MSP#
Meridian Imaging Photometers scanned the sky along magnetic meridians, providing auroral intensities at four wavelengths, including the 486 nm 'Hβ' proton aurora. Three instruments covered from sub-auroral to polar cap latitudes along the 'Churchill Line', while the fourth covered auroral latitudes from Fort Smith, two hours MLT to the west.
4 instruments
Data tree location: https://data.phys.ucalgary.ca/sort_by_project/GO-Canada/GO-Storm/msp/
Acknowledgements PDF: https://data.phys.ucalgary.ca/sort_by_project/GO-Canada/GO-Storm/msp/acknowledgements.pdf
Contact: Eric Donovan