Data Access
This composite image is produced from GUVI radiance data (Level 1C) plotted as a strip image for a complete day. It is a composite of the O I 130.4 nm emission (blue), O I 135.6 nm (green), and LBH Short (140 - 150 nm) (red). White color indicates emission from particles in aurora (all colors), pink areas generally indicate particle precipitation (SAA) or solar glint, blue emissions indicate typical nighttime recombination emissions, light grey typically indicates dayglow emission.
Version:2.2.1
This composite image is produced from GUVI radiance data (Level 1C) plotted as a strip image for a complete day. It is a composite of the O I 130.4 nm emission (blue), O I 135.6 nm (green), and LBH Short (140 - 150 nm) (red). White color indicates emission from particles in aurora (all colors), pink areas generally indicate particle precipitation (SAA) or solar glint, blue emissions indicate typical nighttime recombination emissions, light grey typically indicates dayglow emission.
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Andrew.B.Christensen | |||
| 2. | CoInvestigator | spase://SMWG/Person/Larry.J.Paxton |
his web page allows viewing of individual images or a slideshow of a sequence of images. To request data: select the year and day and the StripDisk Display type then click display for the desired image.
Radiance of each of 3 colors: O I 130.4 nm (displayed as blue), O I 135.6 nm (green), and LBH Short 140 - 150 nm (red).