Solar gamma ray monitor for OSO-H (0.3-10 MeV)

A gamma ray experiment to be flown aboard the OSO-7 spacecraft is described along with a history of the development of the experiment, a description of the gamma ray detector and its operation, and a short preliminary review of the scientific information obtained during the instruments' lifetime. The gamma ray detector operated an average of 18 hours a day for approximately 15 months. The majority of the data was collected in the solar and antisolar direction, but data at right angles to the spacecraft-sun line was also accumulated. In all, at least two full scans of the celestial sphere were completed

A gamma ray monitor for the OSO-7 spacecraft

A 3 in. x 3 in. NaI(Tl) gamma ray (0.3 to 10 MeV) spectrometer with a CsI(Na) charged particle and anti-Compton shield has been developed for the Orbiting Solar Observatory (OSO-7) which was launched September 30, 1971. The instrument, designed for a rotating wheel compartment, utilizes a 377 channel quadratic PHA with accumulation times of 3, 1, or 0.5 minutes. Quick look and calibration data obtained via a direct data link to a minicomputer allows near real time monitoring and control of the experiment. Various commands changing the operating mode can be executed. The functions which can be commanded include: rotation of the quadrants in which data is collected by 90 deg; gain adjustment of the central detector over a 6:1 range; manual or automatic sequencing of calibrations; variations of accumulation times by telemetering selected channels; and selection of reference directions. A small X-ray detector covering the range 7.5 to 120 keV is also included

Documentation of the data analysis system for the gamma ray monitor aboard OSO-H

The programming system is presented which was developed to prepare the data from the gamma ray monitor on OSO-7 for scientific analysis. The detector, data, and objectives are described in detail. Programs presented include; FEEDER, PASS-1, CAL1, CAL2, PASS-3, Van Allen Belt Predict Program, Computation Center Plot Routine, and Response Function Programs

Physical properties, lung deposition modeling, and bioactivity of recombinant GM-CSF aerosolised with a highly efficient nebulizer.

Pulmonary alveolar proteinosis (PAP) is a rare condition characterized by the accumulation of lipoproteinaceous material within air spaces. Although whole lung lavage is the current standard of care, recent advances in our understanding of PAP pathophysiology suggest that the disorder may benefit from inhalation of recombinant granulocyte-macrophage colony-stimulating factor (rGM-CSF). The aim of this study was to determine the physical properties and bioactivity of rGM-CSF aerosolised by the highly efficient AKITA² APIXNEB® nebulizer system. The physical properties of aerosolised rGM-CSF were investigated in terms of droplet size, output and output rate by laser diffraction and gravimetrical analysis. Lung deposition was assessed using deposition modeling (ICRP). Molecular mass before and after aerosolisation was determined by SDS-PAGE, while the bioactivity of rGM-CSF was evaluated by measuring the GM-CSF-stimulated increase in pSTAT5 using mAM-hGM-R cells. Ninety-six \% of the rGM-CSF filling dose was aerosolised with the Akita² Apixneb® nebulizer system. Particle size was highly reproducible, and the amount deposited within the lung was 80.35\% of the delivered dose. The aerosolisation did not alter the molecular structure of rGM-CSF, nor its ability to stimulate the pSTAT5, which increased by 99.5\%, similar to values for rGM-CSF prior to aerosolisation. We conclude that the highly efficient AKITA² APIXNEB® nebulizer system is likely to efficaciously deliver rGM-CSF to the airways of patients with autoimmune PAP