Non-imaging remote sensing data

Details Non-imaging remote sensing data Non-imaging remote sensing data

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2343...72.&link_type=abstract

In its Planetary Data Workshop, Pt. 1 p 72-85 (SEE N84-34366 23-91)

Physics

Data Bases, Measuring Instruments, Planets, Remote Sensing, Space Exploration, Spectrum Analysis, Algorithms, Data Processing, Gamma Rays, High Resolution, Microwaves, Polarization (Waves), Spectral Resolution

Scientific paper

Spectrometric, radiometric and polarimetric remote sensing observations of wavelengths from gamma-rays to microwaves are addressed. The basic form of the data is one dimensional arrays. At the high energy end of the spectrum, data are typically presented as pulse count versus energy, and at lower energies, as intensity versus wavelength. High spectral resolution measurements (better 1% of wavelength) are particularly useful for identifying atomic, molecular, and ionic species while broader band measurements are adequate for identifying minerals and for determining total energy fluxes. Polarization data permit the study of finely divided material such as clouds and surfaces.

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