Standard

Effect of stellar scintillations on the errors in measuring the ozone content of the atmosphere. / Polyakov, A. V.; Timofeev, Y. M.; Gurvich, A. S.; Vorob'ev, V. V.; Kan, V.; Yee, J. H.

In: Izvestiya - Atmospheric and Ocean Physics, Vol. 37, No. 1, 01.01.2001, p. 51-53.

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

Harvard

Polyakov, AV, Timofeev, YM, Gurvich, AS, Vorob'ev, VV, Kan, V & Yee, JH 2001, 'Effect of stellar scintillations on the errors in measuring the ozone content of the atmosphere', Izvestiya - Atmospheric and Ocean Physics, vol. 37, no. 1, pp. 51-53.

APA

Polyakov, A. V., Timofeev, Y. M., Gurvich, A. S., Vorob'ev, V. V., Kan, V., & Yee, J. H. (2001). Effect of stellar scintillations on the errors in measuring the ozone content of the atmosphere. Izvestiya - Atmospheric and Ocean Physics, 37(1), 51-53.

Vancouver

Polyakov AV, Timofeev YM, Gurvich AS, Vorob'ev VV, Kan V, Yee JH. Effect of stellar scintillations on the errors in measuring the ozone content of the atmosphere. Izvestiya - Atmospheric and Ocean Physics. 2001 Jan 1;37(1):51-53.

Author

Polyakov, A. V. ; Timofeev, Y. M. ; Gurvich, A. S. ; Vorob'ev, V. V. ; Kan, V. ; Yee, J. H. / Effect of stellar scintillations on the errors in measuring the ozone content of the atmosphere. In: Izvestiya - Atmospheric and Ocean Physics. 2001 ; Vol. 37, No. 1. pp. 51-53.

BibTeX

@article{7be33f22ab984088b2bea0c3f1062770,
title = "Effect of stellar scintillations on the errors in measuring the ozone content of the atmosphere",
abstract = "Methods and algorithms are developed for the numerical simulation of stellar scintillations in the atmosphere during satellite observations. Estimates of the accuracy of remote measurements of the ozone content in the atmosphere are obtained on the basis of the data on stellar radiation observed from space with allowance made for scintillations under different observation conditions. The dependence of the measurement accuracy on the spectral correlations of scintillations is studied. It is shown that a noticeable increase of errors in determining the ozone content is due to stellar scintillations and may reach, at least, a few percent. Such an increase is out of the limits of errors allowable nowadays in determining the gas content of the atmosphere. The methods of the numerical simulation of stellar scintillations and their consideration in determining the gas content from the results of satellite measurements of the atmospheric transparency require further development.",
author = "Polyakov, {A. V.} and Timofeev, {Y. M.} and Gurvich, {A. S.} and Vorob'ev, {V. V.} and V. Kan and Yee, {J. H.}",
year = "2001",
month = jan,
day = "1",
language = "English",
volume = "37",
pages = "51--53",
journal = "Izvestiya, Atmospheric and Oceanic Physics",
issn = "0001-4338",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "1",

}

RIS

TY - JOUR

T1 - Effect of stellar scintillations on the errors in measuring the ozone content of the atmosphere

AU - Polyakov, A. V.

AU - Timofeev, Y. M.

AU - Gurvich, A. S.

AU - Vorob'ev, V. V.

AU - Kan, V.

AU - Yee, J. H.

PY - 2001/1/1

Y1 - 2001/1/1

N2 - Methods and algorithms are developed for the numerical simulation of stellar scintillations in the atmosphere during satellite observations. Estimates of the accuracy of remote measurements of the ozone content in the atmosphere are obtained on the basis of the data on stellar radiation observed from space with allowance made for scintillations under different observation conditions. The dependence of the measurement accuracy on the spectral correlations of scintillations is studied. It is shown that a noticeable increase of errors in determining the ozone content is due to stellar scintillations and may reach, at least, a few percent. Such an increase is out of the limits of errors allowable nowadays in determining the gas content of the atmosphere. The methods of the numerical simulation of stellar scintillations and their consideration in determining the gas content from the results of satellite measurements of the atmospheric transparency require further development.

AB - Methods and algorithms are developed for the numerical simulation of stellar scintillations in the atmosphere during satellite observations. Estimates of the accuracy of remote measurements of the ozone content in the atmosphere are obtained on the basis of the data on stellar radiation observed from space with allowance made for scintillations under different observation conditions. The dependence of the measurement accuracy on the spectral correlations of scintillations is studied. It is shown that a noticeable increase of errors in determining the ozone content is due to stellar scintillations and may reach, at least, a few percent. Such an increase is out of the limits of errors allowable nowadays in determining the gas content of the atmosphere. The methods of the numerical simulation of stellar scintillations and their consideration in determining the gas content from the results of satellite measurements of the atmospheric transparency require further development.

UR - http://www.scopus.com/inward/record.url?scp=0034770755&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:0034770755

VL - 37

SP - 51

EP - 53

JO - Izvestiya, Atmospheric and Oceanic Physics

JF - Izvestiya, Atmospheric and Oceanic Physics

SN - 0001-4338

IS - 1

ER -

ID: 36222397