Circadian temperature rhythms in clockwise and counter-clockwise rapidly rotating shift schedules.

The purpose of this study was to examine the circadian temperature rhythm in clockwise (CW) and counter-clockwise (CCW) rapidly rotating shift schedules. Arguments against the CCW rotation of shifts are that they result in shortened sleep and promote greater disruption of circadian rhythms. The 3-week study included a week of day shifts (0800-1600) and 2 weeks of shiftwork. The CW 2-2-1 schedule rotated from two early mornings (0600-1400) to two evenings (1400-2200) to one midnight shift (2200-0600) allowing 24 hours off at each shift rotation and a 48-hour weekend. The CCW schedule rotated from two evenings to two early mornings to one midnight shifts allowing only 8 hours off at each shift rotation and an 80-hour weekend. Analysis of the 72-hr periods at the end of each workweek, including the midnight shifts and recovery periods during weeks 2 and 3 were compared to the same 72-hour period at the end of week 1 (baseline). A cosine function that fit the temperature curves by minimizing the sums of squares produced parameters that underwent analysis of covariance procedures. Significant differences were found between rotation conditions for amplitude and acrophase. An attenuation of amplitude and a delay in the acrophase was the found for the counter-clockwise condition. Features inherent in this schedule might explain these effects, particularly, the increased opportunity for "sleeping in" at the beginning of the week and an expanded (2-shift) workday at the end of the week.

Acuity classification in the urgent care setting.

Efforts to control costs but provide accessible services have led to the development of urgent care centers. Viable urgent care centers must provide cost-effective care while maintaining quality. This requires staff allocation appropriate to patient needs as well as volume. Few articles have been written on patient acuity systems that permit optimal urgent care center staffing. Sharp Rees-Stealy Medical Centers have developed an acuity system for use in the urgent care center.

The genetics of a small autosomal region of Drosophila melanogaster containing the structural gene for alcohol dehydrogenase. VI. Induced revertants of scutoid.

Twenty-six induced revertants of Scutoid (Sco), a dominant mutation of Drosophila melanogaster, have been characterized genetically. Sco is an unusual mutation, involving two small reciprocal transpositions within the region 35A4 to 35C5 of chromosome arm 2L. One of these transpositions juxtaposes the noc and l(2)br28 loci. We suggested previously that the Sco phenotype results from the "fusion" of noc and l(2)br28. In support of this idea we now show that 23 of 26 revertants of Sco are noc-, indeed the majority are either chromosome aberrations broken between noc and l(2)br28 or deletions of these loci from the mutant chromosome. However, some revertants of Sco are rather more complex, and their properties suggest an interaction between the pu-noc and l(2)br28-l(2)br37 regions of chromosome arm 2L and also demonstrate the genetic complexity of the el-noc region.

A genetic and developmental analysis of an acid deoxyribonuclease in Drosophila melanogaster.

A deoxyribonuclease, called D Nase-1, that is active at acid pH in the presence of EDTA has been studied in Drosophila melanogaster. The locus for the Enzyme maps genetically to 61.8 on the right arm of the third chromosome. Cytogenetically, DNase-1 has been localized to within five to ten bands between 90C-2 and 90E. This analysis utilizes both electrophoretic variants and the Y-autosome translocations of Lindsley et al. (1972). DNase-1 is present in all stages of the life cycle, and the paternal genome actively contributes DNase-1 to the ambryo between 0 and 1 hr after fertilization.

White Light Coronagraph in OSO-7.

A small, externally occulted Lyot-type coronagraph, designed for use in the seventh unmanned Orbiting Solar Observatory (OSO-7), is described. Optical configuration, suppression of stray light, SEC vidicon detector, and data system are discussed, as well as integration of the instrument into the spacecraft and operation in orbit. Orbital operation produced daily images of the white light corona, from 2.8 to 10 solar radii, at least once per day for 2(3/4) yr. The first records of white light coronal transient events were obtained, and the corona was shown to be constantly changing.