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The Atmospheric Infrared Sounder — called AIRS for short — aboard NASA's orbiting Aqua spacecraft measures temperature and cloud cover by recording infrared emissions across the entire globe twice a day.
An observer on a moving body, such as a spacecraft, measures its so-called rest mass m0, while a fixed observer measures its mass m as which is greater than m0.
The spacecraft measures gravity variations across the surface of the Earth and this information, allied to sea-surface height data, can then be used to work out current directions and speed.
The medium-energy particle experiments—electron analyzer onboard the exploration of energization and radiation in geospace spacecraft measures the energy and direction of each incoming electron in the energy range of 7 87 keV.
The Arase spacecraft measures the fluxes of ions and electrons over a wide energy range and detects electric and magnetic field oscillations over a wide frequency range to gain insight into the interactions between particles of different energies and waves of different frequencies.
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The Voyager spacecraft measured the spot's length at 23,000 km (14,500 miles) in 1979.
These spacecraft measure the very subtle variations in Earth's gravity as they fly around the globe.
Systematical errors of the spacecraft measured high-energy particle fluxes are analyzed.
The speeds were estimated using a cross-correlation analysis of radio frequency fluctuations of the Galileo spacecraft measured simultaneously at widely spaced ground stations.
The CubeSat architecture allows the basic cube design (1U) to be extended into larger sized (cuboid) spacecraft measured as multiples of U (2U, 3U, 6U etc., see Figure 2).
In contrast, the 'solar wind laboratory' is directly measured in situ by a fleet of spacecraft measuring the properties of the plasma and magnetic fields at specific points in space.
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