Mariner 9 ultraviolet spectrometer experiment: seasonal variation of ozone on Mars.

نویسندگان

  • C A Barth
  • C W Hord
  • A I Stewart
  • A L Lane
  • M L Dick
  • G P Anderson
چکیده

Ozone is observed to be present in the polar regions of Mars and to have a seasonal variation. In the summer, the amount present in the polar atmosphere is less than 3 micrometer-atmospheres. In the fall, ozone increases in amount and is found in association with the formation of the polar hood. In winter, the maximum amount of ozone is present, 57 micrometer-atmospheres over the polar hood and 16 over the polar cap. In spring, the amount over the polar cap decreases monotonically until by the beginning of summer the ozone disappears. Ozone is not observed in the equatorial region during any season.

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

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Mariner 9 Ultraviolet Spectrometer Experiment: Vertical Distribution of Ozone on Mars

The vertical distribution of ozone in the atmosphere of Mars is computed from ultraviolet spectra obtained by the Mariner 9 spacecraft. In the Northern Hemisphere the ozone scale height is much smaller than the atmospheric scale height in midlatitudes and increases rapidly to a maximum farther north. At high latitudes (above 60 °) there is no significant difference between the scale heights of ...

متن کامل

Mariner 9 ultraviolet spectrometer experiment: initial results.

The ultraviolet airglow spectrum of Mars has been measured from an orbiting spacecraft during a 30-day period in November-December 1971. The emission rates of the carbon monoxide Cameron and fourth positive bands, the atomic oxygen 1304-angstrom line and the atomic hydrogen 1216-angstrom line have been measured as a function of altitude. Significant variations in the scale height of the CO Came...

متن کامل

Mariner 6, 7, and 9 Ultraviolet Spectrometer Experiment: Analysis of hydrogen Lyman alpha data

Four Lyman a airglow measurements of the limb and disc of Mars, made by ultraviolet spectrometers on Mariner 6 and 7 in 1969 and Mariner 9 in 1971, are analyzed to determine the amount and distribution of atomic hydrogen above 80 km. The variation of atomic hydrogen with altitude is calculated by using time-independent chemical diffusion models from 80 to 250 km, and tin exospheric model is use...

متن کامل

Mariner 6 and 7 Ultraviolet Spectrometer Experiment Analysis of Hydrogen LymanAlpha Data

Mariner 6 and 7 ultraviolet spectrometers that flew by Mars in 1969 observed the Lyman-, dayglow of atomic hydrogen. Data in the altitude range 200 to 24,000 km are analyzed to determine the structure of the Martian exosphere. The classical evaporative theory is applied to calculate a hydrogen density distribution. A spherical model of the dayglow Lyman-a emission, using radiative transfer theo...

متن کامل

ZCARUS 17, 457--468 (1972) Mariner 9 Ultraviolet Spectrometer Experiment: Mars Airglow Spectroscopy and Variations in Lyman Alpha

Mariner 9 ull raviolet spec t rome te r observa t ions show the Mars airglow consists pr incipal ly of emissions t h a t arise f rom the in te rac t ion of solar u l t raviole t radiat ion wi th carbon dioxide, the pr incipal cons t i tuen t of the Mars a tmosphere . Two minor cons t i tuen ts , a tomic hyd rogen and a tomic oxygen, also produce airglow emissions. The airglow measu remen t s sh...

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

عنوان ژورنال:
  • Science

دوره 179 4075  شماره 

صفحات  -

تاریخ انتشار 1973