Developments in upper atmospheric science during the IQSY

Vertical structure and temperature fluctuations in upper atmosphere, anomalies in ionosphere, and whistler identificatio

Mariner 4 and the atmosphere of Mars

Interpretation of data on Martian atmosphere obtained from Mariner

System for collecting world-wide lower thermosphere data

Collecting lower thermosphere data by global satellite network measurements of atmospheric composition, density, temperature, and airglo

Lunar atmosphere

Solar wind, meteoric volatilization, and internal degassing contributing to lunar rarefied atmosphere, and transient contributions produced by rocket gases during lunar mission

Environment for manned planetary missions

Radiation hazards of manned planetary mission

The atmosphere of Mars

Effects of Mariner IV ionospheric data on Mars atmosphere composition prediction

A feasibility study on the use of a coincidence mass spectrometer to determine lunar atmosphere constituents Final report

Coincidence Mass Spectrometer /CMS/ to determine lunar atmosphere constituent

A research in support of NASA's space science

An ion drift meter, extreme ultraviolet spectrometers, an extreme ultraviolet grating photometer, and a soft particle spectrometer were developed

The atmosphere of Venus - A conference review

Data from Mariner 5 and Venera 4, and ground based measurements of Venus atmospher

Evaluation of flat-plate collector efficiency under controlled conditions in a solar simulator

The measured thermal efficiencies of 35 collectors tested with a solar simulator, along with the correlation equations used to generalize the data, are presented. The single correlation used is shown to apply to all the different types of collectors tested, including one with black paint and one cover, one with a selective surface coating and two covers, and an evacuated-tube collector. The test and correlation technique is also modified by using a shield so that collectors larger than the simulator test area can also be tested. This technique was verified experimentally for a shielded collector for which the collector shielded area was 31% of the solar simulator radiation area. A table lists all the collectors tested, the collector areas, and the experimental constants used to correlate the data for each collector