In an exposure of the Fermilab 15' neon (64 atomic %)--H/sub 2/ bubble chamber to a broad band anti ..nu.. beam, 3 ..mu../sup +/e/sup -/X and 6 ..mu../sup -/e/sup +/X events (with estimated backgrounds 1.1 and 0.6 events, respectively) were found with the ..mu../sup +-/ identified in the EMI. The fractions of ..mu../sup +/e/sup -/ and ..mu../sup -/e/sup +/ production relative to anti ..nu../sub ..mu../ and ..nu../sub ..mu../ charged current interactions are respectively anti f = (0.10 +- /sub 0.07//sup 0.13/)% and f = (0.34 +- /sub 0.13//sup 0.23/)%, giving anti f/f = 0.3 +- /sub 0.2//sup 0.5/.

Future industry scenarios for energy consumption in the marine transport industry are projected and the energy savings potential of the research and development program identified in Task III (Efficiency Improvements) against these scenarios is evaluated. The introduction is contained in Chapter I. In Chapter II, the operational, regulatory, and vessel size scenarios for the year 2000 are developed. In Chapter III, future cargo flows and expected levels of energy use for the baseline 2000 projection are determined. In Chapter IV, the research and development programs are introduced into the future US flag fleet and the energy savings potential associated with each is determined. (MCW)

A study was made to examine the effects which raising the ISA from 200 x 200 GeV to 400 x 400 GeV would have on the ''canonical'' experiments. These were ''canonical'' in the sense that they span the full range of foreseeable physics and have served as topics in previous Summer Studies and Workshops which resulted in quite explicit hardware designs and experimental goals. The study results indicate that all of the ''canonical'' experiments survive. Some are actually improved, some are unaffected, and some require changes which are suggested. In general, the 90/sup 0/ experiments are relatively unaffected. The single arm small angle spectrometer, the wide aperture (FATS-WASP) spectrometer and the Coulomb interference experiment have the largest number of modifications suggested. No uniqueness to these solutions are claimed, and there may be more desirable radical approaches. It is, however, felt that the 400 x 400 GeV ISA not only permits the work on conceptual experiments from previous Summer Studies to be taken over entirely, but indicates areas of improvement in many of them. Specifics of the individual experiments are discussed.