Very Low Frequency AstronomyOr how to observe at work on a cloudy day!
The Radio Spectrum
D Layer
E Layer
The Ionosphere
•VLF are opaque to the ionosphere
Therefore VLF Astronomy is by its nature an indirect method of observing
Quiet Sun
Low level of Sky-wave signal Vs. ground-wave
At Night
Erratic level of Sky-wave signal Vs. Constant ground-wave
Active Sun
High level of Sky-wave signal received during flare
Most people think radio astronomy think is complicated
Colin Clements 4Ghz Radio Telescope
But it doesn’t have to be...
Radio Equipment
Receiver Recorder PC
Antenna
Larger the betterMore turns the
better
I have three128 turns 400x400 square
tuned antenna25 turns 600mm Diameter
circle un-tuned150 turns 600mm diameter
circle untuned
Receiver Two approaches
1. radio receiver tuned to a specific station, outputs signal strength
2. PC sound card
RecorderTwo approaches
1. Data logger2. PC
My UKRAA VLF ReceiverAntenna
Aerial Tuning Unit
Receiver
Data logger/controller
Starbase Observatory Software
My Natural Radio Spectrum Set-up
Soundcard
Antenna
SpectrumLab FreewareRunning on an old laptopWin98 (first Edition)192MB RAMPentium II 400MHz processor6GB Harddisk
Live power spectrum, peaks are radio transmitters
Waterfall shows how the power changes with time
Up to 100 plotters can be set to record the power at specific
frequencies / bands of frequency
Radio Stations
• 19.6kHz GBZ, Anthorn,UK• 20.27kHz ICV, Isola di Tavolara, Italy• 20.9kHz FTA, Sainte-Assise, France• 21.75kHz HWU, Rosnay, France• 22.1kHz GQD, 22,.1kHz Skelton, UK• 23.4kHz DHO38 Rhauderfehn, Germany• 24Khz NAA, Cutler, Maine, USA• 37.5kHz, NRK/TFK Grindavik, Iceland• 62.6kHz, La Regine, France• 81kHz, Inskip, UK
VLF receivers currently
monitored
Recording & Interpreting Results– Amplitude of event
• Corresponds (usually) to the flare class, but will be specific to conditions and observer
– Start, Peak & End of event• Recorded as an importance level
Class Energy
X 10-4-10-3W/m2
M 10-5-10-4W/m2
C 10-6-10-5W/m2
B 10-7-10-6W/m2
A 10-8-10-7W/m2
Duration Importance
<18 min 1-
19-25 min 1
26-32 min 1+
33-45 min 2
46-85 min 2+
86 – 125 min 3
>126 min 3+
A text book SIDImportance = 2+2011-02-2812:46 – 12:54 – 13:48Corresponded to a M1 event
Increasing Energy
Typical Quiet Day
Transmitter is turned off at 07:00 – 08:00 every day
SID
Raw Data can be a little confusing
Removing signals after sunset and the signals that are not showing useful information can make it easier to
see what is going on.
SIDs come in many shapes
Res
ult
s
Next Steps for VLF
• Get laptop set-up in shed and connected via wifi to main PC
• Get lap-top controlling UKRAA controller• Build VLF set-up for CMHAS observatory• Experiment with different antenna
configurations• Automate logging and access via web
Future Projects for Radio Astronomy
• Meteor Detection• Solar activity monitor (21Mhz)• Radio Jove (21Mhz)• Radio Imaging