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Linelist of HD16O for study of atmosphere of terrestrial planets (Earth, Venus and Mars)

First results of ground-based Fourier Transform Infrared measurements of the H2O total column in the atmosphere over West Siberia

Study of HDO absorption in the 11,200-12,400 cm-1 range using LED-based Fourier transform spectroscopyA high resolution Fourier transform spectrum of mono-deuterated water vapor was studied between 11

H216O line list for the study of atmospheres of Venus and Mars with a CO2 content of about 95%. In this paper, the line list of H216O is obtained on the basis of the BT

Light-emitting-diode Fourier-transform spectroscopy of HD16O between 11200 and 12400 cm-1 was applied as a source of radiation. Signal to noise ratio was about 104. The spectral line parameters - line

Verification of H2O lines from the HITRAN database for remote sensing of the water vapour isotopic composition've used two following criteria: a quality of the fitting of atmospheric spectra measured at the Ural

Do the processes in near-earth space influence weather and climate? temperature, correlate with Space weather parameters. A straight dependence of the surface temperature from

Problems and perspectives of management and marketing development in digital economy

Десять купцов не стоят одного чиновника (проблемы массового сознания на Востоке в условиях глобализации)

Review: Gusarov V.I. Mediterranean – unclosed ellipse. – M., 2011. – 350 p.

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