Oecologia (2007) 154:247–258 DOI 10.1007/s00442-007-0832-x ECOPHYSIOLOGY Past climate changes and ecophysiological responses recorded in the isotope ratios of saguaro cactus spines Nathan B. English Æ David L. Dettman Æ Darren R. Sandquist Æ David G. Williams Received: 16 May 2007 / Accepted: 19 July 2007 / Published online: 28 August 2007 Springer-Verlag 2007 Abstract The stable isotope composition of spines produced serially from the apex of columnar cacti has the potential to be used as a record of changes in climate and physiology. To investigate this potential, we measured the d18O, d13C and F14C values of spines from a long-lived columnar cactus, saguaro (Carnegiea gigantea). To determine plant age, we collected spines at 11 different heights along one rib from the stem apex (3.77 m height) to the base of a naturally occurring saguaro. Fractions of modern carbon (F14C) ranged from 0.9679 to 1.5537, which is consistent with ages between 1950 and 2004. We observed a very strong positive correlation (r = 0.997) between the F14C age of spines and the age of spines determined from direct and repeated height measurements taken on this individual over the past 37 years. A series of 96 spines collected from this individual had d18O values ranging from 38% to 50% [Vienna standard mean ocean water (VSMOW)] and d13C values from 11.5% to 8.5% [Vienna Peedee belemnite (VPDB)]. The d18O and d13C values of spines were positively correlated (r = 0.45, P \ 0.0001) and showed near-annual oscillations over the Communicated by Frederick C. Meinzer. N. B. English (&) D. L. Dettman Department of Geosciences, University of Arizona, 4810 E 4th Street, Bldg #77, Tucson, AZ 85721, USA e-mail: nenglish@email.arizona.edu D. R. Sandquist Department of Biological Science, California State University, Fullerton, CA, USA D. G. Williams Departments of Renewable Resources and Botany, University of Wyoming, Laramie, WY, USA 15-year record. This pattern suggests that seasonal periods of reduced evaporative demand or greater precipitation input may correspond to increased daytime CO2 uptake. The lowest d18O and d13C values of spines observed occurred during the 1983 and 1993 El Niño years, suggesting that the stable isotope composition recorded in spine tissue may serve as a proxy for these climate events. We compared empirical models and data from potted experimental cacti to validate these observations and test our hypotheses. The isotopic records presented here are the first ever reported from a chronosequence of cactus spines and demonstrate that tissues of columnar cacti, and potentially other long-lived succulents, may contain a record of past physiological and climatic variation. Keywords Stable isotopes Oxygen-18 Carbon-13 Growth rate Carnegiea gigantea Cactus Radiocarbon El Niño southern oscillation (ENSO) Introduction Variation in stable isotope ratios of oxygen (d18O), hydrogen (d2H) and carbon (d13C) in tissues that are incrementally produced and preserved in plants, such as tree-rings, is commonly exploited to reconstruct past environmental changes and investigate associated plant metabolic and physiological responses (e.g., Roberts et al. 1997; Roden et al. 2000; Dawson et al. 2002; McCarroll and Loader 2004; Cernusak et al. 2005; Wright and Leavitt 2006; West et al. 2006). There are few studies documenting isotopic variation in stem succulents, and none that we are aware of that show isotopic variation in tissues that are produced incrementally. Isotope measurements on tissues that are sequentially added and preserved on stem 123 248 succulents, such as spines, could be very useful proxies for reconstructing past climatic events and documenting responses to environmental change, especially in desert regions lacking other suitable proxies for recent climate changes. The massive, long-lived (125–175 years) saguaro cactus [Carnegiea gigantea (Engelmann) Britton & Rose] occurs throughout the Sonoran Desert in southwestern Arizona and western Sonora, Mexico (Turner et al. 1995). In this region, monsoon rains that occur between July and September may provide up to 50% of the mean annual precipitation (Eastoe et al. 2004), with the remainder falling mostly during the winter and spring. The monsoon is an important source of water for saguaro growth in some instances (Drezner 2005). However, stronger correlations have been found between measures of saguaro success (i.e., branching, stem diameter and seedling recruitment) and winter/spring rainfall (Drezner 2003a, b; Drezner and Balling 2002), mediated by the uptake and storage of winter/spring rainfall in the stem or through the prolonged presence of soil moisture in the hot and dry pre-monsoon months. Such precipitation is greatly enhanced during the El Niño phase of the El Niño southern oscillation (ENSO) (Gutzler et al. 2002), but it is unclear how this climatic anomaly has affected, or will affect, saguaro water balance, photosynthetic metabolism, growth and fruit production. Given the relationships with winter/spring precipitation, El Niño years are likely to have a pronounced influence on saguaro growth, reproduction and demography, as well as on the consumers that rely on resources provided by this dominant stem succulent. As in other cacti, saguaro spines develop on areoles near the shoot apical meristem (Mauseth 2006). Areoles and spines are displaced laterally on the large dome-shaped apex of the cactus stem as new areoles are produced (Gibson and Nobel 1986; Mauseth 2006). Spines closer to the apex are therefore younger than spines lower on the stem. Between four and eight areoles, each having about 15 spines, form on each elongate set of fused tubercles (the ‘rib’ of the stem) each year (N. English, personal observation), with the majority of growth occurring during warm periods, i.e., April–October (Steenbergh and Lowe 1983). Spines are highly lignified organs with no secondary growth, as the cells die within days after they are formed (Gibson and Nobel 1986; Mauseth 2006). The lignified spines are very durable and are retained on the plant for decades; thus, isotopic ratios of spines may provide a useful record of environmental and physiological information in a manner similar to that of tree rings. In this paper we: (1) present a theoretical framework that relates the isotopic variation of cactus water and spines to temporal and physical changes in the environment; (2) describe the methods used to collect and prepare cactus 123 Oecologia (2007) 154:247–258 stem-water and spine samples for isotopic analysis; (3) develop and test a model for the isotopic enrichment of cactus stem-water, using experimental potted saguaro plants; (4) demonstrate the accuracy and utility of fractions of modern carbon (F14C) (radiocarbon) dating in establishing growth models and spine formation dates for naturally grown saguaro plants; and (5) evaluate a dated, multi-year record of d18O and d13C values from spines of a naturally occurring cactus and compare these values to local precipitation records. Theory Oxygen and hydrogen isotope variation in cactus water and tissue Large stem succulents in the Sonoran Desert, like saguaro, take up water during very discrete intervals (days) after precipitation events, and then lose water slowly over lengthy dry periods between precipitation events (Gibson and Nobel 1986). Isotopic enrichment of stem water due to evaporation during intervening dry periods in saguaro and other stem succulents can be described by Rayleigh fractionation, expressed as: dsw ¼ ðdi þ 1000Þfeða1v 1Þ 1000 ð1Þ where dsw is the d18O or d2H value of stem water after evaporation, di is the initial d18O or d2H value of water in the stem, fe is the fraction of water lost from the stem due to evaporation, and a1v is the fractionation during evaporation, which is the sum of an equilibrium fractionation related to mean minimum temperature, and a kinetic fractionation related to mean maximum relative humidity (for a lucid demonstration of how to calculate these values, see Clark and Fritz 1997). We use mean minimum temperature and mean maximum relative humidity because these most likely represent night-time values, when stomates are open and the majority of gas exchange occurs for plants with a crassulacean acid metabolism (CAM). This simple model can be used to examine variation in d18O and d2H values of water at the stem apex, where spine development occurs. When new water is added to the stem (recharged) and well mixed, the water isotope value (dsw*) of the new stem is determined by a two-component mixing model: dsw ¼ dsw ð1 fr Þ þ dr ðfr Þ 18 ð2Þ 2 where dsw is the d O or d H value of stem water before recharge (Eq. 1), fr is the fraction of new water added to the stem and dr is the d18O or d2H value of this recharge water (e.g., rainfall). fr can be estimated from changes in stem diameter, since the majority of water in columnar cacti is Oecologia (2007) 154:247–258 249 stored in the cortex and the stem will expand or contract in direct proportion to the amount of water taken up or lost, respectively, by the cortical tissues (McAuliffe and Janzen 1986). The fraction of water taken up (fr), or lost (fe), can, therefore, be calculated from changes in plant diameter, assuming the cactus shape approximates that of a cylinder (Mauseth 2000) or by weighing the plant. The oxygen or hydrogen isotope ratio of spine tissue (d18Ospine or d2Hspine) can be expressed as: dspine ¼ ½f ðdswapex þ 1000Þ abio þ ð1 f Þ ðdswchlorenchyma þ 1000Þ abio 1000 ð3Þ where dsw-apex is the oxygen or hydrogen isotope value of water at the stem apex (dsw or dsw* from the above equations) where spine tissue is synthesized, dsw-chlorenchyma is the isotope value of water at the source of photosynthetic carbon dioxide assimilation in chlorenchyma, abio is the fractionation factor for oxygen (eO) or hydrogen (eH) associated with the biosynthesis of plant tissue, and f is the fraction of carbon-bound oxygen or hydrogen in photosynthetic sugars that undergoes exchange with medium water during spine tissue synthesis (for a thorough discussion of the variables in this model, see Roden and Ehleringer 1999; Roden et al. 2000; McCarroll and Loader 2004). Although f may vary among taxa, for saguaro we apply values reported in the literature for cellulose synthesis in other dicotyledonous plants (i.e., trees, Roden et al. 2000). Note that, if the source of photosynthates for spine formation is near the apex (i.e., dsw-chlorenchyma & dsw-apex), then Eq. 3 simplifies to: dspine ¼ ½ðdswapex þ 1000Þ abio 1000: ð4Þ Carbon isotope variation in cactus tissue Over short-term intervals (i.e., seasons to years), the isotopic variation of carbon in mature photosynthetic organs is most greatly influenced by physiological processes affecting carbon isotope fractionation during CO2 assimilation and compound synthesis (O’Leary 1988) and, to a lesser degree, by seasonal variations in the d13C of atmospheric CO2 (0.2%, Keeling et al. 1979). Crassulacean acid metabolism (CAM) photosynthesis involves the initial fixation of atmospheric CO2 by phosphoenolpyruvate-carboxylase (PEPc) at night, when stomates are open and photosynthate is stored as malate (referred to as CAM phase I; Dodd et al. 2002; Winter and Holtum 2002). At dawn, while the stomates are still open, ribulose-1,5-bisphosphate carboxylase (Rubisco) activity in the chloroplast increases as malate begins to be converted back to CO2 and atmospheric CO2 is also available for assimilation (phase II). This short phase is followed by a prolonged period of malate decarboxylation during the daytime, when stomates are closed, and only malate-released CO2 is fixed by Rubisco in the Calvin cycle (phase III). Near the end of the day, when all the malate has been consumed and internal pCO2 has declined, stomates may open again and allow direct assimilation of atmospheric CO2 by Rubisco (phase IV). Each phase of CAM photosynthesis affects isotopic discrimination of carbon (D13C) to varying degrees and thus influences the isotopic ratio of the plant relative to air (d13Cplant & d13Cair D13C). At night (phase I), D13C is partially determined by changes in the balance of stomatal conductance (CO2 ‘‘supply’’) and PEPc activity (CO2 ‘‘demand’’) during CO2 uptake. During the day, when the stomates are closed (phase III), D13C is moderated by the degree of CO2 leakage out of tissues. These fractionation processes are diffusion-regulated, but enzymatically driven fractionation also affects D13C in CAM plants (Winter and Holtum 2002). When the stomates are open and the sun is up (phases II and IV), atmospheric CO2 taken up by Rubisco (D13C = 27%) modifies D13C as it would in a C3 plant. Enzymatic uptake of CO2 by PEPc (D13C = 2%) when the stomates are open at night (phase I) also modifies D13C (O’Leary 1988; Griffiths 1992). CAM plants grown in mesic environments tend to have more negative values of tissue d13C than do those grown in dry conditions (Schulze et al. 1976; Osmond 1978; Winter and Holtum 2002). Two factors likely account for this pattern: (1) substantial daytime CO2 assimilation and associated expression of Rubisco fractionation with either early morning or late afternoon CO2 uptake during wet periods (CAM phases II and IV), or (2) enhanced leakage of 13 C-enriched CO2 when stomates are closed (phase III; Griffiths et al. 1990; Haslam et al. 2003). A simple model for d13C variation in obligate CAM species (Despain et al. 1970) discounts the impact of daytime CO2 assimilation—a valid assumption for saguaro during extremely dry periods (Lajtha et al. 1997). However, under favorable conditions (moderate temperatures and moist soil), a large stemmed cactus also common to the Sonoran desert [Ferocactus ancanthodes (Lem.) Britt. & Rose] was shown to acquire between 9% and 13% of its CO2 in the early morning and late afternoon (phases II and IV; Gibson and Nobel 1986). Given the large difference in D13C between Rubisco- and PEPc-mediated CO2 uptake, small amounts of CO2 acquired at dawn and in the late afternoon can have a disproportionate impact on the final d13C values of cactus tissues. We predict that the d13C values of spines of saguaro should increase during drought periods on an annual and interannual basis (decreased phase II and IV photosynthesis) and should decline with more favorable conditions (increased phase II and IV photosynthesis), especially in years with 123 250 above-average rainfall, such as during a strong monsoon year or after substantial winter rains (e.g., El Niño years). Oecologia (2007) 154:247–258 vacuum distillation to extract stem water (Ehleringer et al. 2000) for isotope analysis. Boreholes in the stems were plugged with 6-cm-long wooden dowels (10 mm diameter) immediately after sample collection. Methods Experiment with potted saguaro Spine sampling from a naturally occurring saguaro Four 0.8 m tall saguaro plants, purchased from a local nursery in June 2004, were grown in 10-gal (38 l) pots outdoors in full sunlight at the University of Arizona Desert Laboratory, Tucson, AZ, USA (32.22 N, 111.00 W, 800 m elevation). These plants were used to investigate the influence of evaporation and recharge on the d18O and d2H values of water at the stem apex. The plants were allowed to acclimate for 8 months, being frequently watered prior to experimentation (at least once every 1 or 2 weeks, as needed) using Tucson municipal water: d18O = 8.4%; d2H = 61%. In order to induce drought we withheld all irrigation from the cacti between 28 April and 26 July 2005. We excluded meteoric water inputs from the potted soil for the drought cycle by covering the pots around the base of each plant with heavy plastic. Precipitation (recorded daily at Tumamoc Hill by J. Bowers, personal communication) may have reached the soil through gaps in the plastic or by running down the stem, but very little of the 23.4 mm of rainfall (d18O = 1%; d2H = 7%) recorded during the drought cycle reached the soil. After the plastic had been removed (27 July 2005), the cacti took up water from irrigation (provided at the same frequency as before) and natural precipitation through October 2005. We measured stem diameter at 15 cm below the stem apex and total plant mass changes for each plant to calculate water recharge and evaporative losses. We determined plant mass by weighing each plant, plus its pot and soil (altogether 46 kg), on a lysimeter. We used the monthly mass of each plant during the experiment, minus the dry weight of the pot and soil, to determine fe or fr. We subtracted 4 kg from the first and last months of the experiment (April and October, respectively) to account for the mass of water in saturated potting soils (4 l holding capacity in the 10-gal pots). The potting soils were dry during the other months of the experiment when the plants were weighed. We took tissue samples from the stem epidermis and cortex monthly, using a 9-mm-diameter cork borer inserted between ribs slightly below the apex and perpendicular to the plant surface on the north side. The 6cm long cores were divided into two subsamples, representing sections from the surface to 3 cm (chlorenchyma and parenchyma) depth and from 3 to 6 cm depth (parenchyma only, but no wood tissue). The samples were sealed in glass vials and stored in a freezer, and the surface to 3 cm samples were later processed using cryogenic We sampled spines for isotopic analysis from the northernmost rib of Saguaro 162, a 3.7-m-tall, single-stemmed, saguaro cactus whose height had been measured repeatedly over 38 years as part of an effort to establish growth models for saguaro (Pierson and Turner 1998). Saguaro 162 is located at the University of Arizona Desert Laboratory at Tumamoc Hill, Tucson, AZ, USA. We used a 4-m-tall orchard ladder (Stokes Ladders, Kelseyville, CA, USA) and a flexible meter tape to reach and measure the height above ground level of the saguaro apex (Table 1) and of each sampled spine. We used needle-nose pliers and sprue cutters (The Testor Corporation, Rockford, IL, USA) to clip one spine from each areole along the rib (we chose the longest central spine that was most distal from the areolar meristem). This site is on the eastern edge of the Sonoran Desert and receives almost 50% of its mean annual precipitation (284 mm) during the monsoon months of July–September. At least monthly precipitation measurements have been collected 200 m from Saguaro 162 for the last 25 years at Tumamoc Hill (J. Bowers, personal communication). Pierson and Turner (1998) first recorded the height of Saguaro 162 in 1964 and subsequently in the spring of 1970 and 1993 (Table 1). Based on the height growth model established for the saguaro population on Tumamoc Hill (Pierson and Turner 1998), we estimate Saguaro 162 most likely germinated in the 1940s. To serve as a control for potential contamination effects of urban CO2 on F14C values, we sampled a single spine from the apex of another 4-m-tall cacti in Saguaro National Park East, in 2004 (32.22 N, 110.71 W, 843 m elevation; permit #SAGU-2004-SCI-0012), 23 km from downtown Tucson. We compared the measured F14C and the resulting age of this control spine with a similarly sampled spine from Saguaro 162 to determine the impact of urban pollution on radiocarbon measurements yielded by saguaro spines. This control sample was also used to assess the use of stored carbon in spine growth. 123 Stable isotope analyses We performed stable isotope measurements at the Laboratory of Isotope Geochemistry, Department of Geosciences, University of Arizona. We analyzed waters for d18O using a dual-inlet isotope ratio mass spectrometer Oecologia (2007) 154:247–258 251 rate calculated from actual measured heights and years [i.e., between 1964 and 1970, the cactus took 0.2 years to grow 1 cm, thus 77 cm (or 27 cm above the 1964 height) represents 1969.4] Table 1 Height of sampled spine, measured heights recorded by Pierson and Turner (1998), F14C content, and F14C year from spines of Saguaro 162. Italicized values are interpolated from the growth Height (cm) Year at measured height F14Ca b F14C year Corrected F14C year Corrected 2r Corrected + 2r 377 2002.8 1.0698 0.0092 2004.7 2002.8 2000.7 2003.6 325 1993.9 1.1015 0.0039 1996.7 1994.8 1994.0 1995.6 320 1993 – – 287.5 1989.9 1.1363 0.0039 1992.3 1990.4 1989.0 1991.9 255 1986.8 1.1695 0.0041 1989.0 1987.1 1985.2 1988.3 1982.6 1.2051 0.0026 1985.4 1983.5 1982.2 1984.4 1.2105 0.0037 1984.9 1983.0 1982.0 1983.9 Tip 211 211Base – – – – – 151 1976.8 1.3028 0.0038 1979.4 1977.5 1977.0 1977.9 98 1971.7 1.4261 0.0060 1973.9 1972.0 1971.1 1972.9 80 1970 – – 77 50 1969.4 1964 1.5537 – 0.0105 – 1969.5 – 1967.6 – 1966.3 – 1969.6 – – – – – 46 – 1.1991 0.0062 1958.7 1956.8 1956.4 1957.3 40 – 1.1174 0.0060 1957.8 1955.9 1955.6 1956.1 17c – 0.9679 0.0042 1950.0 – – a F14C is corrected to account for Desert Laboratory graphite line blank b Includes 0.1% uncertainty that represents long-term errors on the accelerator mass spectrometer at the University of Arizona This is the most recent possible (2r) calibrated age of a pre-bomb radiocarbon age c (Delta-S, Thermo Finnegan, Bremen, Germany) attached to an automated CO2–H2O equilibration unit. We measured water d2H values on the same mass spectrometer equipped with an automated chromium reduction device (H-Device, Thermo Finnegan) for the generation of hydrogen gas using metallic chromium at 750C. Standardization was based on internal standards calibrated with Vienna standard mean ocean water (VSMOW) and Vienna standard light Antarctic precipitation (VSLAP). Reported values are per mil (%) relative to VSMOW. Precision on repeated analyses of laboratory standard waters was less than 0.08% for d18O and 1% for d2H. A time-ordered series of isotope measurements was created from a vertical series of 96 spines spanning 1.77 m near the apex of Saguaro 162 (hereafter referred to as a spine-series). For each spine, we analyzed the bulk tissue of the top 2 mm (the tip) for d18O and the next 1 mm section below the tip for d13C. d2H of spines was not measured. Spines were dried overnight at 70C and chopped into fine pieces before d18O and d13C analyses. We measured spine tissue d18O and d13C using a thermal combustion elemental analyzer (Thermo Electron Corp., Waltham, MA, USA) and a CHN elemental analyzer (Costech Analytical Technologies, CA, USA), each attached to a continuous flow isotope ratio mass spectrometer (Delta Plus, Thermo Electron Corp.). Reported values are per mil (%) relative to VSMOW for d18O – analyses and ViennaPeedee belemnite (VPDB) for d13C analyses. The precision for our method based on repeated analysis of working standards was 0.2% for d18O and 0.1% for d13C. We measured the effect of tissue processing on d18O values of spines from a saguaro nearby and similar to Saguaro 162. We used ground (40 mesh) spine tissue from 3.7 m, 2.5 m and 1 m above ground level. The d18O values of spine tissue holo- and a-cellulose (Brendel et al. 2000) were 1.1–1.8% more positive than that of bulk spine tissues (95% confidence intervals from 0.4 to 2.9%; three separate two-sample t tests, t8 and 18 [ 3.13, P \ 0.0057). Given the inert nature of dead spine tissue and the relatively small and consistent offset in d18O values, we analyzed raw spine tissue without further processing. At selected heights on Saguaro 162, we used a segment of the remaining raw spine tissue from just below the location of the d18O and d13C sampling on the same spine for F14C analyses. These segments were dried overnight at 70C and bathed in weak HCl acid (0.1 M) in an ultrasonic bath for 30 min. Each of three acid baths was followed by a 30-min soak and then rinse in Milli-Q water (18 Mohm). Spines were dried a second time and then reduced to graphite and analyzed for F14C and d13C (the latter from a gas split of the same graphite sample; Slota et al. 1987) at the University of Arizona Accelerator Mass Spectrometry Laboratory. We used the software program Calibomb 123 252 (Reimer et al. 2004) to calculate possible spine ages from measured F14C values corrected for d13C and line blank. For the age calculations of pre-1999.5 ages, we used the Northern Hemisphere Zone 2 data set (Hua and Barbetti 2004), a 0.2-year sample smoothing term and a resolution of 0.2 years. For one sample with a post-1999.5 age, we used an unpublished update of the same dataset provided by Q. Hua (personal communication). For each F14C value from a spine, Calibomb estimates a number of possible ages, the 95% confidence interval for each possible age, and a probability that each possible age is the correct age (Reimer et al. 2004). To assign a finite date for a sampled spine, rather than a range of dates, we used the average of all the possible ages weighted by the probability of their being correct. We conservatively determined the error of that value to be the youngest and oldest ages from the 95% confidence interval of all the possible ages for each sample (2r age range). The time series was anchored by the 1964– 1965 atmospheric radiocarbon peak and the known height of Saguaro 162 measured in 1964. Thus, for any spines collected from above the 1964 height, we excluded any possible ages that predated the 1964–1965 atmospheric radiocarbon peak and, conversely, for samples taken below the 1964 height. The same was true of our error determinations. This anchor also allowed us to exclude possible dates that did not conform to a unidirectional time series along the spine-series axis. We used JMP IN 5.1.2 (SAS Institute, Cary, NC, USA) to perform statistical analyses and the SSA-MTM Toolkit (singular spectrum analysis/multi-taper method; Ghil et al. 2002; Dettinger et al. 1995) to analyze the power spectra of isotopes in the dated spine-series from Saguaro 162. Singular spectrum analysis (SSA) is a smoothing function that empirically determines stable cycles in time-series data and is useful for short, noisy time series. The multi-taper method (MTM) is used to estimate singular or continuous components (e.g., frequencies or trends) within a time series. We used P = 2 and three data tapers, which has been shown to be suitable for climate time series (Mann and Park 1994). Oecologia (2007) 154:247–258 decreased rapidly thereafter to 11.7% in August. The sharp increase in d18O preceded the artificial drought initiated in late April, beginning when plants were being watered frequently and when plant water content was high. This period also corresponded to the dates when vapor pressure deficit (VPD) increased greatly (Fig. 1). We suspect that an increased rate of evaporation caused by higher VPD began the upward trend of d18O, with desiccation after the cessation of irrigation contributing to even greater d18O values. As expected, d18O decreased in late July and early August after VPD had decreased, heavy rainfall had occurred and irrigation had resumed. Although the effects of climate and treatment were confounded in this experiment, the changes in d18O of stem water appeared to be strongly associated with changes in VPD and the availability of soil water. We used the measured plant mass, night-time temperature and relative humidity to model stem water d18O during periods of evaporation (Eq. 1) and recharge (Eq. 2). We took the measured stem water d18O values from each plant in April and July as initial points for the evaporative and recharge models, respectively (Fig. 2). During the artificial drought (April–July 2005), the cacti lost 40% of their mass, and both modeled and measured d18O values of water at the stem apex increased (Fig. 2a–d). The Rayleigh evaporative model, however, overestimated the final Results and discussion Recharge, evaporation and isotopic composition of potted saguaro The mean d18O value of cortex water near the apex of the four potted saguaro plants varied by 11% over the course of the year (Fig. 1). In general, changes in the d18O values of apex water were small during the cooler months of October through March. However, these values increased rapidly from 11.8% in March to 22.3% in July and 123 Fig. 1 Mean d18O values and 95% confidence intervals of water from stem tissue near the apex of four 0.8-m tall saguaro cacti (top panel). Mean minimum vapor pressure deficit derived from monthly mean minimum temperatures and monthly mean maximum relative humidity at the Tucson International Airport (bottom panel) Oecologia (2007) 154:247–258 253 measured d18O values by 2%. Upon further examination, we found strong vertical gradients (12% for d18O) within the plant stem that may change from month to month and dynamically influence the final isotopic value of water at the apex. The isotopic gradients in these cacti resemble an evaporative chain-of-lakes (Craig and Gordon 1965) in that water becomes more enriched with 18O as it travels upward from the plant base (Fig. 3). For the evaporative model, an increased water flux from the base to the apex may have brought water relatively unenriched in 18O to the apex directly through the pith, thus reducing the d18O value below the modeled value. Alternatively, an error in the mass loss measurement of 7% (3 kg) would also yield a difference in modeled d18O values of 2%. Fig. 3 Local meteoric water line for Tucson, AZ (line, d2H = 5.27 · d18O 11.1) and potted cactus stem-water evaporation line (grey arrow). Mean stem water isotope values and 95% confidence intervals from potted 0.8 m tall cacti (circles, n = 4) at 25 cm, 50 cm and 75 cm height (respectively, from lower left to upper right) moving away from mean irrigation–precipitation water isotope values (square) There was also a strong association between modeled and measured d18O values of water at the apex during recharge from July to October (Fig. 2e–h). For recharge, the twocomponent model (Eq. 2) underestimated the measured d18O value of stem waters by 2.5%. Underestimation of d18O by the recharge model may be a result of continued evaporation after July while recharge occurred. It is clear that, even with these discrepancies, evaporation and recharge have the overall effect of raising and lowering, respectively, the d18O values of stem water at the apex. The waters in a cactus stem, however, are clearly not well mixed, and a more sophisticated spatio-temporal model is needed to describe their isotopic value within the stem and through time, with particular attention to the flux of water through the cactus. F14C derived growth model in a naturally occurring saguaro Fig. 2 Variation over time of measured (filled circles) and evaporative model (open circles) stem water d18O from stem tissue near the apex of four 0.8 m tall saguaro cacti between April and July 2005 (panels a–d). Measured and recharge model d18O between July and October 2005 (panels e–h). Fraction original mass is the fraction of the cactus’ mass compared to the same cactus’ mass in April 2005, for all cases (panels a–h). Time moves from left to right. Top and bottom panels are paired to show data from one cactus each (i.e., the cactus in panel a is the same cactus as in panel e) An individual saguaro spine emerges quickly (within months) from the areole, lengthening up to 0.7 mm each day (N. English, personal observation). F14C ages, measured separately from the tip and base of a mid-1980s spine, further support this observation (Table 1). As in other plants (Reimer et al. 2004), spines incorporate ambient carbon from the immediate atmosphere and appear to use little storage carbon (Table 1). To confirm these observations we measured a newly grown spine collected in 2004 from the top of a plant growing 23 km from 123 254 Fig. 4 F14C age of spine tips (triangles) from Saguaro 162 compared to the age of spines at the same height interpolated from measured heights in 1964, 1970, 1993 and 2002 (Table 1). Line is the one-toone correlation line. Error bars represent 2r age ranges as discussed in the text downtown Tucson, a relatively unpolluted environment. This spine’s F14C age corresponded to 2004 (F14C = 1.0709 0.0016), indicating that, at the apex of this plant, minimal carbon is allocated from previous years’ storage for synthesis of spine tissue. Thus, unlike the needles of pine trees (Wright and Leavitt 2006), the apical spines of saguaro plants do not appear to be constructed from storage carbohydrates that have been assimilated in previous years. In general, production of spines occurs only at the stem apex (Mauseth 2006); however, areoles damaged after their formation will sometimes regrow spines from an axillary bud that has not been used for flowering or arm formation. Fortunately, these are easily identified by a second areole growing either on top of another areole or over an areole scar (N. English, personal observation). For Saguaro 162 there was a one-to-one relationship (95% confidence interval from 0.96 to 1.10) between the age of spines derived from heights measured by Pierson and Turner (1998) and the F14C age of spine tips from heights spanning 77–377 cm (Fig. 4, r = 0.997, P 0.0001). For all the spines that were compared (n = 8), however, the F14C ages were 2.1 years (95% confidence interval from 1.2 to 3.2) more modern than the age interpolated from measured heights. This offset is not due to stored carbon assimilated in previous years (with relatively high F14C) being used to grow new spines, since the spines’ F14C ages would appear to be older not more modern (see also discussion above). Thus, we attribute this offset to either: (1) a discrepancy between our choice of a base for height measurements and that used by Pierson and Turner (1998), or (2) the incorporation of 14C-depleted CO2 from urban fossil fuel emissions (Levin et al. 2003; Eastoe et al. 2004). The former is unlikely, given that a spine grown during the summer of 2002 and collected from the apex of 123 Oecologia (2007) 154:247–258 Saguaro 162 (377 cm) yielded a F14C age of 2004.7, 1.9 years more modern than when sampled and consistent with the offset of samples lower on the plant. However, the incorporation of F14C depleted CO2 from fossil fuels is quite probable, since the field site at Tumamoc Hill is located fewer than 2 km from downtown Tucson and a major interstate freeway. We used the offset measured in 2004 of 1.9 years as a correction factor for earlier F14C ages to account for the input of fossil fuel carbon; however, we also note that using the mean discrepancy of 2.1 years yields similar results. We conclude, therefore, that, with careful calibration, F14C measurements from spines are a promising tool for measuring rates of plant growth and estimating the age of a spine or plant between 1955 and today. Temporal d13C and d18O variations in a spine-series from a naturally occurring saguaro To compare the time series of d18O and d13C of spines from Saguaro 162 to precipitation records on Tumamoc Hill, we used date predictions based on observed heights of Saguaro 162 measured by E. Pierson and R. Turner (personal communication) over the past 38 years (Table 1). This is the more direct time-series measurement, but the results would have been the same if the corrected F14C ages of spines had been used. For dates that precede Pierson and Turner’s measurements, we used the corrected F14C-derived ages. Strong cyclical variations in the d13C and d18O can be seen visually in the spine-series from Saguaro 162, and multiple taper method (MTM, Ghil et al. 2002) and singular spectrum analysis (SSA, Dettinger et al. 1995) confirmed these patterns (Table 2). Periods of low d13C separate each year in the 15-year d13C spine-series record (Fig. 5). Using MTM with F14C-corrected ages from spine heights of 211 cm and 287.5 cm as boundaries, we found statistically significant variance (99% confidence level) in d13C on an annual frequency of 1.08 cycles/year (0.72– 1.52 years/cycle; Table 2). Visually, there appears to be a strong annual cycle in the d18O record of spines over the 15-year record, but based on the MTM analysis the primary spectral peak in d18O occurs above the annual frequency, at 1.63 years/cycle (1.08–2.29 years/cycle; Table 2). These analyses suggest that the d13C variations in the spine-series from Saguaro 162 may reasonably be used as an isotopic chronometer representing annual periodicity, but that the use of d18O for this purpose is less reliable. Spines on saguaro in Tucson generally emerge between April and September (Steenbergh and Lowe 1983) although they are presented and analyzed here as a continuous time series. Periods during which spines do not Oecologia (2007) 154:247–258 255 Table 2 Variables and spectral analysis results using the multiple taper method (MTM) for d13C and d18O in the Saguaro 162 spineseries Time-series variables F14C yearsa Maximum F14C years Minimum F14C years Begins 1980.7 1978.3 1982.5 Ends 1992.4 1996.3 2000.2 Years 15.6 21.9 10.4 Data points 96 96 96 Unit time 0.16 0.23 0.11 Spines per year 6.15 4.38 9.23 13 d C Years/cycle (1st component) 1.08 1.52 0.72 Years/cycle (2nd component)b 1.35 1.90 0.90 1.63 2.29 1.08 d18O spine-series Years/cycle (1st component) a Based on unit-time interpolated and extrapolated from corrected F14C ages at 211 cm and 287.5 cm and assuming year-round spine growth b 1st and 2nd components are significant (a = 0.95) periodicities in a time series in order of greatest significance grow (November–February; N. English, personal observation) will, therefore, not record changes in d13C or d18O due to stem-water recharge or evaporative losses. Given the variable nature of spine growth, we recognize several potential sources of error in our spine-series analyses. Firstly, changes in the number of spines added to the stem each year due to climate or age may change the significance or add or subtract spectral components at decadal scales by altering the resolution of the spine-series. For example, when growing rapidly, a saguaro may produce eight spines per year, thereby providing resolution at a subseasonal scale, but when it is growing slowly, there may be only three spines per year, which can only provide information at the annual scale. Secondly, years with many spines but low isotope variance due to climate factors (i.e., prolonged drought) may be difficult to detect as an annual cycle, thereby altering the spectral character of a time series. This would create the appearance of fewer cycles in a given time period and decrease the strength of an otherwise significant spectral component. We see several potential scenarios of dampened amplitude in our d18O and d13C spine-series. For example, between 290 cm and 310 cm, two dry winters separated by a weak monsoon period yielded a less distinct trough in d18O, so that 2 years appeared to represent only one (Fig. 5). Likewise 2 years appeared as only one between 195 cm and 210 cm, when soil moisture and the premonsoon climate were very wet (El Niño winter of 1982– 1983), resulting in lower d18O and d13C values in spine tissue (Fig. 5). As wet soil conditions persisted until the start of the monsoons, we hypothesize that cacti would continue greater expression of the C3 signal (CAM phases II and IV) through the normally dry period of the year, resulting in the absence of a peak in d13C for that year. The length of the spine isotope record based on the SSA of d13C yields one year fewer than expected based on ages interpolated from measured heights taken in 1970 and 1993 (Table 1; 15 vs 16 years). This discrepancy suggests that either: (1) the SSA of d13C underestimates the number of cycles present in the record, or (2) the rate of growth interpolated from measured heights was an underestimate, and, thus, the age over the spine-series period was overestimated. Saguaro has been observed to grow and reproduce under the harshest of conditions (Steenbergh and Lowe 1977), and SSA results closely match clear peaks and troughs in the isotope record (Fig. 5). For these reasons, we believe the discrepancy results from imprecision of height measurements, giving an underestimation of growth rates. In the context of Pierson and Turner’s (1998) demographic study, measurement errors of 10 cm or 20 cm would have had little effect on the outcome of their studies, due to their large sample sizes and the use of saguaro height classes rather than continuous numeric height data (R. Turner, personal communication). For our purposes, however, the cyclical variations seen in the SSA of d13C was used to assign years (shaded bars in Fig. 5) to spines—using the observed height in 1993 as an anchor for our chronology. Environmental control of d13C and d18O variations in a spine-series from a naturally occurring saguaro The amplitudes of d18O and d13C variation in the spineseries of Saguaro 162 (13% and 3%, respectively) are similar in magnitude and timing to variations seen in the apical stem waters of much smaller potted saguaro cacti and other obligate CAM plants (Roberts et al. 1997). Spine tissue d13C values from Saguaro 162 were positively correlated with d18O (r = 0.45, P \ 0.0001). If stomatal conductance and leakiness were driving d13C values, we would expect them to be negatively correlated to d18O values from the same spine. However, if we assume that variation in d13C in spine tissues is caused only by the photosynthetic pathway used to fix CO2 from the atmosphere, then the 3% variation in spines represents the presence of 10% carbon derived from daytime (C3) photosynthesis, an untested although reasonable conjecture when we consider saguaro analogs like F. acanthodes. Oxygen and carbon isotope values appear to be influenced by anomalous climate conditions through enzymatically driven processes. Two very low d18O excursions occurred in 1983 and 1993. These low values were seen after wet winters of the previous year strongly influenced by ENSO, when the 123 256 Oecologia (2007) 154:247–258 CO2 by Rubisco in the early morning or late afternoon (CAM phases II and IV) and reduces the d13C value of spines grown during these periods. During the dry premonsoon period, saguaro stomates are closed in the morning and late afternoon, increasing the relative contribution of CO2 fixed by PEPc (phase I) and thus increasing the d13C values of spine tissue grown during these periods of drought. Conclusion Fig. 5 A record of isotopic variation in spine tips spanning 1.77 m of Saguaro 162 on Tumamoc Hill, Tucson, AZ. Bars at top (a) are interpolated years based on measured heights in 1970 and 1993 (Pierson and Turner 1998) and filled triangles with lines are corrected F14C ages with 2r age ranges (i.e., F14C age minus 1.9 years; see text). Spine tip d18O values (b) and d13C values (c), plotted by height from the base of the plant, are shown with a singular spectrum analysis (SSA) of d13C for comparison (d). Monthly precipitation values at Tumamoc Hill (e) are shown for October through March (grey bars) and April–September (black bars). The year 1993 of the timescale at the top (a) and on the bottom axis (e) of this figure are anchored to (i.e., in line with) the 320 cm height of Saguaro 162 (c and Table 1, see text for more detail). Increased precipitation in the spring of 1983 and winter of 1992–1993 coincided with El Niño in those years. Shaded bars from top to bottom denote correlated years based on the SSA majority of precipitation ([200 mm) fell between January and March. However, while the d18O of precipitation clearly influences the bulk average d18O of water in the cactus over time, the impact of any single rainfall event on the spine tissue d18O is diminished by admixture with the large reservoir of water in the stem. The unseasonably wet summer of 1982 and ENSO-influenced winter of 1982–1983 also produced the most negative d13C values found in our spine-series. Given the presence of the strong ENSO signal in our record, we suggest that the isotopic variability in this record is due mostly to increased water availability and cooler temperatures at the beginning and end of each growing season that favor direct fixation of atmospheric 123 By efficiently collecting and storing precipitation between long periods of drought, Saguaro, columnar cacti and other succulents in deserts (e.g., Euphorbiaceae in Africa; Cowling et al. 1994) contribute significant amounts of water, nutrients and energy to consumers via flowers, fruits, seeds and stems over the entire year (Markow et al. 2000; Wolf and Martinez del Rio 2003). Climate changes affecting precipitation (NAST 2000) may greatly impact the viability and distribution of saguaro and other species of succulents, as well as their dependants (see, e.g., Houghton et al. 2001). As such, being able to determine how these keystone species have responded to climate variation in the past provides us with a valuable tool for predicting their success in the future. The data from Saguaro 162 and our potted cacti experiments suggest that columnar cacti record changes in and responses to rainfall and VPD in the stable isotopes of their spine tissue. We have yet to quantify fully the interaction of precipitation, humidity, temperature, stem-water flux and other variables, but we have shown that there is good reason to suspect that the variation in d13C and d18O in the spines of cacti are a result of distinct climate properties that include the interaction of these processes. Additionally, we have put forward a new method for establishing the age of columnar cactus, saguaro in this case, using F14C in spines and, consequently, for calculating the stem growth rate. The isotopic chronometers (F14C and d13C), and isotopic signals (d13C and d18O), recorded in spines are just the beginning of many studies that can improve our understanding of climate variation in arid deserts and of the response of these organisms to a changing environment. Acknowledgments This work was funded by an Environmental Protection Agency STAR Fellowship, a William G. McGinnies Scholarship and a Geological Society of America student grant. Jeff Pigati and Christa Placzek processed 14C samples to graphite, and Warren Beck at the NSF-Arizona Accelerator Mass Spectrometry Laboratory provided 14C analyses. Valuable discussions, data and laboratory space were provided by K. Anchukitus, T. Ault, J. Bower, J. Cole, T. Drezner, C. Eastoe, M. Fan, K. Hultine, S. Leavitt, J. Mauseth, J. Overpeck, B. Peachy, E. Pierson, D. Potts, J. Quade and R. Turner. We are also grateful for additional comments from F. C. Oecologia (2007) 154:247–258 Meinzer and two anonymous reviewers. 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