Soft Component in Upper Atmosphere

نویسندگان
چکیده

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Waves in Pluto’s Upper Atmosphere

Observations of the 2007 March 18 occultation of the star P445.3 (2UCAC 25823784; R = 15.3) by Pluto were obtained at high time resolution at five sites across the western United States and reduced to produce light curves for each station using standard aperture photometry. Global models of Pluto’s upper atmosphere are fitted simultaneously to all resulting light curves. The results of these mo...

متن کامل

Mars: upper atmosphere.

The thermal structure of the upper atmosphere of Mars has been theoretically investigated. The exospheric temperature, for a pure CO(2) model atmosphere, lies between 400 degrees and 700 degrees K. The origin of the Martian atmosphere is discussed in the light of these results.

متن کامل

Nonlinear internal waves in the upper atmosphere

This paper considers the large-scale dynamics generated in the upper atmosphere by the destabilization of a linear internal gravity wave and its eventual restabilization through nonlinear processes into a coherent pattern. The assumption of a strongly dissipative medium is relevant to wave propagation in the thermosphere range above 100 km. A parametric instability analysis is carried out invol...

متن کامل

Infrared Scattering Observations in the Upper Atmosphere

Observations of sky emission and absorption in the far infrared (mean wavelength 120 /•) and, simultaneously, sky emission at wavelength 6 • have been made by P. Kuhn (ESSA): from the NASA CV-990 aircraft flying at 12-km altitude over the middle Pacific at latitudes 10ø-15øN. A lack of correlation between the nearand far-infrared data, especially during times of visible cirrus cloud cover above...

متن کامل

Negative ion chemistry in Titan’s upper atmosphere

The Electron Spectrometer (ELS), one of the sensors making up the Cassini Plasma Spectrometer (CAPS) revealed the existence of numerous negative ions in Titan’s upper atmosphere. The observations at closest approach ( 1000 km) show evidence for negatively charged ions up to 10,000 amu/q, as well as two distinct peaks at 2274 and 4478 amu/q, and maybe a third one at 82714 amu/q. We present the f...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Progress of Theoretical Physics

سال: 1950

ISSN: 0033-068X

DOI: 10.1143/ptp.4.578