1 Supporting Material 2 Impact of volcanic stratospheric aerosols on diurnal temperature range (DTR) in 3 Europe over the past 200 years: observations versus model simulations 4 5 Renate Auchmann1, Florian Arfeuille1, Martin Wegmann1, Jörg Franke1, 6 Mariano Barriendos2, Marc Prohom3, Arturo Sanchez-Lorenzo4,5, Jonas Bhend6, 7 Martin Wild4, Doris Folini4, Petr Štěpánek7, and Stefan Brönnimann1 8 9 1 Institute of Geography and Oeschger Centre for Climate Change Research, 10 University of Bern, Switzerland 11 2 Department of Modern History, University of Barcelona, Barcelona, Spain 12 3 Catalan Meteorological Service (SMC, Meteocat), Barcelona, Spain 13 4 Institute for Atmospheric and Climate Science, ETH Zurich, Switzerland 14 5 Department of Physics, University of Girona, Girona, Spain 15 6 CSIRO Marine and Atmospheric Research, Aspendale, Australia 16 7 Global Change Research Centre AS CR, v.v.i., Brno, Czech Republic 17 18 19 Corresponding author: R. Auchmann, Institute of Geography and Oeschger Centre for 20 Climate 21 (renate.auchmann@giub.unibe.ch) 22 Change Research, University of Bern, Switzerland. 23 1. Details on station information and homogeneity of records 24 25 26 Geneva Continuous observations in Geneva began in the late 18th century. During the 27 first period of observations, temperature measurements were performed twice daily 28 (once at sunrise and again at 14:00 LT), approximating the daily minimum (Tn) and 29 maximum (Tx) temperatures, respectively [Auchmann et al., 2012]. Only occasionally 30 were sunset measurements also performed. Within the DigiHom project [Füllemann et 31 al., 2011], all sub-daily observations and measurements from Geneva during the 32 period 1799–1863 were digitized. Internally homogeneous temperature data are 33 available in the period 1799-1821; Auchmann et al. [2012] corrected the temperature 34 data for an artificial trend and standardized the units. During this period, the station 35 was located in the old botanical garden. The same mercury thermometer was used and 36 placed in the shadow of a stake (Bibl. Brit. Vol. 1). 37 Tx and Tn are available from 1863 to present (MeteoSwiss, IDAWEB). Since 38 1863, the station (at that time located at the Observatoire de Genève) has undergone 39 several changes; in April 1959 the station was relocated to the airport (Genève- 40 Cointrin), around 5 km northwest of the city and a new thermometer screen was 41 installed. Until 1966 measurements continued in parallel at the Observatoire de 42 Genève. The relocation and instrumentation change caused inhomogeneities in the 43 series [Z'graggen, 2006]. However, this is outside of our reference periods. In 1980, 44 the English screen was exchanged by a ventilated thermometer, which did not cause 45 significant inhomogeneities [Z'graggen, 2006; Kuglitsch et al., 2012]. 46 Kuglitsch et al. (2012) compiled all documented changes in the Tx/Tn series 47 from metadata and station history records and compared them to the results of three 48 break detection algorithms. We use this information to determine the homogeneous 49 reference periods. 50 Cloud cover observations had been performed twice daily from the very 51 beginning. Until 1863, heterogeneous descriptions (sometimes very detailed) were 52 noted. The original descriptions in the period 1799–1821 have been classified into six 53 categories [Auchmann et al., 2012]. However, the cloud cover series seems to only be 54 homogeneous from around 1812 onwards. In the period from 1874 to present, cloud 55 cover observations have been performed thrice daily and given in octas. Overall, the 56 change in cloud cover categories may lead to inhomogeneities during the study 57 period, which is accounted for when determining homogeneous sub-periods. We use 58 the 7:00 and the 12:00 observations to determine sky conditions at the time of Tx and 59 Tn, respectively. The year 1900 is almost completely missing. In the period 1962–65, 60 around 25% of only the noon series is missing (i.e., mainly weekend observations). 61 This might be a consequence of the relocation to the airport, a possible change in 62 observation practices, or variable observers. In this period, we only use the morning 63 sky observation to determine a clear day. 64 65 66 Basel Continuous observations in Basel began in the mid-18th century [Bider et al., 67 1958]. From 1876 onwards, daily Tn and Tx were measured and are used use in this 68 study. From 1885 to 1897, there is a gap in the series. The station experienced a major 69 relocation in 1929 from the Bernoullianum to Basel-Binningen, which caused an 70 inhomogeneity in the series [Z'graggen, 2006]. In 1966, the Wild screen was replaced 71 by a Stevenson screen [Auchmann and Brönnimann, 2012], introducing an additional 72 inhomogeneity to the series. To account for this inhomogeneity, we set the base 73 period for the Agung eruption (other stations 1960–90) to 1935–65 (Table S2). From 74 1978 onwards, a ventilated thermometer was used, introducing another 75 inhomogeneity, which we considered when determining the base periods (Table S2). 76 Thrice daily cloud cover observations are digitally available from 1864 77 onwards and are given in nine categories (octas). Since 1981, ten cloud cover 78 categories are used (i.e., with the tenth category representing foggy conditions). 79 Again, the change in categories may lead to inhomogeneities, which are accounted for 80 when determining the homogeneous sub-periods. Nothing is known about changes in 81 observers, which might be a further reason for inhomogeneities. A visual inspection 82 of the series homogeneity reveals a possible change in the frequency distribution in 83 1929 (i.e., coincident with the relocation of the station). 84 85 86 Prague The station Prague-Klementinum started continuous meteorological 87 measurements in 1775. Prague-Klementinum is located in the Old Town of Prague in 88 the College of St. Clement. Hence, the station has always been urban [Brázdil and 89 Budiková, 1999]. In the beginning of the series, temperature was measured near the 90 window of a second-story flatin a metal screen attached to a north-facing wall (11 m 91 above ground) in a closed courtyard [Brázdil and Budiková, 1999]. From 1775 to 92 1889, the thermometer has shifted several times between the second and first floors. 93 Since then, the thermometer has been permanently installed on the first floor [Brázdil 94 and Budiková, 1999]. Also some “structural changes in the courtyard” [Brázdil and 95 Budiková, 1999] were reported in 1863, 1924, and 1929. According to Hlaváč [1937] 96 [Brázdil and Budiková, 1999] none of those changes caused inhomogeneities in the 97 series. However, as an urban site, urban heating effects have biased the temperatures 98 series [Brázdil and Dobrovolný, 1993; Brázdil and Budiková, 1999] . Because we 99 consider anomalies in contemporary (short) reference periods, this is assumed to be 100 irrelevant. We use the Tn and Tx series, which represent minimum and maximum 101 temperatures for a period of 24 hours, from 21 to 21 UTC+1 (ECA&D). 102 Cloud cover observations have also been performed from the beginning of the 103 series. However, the data has not been analyzed or used for any studies so far (email 104 communication, Nemec, L., 2011). Cloud cover is given in tenths throughout the 105 period. Missing values only occur in 1870, 1903 (ca. 25 values), 1939 (ca. 4 months), 106 and during a longer period (1961–91) during which no morning cloud cover 107 observations are available. For the latter, we selected clear-sky days based only on the 108 noon cloud cover observations. Nothing is known about the changes in observers, 109 which may lead to inhomogeneities in the series. We visually inspected the temporal 110 homogeneity of the cloud cover series and found the period 1840 to1843 very likely 111 to be inhomogeneous. Another noticeable period starts around 1897 and ends (for the 112 morning series) around 1919, when more fully covered days were observed. However, 113 the transition is gradual and there is no clear evidence of an inhomogeneity. We 114 determine the reference periods accordingly, for instance, for Krakatau (Table S2). 115 116 117 Barcelona Meteorological observations in Barcelona started in 1780 [Trigo et al., 2009], 118 but little is known about instruments and observational techniques [Rodríguez et al., 119 2001]. Three observations are taken per day (i.e., at 7:00, 12:00, and 22:00). 120 However, nothing is known about the exactness of observation times. In our study, we 121 use the 7:00 and 12:00 temperature series, assuming that the morning series 122 approximate daily minimum temperatures and that the noon series are close to the 123 daily maximum temperatures. It has been reported that, at least during the first period, 124 observations were taken outside and on a north-facing wall [Trigo et al., 2009]. In 125 1885, the first official observations were made [Rodríguez et al., 2001; Trigo et al., 126 2009]. At the moment, data for the early period are only available in digital format 127 from1780 to 1825. Several efforts are made to complete both the temperature and 128 cloud cover sub-daily series following the study proposed in Prohom et al. [2012]. 129 These and should be available shortly. 130 Throughout the 19th century many changes are reported making the Barcelona 131 series discontinuous [Trigo et al., 2009]. For this early period, cloud cover 132 observations are reported in three categories: clear, presence of clouds (different 133 density), and total sky coverage . However, the data had not yet been explored. We 134 inspected the cloud cover series visually and found the early series to be 135 homogeneous. 136 Tx and Tn series are available from 1924 onwards (ECA&D). However, there 137 is a gap starting on December 1, 1927 and lasting until 1943. Measurements after 138 1943 were taken at the airport [Rodríguez et al., 2001]. 139 For the period 1961–2011, cloud cover is only available as a daily mean 140 (calculated as the mean of the 7:00, 13:00, and 18:00 observations) and is given in 141 nine categories. Nothing is known about the changes in observers, which may lead to 142 inhomogeneities in the series. A visual homogeneity inspection did not reveal any 143 notable breaks in the series. 144 145 146 Hohenpeissenberg Hohenpeissenberg is situated in Bavaria, southern Germany, in the northern 147 pre-Alps. Meteorological measurements and observations at Hohenpeissenberg started 148 in 1781 (at that time a monastery). Hence, Hohenpeissenberg is one of the oldest 149 mountain observatories in Europe and worldwide. Many of the records are available 150 without discontinuities since the beginning of the measurements [Winkler, 2009]. In 151 contrast to many other European stations the location of the station did not change 152 over time (i.e., no large station relocations were undertaken). The station of 153 Hohenpeissenberg is located on a mountain (Hoher Peissenberg; 985 m a.s.l.), which 154 offers several advantages. First, the environment around the station has not changed 155 considerably over the past 200 years. Relative to stations located within city centers or 156 suburbs, the temperature series of the isolated Hohenpeissenberg are independent of 157 urban heating effects [Mitchell, 1953; Winkler, 2009]. Second, due to the location on 158 a stand-alone mountain, daily variability is damped compared to surrounding stations 159 in the valley, which are heavily influenced by ground-level cold air during the 160 nighttime [Winkler, 2009]. 161 162 163 164 Thrice daily measurements have been taken since 1781. However, Tn and Tx measurements and cloud cover observations have been continuously taken since 1879. Auer et al. (2007) homogenized monthly mean temperature series for the ‘Greater Alpine Region’ including Hohenpeissenberg. We compared the 165 homogenized monthly series to monthly averages calculated from our data (with daily 166 mean = (Tx+Tn)/2) and show the difference series (homogenized minus our raw data) 167 in Figure S1. We use metadata from Hohenpeissenberg together with Figure S1 to 168 define homogeneous sub-periods as reference periods. 169 Cloud cover is observed thrice daily (at 6:00, 12:00, and 18:00 UTC) 170 throughout the period 1879–2009 and given in nine categories (octas). Times are 171 given in UTC throughout the paper unless otherwise noted. Comprehensive metadata 172 and information on the station history, instruments, data quality, and observers are 173 available for Hohenpeissenberg. A detailed compilation and summary of the available 174 material and sources was performed by the DWD and Winkler [2009, and references 175 therein]. Large changes at Hohenpeissenberg that could have affected the Tx and Tn 176 series or the cloud cover observations are listed in Table S1. 177 We visually inspect the homogeneity of the cloud cover series, which reveals 178 an overall general change in the distribution of the cloud cover frequencies around the 179 mid- to end of the 1930s. A change in general measurement techniques and 180 responsibilities on December 1, 1936 [Winkler, 2009; see Table S1] may be the 181 reason for this change in the frequency distribution. From 1879 to 1936, 12 different 182 official observers (usually priests or vicars) were in charge. However, usually the 183 measurements were read and observations were also done by helpers (e.g., teachers or 184 the cook of the parish; see Table S1). From 1937 to 1940, five technical employees of 185 the “Reichswetterdienst” made the observations (DWD station history). From 1940 186 until now, employees of the mountain station have been in charge of the observations. 187 Also in 1940, a small relocation of the station was undertaken, including a vertical 188 shift of 10m (DWD station history), which could have affected the Tx and Tn series. 189 In addition, a change in the extreme thermometers was reported around 1937. In 1971, 190 electronic data processing equipment was installed. 191 192 2. Base and reference periods 193 194 195 References Auchmann, R. and S. Brönnimann (2012), A physics-based correction model 196 for homogenizing sub-daily temperature series, J. Geophys. Res., 117(D17), D17119, 197 doi:10.1029/2012JD018067. 198 Auchmann, R., S. Brönnimann, L. Breda, M. Bühler, R. Spadin, and A. 199 Stickler (2012), Extreme climate, not extreme weather: the summer of 1816 in 200 Geneva, Switzerland, Clim. Past, 8(1), 325–335, doi:10.5194/cp-8-325-2012. 201 Auer, I., Böhm, R., Jurkovic, A., Lipa, W., Orlik, A., Potzmann, R., Schöner, 202 W., Ungersböck, M., Matulla, C., Briffa, K., Jones, P.D., Efthymiadis, D., Brunetti, 203 M., Nanni, T, Maugeri, M., Mercalli, L., Mestre, O., Moisselin, J.-M., Begert, M., 204 Müller-Westermeier, G., Kveton, V., Bochnicek, O., Stastny, P., Lapin, M., Szalai, S., 205 Szentimrey, T., Cegnar, T., Dolinar, M., Gajic-Capka, M., Zaninovic, K., Majstorovic, 206 Z., and E. Nieplova (2007), HISTALP – Historical instrumental climatological 207 surface time series of the greater Alpine region 1760-2003, Int. J. Climatol., 27, 17-46, 208 doi: 10.1002/joc.1377. 209 Bider, M., M. Schüepp, and H. Rudloff (1958), Die Reduktion der 200jährigen 210 Basler Temperaturreihe. Archiv für Meteorologie, Geophysik und Bioklimatologie, 211 Serie B, 9(3–4): 360–412, LA – German, doi:10.1007/BF02243047. 212 Brázdil, R. and M. Budiková (1999), An urban bias in air temperature 213 fluctuations at the Klementinum, Prague, The Czech Republic, Atmospheric 214 Environment, 33 (24–25), 4211–4217. 215 Brázdil, R. and P. Dobrovolný (1993), The utilization of long temperature 216 series for studying climatic fluctuations in central Europe, Zeszyty Naukowe 217 Uniwersytetu Jagiellonskiego, Prace Geogr., 95, 151–162. 218 Fischer, E. M., J. Luterbacher, E. Zorita, S. F. B. Tett, C. Casty, and H. 219 Wanner (2007), European climate response to tropical volcanic eruptions over the last 220 half millennium, Geophys. Res. Lett., 34(5), L05707, doi:10.1029/2006GL027992. 221 Füllemann, C., M. Begert, M. Croci-Maspoli, and S. Brönnimann (2011), 222 Digitalisieren und Homogenisieren von historischen Klimadaten des Swiss NBCN 223 Resultate aus DigiHom, Technical report, Arbeitsber. MeteoSwiss, Zürich, 224 Switzerland. 225 Hlaváč, V. (1937), Temperature Patterns of the Capital of Prague, Praha, 95. 226 Kuglitsch, F. G., R. Auchmann, R. Bleisch, S. Brönnimann, O. Martius, and 227 M. Stewart (2012), Break detection of annual Swiss temperature series, J. Geophys. 228 Res., 117, D13105, doi:10.1029/2012JD017729. 229 230 Mitchell, J. (1953), On the causes of instrumentally observed secular temperature trends, J. Met., 10, 244–261. 231 232 Pfister, C. (1999), Wetternachhersage - 500 Jahre Klimavariationen und Naturkatastrophen (1496–1995), Bern: Paul Haupt. 233 Prohom, M., Barriendos, M., Aguilar, E. and Ripoll, R. (2012), Recuperación 234 y análisis de la serie de temperatura diaria de Barcelona, 1780-2011. Cambio 235 climático. Extremos e impactos. Publicaciones de la Asociación Española de 236 Climatología (AEC), Serie A, nº 8. Salamanca, ISBN: 978-84-695-4331-3, pp. 207– 237 217. 238 Rodríguez, R., M. Barriendos, P. D. Jones, J. Martín-Vide, and J. C. Peña 239 (2001), Long pressure series for Barcelona (Spain), Daily reconstruction and monthly 240 homogenization, Int. J. Climatol., 21(13), 1693-1704, doi:10.1002/joc.696. 241 242 Trigo, R. M., J. M. Vaquero, M.-J. a. Alcoforado, M. Barriendos, J. a. Taborda, R. García-Herrera, and J. Luterbacher (2009), Iberia in 1816, the year without a 243 summer, Int. J. Climatol., 29(1), 99–115, doi:10.1002/joc.1693. 244 Winkler, P. (2009), Wissenschaftshistorische Untersuchungen zur Geschichte 245 und insbesondere zur Datenqualität der langen meteorologischen Reihen des 246 Observatoriums Hohenpeissenberg, Berichte des Deutschen Wetterdienstes, 233(1), 247 187 pp, doi:10.1007/s00704-009-0108-y. 248 Z'graggen, L. (2006), Die Maximaltemperaturen im Hitzesommer 2003 und 249 Vergleich zu früheren Extremtemperaturen, Arbeitsberichte der MeteoSchweiz, 212, 250 74 pp. 251 252 253 254 255 256 257 258 259 Table S1. Large changes at the site Hohenpeissenberg. Date Type of change Change 1936 Measurement technique 1.12.1936 1937 1940 Official competence Instrument Observer 1971 Measurement technique Window screen (outside window on northern wall of house on second floor) replaced by free-standing shelter screen “Reichswetterdienst” Change in the extreme thermometers Employees of the mountain station were in charge of the observations Electronic data processing equipment was installed Possibly affected Tx and Tn Cloud cover Tx and Tn Cloud cover Tx and Tn 260 261 262 263 264 265 266 267 268 269 Table S2. Base periods (length of reference periods in parentheses) provided in years. Krakatau 1883 1874– 99 (23) 1871– 96 (23) 1879– 1901 (20) Santa Maria 1902 1890– 1920 (25) 1897– 1919 (17) 1890– 1920 (25) 1800–21 (16) — — — 1961–90 (24) — 1876– 1920 (25) 1876– 1920 (25) 1898– 1927 (25) 1938–65 (25) Unknown Tambora 1809 1815 GE — 1812–21 (7) PR 1799– 1825 (21) 1799– 1825 (21) HP — — BC 1800–21 (16) BS — Katmai Agung 1912 1897– 1927 (26) 1897– 1919 (17) 1897– 1927 (26) 1963 1939–65 (24) 1961–91 (25) 1960–90 (25) El Chichón 1982 1970– 2000 (25) 1970– 2000 (25) Pinatubo 1991 1980– 2010 (25) 1980– 2010 (25) 1971–99 (23) 1971–99 (23) 1970– 2000 (25) 1980– 2010 (25) 1970– 2000 (25) 1980– 2010 (25) 285 Figure S1: Difference series of homogenized monthly temperature series from 286 Hohenpeissenberg from the HISTALP (Historical Instrumental Climatological 287 Surface Time Series of the Greater Alpine Region) project by Auer et al. (2007) 288 minus raw monthly mean temperatures calculated from the data used in this study. T diff [histalp - study] (°C) -4 -3 -2 -1 0 1 2 1879/1 1880/1 1881/1 1882/1 1883/1 1884/1 1885/1 1886/1 1887/1 1888/1 1889/1 1890/1 1891/1 1892/1 1893/1 1894/1 1895/1 1896/1 1897/1 1898/1 1899/1 1900/1 1901/1 1902/1 1903/1 1904/1 1905/1 1906/1 1907/1 1908/1 1909/1 1910/1 1911/1 1912/1 1913/1 1914/1 1915/1 1916/1 1917/1 1918/1 1919/1 1920/1 1921/1 1922/1 1923/1 1924/1 1925/1 1926/1 1927/1 1928/1 1929/1 1930/1 1931/1 1932/1 1933/1 1934/1 1935/1 1936/1 1937/1 1938/1 1939/1 1940/1 1941/1 1942/1 1943/1 1944/1 1945/1 1946/1 1947/1 1948/1 1949/1 1950/1 1951/1 1952/1 1953/1 1954/1 1955/1 1956/1 1957/1 1958/1 1959/1 1960/1 1961/1 1962/1 1963/1 1964/1 1965/1 1966/1 1967/1 1968/1 1969/1 1970/1 1971/1 1972/1 1973/1 1974/1 1975/1 1976/1 1977/1 1978/1 1979/1 1980/1 1981/1 1982/1 1983/1 1984/1 1985/1 1986/1 1987/1 1988/1 1989/1 1990/1 1991/1 1992/1 1993/1 1994/1 1995/1 1996/1 1997/1 1998/1 1999/1 284 283 282 281 280 279 278 277 276 275 274 273 272 271 270