A dense winter bloom of the dinoflagellate Heterocapsa triquetra was observed at a fixed station (44°35.3'S; 72°43.6'W) in the Puyuhuapi Fjord in Chilean Patagonia during July 2015. H. triquetra dominated the phytoplankton community in the surface waters between 2 and 15 m (13-58 × 10 9 cell m -2 ), with abundances some 3 to 15 times higher than the total abundance of the diatom assemblage, which was dominated by Skeletonema spp. The high abundance of dinoflagellates was reflected in high rates of gross primary production (GPP; 0.6-1.6 g C m -2 d -1 ) and chlorophyll-a concentration (Chl-a; 70-199.2 mg m -2 ) that are comparable to levels reported in spring diatom blooms in similar Patagonian fjords. We identify the main forcing factors behind a pulse of organic matter production during the non-productive winter season, and test the hypothesis that low irradiance levels are a key factor limiting phytoplankton blooms and subsequent productivity during winter.Principal Component Analysis (PCA) indicated that GPP rates were significantly correlated (r = -0.8, p< 0.05) with a decrease in salinity/temperature and the presence of the Heterocapsa bloom. The bloom occurred under low surface irradiance levels characteristic of austral winter and was accompanied by strong northern winds, associated with the passage of a low-pressure system, and a water column dominated by double diffusive layering. To our knowledge, this is the first report of a dense dinoflagellate bloom during deep austral winter in a Patagonian fjord, and our data challenge the paradigm of light limitation as a factor controlling phytoplankton blooms in this region in winter.
Abstract. In the Southern Hemisphere, macroscale atmospheric systems such as westerly winds and the southeast Pacific subtropical anti-cyclone (SPSA) influence the wind regime of the eastern austral Pacific Ocean. The average and seasonal behaviors of these systems are well known, although wind variability at different time and distance scales remains largely unexamined. Therefore, the main goal of this study was to determine the variabilities of surface winds on a spatiotemporal scale from 40 to 56∘ S, using QuikSCAT, Advanced Scatterometer (ASCAT), and the fifth major global European Centre for Medium-Range Weather Forecasts (ECMWF) reanalysis (ERA5) surface-wind information complemented with in situ meteorological data. In addition, interactions between the atmospheric systems, together with the ocean–atmosphere response, were evaluated for the period 1999–2018. The empirical orthogonal function detected dominance at the synoptic scale in mode 1, representing approximately 30 % of the total variance. In this mode, low and high atmospheric pressure systems characterized wind variability for a 16.5 d cycle. Initially, mode 2 – which represents approximately 22 % of the variance – was represented by winds from the west/east (43–56∘ S), occurring mostly during spring and summer/fall and winter at an annual timescale (1999–2008) until they were replaced by systems cycling at 27.5 d (2008–2015). This reflects the influence of the baroclinic annular mode in the Southern Hemisphere. Mode 3, representing approximately 15 % of the variance, involved the passage of small-scale low and high atmospheric pressure (LAP and HAP) systems throughout Patagonia. Persistent Ekman suction occurred throughout the year south of the Gulf of Penas and beyond the Pacific mouth of the Strait of Magellan. Easterly Ekman transport (ET) piled these upwelled waters onto the western shore of South America when winds blew southward. These physical mechanisms were essential in bringing nutrients to the surface and then transporting planktonic organisms from the oceanic zone to Patagonian fjords and channels. In the zonal band between 41 and 43∘ S, the latitude of Chiloé Island, upward Ekman pumping and Ekman transport during spring and summer favored a reduced sea surface temperature and increased chlorophyll a (Chl a) levels; this is the first time that such Ekman upwelling conditions have been reported so far south in the eastern Pacific Ocean. The influence of the northward-migrating LAP systems on the ocean–atmosphere interphase allowed us to understand, for the first time, their direct relationship with recorded nighttime air temperature maxima (locally referred to as “nighttime heatwave events”). In the context of global climate change, greater attention should be paid to these processes based on their possible impact on the rate of glacier melting and on the austral climate.
Abstract. In the southern hemisphere, macroscale atmospheric systems such as the westerly winds and the Southeast Pacific Subtropical anti-cyclone (SPSA) influence the wind regime of the eastern Austral Pacific Ocean. The average and seasonal behaviors of these systems are well known, although wind variability at different time and distance scales was previously unexamined. The main goal of this study was, therefore, to determine the space and time scale variabilities of surface winds from 40° to 56° S, using QuikSCAT, ASCAT, and ERA-Interim surface wind information, complemented by in situ meteorological data. In addition, interactions between atmospheric systems, together with the ocean–atmosphere dynamics, were evaluated, from 1999 to 2015. The empirical orthogonal function detected dominance at the synoptic scale in mode 1, representing approximately 30 % of the total variance. In this mode, low and high atmospheric pressure systems characterized wind variability, with a cycle length of 16.5 days. Initially, mode 2, representing approximately 22 % of the variance, was represented by westerly winds (43° to 56° S), which occurred mostly during spring and summer, with an annual time scale (1999–2008), until they were replaced by systems cycling at 27.5 days (2008–2015), reflecting the influence of the Southern Hemisphere's baroclinic annular mode. Mode 3, representing approximately 15 % of the variance, involved passage of small scale, low and high atmospheric pressure (LAP, HAP) systems throughout Patagonia. Persistent Ekman suction south of the Gulf of Penas, and up to and beyond the Pacific mouth of the Magellan Strait, occurred throughout the year. Easterly Ekman transport (ET) piled these upwelled waters onto the western shore of South America, when the winds blew southward. These physical mechanisms were essential in bringing nutrients to the surface, and then transporting planktonic organisms from the oceanic zone into Patagonian fjords and channels. In a variation, between 41° and 43° S, surface wind from the SPSA produced offshore ET during spring and summer, causing reduced sea surface temperature, and increased chlorophyll-a; this is the first time that such upwelling conditions have been reported so far south, in the eastern Pacific Ocean. The influence of northward migrating LAP systems on the ocean–atmosphere interphase allowed us to understand, for the first time, their direct relationship with recorded night time air temperature maxima (locally referred to as Nighttime heat wave events). In the context of global climate change, greater attention should be paid to these processes, based on their possible impact on the rate of glacier melting, and on the austral climate.
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