Geoscientific Instrumentation, Methods and Data Systems
Geoscientific Instrumentation, Methods and Data Systems
GI
Articles | Volume 5, issue 2
Articles | Volume 5, issue 2
https://doi.org/10.5194/gi-5-493-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/gi-5-493-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
Articles | Volume 5, issue 2
Research article
 | 
06 Oct 2016
Research article |  | 06 Oct 2016

Auroral meridian scanning photometer calibration using Jupiter

Brian J. Jackel, Craig Unick, Fokke Creutzberg, Greg Baker, Eric Davis, Eric F. Donovan, Martin Connors, Cody Wilson, Jarrett Little, M. Greffen, and Neil McGuffin

Viewed

Total article views: 1,953 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,125 702 126 1,953 115 118
  • HTML: 1,125
  • PDF: 702
  • XML: 126
  • Total: 1,953
  • BibTeX: 115
  • EndNote: 118
Views and downloads (calculated since 23 Mar 2016)
Cumulative views and downloads (calculated since 23 Mar 2016)

Cited

Latest update: 14 Sep 2024
Download
Short summary
In order to compare auroral observations, it is necessary to ensure that all instruments are properly calibrated. This can be difficult to achieve with different instruments operated for extended intervals at remote field sites under harsh conditions. Astronomical sources can be used for independent absolute calibration procedures. Under ideal conditions Jupiter is an excellent source, as it can provide more light than the brightest star. We use Jupiter to calibrate an auroral MSP network.
Read more