This image has not been optimised to highlight the complete solar radio burst.
This image has not been optimised to highlight the complete solar radio burst.
This image has not been optimised to highlight the complete solar radio burst.
This image has not been optimised to highlight the complete solar radio burst.
This image has not been optimised to highlight the complete solar radio burst.
This image has not been optimised to highlight the complete solar radio burst.
These images have been optimised to highlight the complete solar radio burst (where possible) utilising the full frequency range of the Solar Radio Spectrometers at Sunnydale. While each spectrometer scans a different frequency range, the image is probably a composite in either frequency or time.
These images have been optimised to highlight the complete solar radio burst (where possible) utilising the full frequency range of the Solar Radio Spectrometers at Sunnydale. While each spectrometer scans a different frequency range, the image is probably a composite in either frequency or time.
These images have been optimised to highlight the complete solar radio burst (where possible) utilising the full frequency range of the Solar Radio Spectrometers at Sunnydale. While each spectrometer scans a different frequency range, the image is probably a composite in either frequency or time.
These images have been optimised to highlight the complete solar radio burst (where possible) utilising the full frequency range of the Solar Radio Spectrometers at Sunnydale. While each spectrometer scans a different frequency range, the image is probably a composite in either frequency or time.
These images have been optimised to highlight the complete solar radio burst (where possible) utilising the full frequency range of the Solar Radio Spectrometers at Sunnydale. While each spectrometer scans a different frequency range, the image is probably a composite in either frequency or time.
If you are a returning viewer, this page probably looks considerably different from your last visit. I am trialing a new Python software tool developed by Sahan Liyanage, BSc (Hons) in Physics, Faculty of Science, University of Colombo Sri Lanka.
The page may take a while to settle down as I explore the capabilities and features of this tool.