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   81407
   We propose a 14-day continuous observation of SS 433 with ASCA to cover
   its one full orbital period. The goals are: (1) mapping of the
   structure of the super-critical accreting flow using the X-ray jet
   emission as the light source of X-ray tomography, (2) measurement of
   the time variation of the jet kinetic power and its correlation with
   the optical and radio flux variation, and (3) cross-calibration of
   ASTRO-E and XMM with ASCA using the strong emission lines of SS 433.
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