FOS Scattered Light

• Analysis of UV spectra

  • cools sources had excess flux in UV
  • level and shape unphysical
  • comparison with other experiments ( rocket data, Copernicus, IUE, HUT)
  • comparison with atmosphere models
  • error bars are scaled by a factor 100 to become visible

• Obvious source

  • scattered red light

• Questions

  • anything wrong with instrument
  • what can be done to cure the data

Previous slide

Next slide

Back to first slide

View graphic version