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The Diffuse Radiation Field at High Galactic Latitudes

  • Authors: M. S. Akshaya, Jayant Murthy, S. Ravichandran, R. C. Henry, and James Overduin

2018 The Astrophysical Journal 858 101.

  • Provider: AAS Journals

Caption: Figure 9.

Modeled surface brightness for the NGP in the FUV (a = 0.4, g = 0.6) and NUV (a = 0.4, g = 0.5) at a resolution of 30′. The maps are in photon units. The NGP is at the center with lines of latitude at 80° and 85° and lines of longitude every 60° starting from 0° at the top and increasing clockwise.

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