ACRIM‐gap and TSI trend issue resolved using a surface magnetic flux TSI proxy model

@article{Scafetta2009ACRIMgapAT,
  title={ACRIM‐gap and TSI trend issue resolved using a surface magnetic flux TSI proxy model},
  author={Nicola Scafetta and Richard C. Willson},
  journal={Geophysical Research Letters},
  year={2009},
  volume={36}
}
The ACRIM‐gap (1989.5–1991.75) continuity dilemma for satellite TSI observations is resolved by bridging the satellite TSI monitoring gap between ACRIM1 and ACRIM2 results with TSI derived from Krivova et al.'s (2007) proxy model based on variations of the surface distribution of solar magnetic flux. ‘Mixed’ versions of ACRIM and PMOD TSI composites are constructed with their composites' original values except for the ACRIM gap, where Krivova modeled TSI is used to connect ACRIM1 and ACRIM2… 
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