Titlebook: Atmospheric Physics from Spacelab; Proceedings of the 1 J. J. Burger,A. Pedersen,B. Battrick Conference proceedings 1976 D. Reidel Publishi

Nonchalant

書目名稱Atmospheric Physics from Spacelab影響因子(影響力)




書目名稱Atmospheric Physics from Spacelab影響因子(影響力)學(xué)科排名




書目名稱Atmospheric Physics from Spacelab網(wǎng)絡(luò)公開度




書目名稱Atmospheric Physics from Spacelab網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Atmospheric Physics from Spacelab被引頻次




書目名稱Atmospheric Physics from Spacelab被引頻次學(xué)科排名




書目名稱Atmospheric Physics from Spacelab年度引用




書目名稱Atmospheric Physics from Spacelab年度引用學(xué)科排名




書目名稱Atmospheric Physics from Spacelab讀者反饋




書目名稱Atmospheric Physics from Spacelab讀者反饋學(xué)科排名

BET

High-Latitude Ionosphere-Atmosphere Interactionsscussed in relation to the formation of the ionospheric F-layer trough and the higher altitude plasma-pause. With regard to thermospheric dynamics, the effects of ion drag and Joule and particle heating were considered. Some emphasis was given to recent measurements which provide evidence for a hors

輕浮思想

Solar Radiation Variation and Climatelation between solar activity and atmospheric parameters at different heights are shown. The interest of studying the correlation that exists between important atmospheric parameters (physical and chemical) with the variations of the Sun flux at different wavelengths is stressed.

anesthesia

Obstacle

Synchronism

Basic Processes in the Stratosphere and the Mesospherewere discussed. Emphasis was placed on identifying the regions in which particular reaction cycles involving OX, ClX, HOX and NOX are dominant and feedback effects that may occur when sources of these species are altered. In particular, the implications of recent measurements of height profiles for

細(xì)胞

使饑餓

Measurements of Minor Constituents in the Stratosphereension to investigations of the earth homosphere from space. The use of more sophisticated instruments will be possible as well as their association allowing comparison between various types of measurements that will lead to a better accuracy of the data gathered on a global basis.

反感

High Resolution Atmospheric Extinction Measurements from the French Experiment on Board the NASA Spac to 6″ x 2′ of arc) simultaneously in the Ca II, Mg II, Ly α, Ly β lines..Using a classical inversion technique as described by Roble and Hays (1972) it has been possible to invert some extinction profiles..The quality of the data appears to give a 500 m vertical resolution both for O. and O.. O. i

Foregery

High Resolution Atmospheric Emission Spectroscopy at 120 cm -1 and 535 cm -1, with a Rapid Scan Inteescope on NASA’s G.P. Kuiper airborne observatory. Technical details have been described elsewhere. and the measurement of ionic lines from the Orion Nebula will be the subject of further published work. The system attains a spectral resolution of 0.02 cm. within a helium-cooled filter passband of Δ