Standard

Ozone profile determination by occultation sounding from the Mir space station : 1. Instrumentation and data processing method. / Poberovskii, A. V.; Polyakov, A. V.; Timofeev, Yu M.; Mansurov, I. I.

In: Izvestiya - Atmospheric and Ocean Physics, Vol. 35, No. 3, 01.01.1999, p. 282-290.

Research output: Contribution to journal › Article › peer-review

Harvard

Poberovskii, AV, Polyakov, AV, Timofeev, YM & Mansurov, II 1999, 'Ozone profile determination by occultation sounding from the Mir space station: 1. Instrumentation and data processing method', Izvestiya - Atmospheric and Ocean Physics, vol. 35, no. 3, pp. 282-290.

APA

Poberovskii, A. V., Polyakov, A. V., Timofeev, Y. M., & Mansurov, I. I. (1999). Ozone profile determination by occultation sounding from the Mir space station: 1. Instrumentation and data processing method. Izvestiya - Atmospheric and Ocean Physics, 35(3), 282-290.

Vancouver

Poberovskii AV, Polyakov AV, Timofeev YM, Mansurov II. Ozone profile determination by occultation sounding from the Mir space station: 1. Instrumentation and data processing method. Izvestiya - Atmospheric and Ocean Physics. 1999 Jan 1;35(3):282-290.

Author

Poberovskii, A. V. ; Polyakov, A. V. ; Timofeev, Yu M. ; Mansurov, I. I. / Ozone profile determination by occultation sounding from the Mir space station : 1. Instrumentation and data processing method. In: Izvestiya - Atmospheric and Ocean Physics. 1999 ; Vol. 35, No. 3. pp. 282-290.

BibTeX

@article{6ae7090287db4f63b4d99340eb191c18,
title = "Ozone profile determination by occultation sounding from the Mir space station: 1. Instrumentation and data processing method",
abstract = "The instrumentation, interpretation procedure, and some examples of ozone profile retrieval in space experiments with the Priroda module of the Mir space station are described. The Ozon-Mir spectrometer measured solar radiation absorption along tangent paths in a large number of spectral channels within the range from 265 to 1130 nm at sunsets. Different stages of telemetric information processing are considered. The atmospheric radiative model used for computations and the algorithm of data inversion are discussed. Measurements in oxygen absorption bands provided an independent way of referring the data of transmission function measurements to heights. Errors in ozone content determination that are due to different factors are estimated. By and large, the experimental results correlate well with climatic data. At the same time, significant variations in the ozone content were observed. They may be explained by the natural variability of characteristics of atmospheric gaseous composition and also by retrieval errors.",
author = "Poberovskii, {A. V.} and Polyakov, {A. V.} and Timofeev, {Yu M.} and Mansurov, {I. I.}",
year = "1999",
month = jan,
day = "1",
language = "English",
volume = "35",
pages = "282--290",
journal = "Izvestiya - Atmospheric and Oceanic Physics",
issn = "0001-4338",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "3",

}

RIS

TY - JOUR

T1 - Ozone profile determination by occultation sounding from the Mir space station

T2 - 1. Instrumentation and data processing method

AU - Poberovskii, A. V.

AU - Polyakov, A. V.

AU - Timofeev, Yu M.

AU - Mansurov, I. I.

PY - 1999/1/1

Y1 - 1999/1/1

N2 - The instrumentation, interpretation procedure, and some examples of ozone profile retrieval in space experiments with the Priroda module of the Mir space station are described. The Ozon-Mir spectrometer measured solar radiation absorption along tangent paths in a large number of spectral channels within the range from 265 to 1130 nm at sunsets. Different stages of telemetric information processing are considered. The atmospheric radiative model used for computations and the algorithm of data inversion are discussed. Measurements in oxygen absorption bands provided an independent way of referring the data of transmission function measurements to heights. Errors in ozone content determination that are due to different factors are estimated. By and large, the experimental results correlate well with climatic data. At the same time, significant variations in the ozone content were observed. They may be explained by the natural variability of characteristics of atmospheric gaseous composition and also by retrieval errors.

AB - The instrumentation, interpretation procedure, and some examples of ozone profile retrieval in space experiments with the Priroda module of the Mir space station are described. The Ozon-Mir spectrometer measured solar radiation absorption along tangent paths in a large number of spectral channels within the range from 265 to 1130 nm at sunsets. Different stages of telemetric information processing are considered. The atmospheric radiative model used for computations and the algorithm of data inversion are discussed. Measurements in oxygen absorption bands provided an independent way of referring the data of transmission function measurements to heights. Errors in ozone content determination that are due to different factors are estimated. By and large, the experimental results correlate well with climatic data. At the same time, significant variations in the ozone content were observed. They may be explained by the natural variability of characteristics of atmospheric gaseous composition and also by retrieval errors.

UR - http://www.scopus.com/inward/record.url?scp=0032888384&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:0032888384

VL - 35

SP - 282

EP - 290

JO - Izvestiya - Atmospheric and Oceanic Physics

JF - Izvestiya - Atmospheric and Oceanic Physics

SN - 0001-4338

IS - 3

ER -

ID: 36223266