System Under Maintenance / Upgrades from July 19, to July 25, 2017
Installing new receiver matrix
Please expect some interruption to normal service
The above real-time trace is updated every 60 seconds and shows meteors detected over the presceding two minute period.
Time is shown as Universal Coordinated Time (UTC) which is an intenational time standard equivalent to GMT. This avoids regional confusion with local time zones.
"This Hour" is the number of counts since the beginning of the hour. "Prev Hour" is the number of counts in the last full hour. "PHR (15 min)" is the "present hourly rate" based on a 15 minute sample.
The graph shows hourly counts throughout the last 24 hour period. Click on graph to see larger image.
Meteors Last 24 hours (Click for larger image)
When a meteor strikes Earth’s atmosphere it decelerates rapidly. The friction created by the air causes the meteor to burn up at extremely high temperatures creating the white “shooting star” that we are all familiar with. This process also ionises the atmosphere along the trail making it possible to reflect radio waves.
Utilising a high powered VHF radar signal sent into the sky, we are able to detect reflected waves from these ionisation trails. Because the meteor is moving very fast, the reflected signal is shifted in frequency, by an amount according to it’s speed. This Doppler shift is also heard as an audible ping by the station operator.
Our system translates the reflected wave into three main parameters - Amplitude (strength), Frequency shift (Doppler shift) and decay time. This allows us to determine the relative size of the meteor strike (vertical scale) and the relative approximate speed and deceleration (width of the trace).
You can see the output from our system above in real time. the graph shows the presceding one minute period. During a meteor shower this trace will be full of meteor strike traces, but it is also surprising how many meteors are striking Earth’s atmosphere all of the time.
Typical Meteor Strike
Here you can see a typical meteor strike. The trace starts high in frequency (right of graph) and rapidly drops to the radar carrier frequency as the meteor decelerates in the atmosphere, increasing in strength (ionisation) as it burns up. This creates this typical triangular shape you can see here. The width, height and shape tell us a lot about the meteor strike. The blue is the baseline atmospheric noise.
Meteor Showers in
- Quadrantids - January 3rd
- Lyrids - April 21/22
- Eta Aquarids - May 5/6th
- Perseids - August 12th
- Orionids - October 21st
- Leonids - November 17th
- Geminids - December 13th
These are the main events visible with the naked eye. There are many smaller meteor showers throughout the year.