Abstract

The zonal averages of temperature (the so-called normal temperatures) for numerous parallels of latitude published between 1852 and 1913 by Dove, Forbes, Ferrel, Spitaler, Batchelder, Arrhenius, von Bezold, Hopfner, von Hann, and Börnstein were used to quantify the global (spherical) and spheroidal mean near-surface temperature of the terrestrial atmosphere. Only the datasets of Dove and Forbes published in the 1850s provided global averages below 〈T〉=14°C, mainly due to the poor coverage of the Southern Hemisphere by observations during that time. The global averages derived from the distributions of normal temperatures published between 1877 and 1913 ranged from 〈T〉=14.0°C (Batchelder) to 〈T〉=15.1°C (Ferrel). The differences between the global and the spheroidal mean near-surface air temperature are marginal. To examine the uncertainty due to interannual variability and different years considered in the historic zonal mean temperature distributions, the historical normal temperatures were perturbed within ±2σ to obtain ensembles of 50 realizations for each dataset. Numerical integrations of the perturbed distributions indicate uncertainties in the global averages in the range of ±0.3°C to ±0.6°C and depended on the number of available normal temperatures. Compared to our results, the global mean temperature of 〈T〉=15.0°C published by von Hann in 1897 and von Bezold in 1901 and 1906 is notably too high, while 〈T〉=14.4°C published by von Hann in 1908 seems to be more adequate within the range of uncertainty. The HadCRUT4 record provided 〈T〉≌ 13.7°C for 1851-1880 and 〈T〉=13.6°C for 1881-1910. The Berkeley record provided 〈T〉=13.6°C and 〈T〉≌ 13.5°C for these periods, respectively. The NASA GISS record yielded 〈T〉=13.6°C for 1881-1910 as well. These results are notably lower than those based on the historic zonal means. For 1991-2018, the HadCRUT4, Berkeley, and NASA GISS records provided 〈T〉=14.4°C, 〈T〉=14.5°C, and 〈T〉=14.5°C, respectively. The comparison of the 1991-2018 globally averaged near-surface temperature with those derived from distributions of zonal temperature averages for numerous parallels of latitude suggests no change for the past 100 years.

Highlights

  • Analyses of global surface-temperature change have been routinely carried out by several groups, including the NASA Goddard Institute for Space Studies (NASA GISS), the NOAA National Climatic DataCenter (NCDC), and a joint effort of the UKMet Office Hadley Centre and the University of East AngliaClimatic Research Unit (HadCRU) [1]

  • Based on Equation (4), the integration of Ts (θ ) from θ = 0 to θ = π provided Ts = 157.2 K. This global mean surface temperature substantially agrees with result of Gerlich and Tscheuschner [91], even though we considered an obliquely rotating Earth in the absence of its atmosphere

  • We used Equation (23) to calculate the respective spheroidal mean near-surface temperature to assess the accuracy of spherical averaging as compared to spheroidal averaging

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Summary

Introduction

The latter two temperature-anomaly records were originally expressed with respect to the CLINO. The first series of the HadCRU observational surface-temperature data set is related to Jones [5]. Since Jones et al [6] found for this

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