Research article
Received: 01 January 2017
Accepted: 07 August 2018
DOI: https://doi.org/:10.5027/andgeoV46n1-3087
Abstract: Prior to the 24-26 March 2015 extreme precipitation event that impacted northern Chile, the scenarios for Pleistocene and Holocene wetter paleoclimate intervals in the hyperarid core of the Atacama Desert had been attributed to eastern or southwestern moisture sources. The March 2015 precipitation event offered the first modern opportunity to evaluate a major regional precipitation event relative to those hypothetical paleoclimate scenarios. It was the first opportunity to determine the 18O and 2H composition of a major precipitation event that might eventually be preserved in geological materials. The driver for the March 2015 event was a synoptic-scale weather system, a cutoff cold upper-level low system that traversed the Pacific Ocean at a time of unusually warm temperatures of Pacific surface water. Ground-based precipitation data, stable isotopes in precipitation and river samples, NCEP/NCAR reanalysis atmospheric data and air mass tracking are utilized to connect the Earth surface processes to atmospheric conditions. The δ18O and δ2H of the precipitation and ephemeral rivers were significantly heavier than the rain, snow and ephemeral rivers fed by more frequent but less voluminous precipitation events registered prior to March 2015. Consistent with the atmospheric analyses, the rain isotopic compositions are typical of a water vapor whose source was at more equatorial latitudes of the Pacific and which moved southward. The late March 2015 system was an unforeseen scenario even for El Niño Pacific ocean conditions. Furthermore, the late summer season warmth led to greater potential for erosion and sediment transport than typical of more common moderate precipitation scenarios which usually include widely distributed snow. A comparison of the March 2015 scenario to the spatial distribution of wetter paleoclimate intervals leads to the hypothesis that the March 2015 scenario likely better fits some parts of the paleoclimate record of the continental interior hyperarid Atacama Desert than do the eastern or southwestern moisture source paleoclimate scenarios deduced previously.
Keywords: Extreme precipitation, Atacama Desert, O and H isotopes, Chile, Paleoclimate, Groundwater.
Resumen: Previo al evento de precipitación extrema que ocurrió entre el 24 y el 26 de marzo de 2015 y que impactó fuertemente en el norte de Chile, los escenarios de los intervalos paleoclimáticos más húmedos del Pleistoceno y Holoceno en el núcleo hiperárido del desierto de Atacama se habían atribuido sólo a fuentes de humedad provenientes del este o suroeste. El evento de precipitación de marzo de 2015 es la primera oportunidad de evaluar un hecho de precipitación regional importante en relación con los hipotéticos escenarios de paleoclima investigados previamente. Además, era la primera oportunidad de determinar la composici ón isotópica de 18O y 2H correspondiente a un evento mayor de precipitación que pudo, eventualmente, ser preservado en materiales geológicos. El evento de precitación de marzo de 2015 fue un sistema meteorológico de escala sinóptica, del tipo núcleo frío en altura que cruzó el oceáno Pacífico cuando las temperaturas superficiales del océano eran inusualmente elevadas debido al fenómeno de El Niño. Para comprender las relaciones entre los procesos desencadenados en la superficie de la Tierra y las condiciones atmosféricas prevalentes, se utilizaron datos de precipitación registrados en estaciones meteorológicas distribuidas regionalmente, is ó topos estables de muestras de lluvia y ríos, el desarrollo de un reanálisis de datos atmosféricos NCEP/NCAR y un seguimiento de las masas de aire. Los valores isotópicos de δ18O y δ2H de la precipitación y los ríos efímeros fueron significativamente más pesados que la lluvia, la nieve y los ríos efímeros alimentados por precipitaciones más frecuentes, pero menos voluminosos que los registrados antes de marzo de 2015. Estas composiciones isotópicas coinciden con el análisis atmosférico en el sentido que son típicos de vapor de agua proveniente del oceáno Pacífico tropical. El evento extremo de marzo de 2015 no corresponde a los escenarios previstos para precipitaciones en el norte de Chile vinculadas a las condiciones El Niño. Además, su ocurrencia bajo temperaturas estivales provocó mayor capacidad de erosión y transporte de sedimentos, comparado con escenarios de precipitaciones más comunes y menos abundantes, que usualmente incluyen nieve ampliamente distribuida. De una comparación entre la distribución de precipitación en 2015 con mapas paleoclimáticos de intervalos más húmedos surge la hipótesis que el escenario de marzo de 2015 coincide mejor con ciertas partes del registro paleoclimático del desierto hiperárido de Atacama que los escenarios anteriormente propuestos.
Palabras clave: Precipitación extrema, Desierto de Atacama, Isótopos de O y H, Chile, Paleoclima, Agua subterránea.
1. Introduction
An uncommon precipitation event impacted northern Chile from 24-26 March 2015 (Fig. 1), at the end of the southern hemisphere summer season and at the onset of El Niño conditions in the Pacific Ocean. Because of the warm season, much of the precipitation fell as rain even in the high mountains where snowfall historically dominates. Whereas snow permits delayed and slowed surface run-off, the 24-26 March 2015 region-wide run-off was rapid. The impacts included severe flooding of river valleys that drain the Andes to the Pacific coast with associated debris flows, tens of deaths, and widespread property damage (e.g., cities of Chañaral and Copiapó, Fig. 2) (Wilcox et al., 2016). Yet for regions of low relief or internal drainage there was little change of the land surface materials despite high rain totals (Jordan et al., 2015; Tapia et al., 2015; Wilcox et al., 2016; Scott et al., 2017). It is anticipated that groundwater was recharged, though spatial variations in recharge amount are not known.
Where precipitation is extremely infrequent and where historical documentation is incomplete, as in Chile’s Atacama Desert, it is difficult to place an extreme precipitation event in a historical context. Viewed from the perspective of the last century, the March 2015 precipitation event was unprecedented, leading to questions such as: Was it representative of the normal weather fluctuations of late Holocene climate? Was it typical of past wetter conditions of the Late Pleistocene or Holocene? Does it herald the initiation of an unprecedented new climate state?
Details about paleoclimate, geomorphology or groundwater hydrology are valuable in answering these questions by providing a longer chronicle of precipitation and its spatial and temporal variability. However, published studies to date have not considered the March 2015 hydrometeorological scenario as a mechanism for late Pleistocene and Holocene wet paleoclimate periods (e.g., Gayó et al., 2012; Sáez et al., 2016). The objectives of this paper are to lay the foundation for reconsideration of existing paleoclimate and groundwater data sets and to show the need for the collection of new data from paleorecords that would enable comparison to the March 2015 precipitation event.
Climatologists underestimated the precipitation event: precipitation in the core of the hyperarid Atacama Desert had not previously been attributed to the set of atmospheric and oceanic circumstances which played out in March 2015. The event differed from all the previously documented precipitation scenarios expected in Chile during an El Niño event (Vargas et al., 2006). In mid March 2015 a southern hemisphere mid-latitude atmospheric wave disturbance evolved into a cold upper level cutoff low (Barrett et al., 2016) that traversed the Pacific Ocean (Fig. 1), reaching the South American coastline when subtropical and tropical eastern Pacific surface water was 1-3 °C warmer than the mean for March (Barrett et al., 2016; Bozkurt et al., 2016). From 24-26 March rain and snow fell across approximately 400,000 km2 of subtropical Chile and western Argentina, 22-32° S latitude (Fig. 2; Appendix Table A1), covering zones with hyperarid to semi-arid climates (Fig. 1). The boundary of transition from rain to snow near 3,600 m a.s.l. was uncommonly high.
In the hyperarid core of the Atacama Desert, the rain generated by this event exceeded decades of mean annual precipitation (Table 1). For example, historically (1988-2014) at the Aguas Verdes station (25.4° S, 69.96° W) no March registered precipitation and, among December, January and February data, a single February (1998) registered 3.5 mm. However, over the three days from 24-26 March 2015, this station received 85 mm. In the hyperarid core of the desert, an event of this magnitude or greater likely dominates the modification of small scale landforms and the recharge of groundwater. Following this single event vegetation and flowering plants in particular covered wide areas in multiple locations, some of which had been barren for decades. An increase in vegetation on this scale becomes part of the paleoclimate record through storage of plant residue in rodent middens (e.g., Latorre et al., 2002; Latorre et al., 2006; Maldonado et al., 2005; Díaz et al., 2012; Gayó et al., 2012).
This paper documents the isotopic composition of precipitation from this rare event based on analyses of a unique set of rain and stream samples. The isotopic results are combined with analyses of atmospheric conditions to reveal the factors that produced the extreme precipitation and its isotopic fingerprint. The isotopic data for this event in combination with data from more commonplace events in northern Chile now offer diagnostic criteria for connecting past precipitation to atmospheric conditions.


2. Hydroclimate zones and anticipated isotopic compositions
The values of δ18O and δ2H in precipitation over the Andes Cordillera and intermediate elevation terrain between the Andes and the Pacific coast reflect multiple atmospheric water vapor transport paths and the orographic effects of the Andes (Fig. 2A). The dominant water vapor transport paths to the northern and southern ends of the region impacted by the March 2015 event are different, tied to latitudinal gradients in hemispheric-scale atmospheric circulation, sea surface temperature gradients, and topography.
Atmospheric water vapor that leads to precipitation comes from at least three spatially separated sources (Aceituno, 1988; Rutllant and Fuenzalida, 1991; Houston and Hartley, 2003; Garreaud et al., 2009) (Fig. 2A) which define three separated climate zones (Zone I, Zone II and Zone III, Fig. 2B). The area between climate zones I, II, and III constitutes the hyperarid core of the Atacama Desert, zone IV. South of 22° S (northern part of the political division “II Region of Antofagasta”), Pacific-sourced water vapor leads to precipitation in the Andes Mountains dominantly in winter (June-July-August) (zone III) (Houston and Hartley, 2003; Burgener et al., 2016). Through cutoffs and fronts from the mid-latitude westerlies (Vuille and Ammann, 1997) a decreasing amount of precipitation reaches progressively northward. North of 25° S (southern part of the political division “II Region of Antofagasta”), the persistent southeast Pacific subtropical high pressure system so effectively blocks the entry of fronts in the westerlies onto the continent (Rutllant and Fuenzalida, 1991) that this winter Pacific-sourced precipitation beyond 25° S is of very small amount, and we designate that to be the northern boundary of zone III. Along a coastal strip (zone II), low level stratocumulus clouds beneath a persistent temperature inversion produce Pacific-sourced fog, especially during the winter (Houston and Hartley, 2003). The third typical moisture source, of Atlantic origin via the Amazon basin, is responsible for providing precipitation to zone I during summer months. During summer the change in the strength of the South American Low Level Jet (SALLJ, Fig. 2A) and southward shift of the intertropical convergence zone lead to an enhanced supply of moisture to the high altitude plateau (Altiplano) within the southern tropics (Garreaud et al., 2009). Under conditions of diminished westerly flow over northernmost Chile, that Atlantic-sourced tropical air mass spreads westward, providing summer precipitation to the western Andean cordillera (Garreaud et al., 2009). Although another path of summer season water vapor delivery from the South American lowlands southeast of the Atacama Desert was established by Vuille and Keimig (2004) which would contribute to zones I and III, a lack of documentation of specific cases in which this mode caused rain in the Atacama Desert suggests that it may contribute less to total rainfall than the other sources.

For the west coast of South America, the δ18O and δ2H of precipitation derived from Pacific-sourced water vapor (Fig. 3A) vary from tropical sites that are only slightly lower than SMOW (Standard Mean Ocean Water) (Esmeraldas and La Cuca, Ecuador) to sub-tropical and mid-latitude sites (La Serena and Valparaíso, Chile), whose monthly isotopic values are much more variable and generally more negative. Data for the stable isotope compositions of precipitation in the hyperarid part of the Atacama Desert are sparse (Fritz et al., 1981; Alpers and Whittemore, 1990; Aravena et al., 1999). Summer rain that falls on the western slope of the Andes tends to be less depleted in heavy isotopes than rains east of the topographic divide in the Altiplano (Fig. 3B) (Fritz et al., 1981; Chaffaut, 1998; Aravena et al., 1999; Uribe et al., 2015). Over the eastern Andes, precipitation at low elevations has δ18O of -2 to -8‰ but δ18O becomes depleted toward the west as vapor is lifted across the Eastern Cordillera of the Andes (Fig. 4) (Fiorella et al., 2015; Gonfiantini et al., 2001; Rohrmann et al., 2014). The dominant Altiplano summer rain has d18O values of -8‰ to -15‰. Published isotopic data for rain in Chile south of the study area reveal moderately depleted coastal rain (-4‰ to -10‰; Fig. 3A) and progressive depletion at increasing elevations (Fig. 4) (Burgener et al., 2016). These characteristic isotopic values for locations along the principal water vapor paths to the Atacama Desert (Fig. 2A) lead to the expectation that precipitation in the hyperarid region should be moderately to strongly depleted at all elevations, perhaps δ18O of -10‰ to -15‰. These hypothetical values are similar to the winter precipitation within the study area (Alpers and Whittemore, 1990) and in the slightly less arid high elevation mountains >450 km to the north of our study area (Fritz et al., 1981; Aravena et al., 1999). Some summer precipitation 450-700 km to the north of our study area at elevations between 2,380-3,360 m a.s.l. defies this expectation (Fig. 4A) (Aravena et al., 1999) and is discussed later.


3. Materials and methods
Five rainwater samples from the March, 2015, precipitation event were obtained from containers designed to retrieve and store precipitation. Locations and sampling dates of two samples collected near the coast in the city of Antofagasta and three in the Andean foothills are shown in figure 2b and detailed in table 2. During the precipitation event, the coastal samples were transfered to 100 ml and 1 L polyethylene bottles, depending on the volume of recovered sample. The rain in the very remote Andean locations was captured in tubs adapted with a funnel and a 2.5 cm thick layer of pure vaseline oil to prevent evaporation. These were retrieved one week (two locations) and one month (one location) after the event (Table 2). Using a syringe the water, without vaseline, was also transfered to 100 ml and 1 L polyethylene bottles. Three stream samples were collected a few days after the March 24-26, 2015 precipitation event (Table 2). Stream samples were not filtered before being sent to external laboratories for analysis. The high suspended load of the Salado River (Atacama Region) was separated by decanting the water after allowing the particles to settle. All sample bottles were completely filled, capped tightly, and the cap then taped to prevent evaporation until analysis. The samples were stored in a refrigerator at 4 °C before they were sent to the laboratory for analysis. Two rain samples were collected following the same collection standards at the same coastal location during August 2015, to provide a basis for comparison to a more ordinary precipitation event.

The stable isotope compositions of most water samples were analyzed at the Environmental Isotope Laboratory from the University of Arizona; two stream samples were analyzed by the Cornell University Stable Isotope Laboratory. At Arizona, measurement was done with a gas-source isotope ratio mass spectrometer (Finnigan Delta S). For hydrogen, samples were reacted at 750 °C with Cr metal using a Finnigan H/Device coupled to the mass spectrometer. For oxygen, samples were equilibrated with CO2 gas at approximately 15 °C in an automated equilibration device coupled to the mass spectrometer. Standardization is based on international reference materials Vienna Standard Mean Ocean Water (VSMOW) and Standard Light Antarctic Precipitation (SLAP). The analytical uncertainty (one standard deviation) is 0.9 ‰ for δ2H and 0.08 ‰ for d18O on the basis of repeated internal standards. At Cornell, measurement was done using an equilibration technique on a Thermo Scientific Gas Bench II coupled to a Thermo Scientific Delta V mass spectrometer. In the case of deuterium, 2% H2 gas was added into the headspace and the sample was equilibrated with this H2 with the aid of a platinum Hokko bead catalyst (Shoko Co. Ltd, Japan). For this analytical run the overall standard deviation for the internal deionized water standard was 3.44 ‰ for δ2H and 0.18 ‰ for δ18O. Isotope corrections were performed based on a two-point normalization (linear regression) using one in-house standard (Mauna Kea) and VSMOW.
Daily sums of liquid precipitation corresponding to 23-29 March 2015 at 114 stations in Chile and three stations in Argentina between 20°-32° S were compiled (Appendix Table A1) from two Chilean government agencies, five mining companies, a commercial weather forecasting service and university-hosted weather stations. Examination of the data revealed an apparent reporting inconsistency with one public data source that limits the temporal resolution of the full data set (Appendix Table A1 note). Therefore, we report the spatial distribution of amount for a span of days that exceeds the precipitation event. Total precipitation quantities for four other stations are available (Appendix Table A1, items 35-38), three of which were rain catchers described above. The full set of station data were manually contoured (Fig. 2B) as lines of equal precipitation. Because only two of the meteorological stations captured snow (Appendix Table A2) the total precitation is under reported. The spatial coverage of snow on 27 March 2015 was traced from a MODIS satellite image (https://earthdata.nasa.gov/labs/worldview/ (last visit 16/06/2015)).
We examined the atmospheric circulation at 0000 and 1800 Coordinated Universal Time (UTC) 25 March 2015 over a region of interest greatly exceeding the region of precipitation (0°-60° S latitude; 0°-120° W longitude) (Fig. 1). Atmospheric conditions are derived from National Centers for Environmental Prediction/National Center for Atmospheric Research (NCEP/NCAR) reanalysis data (Kalnay et al., 1996). These data are resolved to point locations spaced 2.5-degrees latitude and longitude every six hours on 17 pressure levels (1,000 mb through 10 mb) for geopotential height (Z), temperature (T) and horizontal wind components (u, v), twelve vertical levels (1,000 mb through 100 mb) for vertical pressure velocity (omega) and eight levels (1,000 mb through 300 mb) for specific humidity, from which water vapor mixing ratio and equivalent potential temperature are calculated.
Atmospheric stability was assessed with a calculation of the vertical gradient of equivalent potential temperature (theta-e). Long-term (1981-2010) mean values of theta-e were calculated at each grid point from the long-term mean values of temperature and water vapor mixing ratio at that grid point. The long-term mean theta-e was then subtracted from the actual theta-e to obtain theta-e anomalies. The vertical gradient of theta-e anomalies provides an assessment of the anomalous stability or instability of the environment.
To document the source of air arriving over the precipitation-event region, air parcel trajectories were calculated with the on-line web version of the HYSPLIT model (Stein et al., 2015; Rolph, 2016). HYSPLIT calculates the movement of a single Lagrangian particle according to the three-dimensional mean wind field. This analysis used Global Data Assimilation System meteorological data resolved at 0.5 degrees latitude and longitude.
Neither the atmospheric stability analysis nor the air parcel trajectory analysis includes consideration of turbulence.
4. Results
4.1. Precipitation distribution
The geographic limits of heavy rain (>30 mm) during the 24-26 March 2015 event were near 23° S and 32° S (Fig. 2B). North of 26° S heavy rain spanned over 150 km from the Pacific to the Andean highlands. This included the core of the hyperarid Atacama Desert (zone IV, Fig. 2B). South of 26° S, greater than 30 mm fell on a 50-100 km wide continental interior region up to about 3,400 m a.s.l. that lies in climate zone III (Fig. 2B) and constitutes steep Andean upland catchment basins. An elongate region of rainfall exceeding 50 mm extended along the Andes Mountains from 24° to 30° S. At higher elevations and farther east, snow from 23° S to 32° S covered 88,000 km2 (Fig. 2B); areas covered by snow may also have received rain (Wilcox et al., 2016). North of 32° S, areas with any amount of rain but no snow totaled approximately 175,000 km2 of Chile and, based on very sparse data, about 140,000 km2 of lowland Argentina west of 66° W (Appendix Table A1).
4.2. Isotopic composition of rain and runoff
The March 2015 rain samples included a Pacific coast site and three sites close together >115 km inland; the inland sites range in elevation from 2,939-3,962 m a.s.l. (Table 2). The two coastal rain samples are little displaced from Vienna Standard Mean Ocean Water (VSMOW) and differ from one another in the d18O -d2H plot (Fig. 3A) along a line with a slope of 4, considerably less than the Global Mean Water Line (GMWL). The coastal rain water was similar to rains of coastal Ecuador, and not the rains of mid-latitude coastal Chile (Fig. 3A).
The three high elevation samples have lower d18O and d2H than rain at the coast (Fig. 3A and 4A) and become progressively lower with increasing elevation of the rain sampling location. The excess deuterium (dxs) of coastal sites is between 7.0 and 11.2, and for inland sites between 15.0 and 17.3 (Table 2).
Of three stream samples (Fig. 2B; Table 2), those from the Salado River (Atacama Region, 26.4° S) and the Los Vientos stream are considered to be dominated by the March rain because both streams had been dry beforehand. The third stream sample, the perennial Salado River (Antofagasta Region, 22.3° S), is considered to be a mixture of groundwater baseflow and recent precipitation. The Los Vientos stream isotopes are consistent with the rain water in the same small drainage basin, with d18O higher by 4‰ and d2H by 13‰, due to evaporation as water flowed overland to the stream. The Salado River (Atacama Region), sampled at a position far downstream in a large catchment that drains the Andes, has d18O intermediate between the coastal and Andean rains (Fig. 4A; Table 2). If the effect of evaporative enrichment of 18O and 2H in streams relative to precipitation is similar to the Los Vientos stream, the Salado (Atacama) sample indicates that run-off from rain that fell above 3,000 m a.s.l. in the Andes was the dominant streamwater source.
4.3. Atmospheric conditions
The key atmospheric circulation feature at 0000 UTC 25 March 2015 (local time 21:00 h, 24 March) is the “cutoff low” at middle to upper levels of the troposphere near 75° W, 30° S (Fig. 1). To the south is a persistent anticyclonically breaking wave in the height field near 45° S that caused atmospheric blocking (Barrett et al., 2016). A high content of precipitable water in the atmosphere over the eastern equatorial Pacific was a second key attribute in setting up the extreme precipitation event (Barrett et al., 2016). As a consequence of both features, upper level winds were from the northwest over the north Chilean Pacific coast and transported anomalously moist air into the region.
This air motion was confirmed by a set of backward trajectory calculations of air arriving at 0000 UTC 26 March (21:00 local time on 25 March) to positions 500 m above ground level at five locations (Fig. 5A). Unlike typical conditions within the southeast Pacific anticyclone, the air mass turned cyclonically. At 1800 UTC on 25 March, there was ascending air at the 600 mb level, centered at 29° S, 70° W, which covered the region from 25-31°S across which large amounts of precipitation fell (Fig. 5B). The ascent coincided with abnormally unstable air (anomalously upward-decreasing equivalent potential temperature; Fig. 5B). Consequently, water-vapor saturated air parcels (e.g., as illustrated in figure 5A) that reached the continental interior likely would have become buoyant and accelerated upwards, precipitating water as excess precipitation. The abnormal instability was due to both abnormally cold air aloft and above-normal water vapor mixing ratios at lower levels (not shown). This situation is suitable to explain the Elqui Algarrobal rainfall intensity peak at local time 15:00 (Fig. 6).
Figure 5A illustrates that the air parcel tracks are not all parallel. Specifically, the track to the southernmost location, Elqui Algarrobo, began at the northernmost source location, offshore southern Perú, and crossed the other tracks at a higher altitude. Complexities like this are expected because air parcels which began the time interval of interest at varying locations and heights experienced differing wind strengths and directions. Ultimately the precipitation from a storm like this is the product of a complex mixture of differing paths, as well as turbulence which is not captured in these models. The isotopic composition evolves within these air masses, and it is not possible to differentiate these details based on our isotopic data.


5. Discussion
5.1. Isotopic values
The March northern Chile coastal rain O and H isotopic composition are very similar to those of Ecuador (Fig. 3A), with compositions that fit expectations for rain produced from rapidly evaporated ocean water (Dansgaard, 1964). This result is consistent with humid air that traveled from the tropical to subtropical eastern Pacific Ocean off the coasts of Perú and northern Chile under conditions 1-2 °C warmer than normal, as suggested by the air parcel tracks (Fig. 5A).
The d18O and d2H values of inland sites remain close to the Global Mean Water Line, which is consistent with little evaporative loss either as the rain fell or from the samplers. Consequently, we interpret that these samples provide robust data for air mass interpretation. The pattern of decreasing d18O and d2H values away from the coast and with increasing elevation in combination with the changes in water vapor saturation and wind directions point unequivocally toward the Pacific Ocean as the only significant source of the precipitation. The advection of moist subtropical to tropical eastern Pacific air (Barrett et al., 2016) and its rise across the Coastal Cordillera and then the Andes Mountains triggered the instability (Fig. 5B) that resulted in prolonged and widespread rain and snow (Fig. 2B).
The only published precipitation isotope data close to our samples from March 2015 are for winter season precipitation. Snow and rain collected during June 1984 had much lower mean d18O and d2H values of -13.8‰ and -92.8‰, respectively (Alpers and Whittemore, 1990). Further to the south at 30° S, amount-weighted d18O and d2H available for primarily winter precipitation events (Table S1 of Burgener et al., 2016) are also much lower than for the March 2015 event. At low elevations from the coast to 1,300 m a.s.l., values of d18O ranged between -9.0‰ and -12.3‰ and d2H between -64.9‰ and -91.2‰. At high elevations (2,100-3,100 m a.s.l.), values of d18O ranged between -13.5 to -13.6‰ and d2H between -104.9‰ and -100.3‰. In the Altiplano plateau outside the area of rain in March 2015, the variability is sufficient that those rains overlap with the inland March 2015 rain samples (Fig. 4) (Gonfiantini et al., 2001; Fiorella et al., 2015; Herrera et al., 2016).
In comparison, Chilean rain data at locations >450 km to the north of our study area (Fritz et al., 1981; Aravena et al., 1999) revealed that amount-weighted means of d18O of Andean precipitation varied during summer months (1973-1975; 1984-1986) between -4.5‰ to -20.2‰, and rare rains in winter (June) 1984 between -11.1‰ to -12.5‰, with an unusually strong dependence upon elevation (Fig. 4). For comparable elevations, the March 2015 samples were isotopically less depleted (Fig. 4). However, examined in detail, summer precipitation at elevations of 2,000-3,000 m a.s.l. was much less depleted than same-day precipitation at altitudes greater than 3,000 m (Aravena et al., 1999). Aravena et al. (1999) noted that these low-elevation summer values (e.g., d18O -4 to -7‰) cannot be explained by a model in which water vapor is derived from the east and crosses the Andes (Fig. 2A). Consequently, Aravena et al. (1999) suggested that some summer storms driven by eastern-sourced upper air masses simultaneously drew in low-altitude tropical Pacific moisture by dynamics not captured in coarse grid meteorological analyses. The much larger scale March 2015 synoptic storm system delivered eastern equatorial Pacific water vapor of similar isotopic values.
Despite proximity, the isotopic composition of the Salado River (Atacama Region) stream water in March 2015 is not comparable to water from streams located between 28.5°-31° S sampled in November 2006 (Fig. 4) (Strauch et al., 2009). Those springtime 2006 δ18O values (mean -12.8‰) are significantly lower than the March 2015 stream, and consistent with the isotopically depleted precipitation that more frequently falls on the Andes in winter (Fig. 4) (Burgener et al., 2016).
5.2. Comparison of the March 2015 extreme event to common precipitation scenarios
Climatological analyses have shown that all documented modern precipitation events of significance in coastal regions of northern Chile were associated with atmospheric wave disturbances that move generally eastward across the Pacific Ocean at mid-latitudes (Vargas et al., 2006). The March 2015 event shared this commonality with prior precipitation events. However, the typical major precipitation event of coastal northern Chile occurs during the winter season of an El Niño event, not in the late summer. Vargas et al. (2000, 2006) determined that rainfalls in Antofagasta city strong enough to cause significant flooding occurred in May (1982), June (1940, 1991), July (1925, 1940, 1987) and August (1930, 1982). In those cases, the intensity of rainfall has been cited as a key feature which led to the development of landslides along the Coastal Escarpment (20-40 mm per 3-hour-period) (Hauser, 1997; Vargas et al., 2000, 2006). The March 2015 event caused stream run-off floods which caused great damage to coastal cities (e.g., Chañaral), but produced much less landsliding along the Coastal Escarpment than typical intense rain events.
As the 2015 El Niño event advanced, a second significant precipitation event was generated during early August. From August 8-11 a coastal strip of Chile north of 26° S received up to 29.4 mm of rain. During the same interval, interior regions recorded little rain and the snow on the high Andes (Fig. 7A, 22° to 26° S) was thin enough to fade from the daily satellite images within a few days. These rains in the hyperarid Atacama Desert occurred simultaneously with much more widespread cold-front related precipitation which impacted the semi-arid to arid parts of Chile, such as the Elqui valley. North of 25° S the August 2015 intense rain focused on the steeply inclined western slope of the Coastal Cordillera, where it generated mudslides that caused deaths in Tocopilla and significant property loss. That August 2015 event fits well the generalizations given by Vargas et al. (2000, 2006) for precipitation events during prior El Niño events: it occurred during the winter and it was intense only in a narrow strip near the Pacific coast.
Rain water sampled in Antofagasta city near the coast on August 9, 2015 (Table 2) was isotopically depleted by -2 ‰ for d18O (-3.4 and -4.4‰) and -11‰ for d2H (-12.2 and -19.9‰) compared to the March 2015 rain. The August data indicate a Pacific water vapor source as inferred from atmospheric circulation during the storm, but from a latitude further south which is more typical of rain for northern Chile (Fig. 3). This is in contrast to the low latitude Pacific water vapor source for March 2015 precipitation.
Another significant winter season precipitation event June 6-7, 2017 brought up to 40 mm of rain to part of the hyperarid Atacama Desert and regionally extensive snow above about 2,700 meters elevation above sea level (Fig. 7B). This event is not reported to be related to El Niño conditions nor to anomalous warmth in the eastern equatorial Pacific. The June 2017 event fits well the cold-front scenario of winter season precipitation described by Vuille and Ammann (1997). It had larger impact on the Atacama Desert than most cold fronts: less than 20% of all winter cold fronts in years 1984, 1986, and 1990-1993 (Vuille and Ammann, 1997) extended as far north as the June 2017 snow cover (Fig. 7B).

5.3. Geological differences among March 2015 precipitation scenario and other scenarios
Comparison of the March 2015, August 2015, and July 2017 precipitation events reveals that the three hydrometeorological scenarios have multiple differences that may be recorded in geological materials or landforms. Relative to the typical El Niño Southern Oscillation (ENSO)-related August 2015 event, the March 2015 scenario generated a much larger regional footprint and volume of precipitation and, for interior high elevation areas, much faster surface run-off. Therefore, across the core of the hyperarid Atacama Desert, the March 2015 scenario would have greater geomorphological consequences than would the August 2015 scenario. The isotopic record that might be preserved in plant waxes or groundwater would differ only subtly between the two situations, with slightly more enriched oxygen and hydrogen isotopic values for the March 2015 scenario. Whereas rain intensity at Taltal reached approximately 20 mm per-3-hours during the March 2015 event (Fig. 6), which is the lower limit in the range of intensities shown to cause Coastal Escarpment mudslides near Antofagasta (Vargas et al., 2000, 2006), mudslides from the Coastal Escarpment were not a major consequence. Paleo-mudslide deposits along the toe of the Coastal Escarpment would be more likely products of the August 2015 scenario than the March 2015 scenario.
The June 2017 cold front winter storm produced more widespread precipitation in the hyperarid Atacama Desert than did the August 2015 event and less widespread than during the March 2015 extreme event (Fig. 7). Like most winter season cold fronts and cut-off lows, the temperature-controlled elevation of change from rain to snow was low and thus run-off from the Andes Mountains was delayed and diminished. Consequently, less regionally extensive erosion in ephemeral stream beds would be expected compared to the March 2015 event, a hypothesis borne out by field observations in June 2017.
5.4. Paleoclimate implications
The March 2015 precipitation event offers criteria for use in paleoclimate, groundwater hydrology, and archeological studies, with which to elucidate whether it is a scenario that was significant during intervals of wetter climate in the past. Each discipline looks to modern climate to explain the factors responsible for past climate states but conditions in late March 2015 had not been encountered since records and observations started. Consequently, this hydrometeorological scenario has not been considered among the explanations for millennial-duration late Pleistocene to Holocene wet paleoclimate periods.
In climate zone I, in zone III north of 26° S, and along the eastern margin of the hyperarid Atacama Desert (zone IV), between 18 ka and 9 ka B.P. prolonged intervals of wetter climate occurred in the Andes Mountains above 2000 m a.s.l. (Grosjean et al., 2001; Latorre et al., 2002, 2006; Rech et al., 2002; Placzek et al., 2009; Nester et al., 2007; Quade et al., 2008; Díaz et al., 2012; Gayó et al., 2012), referred to as the Central Andean Pluvial Event (CAPE) (Fig. 8). Contemporaneous groundwater-fed wetlands are reported in the Coastal Cordillera (Díaz et al., 2012). South of 25° S, wetter conditions in the Andean highlands during the Late Glacial Maximum, approximately 28-18 Ka B.P., are recognized (Lamy et al., 1998; Lamy et al., 2000; Maldonado et al., 2005; Díaz et al., 2012). Usually these paleoclimate intervals are assumed to be explained by one of three conditions known to have been modes of interannual variability during the 20th century (e.g., Lamy et al., 1998, 2000; Latorre et al., 2002, 2006; Maldonado et al., 2005; Quade et al., 2008; Garreaud et al., 2009; Placzek et al., 2009; Gayó et al., 2012; Díaz et al., 2012; Sáez et al., 2016). Two of these modes have been associated with enhanced precipitation on the margins of the Atacama Desert: the increased frequency of northward incursion of Pacific-sourced winter rains from mid-latitude weather systems, and more frequent westward spill-over of summer rains from Amazon-sourced air masses. The third mode, greater summer season supply of water vapor from the Argentine plains southeast of the Atacama Desert (Vuille and Keimig, 2004), is discussed in depth below. Not included among the paleoclimate options was the March 2015 scenario.

Because of location and season, a comparison of the March 2015 precipitation event to the scenarios for precipitation south of 22° S in the Central Andes evaluated by Vuille and Keimig (2004) is relevant. Vuille and Keimig (2004) demonstrated that summer precipitation during wetter-than-average years between 1983 to 1999 was commonly anti-phased north and south of a latitudinal limit near 22° S. They compared summer season rain station data for sparsely distributed Peruvian, Bolivian, Argentine and Chilean sites to satellite information indicative of convective cloud activity and demonstrated that the spatially extensive satellite data could be used as a precipitation proxy. The region north of 22° S behaves as described by earlier studies (Aceituno 1988; Rutllant and Fuenzalida, 1991; Houston and Hartley, 2003; Garreaud et al., 2009) (Fig. 2A), whereby Amazon lowland water vapor is transported westward to the Andean crest and western slope of the Andes whenever the balance between the dominant westerly winds and easterly flow shifts to allow westward translation of the eastern air mass. However, south of 22° S the satellite rain proxy data across the whole width of the Andes and corresponding atmospheric data suggest that summer rain is most likely when two anomalous conditions coincide: the low-level (below 700 hPa) air mass over the Argentine Pampas has anomalously high water vapor, and there exists easterly flow aloft (above the 500 hPa pressure level) (for reference, the crest of the Andes Mountains occurs at approximately the 600 hPa air pressure level). That situation was met (summers of 1983-1998) when the center of an upper level anticyclone was located near 37° S over the mid-latitude Argentine Pampas, which drove high altitude easterly winds on the north side of that anticyclone.
This scenario does not fit the 24-26 March 2015 precipitation event. Consistent with the Vuille and Keimig (2004) scenario, there was an area of enhanced precipitable water vapor over the Pampas near 28°-30° S on the first two days of the rain event (Bozkurt et al. 2016). Furthermore, there was an anticyclonic high over southern Argentina (onshore center near 46° S), which played a key role by setting up blocking that dictated the unusual path across the Andes taken by the equatorial Pacific air mass (Fig. 1 and Barrett et al., 2016). However, the pressure field to the north of that anticyclone resulted in a strong westerly flow at 600 mb, allowing Pacific-sourced water vapor to cross the crest of the Andes and enter the eastern lowlands (Fig. 8), not the more commonly assumed reverse direction of flow.
Several authors have called upon the anti-phasing of modern precipitation in the Central Andes (Vuille and Keimig, 2004) as an explanation for variability of the time-space pattern displayed by CAPE. For example, whereas a first CAPE stage (18-14.2 ka B.P.) was widespread north of 26 ° S (Fig. 8), at most locations south of 23° S the second stage (13.8-9.7 ka B.P.) was wetter (Gayó et al., 2012). The general spatial similarity between millennial-scale anti-phasing and the interannual anti-phasing led to the hypothesis that intervals like the second CAPE stage represent times of enhanced water vapor delivery to the southern Atacama Desert from the Argentine plains southeast of the Atacama (Placzek et al., 2009; Quade et al., 2008; Gayó et al., 2012; Sáez et al., 2016). An alternative explanation that should be evaluated is that enhanced frequency of conditions like those of late March 2015 was responsible for CAPE 2.
Times of wetter conditions documented in the central lowland (<3,000 m a.s.l.) core of the Atacama Desert (zone I) also merit reexamination in search of better understanding of the precipitation sources for the CAPE and Holocene vegetation. As summarized by Díaz et al. (2012), in the lowland region water supplies in excess of 20th century quantities on which paleo-plant growth depended might have come from four sources: i) local rainfall at the site where the paleo-vegetation grew; ii) increases in fog intensity or extent; iii) extreme rainfall at high elevations that caused flash floods in the hyperarid lowlands; iv) higher groundwater levels feeding perennial streams and wetlands in the lowlands due to recharge by persistent rainfall at high elevations. Among those options, the March 2015 precipitation event provided rain water locally (situation i) as well as at high elevations (iii, iv). If frequent repetition during the 21st century of the March 2015 conditions were to lead to the extent of environmental change recorded by paleoclimate records, then the flash-flood scenario (iii) and the groundwater recharge-discharge scenario (iv) may grow more easily differentiable. For the Late Pleistocene and Holocene sites with rodent middens as climate proxies, details of vegetation types can reveal the seasonality of precipitation and allow stream- or groundwater-fed oasis plants to be differentiated from hillslopes plants representative of local rainfall (e.g., at 3,000 m a.s.l., 22° S; Latorre et al., 2006; Gayó et al., 2012). The adoption of proxies that conserve information about the water isotope variations, such as rodent teeth or plant wax, would be invaluable to further investigate the regional paleoclimate system.
An additional historical perspective on precipitation pathways may be available in groundwater. Groundwater isotopic compositions reflect a time-integrated amount-weighted average of precipitation (Aravena, 1995; West et al., 2014). In some areas of the Atacama Desert groundwater recharge continued during the latter half of the 20th century (e.g., Houston, 2007), whereas other aquifers primarily recharged hundreds to thousands of years ago (Aravena, 1995; Herrera and Custodio, 2014; Herrera et al., 2018). Within that spectrum of recharge are insights to both recent climate and paleoclimate states. For example, spring water for coastal Antofagasta province (climate zone II) of apparent mid-Holocene age (Herrera and Custodio, 2014; Herrera et al., 2018) (Fig. 3A) has δ18O near zero (+0.2‰ to -2.2‰), evidence that those coastal springs recharged by precipitation derived from the adjacent Pacific Ocean. That composition is much like the March 2015 rain (Fig. 3A).
The middle Holocene record deserves new consideration in light of the March 2015 extreme rain scenario. In addition to the coastal springs, rodent middens with vegetation debris of similar age (3.7 ka B.P.) are reported 20 km inland (Díaz et al., 2012), paleo-spring deposits occur 140 km inland (3.1-4.7 ka B.P.) (Sáez et al., 2016), and paleowetlands occur 260 km inland (3.1-7.4 ka B.P.) (Rech et al., 2002). Collectively, these sites appear to define a region of enhanced precipitation stretching from the coast to the Andes (Fig. 8). If a discrete time interval of wet conditions did extend inland across the core of hyperarid zone IV, a reasonable interpretation would be that rains like those of March 2015 were common 3,000-5,000 years ago but not in more recent times. A similar paleoclimate history has been demonstrated for the west coast of South America farther north. Carré et al. (2014) showed that El Niño conditions began to deliver important quantities of rain to coastal Perú approximately 4.7 ka BP, after having been suppressed between 5-7 ka BP. Nevertheless, continuity of wetter conditions from the coast to the Andes across the hyperarid Atacama Desert at 22°-25° S during the same time is speculative. Both the spatial continuity of precipitation events across the Atacama Desert during the latter middle Holocene and the hypothetical linkage to warm SST conditions could be better evaluated if oxygen or hydrogen isotopic data from groundwater or middens of appropriate age become available.
Broadly, the March 2015 storm shows a need for reconsideration of paleoclimate interpretations that are linked to ENSO phase. A connection to changed or enhanced paleo-ENSO variability has been postulated to contribute to paleoclimate variability during the last 20,000 years in climate zone IV (Vargas et al., 2006; Latorre et al., 2006). During the last century La Niña conditions have enhanced summer rainfall on the Altiplano (zone I) whereas El Niño conditions increased winter precipitation in central Chile (zone III) (Aceituno, 1988; Rutllant and Fuenzalida, 1991; Garreaud et al., 2009). For coastal northern Chile (zone II) a correlation between precipitation and El Niño conditions is positive only for winter rain along the coastline (Ortlieb, 1995; Vargas et al., 2006; Bozkurt et al., 2016). While it is reasonable that an increase in rain in any of those neighboring zones would increase the likelihood of increased rain in the core of the Atacama Desert, the case is not strong for attributing past wet intervals in zone IV to a given ENSO phase. The March 2015 rain, for summer season at the onset of an El Niño, demonstrates that preconceived notions about how ENSO might modulate rain in the hyperarid Atacama Desert should be applied judiciously to paleoclimate interpretation.
Much longer duration paleoclimate variations can also be illuminated by the March 2015 event. Amundson et al. (2012) present the history of aridity in the Atacama Desert recorded in landforms between 23°-25° S (Fig. 8, box with dashed black border). The northern 100 km of the region of heavy rain (>30 mm) during the March 2015 event coincided with the Amundson et al. (2012) study area. They deduced that less arid conditions prior to circa 2 Ma corresponded to warmer SSTs in the eastern equatorial Pacific and a diminished east-west temperature gradient (a persistent El Niño state), whereas hyperarid conditions since that time corrresponded to overall cooler SSTs and an east-west gradient characteristic of La Niña conditions. Given the prominent geomorphological tranformations that resulted from that climate change, Amundson et al. (2012) drew attention to the possibility that future climate warming might increase rainfall in northern Chile. The late March 2015 conditions and consequences align well with their prediction.
The fact that the δ18O and δ2H of March 2015 rain are readily differentiated from other historical rains (Fig. 4) and are diagnostic of a tropical Pacific source should stimulate reexamination of Atacama Desert paleoclimate records. Mapping of the spatial patterns of δ18O and δ2H in paleo-precipitation proxies or of long residence-time groundwater would enable better differentiation of times and regions impacted by rain like that of March 2015.
6. Conclusions
From 24-26 March 2015 heavy rain fell across a very wide area of northern Chile’s Atacama Desert. The driver for this rare and high-impact event was an unusual weather system that traversed the Pacific Ocean at a time that the ocean’s surface water was unusually warm. Isotopic values of rain water and river samples demonstrate that the March 2015 precipitation event supplied water that was outside the isotopic range expected for the western slope of the Andes between 23°-30° S, and therefore similar past events should be recognizable in paleohydrological records. In combination, the stable isotopes and atmospheric conditions show that the eastern subtropical and tropical Pacific Ocean was the source of the water vapor. The conditions that produced the March 2015 rain in the hyperarid Atacama Desert had not been included among scenarios for interannual variability of modern climate states. Likewise, the March 2015 scenario was overlooked as a possibility to explain documented wetter intervals in the Atacama Desert during the late Pleistocene and Holocene. Here we show that a comparison of the spatial distribution of areas with proxies indicative of past wetter conditions to the distribution of precipitation from modern major events is one clue to the plausible water vapor source area. Nevertheless, future incorporation of isotopic evidence that could fingerprint paleo-water vapor pathways like that of March 2015 will help to disentangle spatially overlapping phenomena and improve interpretations of causation of past climate change.
Acknowledgments
This study was supported by Anillo Project ACT1203 of CONICYT (Chile). CONICYT/FONDAP Grant 15110017 (National Research Center for Integrated Natural Disaster Management) supported rapid response task forces shortly after the March and August 2015 precipitation events. The investigation was also funded by Ph.D. grants from CONICYT-PCHA/Doctorado Nacional, number 2016-21160152 for author C. Gamboa P. and 2015-21150951 for author J. Urrutia M. We are grateful to the Air Resources Laboratory of NOAA (USA) for developing HYSPLIT and providing online access. Technical assistance by staff of University of Arizona and Cornell University stable isotope laboratories is appreciated, and by R. Riquelme, H. Ramos, L. Tapia, K. Centellas, I. Del Río, M. Pulgar (Universidad Católica del Norte, Antofagasta) and J. Gironás L. (Pontifícia Universidad Católica de Chile). Reviews of an earlier draft of this paper by I. Aguirre and M. Rojas resulted in significant improvements.
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Notes
Author notes
tej1@cornell.edu