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An overview of the applications of the field electrophoretic instruments is provided, including environmental science and planetary investigation.
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The benefits of instrument combinations and integration into instrument suites are discussed, and examples of potential exploration suites are given for the investigation of planetary shape, size, and mass, their surface and subsurface properties, moons and rings, and the analysis of planetary atmospheres, exospheres, ionospheres, and magnetospheres.
The benefits of instrument combinations and integration into instrument suites are discussed and examples of potential exploration suites are given for the investigation of planetary shape, size and mass, their surface and subsurface properties, moons and rings and the analyzing of planetary atmospheres, exospheres, ionospheres, and magnetospheres.
To address these topics, CAWSES-II uses a research strategy that includes comparisons with other stellar and planetary environments to inform investigations into solar-terrestrial science.
From the multi-temporal planetary image database and investigations based on multi-temporal observations we will better understand the interactions between the surface of Mars and external forces, including the atmosphere.
They are all instruments of exploration and investigation, models of planetary and stellar motion, surveying instruments and mapmaking equipment.
The orbital period indicates that the planet is located close to a 1 3 mean motion resonance with 55 Cancri c, however investigations of the planetary parameters in a Newtonian simulation indicate that while the orbital periods are close to this ratio, the planets are not actually in the resonance.
Topographic information is of fundamental importance for various scientific investigations in lunar and planetary exploration.
This development program is accompanied by an in-depth methodical investigation of this technique under planetary environmental conditions.
We developed a compact time-of-flight mass spectrometer (TOF-MS) for the sensitive investigation of gas samples in planetary missions.
This paper presents an experimental investigation of mixing in a planetary mixer, and a comparison with numerical simulations based on a simple mathematical model of the flow.
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