal in a direction where there are few listeners. Secondly it avoids beaming a signal towards another station where listeners might experience interference between two signals. Thirdly a directional radiation pattern allows a station to focus its energy on a distant target audience.

Background to antenna patterns

Radio engineers have known for many years how to create broadcasting antennas with a directional pattern but they inevitable are more complex and expensive than a simple antenna that radiates omni-directionally (i.e in all directions). These antennas also need careful maintenance to maintain their design performance.

In countries like the USA there was huge growth in demand for AM radio stations in the 20th century. The challenge was to ensure that 50kW “clear” channel stations could co-exist with 1kW small town stations without filling the MW radio dial with lots of mutual interference. Directional broadcast antennas have been in use from the early 1930s and today many sophisticated antenna arrays exist across North America, and to a lesser extent on other continents.

Inevitably the use of directional radiation patterns came to the rescue and enabled the growth of MW broadcasting. Today there are around 5000 AM stations operating in the MW band in North America.

What is a directional pattern?

At its simplest, a broadcasting antenna radiates its signal equally in all directions like the diagram for KOA in Denver Colorado. In practice local terrain and obstructions can influence the real radiation pattern, making it not quite circular. Maps usually show two contours which mark the limit of strong signal and weak signal reception.

KOA 850kHz Denver, Colorado – daytime omni-directional coverage map

Directional radiation patterns involve more complicated antennas to generate a desired radiation pattern. An example is WBBR 1130kHz which at night beams most of its signal east to avoid causing co-channel interference west of New York. DXers in Europe benefit from this and the map shows why reception of WBBR is frequently possible on portable radios or car radios in the UK.

WBBR 1130kHz New York – night-time coverage map

Other directional patterns are designed to target a specific audience. Although WAQI 710 is a Spanish language radio station licensed to Miami its radiation pattern reveals where its target audience really is located!

WAQI 710kHz Miami FL – daytime coverage map

Impact on DXers

If you are DXing you might assume that what seems to be a high power station would be any easy catch. But the total radiated power is only half the story. What really matters is the amount of power actually being radiated towards your receiving antenna. There are examples of stations radiating 50000W in total which have radiation patterns that reduce the effective radiated power in certain directions to as little as 50W.

Many broadcasters change their antenna radiation pattern between night and day (this often coincides with a change in transmitter power as well). Some even have a third pattern used during “critical hours”, i.e. during the transition between day & night.

You can take advantage of changes in power and changes in broadcast radiation pattern to hear a particular station – sometimes for only a brief period of time. But of course this is only possible if you have accurate up to date information at your fingertips.

Sometimes anomalies arise which can be of great interest to DXers. There are circumstances where a station fails to use the radiation pattern it is supposed to. For example a station might accidentally or deliberately use its daytime pattern at night. This is can create a short-lived opportunity for the dedicated listener to hear an otherwise inaudible station. These opportunities can be deliberate due to a pre-arranged DX test, or planned antenna maintenance. Or they can be unexpected as a result of equipment failure, storm damage or vandalism.

Data Source

In the USA fortunately the technical specification of every MW radio station and their antennas is made publicly available by the Federal Communications Commission (FCC). All this data is available online via the FCC website. However the data is not in a format that is helpful to the DXer.

Mapping tool

It’s one thing having data, but quite another turning it into something useful. We are pleased to say that Bill Scott has done a fantastic computer programming job to make this data valuable. He has created a tool called Radio Data MW (RDMW) which uses the FCC and other data to map the radiation pattern of every MW station in the USA and Canada. And then he has integrated this with Google Maps for your benefit.

That means for every MW channel in North America you can see a map showing the radiation pattern of every station. You can view the whole continent or zoom in to great detail. In fact you can zoom in and actually see the antenna masts!

In fact for every MW channel Bill has created two maps: daytime and nighttime supplemented by 44 maps showing critical hours. In total there are 280 maps.

Daytime maps

The daytime maps show expected ground-wave coverage patterns at two levels, out to the 1.0mV/m and 0.1mV/m field strength contours (60 dBu and 40 dBu respectively). These levels were chosen to closely match those which might be helpful to the MW DXer. For daytime signal maps, Radio Data MW generates a real pattern plot based on transmitter power, antenna array efficiency and directivity, ground conductivity and ground dielectric constant of the path to the receiver. Increased conductivity of water paths over the Great Lakes and the oceans are also accounted for. It is exceptional to find a program that takes all these factors into account.

Nighttime maps

Nighttime maps show expected skywave coverage patterns. These represent the standard SS+6 (sunset plus 6 hours, or approximately midnight Central Standard Time), 50% signal probability of 0.1mV/m (40 dBu) field strength. Note also that nighttime reception of signals out to and beyond the depicted pattern is very possible, and in fact quite likely for a skywave signal. The maps represent a signal strength at the fringe level. Bill chose this signal level to give a good representation of what is possibly received by most DXers on an average evening. For skywave signal maps, predicted signal levels are calculated in accordance with current FCC or ITU methods of recent years (1999 onward).

Other features

Bill has added a feature where you can trace a path on the map from transmitters to your listening post. This shows the great circle path that the signal would take and also reveals the relative signal strength radiating in your direction. And with a map at hand showing the traces you’ll quickly see which signals might be audible at your location. The example below shows how stations on 870kHz could propagate to the UK. A UK-based listener could easily see which stations might be affected by polar signal absorption and could also see where to point their receiving antenna for best reception.

We have created 6 regional editions in which a default receiving location has been pre-programmed to simplify ray tracing to your part of the world. However you can always enter any latitude and longitude to represent any receiving location and get the program to redraw the map for you. If you are more interested in coverage maps than ray tracing to a receiving location outside the USA, then you should opt for the US Edition because the continental US appears as the default map.

Furthermore, if you hover your mouse/pointer over any station flag pin it will show you the calculated great circle distance (km) from your listening post to the radio station’s antenna.

Map showing the direct path from every station on 870kHz to a receiver in York, England

Download “Radio Data MW

Now that most people have broadband internet connections we can distribute Radio Data MW via the internet from the Circle website. You can order your personal copy by clicking the shopping cart button below.

For only £3, ~€4 or ~$4.50** you can have your own copy. You can pay with a Debit or Credit Card. Payment is through a PayPal gateway and is safe and secure. You do not need a PayPal account to use this facility. If you don’t have a Paypal account or have one and don’t want to use it then you can use the Paypal guest check-out where you can enter credit/debit card details. Prices are given in UK Sterling with approximate Euro and US Dollar equivalents. Paypal will convert to your home currency automatically. There is no surcharge for payment by PayPal.

Purchasing online is safe and secure using the Paypal gateway and you always have protection provided by Paypal and/or your credit card company. We do not collect or store any of your payment details.

Please respect the copyright of the content and do not reproduce, replicate or transmit the content in any form to anyone else; this program is intended for your own personal use. Commercial use is strictly forbidden!

Thanks to Bill Scott the creator of Radio Data MW for giving permission to include his hard work & creative efforts here.

IMPORTANT: After payment is complete click the “Return to Seller” or “Return to Merchant” button and you will be directed to a page from where you can download Radio Data MW. Please note that this is delivered as a 60MB zip file to your computer or smartphone ready for you to enjoy immediately.

Just select your option and click your (one) preferred button below. (The editions show their default receiving location; they are all identical apart from the default receiver location.)

British Edition
54.00N 2.50W
   
Central Europe Edition
47.59N 7.59E 
   
Southern Scandinavia
57.78N 14.16E   
   
Arctic Scandinavia
66.57N 23.85E 
   
Japan
36.65N 138.19E 
   
USA 
39.83N 98.58W 
   
New Zealand 
-40.92S 175.27E 
   

** your payment contributes to the cost of bandwidth, our servers and the maintenance and security of the Circle’s website – thank you!

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