Models for the atmosphere of Mars based on the Mariner 4 occultation experiment.
Mars atmosphere models based on Mariner IV OCCULTATION deriving electron number density, temperature, pressure, mass density, etc, noting carbon dioxide presence
Engineering topics
Publications and source records attributed to Eshleman, V. R..
Mars atmosphere models based on Mariner IV OCCULTATION deriving electron number density, temperature, pressure, mass density, etc, noting carbon dioxide presence
Radio and radar astronomical studies on lunar and planetary ionospheres and atmospheres, and solar activity
Mars atmospheric models based on Mariner IV OCCULTATION experiment
Frequency, phase, and amplitude changes of Mariner IV radio signal through atmosphere and ionosphere of Mars observed before and after planetary occulatation
Coherent radio transmission to probe atmosphere and ionosphere of Mars including density, temperature, scale height, etc
Two lunar radars used to measure total integrated electron density between Earth and Moon during three nights and two mornings in December 1964
Two-frequency bistatic radar-occultation technique to investigate planetary atmospheres
Lunar radar echo measurments to determine size and electron density of earth magnetospheric wake
Mars atmosphere and ionosphere measurements using 2300-mc telemetry signal from Mariner IV SPACECRAFT occultation experiments
Diffraction and refraction of radio waves to study planetary atmosphere
Radio and radar astronomy - lunar and planetary ionospheres, atmospheres, and surfaces, and radar studies of sun and interplanetary medium
Radar measurement of total cislunar electron content
Method for study of planetary ionospheres based on radio wave propagation between earth and spacecraft
Bistatic radar-occultation method for planetary atmosphere study
Radio and radar astronomy studies of lunar and planetary atmospheres and surfaces, and radar studies of sun and interplanetary medium
Ionized gases of solar system studied by radar astronomy
Planetary-solar-interplanetary gaseous regions studied by monostatic and bistatic radar astronomy techniques