The parametric model NEOPLANTA was used to study the effects of various
atmospheric conditions on terrestrial spectral UV irradiance. The capability of the model to correctly reproduce processes in the atmosphere is tested by changing input parameters such as ozone content, solar zenith angle, amount and type of aerosols, and altitude. The results of the model testing on input parameter change were satisfactory. As is expected, the amount of UV radiation reaching the surface is the most dependable on ozone layer thickness and solar zenith angle. Erythemal irradiance is more dependent on changes in the amount of ozone in the atmosphere than spectral UV irradiance, showing a significantly greater impact of UV-B radiation on human skin than radiation in the UV-A part of the spectrum.
Source:
IV Meeting on Astrophysical Spectroscopy - A&M DATA – Atmosphere. Book of Abstracts and Contributed Papers, 2022, 10-15
TY - CONF
AU - Malinović-Milićević, Slavica
PY - 2022
UR - https://dais.sanu.ac.rs/123456789/13299
AB - The parametric model NEOPLANTA was used to study the effects of various
atmospheric conditions on terrestrial spectral UV irradiance. The capability of the model to correctly reproduce processes in the atmosphere is tested by changing input parameters such as ozone content, solar zenith angle, amount and type of aerosols, and altitude. The results of the model testing on input parameter change were satisfactory. As is expected, the amount of UV radiation reaching the surface is the most dependable on ozone layer thickness and solar zenith angle. Erythemal irradiance is more dependent on changes in the amount of ozone in the atmosphere than spectral UV irradiance, showing a significantly greater impact of UV-B radiation on human skin than radiation in the UV-A part of the spectrum.
PB - Belgrade : Institute of Physics Belgrade
C3 - IV Meeting on Astrophysical Spectroscopy - A&M DATA – Atmosphere. Book of Abstracts and Contributed Papers
T1 - Clear-sky spectral UV radiation modelling
SP - 10
EP - 15
UR - https://hdl.handle.net/21.15107/rcub_dais_13299
ER -
@conference{
author = "Malinović-Milićević, Slavica",
year = "2022",
abstract = "The parametric model NEOPLANTA was used to study the effects of various
atmospheric conditions on terrestrial spectral UV irradiance. The capability of the model to correctly reproduce processes in the atmosphere is tested by changing input parameters such as ozone content, solar zenith angle, amount and type of aerosols, and altitude. The results of the model testing on input parameter change were satisfactory. As is expected, the amount of UV radiation reaching the surface is the most dependable on ozone layer thickness and solar zenith angle. Erythemal irradiance is more dependent on changes in the amount of ozone in the atmosphere than spectral UV irradiance, showing a significantly greater impact of UV-B radiation on human skin than radiation in the UV-A part of the spectrum.",
publisher = "Belgrade : Institute of Physics Belgrade",
journal = "IV Meeting on Astrophysical Spectroscopy - A&M DATA – Atmosphere. Book of Abstracts and Contributed Papers",
title = "Clear-sky spectral UV radiation modelling",
pages = "10-15",
url = "https://hdl.handle.net/21.15107/rcub_dais_13299"
}
Malinović-Milićević, S.. (2022). Clear-sky spectral UV radiation modelling. in IV Meeting on Astrophysical Spectroscopy - A&M DATA – Atmosphere. Book of Abstracts and Contributed Papers
Belgrade : Institute of Physics Belgrade., 10-15.
https://hdl.handle.net/21.15107/rcub_dais_13299
Malinović-Milićević S. Clear-sky spectral UV radiation modelling. in IV Meeting on Astrophysical Spectroscopy - A&M DATA – Atmosphere. Book of Abstracts and Contributed Papers. 2022;:10-15.
https://hdl.handle.net/21.15107/rcub_dais_13299 .
Malinović-Milićević, Slavica, "Clear-sky spectral UV radiation modelling" in IV Meeting on Astrophysical Spectroscopy - A&M DATA – Atmosphere. Book of Abstracts and Contributed Papers (2022):10-15,
https://hdl.handle.net/21.15107/rcub_dais_13299 .
