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Usually the measurement instruments dedicated to power quality assessment contain a transient detection stage that is activated only when it is necessary.
With these instruments dedicated to meteorological study, we are planning a systematic observation sequence to detect dynamical processes with various temporal and spatial scales.
Akatsuki will explore the Venusian atmosphere using a set of sophisticated optical instruments dedicated to meteorological study and radio occultation technique.
With the emergence of new biomaterials and elastography imaging techniques, there is a need for innovative instruments dedicated to viscoelasticity measurements.
The Upper Atmospheric Research Satellite UARSS) carries two instruments dedicated to monitoring long-term solar UV irradiance: the Solar Ultraviolet Spectral Irradiance Monitor (SUSIM) and the Solar Stellar Intercomparison Experiment (SOLSTICE).
This diagnostic approach can be used: (i) to guide users in choosing the most appropriate imagery for their application, (ii) to evaluate the adequacy of existing remote sensing systems for monitoring agriculture in different regions of the world and (iii) to provide guidelines for space agencies to design future instruments dedicated to agriculture monitoring.
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There is no established psychometric instrument dedicated to the measurement of severity in psychotic depression (PD).
Archeops1 is a balloon-borne instrument dedicated to measuring the Cosmic Microwave Background (CMB) temperature anisotropies over a large fraction (30%) of the sky, in the (sub millimetre domain (from 143 to 545 GHz).
ARCHEOPS is a balloon-borne instrument dedicated to measure cosmic microwave background (CMB) temperature anisotropies at high angular resolution (about 10′) over a large fraction (30%) of the sky in the (sub millimetre domain (from 143 to 545 GHz).
Global ozone monitoring by occultation of stars (GOMOS) on ENVISAT is the first space instrument dedicated to the study of the atmosphere of the Earth by the technique of stellar occultations (global ozone monitoring by occultation of stars).
Since FIS is an instrument dedicated to FIR, λ = 50 180 μ m, all the AKARI FIS bands are in the FIR wavelengths: N60 (65 μ m), WIDE-S (90 μ m), WIDE-L (140 μ m), and N160 (160 μ m) (Kawada et al., 2007).
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