Skip to Main Content

Audio Eclipse May Fill the Sky

Pin it
return to NASA Science News
Space Science News home

Audio Eclipse May Fill the Sky

Hams around the world can track the August 11, 1999 total solar eclipse by monitoring changes in atmospheric radio propagation.

Aug 7, 1999: UPDATE - A special transmission of the BBC World Service will be broadcast from Rampisham, England near the path of totality to assist NASA efforts to monitor atmospheric radio propagation conditions during the eclipse. [details]

August 4, 1999: During a total solar eclipse, day becomes night for a few precious minutes. The temperature drops, birds stop singing, and bees return to their hives for a premature rest. An eerie quiet envelopes the landscape inside the path of totality.

However, from the unique perspective of a ham radio operator, night is anything but quiet - and neither is a solar eclipse. Many shortwave radio stations that are undetectable in daytime are easy to pick up at night. The reason has to do with the Sun's effect on Earth's atmosphere. During the day, solar UV radiation ionizes atoms and molecules in the upper atmosphere, creating a zone called the "ionosphere." The uppermost part of the ionosphere, called the F layer, is so thoroughly ionized that some free electrons exist there - even at night - when the UV source (the Sun) is not present. The F layer is like a mirror for radio waves with frequencies below about 20 MHz. Shortwave transmissions from earth hit the F layer and bounce back down. In fact, many such bounces can occur, and this is the reason why over-the-horizon transmissions are possible at short wave frequencies.

Interestingly, the ionosphere -- so important for long distance radio communication -- can also reduce the energy in radio waves. In the D and E layers the degree of ionization is not as great as in the F layer. Partial ionization cause these layers to act more like a resistor than a mirror. Short waves passing through them are attenuated rather than reflected. Signals at some frequencies are damped out altogether. Fortunately, the level of ionization in the D layer is small, and when the sun sets at night, all the molecules and free electrons can recombine, and the D layer disappears! Stations that were damped out during the day can then propagate around the world.

This well-known atmospheric cycle takes place every day. On August 11, 1999 it will happen twice.

As the path of totality slices through Earth's atmosphere, ions and electrons in the vicinity of the shadow will begin to recombine. The reflecting F layer may not be greatly affected, but ionization in the attenuating D layer could vanish. Shortwave radio stations that were restricted in range to sites in Europe just moments earlier may be able to skip over the horizon and be heard on the other side of the Atlantic.

Solar Disk Jockeys

Scientists at NASA/Marshall are putting this phenomenon to the test by inviting Science@NASA readers to become "Solar Disk Jockeys," who will report the effects of the August 11th solar eclipse not by watching for it, but by listening for it. Since England and middle Europe offer unpredictable visual conditions, the audio eclipse may prove the most reliable observation, particularly when heard from thousands of miles away.

The BBC World Service will be a good choice for many radio listeners. BBC transmitters are located mostly in the UK relatively near the path of totality, and they transmit at frequencies between 5 and 15 MHz that are favorable for probing changes in the D-layer. The table, below, shows BBC frequencies and suggested monitoring times. European Voice of America transmitters may also be suitable. A list of VOA frequencies for Europe is given at http://www.voa.gov/europe.html.

Time (UT), August 11 Frequency(s) kHz  Site(s) Target of Broadcast

 09-1000
7325, 15190 Rampisham (special broadcast), Ascension N America, S America
10-1100 5965, 6195, 7325 Sackville, Antigua, Rampisham (special broadcast) N America, C N America, N America
11-1200 5965, 15220, 15190, 6195, 5975 Sackville, Antigua, Ascension, Cyprus, Greenville N America, Americas&Carib, S America, C N America (begins 11:30 UT), C S America
12-1300 9515, 6195, 15220 Sackville, Cyprus, Antigua N America, C N America (begins 12:16 UT), N C S America (begins 12:16 UT)
13-1400 15220, 9515, 6195 Antigua, Sackville, Cyprus N C S America, N America, C N America

Above: This table lists some short-wave frequencies for the British Broadcasting Corporation (BBC) world service. The table suggests the times (in Universal Time) when hams may detect the clearest transmission during the eclipse event. Note the target of transmission - we suggest selecting a target closest to home. European Voice of America transmitters may also be interesting. Ham operators should experiment before August 11 to select frequencies to log during the eclipse. Click for a more complete table showing times and targets of BBC shortwave broadcasts (including worldwide targets) during the eclipse. (Source of information for tables: Dan Ferguson, Spectrum Management Division, International Broadcasting Bureau)

Interested readers should use their shortwave receivers to experiment with different stations. The best ones for eclipse listening will be transmitters that can be heard at night, but not at all during the day. The eclipse will begin over Europe around 10:10 UT when it is still night over most of North America. Thus, when the daytime ionosphere begins to diminish over Europe, there is a good chance that European shortwave broadcast stations will be able to propagate great distances into the Western Hemisphere.

Recording useful data is easy: Simply note the following information: The station's signal strength as displayed on the receiver's S meter at night and during the local time of the eclipse for a week centered on Aug 11. Then email your logs, your audio recordings (if any), and your position (latitude and longitude) to Marshall Space Flight Center's Eclipse mailbox. The data will be analyzed to help determine ionospheric properties, and used for a future story from Science@NASA.

Special Live Audio Webcast

Thanks to the assistance of the International Broadcasting Bureau, the UK's Merlin Communications is joining forces with Science@NASA for a special broadcast of the BBC World Service to probe atmospheric conditions during the eclipse. The transmitter is located at Rampisham in southern England (50o 48' N, 2o 38' W), not far from path of totality. The 500 kW signal will be broadcast at 7325 KHz over a 4x4 curtain antenna with a 30 deg horizontal beam width. The antenna will be pointing toward 285o azimuth, approximately in the direction of Washington DC as viewed from Rampisham.

Transmission times:
  • regular evening show at 2:45 to 3:45 UTC (10:45 p.m. to 11:45 p.m. Central Daylight) braodcast daily
  • special broadcast: August 10 0900-1100 UTC (4 a.m. to 6 a.m. CDT) the day before the eclipse
  • special broadcast: August 11 0900-1100 UTC (4 a.m. to 6 a.m. CDT) during the eclipse!
The special broadcasts on August 10 and August 11 will be replayed in near real time at EclipseCast.com


Right: A map of the expected changes in radio MUF (maximum usable frequency) caused by the August 1999 solar eclipse. The striking aspect of these University College London simulations is that the changes are global, not local to the path of totality. With times shown at top, the numerical simulation, performed by University College, London, will be used to support a collaborative experiment between UCL and the Rutherford-Appleton Lab, in which radio signals between Spain and England will probe the eclipse on selected MW frequency and radios tuned by the public. [more information from Rutherford-Appleton Labs]

"A total eclipse of Sun is about as close to a controlled experiment as atmospheric research can hope for."
Marcos A., Penaloza M.,University of Essex, Institute for Environmental Research

The possibility of "listening" to the August 1999 eclipse from afar has more than novelty value. Scientists are interested, too, because the results of a global monitoring experiment could give them new insight into the physics of the upper atmosphere.

Educators!
visit Thursday's Classroom
Please visit
Thursday's Classroom
for lesson plans and activities related to the August 11, 1999 total solar eclipse.
As the Moon's shadow moves across the earth the temperature in the upper atmosphere will drop, changing the wind pattern as air contracts in on the eclipse region. In the absence of UV radiation from the Sun, the ionosphere rapidly begins to decay. The shadow of the moon races through the atmosphere at supersonic speeds, causing wind and waves of electron-ion recombination to spread through the atmosphere from the eclipse region. The effects could be global.

All of these phenomena have been predicted by theory, and some have been observed during previous eclipses. On August 11, European scientists and amateur radio operators will attempt to refine physical models of the ionosphere by attempting to monitor changes in the D layer absorption of radio beacons. The public is invited to participate (see "related links" below).

Theoretical physics will benefit from an improved understanding of the ionosphere, and so will radio broadcasters. In many atmospheric models the attenuation of the D layer is overestimated, with the result that radio transmitters are often operated at a higher power than necessary. This, in turn, costs money, wastes energy, and pollutes the already cluttered airwaves with more RFI (radio frequency interference). Improved models of radio absorption in the ionosphere could lead to lower power broadcasts during much of the day.

"With the measurements of absorption obtained during the eclipse, scientists and engineers hope to have a better understanding of the nature of the ionospheric absorption which may ultimately lead to less interference in the future." (quote from Rutherford-Appleton Lab, UK.)


Calling All Solar Disk Jockeys

For sky watchers in North America and other areas not touched by the path of totality, August 11, 1999 offers a unique opportunity to sense the eclipse from a distance (or perhaps from beneath a cloud if you live in Britain). Science@NASA encourages readers to tune into the eclipse using shortwave radios and to report their results for scientific analysis. Reader suggestions concerning appropriate frequencies and observing procedures are welcomed and will be distributed to other "Solar Disk Jockeys" prior to totality.

Science@NASA will need the following information for a meaningful record of observations.

a) the frequency of the radio station(s),
b) the station's signal strength(s) as displayed on the receiver's VU meter at night and during the local time of the eclipse for a week centered on Aug 11,
c) your location (latitude and longitude).

Send these logs and your audio recordings (if any) to Marshall Space Flight Center's Eclipse mailbox. The data will be analyzed to help determine ionospheric properties, and used for a future story from Science@NASA.

For more information about the August 11, 1999 solar eclipse, please visit Goddard Space Flight Center's Solar Eclipse home page.

External Web Links

Radio frequencies reference - Voice of America's European stations
Project for study of Atmospheric and Ionospheric effects - prepared by Marcos and Penaloza at the Institute for Environmental Research Central Campus. England, U. K.

Rutherford-Appleton Laboratory (UK) research on eclipse effects:

Upper atmospheric research during the eclipse - R.A. Lab's home page for the upper atmospheric research during the Aug. 11 eclipse
Temperatures in upper atmosphere - Temperature variations at 240 km during an eclipse
Wind patterns - Atmospheric winds during an eclipse
Wind and Waves - in the ionosphere during an eclipse
Public participation - Public opportunities, through R.A. Lab to participate in measuring eclipse effects

Links & References

Further reading: [1] Journal of Atmospheric and Terrestrial Physics Volume: 38 Page: May 1976 Meisel, D. D. (New York, State University) Duke, B. (Canadian Broadcasting Corp.) Aguglia, R. C. (Buffalo Museum of Science) Goldblatt, N. R. (Rochester Institute of Technology) p. 8

[2] Kolokolov, L. E. Legen'ka, A. D. Pulinets, S. A. (IZMIRAN) Geomagnetizm i Aeronomiia Volume: 33 Issue: 1 Page: p. 49-57. Feb 01, 1993

[3] Zaitseva, N. A. Elanskii, N. F. Matveev, A. D. Vartanian, V. A.Meteorologiia i Gidrologiia Page: 45-50 Jun 01, 1984

More Space Science Headlines - NASA research on the web

NASA's Office of Space Sciencepress releases and other news related to NASA and astrophysics


Science Notes from Previous Eclipses

A multifrequency sounding experiment bounced high-power radio waves off the Earth's atmosphere during the July 10, 1972 eclipse, and a research team led by New York State University and the Canadian Broadcasting Corporation found: "A definite correlation of very low frequency (VLF) phase, high frequency (HF) signal strength, and geomagnetic field behavior on eclipse day."

For the March 18, 1988 eclipse, a vertical sounding experiment bounced signals between Japan and Russia and indicated that the uppermost layers of the ionosphere (the F2 layer) changed "only 30-35 minutes after the maximal phase of solar eclipse." But little to no weather change was indicated "during the solar eclipse of July 31, 1981", either for atmospheric temperature or ozone.

BACK TO THE STORY

 


flash!Join our growing list of subscribers - sign up for our express news delivery and you will receive a mail message every time we post a new story!!!
More Headlines
For more information, please contact:
Dr. John M. Horack , Director of Science Communications
Author: Tony Phillips
Curator: Linda Porter
NASA Official: M. Frank Rose