1995
DOI: 10.1017/s0376892900010663
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Atmospheric Ozone Trends and Other Factors of Surface Ultraviolet Radiation Variability

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Cited by 70 publications
(16 citation statements)
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“…It is important to remember that snow albedo is most sensitive to impurities. Very recently, Hadley and Kirchstetter (2012) performed laboratory measurements in an effort to quantify the reduction in snow albedo as a function of its contamination with black carbon, which is an important parameter in the available atmospheric solar radiative transfer and climate models (Alexandris et al, 1999;Brandt et al, 2011;Doherty et al, 2010;Flanner et al, 2007;Gallet et al, 2009;Katsambas et al, 1997;Kondratyev et al, 1995;Varotsos, 1995a, b, 1996a, b;Monks et al, 2004;Varotsos et al, 1995). According to Hadley and Kirchstetter (2012), 200 ppb of black carbon is required to decrease the snow albedo by 5 %.…”
Section: A Varotsos Et Al: New Spectral Functions Of Near-groundmentioning
confidence: 99%
“…It is important to remember that snow albedo is most sensitive to impurities. Very recently, Hadley and Kirchstetter (2012) performed laboratory measurements in an effort to quantify the reduction in snow albedo as a function of its contamination with black carbon, which is an important parameter in the available atmospheric solar radiative transfer and climate models (Alexandris et al, 1999;Brandt et al, 2011;Doherty et al, 2010;Flanner et al, 2007;Gallet et al, 2009;Katsambas et al, 1997;Kondratyev et al, 1995;Varotsos, 1995a, b, 1996a, b;Monks et al, 2004;Varotsos et al, 1995). According to Hadley and Kirchstetter (2012), 200 ppb of black carbon is required to decrease the snow albedo by 5 %.…”
Section: A Varotsos Et Al: New Spectral Functions Of Near-groundmentioning
confidence: 99%
“…The comparison of the theoretical algorithm's results with the corresponding experimental data showed a very good agreement. The theoretical algorithm gave us the chance of studying the fluctuations not only of the direct and diffuse UV radiation but also of the entire radiation, in different spectral areas (Kondratyev et al 1995.…”
Section: Measurements Of the Erythemal Uv Radiation At Various Atmospmentioning
confidence: 99%
“…As the temperature of an emitting surface increases, the maximum wavelength of the emitted radiation increases too. Smith and Gottlieb (1974) re-examined the subject of photon solar flux and its variations vs. wavelength and showed that variations in the extreme ultraviolet (UV) spectrum and in the X-ray of solar flux may reach high orders of magnitude causing significant changes in the Earth's ionosphere, especially during major solar flares (Kondratyev et al, 1995;Kondratyev and Varotsos, 1996;Ziemke et al, 2000;Varotsos et al, 2001;Melnikova, 2009;Tzanis et al, 2009;Xue et al, 2011;Cracknell et al, 2014). Solanki and Unruh (1998) proposed simple models of the total solar irradiance variations vs. wavelength showing that variations on solar flux are mainly caused by magnetic fields at the solar surface.…”
Section: Introductionmentioning
confidence: 99%