Under-Ice Phytoplankton Blooms: Shedding Light on the “Invisible” Part of Arctic Primary Production

Abstract

The growth of phytoplankton at high latitudes was generally thought to begin in open waters of the marginal ice zone once the highly reflective sea ice retreats in spring, solar elevation increases, and surface waters become stratified by the addition of sea-ice melt water. In fact, virtually all recent large-scale estimates of primary production in the Arctic Ocean (AO) assume that phytoplankton production in the water column under sea ice is negligible. However, over the past two decades, an emerging literature showing significant under-ice phytoplankton production on a pan-Arctic scale has challenged our paradigms of Arctic phytoplankton ecology and phenology. This evidence, which builds on previous, but scarce reports, requires the Arctic scientific community to change its perception of traditional AO phenology and urgently revise it. In particular, it is essential to better comprehend, on small and large scales, the changing and variable icescapes, the under-ice light field and biogeochemical cycles during the transition from sea-ice covered to ice-free Arctic waters. Here, we provide a baseline of our current knowledge of under-ice blooms (UIBs), by defining their ecology and their environmental setting, but also their regional peculiarities (in terms of occurrence, magnitude, and assemblages), which is shaped by a complex AO. To this end, a multidisciplinary approach, i.e., combining expeditions and modern autonomous technologies, satellite, and modeling analyses, has been used to provide an overview of this pan-Arctic phenological feature, which will become increasingly important in future marine Arctic biogeochemical cycles.

Historical Perspective: Under-Ice Blooms, an Overlooked Phenological Feature

The idea of phytoplankton blooms developing underneath an ice cover, also called under-ice blooms (UIBs), had been sporadically reported in the past (see below) but became widely accepted by the scientific community only after a massive UIB was reported in the Chukchi Sea (Arrigo et al., 2012, 2014). The hypothesis that light inhibits the development of phytoplankton blooms under a snow, ice, and ice algal cover had previously prevailed in the Arctic scientific community’s thinking. This assumption has likely led to significant errors in estimates of Arctic-wide production and phytoplankton phenology. For example, it was suggested that net primary production over Arctic shelves could be up to an order of magnitude larger than currently estimated from open water measurements (Arrigo et al., 2012). However, the assumption is not new. In fact, studies in the early part of the last century concluded that thick ice and low temperatures limited the development of phytoplankton under the central Arctic ice pack (Nansen, 1902; Gran, 1904; Sverdrup, 1929).

Noted by English (1961), it was Braarud (1935) who first put forward the idea that, although limited by light, phytoplankton can still grow under the Arctic pack ice. It was suggested that the use of phytoplankton nets with relatively coarse mesh size at the time may have missed the abundant but smaller sized fraction of the phytoplankton community. Confirming the hypothesis of under-ice phytoplankton production, Shirshov (1944) showed that a seasonal cycle of phytoplankton development occurred northeast of Greenland under the 3 m thick permanent ice pack with maximum chlorophyll a (Chl a) concentrations reaching 0.4 mg m^–3 in the upper 20 m of the water column. Again, one of the limitations of this work was the use of nets to collect phytoplankton samples, the tool available at the time.

It was not until two decades later, during the 1957–58 International Geophysical Year (IGY) drift station expeditions, that the opportunity arose to observe annual cycles of phytoplankton standing stocks and production using the more modern techniques of the time. The end result of this work was nothing less than an incredible first glimpse of UIBs occurring in the central Arctic (Apollonio, 1959; English, 1961). Both studies demonstrated the progression of what we term “classical” UIBs, where bloom development begins slowly under a melting snow cover and fully develops under melt pond-covered sea ice. Unfortunately, both of these papers have remained in relative obscurity, the first having been published as a short note in the IGY Bulletin (Apollonio, 1959), and the second as a scientific report (English, 1961). In other words, both research papers are difficult to access using today’s online search engines, which limited their use in the flourish of papers on UIBs over the last decade. It is for this purpose that we include key data from these studies in Figure 1 to showcase their relevant observations.

FIGURE 1

The two separate drift stations, Alpha and Bravo, drifting on opposite sides of the Beaufort High Gyre, showed surprisingly similar results (Figure 1). Both sites had a 3 m thick multiyear ice cover with hummocks reaching more than 9 m thick and ∼1% lead coverage (estimates by aircraft; Apollonio, 1959; English, 1961). At both sites, the observed UIBs were initiated during the snowmelt period in July after the solstice insolation peak and quickly ended when snow began to accumulate. This prevailing light limitation driven by the snow cover is particularly evident when comparing the 1957 and 1958 UIBs at Alpha station. A longer snow-free period during summer led to a longer lasting UIB. It is impossible to quantitatively compare integrated Chl a values between these years due to inconsistencies in sampling depths (Figure 1A). Melt ponds started to form during the first week of July at Alpha station in both 1957 and 1958, covering 15–30% of the ice pack surface. This melt pond coverage closely matches more recent reports for multiyear ice ranging from 6.8 to 25% (Fetterer and Untersteiner, 1998; Nicolaus et al., 2012; Huang et al., 2016). Of course, the most dramatic change is the loss of multiyear ice (MYI) and its replacement by first-ice year ice (FYI) and the resulting increase in light transmission during the melt period (Nicolaus et al., 2012; Horvat et al., 2017).

A comparison between Alpha and Bravo stations in 1957 suggests that production of phytoplankton biomass was greater at Alpha station, where the maximum Chl a concentration was >1.5 mg m^–3 (Figure 1A; English, 1961) versus at Bravo station where it was only 0.37 mg Chl a m^–3 just under the ice (Apollonio, 1959). Furthermore, while the integrated Chl a biomass was estimated over a depth interval of 100 m at Bravo station, the maximum biomass was only ∼21 mg m^–2 versus the >30 mg Chl a m^–2 estimated at Alpha station and only integrated over the upper 20 m. Similarly, averaged daily production, directly estimated by ¹⁴C incubation at Bravo station, was about half that of a more conservative estimate derived from the net Chl a accumulation rate at the Alpha station (Table 1). The central Arctic ice pack tends to be more convergent along the northern edge of the Canadian Archipelago (Haas et al., 2017). It is likely that drift station Bravo had more deformed (hummock) ice with a thicker ice cover and hence greater light limitation that would help to explain the observed lower Chl a concentrations. Both studies concluded that light limitation controlled under-ice primary production. In fact, English (1961) conducted a nutrient addition experiment and found no response, suggesting that nutrients were not limiting. However, Apollonio (1959) concluded that although light availability controlled phytoplankton production, the nitrogen-depleted upper 150 m water column, with NO₃:PO₄ ratios averaging 7:1 relative to the Redfield ratio of 16:1 (Redfield et al., 1963), would ultimately constrain the central Arctic to have one of the lowest productivities in the world even if light limitation was not a prime factor.

Since those early studies, UIBs in the Arctic have received a modest amount of attention based on the number of times those features have been described in the literature (Table 1 and Figure 2). Additional datasets from online and unpublished data sources confirm the occurrence of UIBs. Table 1 shows that after the IGY studies, there was a period of more than three decades before direct documentation of UIBs were published (e.g., Michel et al., 1993, 1996; Strass and Nöthig, 1996; Gosselin et al., 1997). However, it is clear that UIBs were occurring during this gap of published literature. In fact, UIBs were observed in the early 1960s in Jones Sound (Apollonio and Matrai, 2011) and from the mid-1980s to the 1990s near Resolute Bay in the Canadian Arctic Archipelago (Table 1). Reports of UIBs after the mid-1990s remained relatively sporadic (e.g., Yager et al., 2001; Fortier et al., 2002; Mundy et al., 2009; Leu et al., 2011) until the last decade when the occurrence of UIBs was documented for almost all Arctic and sub-Arctic marine regions (Table 1). The recent effort to improve our understanding of UIBs has led to dedicated scientific programs [e.g., Arctic-ICE (Mundy et al., 2014), FAABulous (Leu et al., pers. comm.), Green Edge (Oziel et al., 2019; Randelhoff et al., 2019), ICESCAPE (Arrigo et al., 2012), N-ICE (Assmy et al., 2017), SUBICE (Arrigo et al., 2017)] as well as the deployment of new monitoring technologies (Laney et al., 2014; Hill et al., 2018; Mayot et al., 2018; Boles et al., 2020; Randelhoff et al., 2020) and directed modeling efforts (e.g., Palmer et al., 2014; Zhang et al., 2015; Horvat et al., 2017; Lowry et al., 2018; Kinney et al., 2020). In this paper, we attempt to provide the state of the art of our knowledge of UIBs, by focusing on their ecology and environmental control, but also their regional specificities (in terms of occurrence, magnitude, and assemblages), which are shaped by the complexity of the rapidly changing Arctic physico-chemical environment. To this end, a multidisciplinary approach, i.e., combining expeditions and modern autonomous technologies (see “Box 1: New technologies: More insights on under-ice biogeochemical cycles and blooms”), satellite, and modeling analyses, has been used to provide an overview of this pan-Arctic phenological feature, which should become increasingly important in future Arctic biogeochemical cycles.

FIGURE 2

Changing Under-Ice Light Regime, Precursor to Under-Ice Blooms?

Large-Scale Under Sea-Ice Light Regimes

As a consequence of a warming Arctic climate, Arctic sea ice melts earlier and more widely, leading to Arctic-wide reductions in sea-ice thickness and age (Kwok, 2018; Stroeve and Notz, 2018). Arctic sea ice is now predominantly thin, first or second-year ice, and large areas formerly covered by sea ice year-round are now ice-free in summer (Kwok, 2018; Stroeve and Notz, 2018). Arctic warming also leads to an earlier transition from snow- to melt pond-covered ice, which significantly reduces the albedo of the ice-covered Arctic Ocean (AO) earlier in the year, and closer to peak insolation of the annual solar cycle (Perovich et al., 2007). Reduced surface albedo due to a greater melt pond coverage of FYI compared to MYI (Nicolaus et al., 2012; Perovich and Polashenski, 2012) and reduced attenuation by thinner ice are crucial for the initiation of UIBs (Arrigo et al., 2012, 2014; Oziel et al., 2019; Ardyna et al., 2020). Together, these factors lead to a substantial increase in the availability of photosynthetically active radiation (PAR; 400–700 nm) for primary production in the ice-covered upper ocean, making widespread UIBs a possibility that was hypothesized by Mundy et al. (2009) and recently recognized (Horvat et al., 2017; Kinney et al., 2020).

Due to the lack of long-term observations of the under-ice light field, climate model hindcasts can provide a useful tool for examining trends in light availability in the ice-covered Arctic surface layer. Here, we analyze the ensemble climate model statistics from 11 historical (1850–2014) CESM2 simulations submitted to CMIP6 for each month between June and August (panels from left to right; Figure 3). Note that the CICE5.1 model used in CESM2 employs a Delta-Eddington scheme for reflection, absorption, and transmission of solar radiation as a function of sea-ice thickness, surface type, and sea-ice inherent optical properties. This scheme has been extensively validated, accurately reproducing optical properties of Arctic sea ice (Briegleb and Light, 2007; Light et al., 2008). Figures 3A–C show the total extent of sea ice and the total extent of the compact ice zone (CIZ), defined as the total area where the concentration of sea ice is greater than 80%, and thus the area where there is sufficient sea ice for UIBs to be relevant. The modeled trend in the loss of CIZ extent reflects and exceeds the loss in total sea-ice extent, resulting in a larger fraction of the Arctic being covered with low concentration sea ice (a result found across CMIP6 models), and little sea ice in CESM2 is considered “compact” by August.

FIGURE 3

The remaining compact ice, however, is more transparent. The Arctic-average PAR flux (μmol photons m^–2 s^–1) through sea ice in the CIZ has increased dramatically (Figures 3D–F), doubling in June and July, when the transitions in sea-ice surface type are most dramatic. These model results are consistent with recent observations by Castellani et al. (2020) who measured the highest daily integrated under-ice PAR levels (i.e., 4.46–20.71 mol photons m^–2 d^–1) in the central Arctic in June–July. To estimate what fraction of the CIZ could support UIBs, we used a simple critical depth model (Sverdrup, 1953; and a threshold value for PAR flux of 34 μmol photons m^–2s^–1 with a 20 m deep mixed layer; see Horvat et al. (2017) for the choice of all parameters used here). Up to 2.5 × 10⁶ km² of the ice-covered AO permitted UIBs in June (Figure 3G), compared to 3.5 × 10⁶ km² in July (Figure 3H), despite the declining area of the CIZ in July (Figure 3B). During this month, in up to 100% of the CIZ, under-ice PAR levels were above the threshold of 34 μmol photons m^–2s^–1, which allows for net phytoplankton growth and biomass increase. Interestingly, large portions of the AO may have permitted UIBs in the surface layer in the past, amounting to about 2 × 10⁶ km² in July or between 30 and 40% of CIZ area (10–20% of total sea-ice extent). This can help explain why sporadic UIBs were recorded in the past (see the section “Historical Perspective: Under-Ice Blooms, an Overlooked Phenological Feature”). That is, historical light conditions could occasionally be sufficient for UIBs to develop, though their frequency has likely greatly increased over the past several decades.

The geographical pattern of modeled light field changes for the months of June to August also provides some interesting insights (Figure 4). The 2010–2014 average ensemble mean downwelling PAR through sea ice demonstrates that the regions permitting UIBs are confined to the periphery of the CIZ in June, but extend over most of the Arctic in July. This is a recent change; historically during July (Figure 4E), the areas supporting UIBs lay outside of the modern CIZ, and UIBs were only found on the periphery of the (historical) July CIZ. The difference between these two areas is largely broad-based and non-regional, with the signature of larger changes in sea-ice thickness and melt state rather than the imprint of regional variability.

FIGURE 4

While the overall under-ice light availability increased with decreasing ice thickness over recent decades, small-scale sea-ice features such as the geometry of melt ponds at the ice surface, ridges, hummocks, leads, and the horizontal distribution of light absorbing ice impurities cause spatial heterogeneity in PAR transmission (Ehn et al., 2008, 2011; Light et al., 2008; Frey et al., 2011; Katlein et al., 2014, 2016; Matthes et al., 2019; Horvat et al., 2020). The resulting complexity of the under-ice light field creates difficulties in measuring and estimating light availability for UIB phytoplankton since algal cells drifting in under-ice surface waters are exposed to large variations in PAR throughout the day. Overlooking the complexity of the under-ice light field and its characteristic optical parameters can oversimplify model development and our general understanding of UIB phenology.

Small-Scale Heterogeneity in Light Propagation Through Arctic Sea Ice

After the return of the sun in spring, transmission of PAR through refrozen leads in the dynamic ice cover can trigger early season phytoplankton blooms beneath the still snow-covered sea ice (Assmy et al., 2017). Later, during melt pond formation, regional PAR transmission through FYI increases rapidly to 25–31% (Figure 5, Katlein et al., 2019; Matthes et al., 2020), which marks the potential onset of an UIB and, simultaneously, the termination of the ice algal bloom (Oziel et al., 2019). Earlier bottom ablation and termination of the ice algal bloom also improves the under-ice light climate for phytoplankton and can contribute to the initiation of UIBs (Mundy et al., 2014). Another key prerequisite for the initiation of an UIB is stratification of the surface layer induced by melt water addition (Oziel et al., 2019) as already suggested by Legendre et al. (1981).

FIGURE 5

As the euphotic zone starts to deepen until enhanced light attenuation by blooming phytoplankton reverses this process (Figure 5, Oziel et al., 2019), the increasing difference in light transmittance through ponded versus bare ice, combined with the lateral spreading of photons within the ice layer, create large fluctuations of up to 43% in under-ice PAR levels for drifting phytoplankton communities in the upper ocean beneath landfast sea ice (Matthes et al., 2020). Higher light transmission through more transparent nearby structures (i.e., refrozen leads, melt ponds, and bare ice) impacts the vertical radiation transfer in the water column causing edge effects at the ice bottom and subsurface irradiance maxima beneath bare ice adjacent to melt ponds (Ehn et al., 2011; Frey et al., 2011; Katlein et al., 2016).

During the melt season, the under-ice light field can change over a relatively short time and, in turn, can cause a large error in regional estimates of under-ice PAR availability for marine primary production. Single-location transmittance measurements beneath one ice surface type may not be representative of the average PAR experienced by phytoplankton cells that drift at a different rate and direction relative to the overlying sea ice. Perovich (2005) was the first to define the spatial scale of the minimal variation in the partitioning of incident solar radiation as an “aggregate scale”. Using this approach, regional light transmission can be calculated as the sum of average transmission values for each surface type (melt ponds, bare ice, open water) multiplied by its areal fraction (e.g., Taskjelle et al., 2017; Katlein et al., 2019; Massicotte et al., 2019; Matthes et al., 2020).

Figure 5 highlights the complexity of the radiation field beneath the ice cover that creates large variations in the apparent optical properties, such as the diffuse vertical attenuation coefficient (K_d) and the average cosine coefficient (μ_d) of downwelling irradiance, which are used to calculate the depth of the euphotic zone and thereby the accessibility to subsurface inorganic nutrients for primary production. Subsurface maxima in PAR from higher light transmission through adjacent melt pond-covered ice alter the vertical light distribution, resulting in a non-exponential decrease in PAR with depth and difficulties in estimating K_d (Ehn et al., 2011; Frey et al., 2011; Katlein et al., 2016; Laney et al., 2017). Several studies investigated separation of the effects of water column attenuation from local spatial heterogeneity in transmittance through sea ice using semi-empirical models (Frey et al., 2011; Laney et al., 2017) or by deriving K_d from upwelling radiation (Massicotte et al., 2018). Besides a more robust K_d, the angular distribution of light in the surface water layer needs to be considered in the parametrization of the under-ice light field due to multiple scattering in the overlying snow and ice cover and/or enhanced backscattering of algal cells under bloom conditions (Ehn et al., 2011; Arrigo et al., 2014; Katlein et al., 2014; Pavlov et al., 2017). Considering this lateral photon transport, scalar radiometers with a spherical collector that capture PAR from all directions provide a more realistic measurement of light availability for primary production (Morel and Gentili, 2004; Pavlov et al., 2017; Matthes et al., 2019). If only downwelling planar PAR can be measured beneath the ice, a μ_d between 0.56 and 0.7 can be used to convert these measurements into downwelling scalar PAR (Arrigo et al., 1991, 2014; Ehn and Mundy, 2013; Katlein et al., 2014; Pavlov et al., 2017; Matthes et al., 2019).

Underestimating light availability in the ice-covered water column has large implications on the calculation of the euphotic zone (depths where PAR is >0.2–1% of surface PAR) or isolume (integrated daily irradiance of 0.4 mol photons m^–2 d^–1, Letelier et al., 2004) depths and the investigation of the UIB onset. During pre-bloom conditions, light availability limits photosynthesis and under-ice phytoplankton communities are acclimated to low-light conditions. In this time period, the impact of errors in the under-ice light field parametrization on calculated primary production rates is largest due to the linear relationship between the rate of photosynthesis and increasing light levels before reaching saturation levels (Matthes et al., 2019).

Physiological Phytoplankton Assemblage Responses to Varying Light Regimes

Phytoplankton are well acclimated to the low-light under-ice environment by maximizing light absorption and photosynthetic capacity (Palmer et al., 2011, 2013; Lewis et al., 2019). As light transmission increases through melt pond formation and sea-ice melt, phytoplankton cells modify their pigment composition (Hill et al., 2005; Johnsen et al., 2018; Kauko et al., 2019), the number and size of their photosynthetic units (Matsuoka et al., 2009, 2011; Lewis et al., 2019) and through those adjustments change their measurable photosynthetic parameters of the photosynthetic machinery to maximize light utilization. Changes in the photoprotective to photosynthetic pigment ratio of under-ice phytoplankton communities to acclimate to the changing light availability have been observed as blooms progress. During pre-bloom and early bloom conditions, intracellular concentrations of Chl a and accessory pigments increase, supported by the abundant nutrients in the surface layer required for biosynthesis (Geider et al., 1998; Lewis et al., 2019). Although the high nutrient availability further supports large cell sizes, phytoplankton cells are heavily packed with pigments resulting in reduced cross sectional absorption (when absorption is normalized to pigment) due to self-shading (package effect; Morel and Bricaud, 1981; Hill et al., 2005; Matsuoka et al., 2011). Nevertheless, these pre-bloom communities are well adapted to achieve high rates of photosynthesis for small increases in under-ice light levels through a high photosynthetic efficiency, α, typical of low-light environments, paired with a high maximum rate of carbon fixation, P_max (Palmer et al., 2013; Lewis et al., 2019). Interestingly, the light saturation parameter, E_k, was found to be higher than the available average light intensity (Johnsen et al., 2018; Lewis et al., 2019). Lewis et al. (2019) concluded that under-ice phytoplankton communities are “primed” for later season increases in light availability. Hence, shade-acclimation allows algae to maximize their growth rate and to utilize the limited nutrient reservoir immediately once light levels increase through melt pond formation and ice melt. This acclimation strategy also enables phytoplankton to adjust quickly to the higher light conditions at ice edges (e.g., leads and polynyas; Palmer et al., 2011; Assmy et al., 2017; Lowry et al., 2018). In particular, pelagic diatoms were found to be able to rapidly acclimate successfully to drastically increased light conditions, in strong contrast to that of sea-ice diatoms (Kvernvik et al., 2020).

During bloom conditions at higher light intensities, under-ice communities increasingly synthesize photoprotective carotenoids (Hill et al., 2005; Joy-Warren et al., 2019; Kauko et al., 2019) and mycosporine-like amino acids (Elliott et al., 2015) that dissipate excess light energy as heat instead of channeling it to photosystems. This process of non-photochemical quenching enables a high degree of plasticity of the photosynthetic performance of bloom-forming species such as Phaeocystis, promoting its dominance under highly variable light regimes (Arrigo et al., 2010; Assmy et al., 2017; Joy-Warren et al., 2019). However, nitrate that is needed to synthesize proteins and pigments is often depleted during the late stage of an UIB, and thus impedes the photo-acclimation responses to increasing light levels by reducing the number of functional reaction centers and the photochemical efficiency of the photosynthetic machinery (Lewis et al., 2019, and citations therein). As shade-acclimated phytoplankton transition from a low-light regime beneath the ice into a high-light regime in open water, carbon fixation rates can decrease due to super-saturating light intensities (Figure 5, Palmer et al., 2011). According to the observations by Palmer et al. (2011), communities were able to acclimate to the high-light environment in the surface water after 4–10 days while phytoplankton at the subsurface chlorophyll maximum (SCM) remained shade-acclimated with comparable α and P_max to those of under-ice communities.

Contrasted Regional Environmental Settings Favoring UIBs

The AO is surrounded by land and has a complex topography of shelves, slopes, basins, channels, and sills. These features strongly constrain ocean circulation, primarily driven by both wind and buoyancy processes (Timmermans and Marshall, 2020) and are influenced by the Atlantic and Pacific inflows. These warmer and saltier inflows are the main source of inorganic nutrients for the colder and fresher Arctic domain. Stratification is generally driven by salinity rather than temperature in the AO (beta rather than alpha oceans; sensuCarmack, 2007). Indeed, the AO generally acts as a freshwater reservoir especially in the anticyclonic Beaufort Gyre (Proshutinsky et al., 2019). Most (>50%) of this freshwater is received from rivers and, to a lesser extent, sea-ice melt and precipitation (Haine et al., 2015). Light availability above the sea-ice surface is dictated by the annual light cycle, which itself depends on latitude. However, the light transmitted to the ocean surface is controlled to a large extent by the properties of clouds (Bélanger et al., 2013), as well as sea ice and its overlying snow cover (see the section “Small-Scale Heterogeneity in Light Propagation Through Arctic Sea Ice”).

The occurrence of UIBs, like open water phytoplankton blooms, is governed by bottom-up (e.g., temperature, light and nutrient availability, water column stability) and top-down (e.g., zooplankton grazing, viral infection, parasite infestation) controls. UIBs appear to be an ubiquitous feature of the Arctic spring bloom (see the section “Historical Perspective: Under-Ice Blooms, an Overlooked Phenological Feature”), but the mechanisms underlying their formation, as well as their phenology and species succession may be diverse due to regional specificities. Here we synthesize the currently available knowledge on the atmosphere-snow-ice-ocean processes that have been shown to control UIB dynamics. This approach enables both an assessment of the relevance of regional specificities (bathymetry, tides), as well as the influence of changing environmental conditions (i.e., sea ice, snow, ocean circulation, wind regimes) for future developments in UIB distribution and phenology (Figures 6, 7).

FIGURE 6

FIGURE 7

Upwelling Systems

Wind-driven upwelling along the continental shelves, shelf breaks, and ice edges are a source of substantial change in water masses and cross-shelf transport (Williams and Carmack, 2015). They allow nutrient-rich subsurface water masses to shoal up to the surface over shelves. Such processes have been documented in several regions such as the Beaufort (Pickart et al., 2009; Jackson et al., 2015) and the Chukchi (Arrigo et al., 2014; Spall et al., 2014) seas. There, these upwelling systems are characterized by an eastward flowing Pacific shelf break jet overlying the offshore Atlantic boundary current (see Figures 6A, 7).

The continental slope of the Beaufort Sea appears to present the most favorable upwelling conditions (Carmack and Chapman, 2003) for inducing UIBs because: (1) the shelf break is the shallowest and steepest of the AO (see Figure 6A; Randelhoff et al., 2018); (2) the region is characterized by persistent zonal wind regimes determined by the atmospheric circulation patterns of the Beaufort High and Aleutian Low; and (3) upwelling along the Canadian continental slope of the Beaufort Sea is favored by northeasterly wind regimes oriented along the bathymetric slope (Kirillov et al., 2016) and a westerly inversion of the normally eastward-flowing Pacific shelf break jet (Spall et al., 2014). Thus, when the wind regime allows it, nutrients are upwelled from the Beaufort basin at depth (typically winter Pacific or Atlantic waters; Schulze and Pickart, 2012; Pickart et al., 2013) and stimulate primary production on the Beaufort shelf (Carmack et al., 2004; Tremblay et al., 2011; Ardyna et al., 2017). On the Atlantic side, the presence of warm and nutrient-rich Atlantic waters at the surface in the region north and west of Svalbard during winter has been attributed to upwelling (Falk-Petersen et al., 2015), but later oceanographic campaigns have not found such evidence (Randelhoff et al., 2018). The occurrence of wind-driven upwelling in the European sector is rather unlikely because the area is not subject to upwelling-favorable winds (i.e., northeast winds) and the shelf slope is much deeper (Randelhoff and Sundfjord, 2018). By contrast, the Atlantic sector is much more sensitive to vertical mixing, wintertime convection and advection (Lind et al., 2018).

Advective Systems of the Atlantic Sector

The European sector is the most dynamic region of the AO, particularly along the Atlantic waterway which closely follows the slope of the Barents Sea continental shelf. At the very end of one of the branches of the Atlantic Current (i.e., the Svalbard branch), the Atlantic waters flow beneath the more buoyant polar surface waters, which are generally sea-ice covered until spring. This is a place where UIBs have been documented (Figure 6B) but the most important evidence of UIBs in this region was reported during the N-ICE expedition (Assmy et al., 2017). The authors suggested that Atlantic waters could play a second order role in seeding polar surface waters with phytoplankton cells from below and that light penetration through leads is likely to be the main environmental driver behind initiation of the UIB. Other studies have highlighted advective origins of UIBs in the region north of Svalbard (Johnsen et al., 2018). The ongoing “Atlantification” of the region is weakening the cold halocline and could favor the shoaling of nutrient-rich intermediate Atlantic waters (Polyakov et al., 2017).

Outflow Shelves

The Arctic outflow shelves are highly heterogeneous (Michel et al., 2015). Arctic sea ice advected over the East Greenland shelf extends offshore from the shelf break. Mayot et al. (2018) argued that UIBs in this offshore region are the result of local processes and may contribute up to 50% of annual primary production. These UIBs that occur in the Canadian Archipelago are typically driven by mixing (nutrient availability) processes and increased light availability during the spring ice melt (Figure 6C). The most recent studies collecting time series under landfast sea ice in the Canadian Archipelago (Resolute Bay: Mundy et al., 2014; Baffin Bay: Oziel et al., 2019) also concluded that the biomass was locally produced on these shelves. These sea ice camp studies helped resolve early temporal evolution of UIBs and revealed different key processes. Both the deepening of the euphotic zone due to increased light transmission and mixing/stratification processes acted together to trigger and drive UIB dynamics. Snow accumulation on landfast sea ice plays a critical role for UIB development by controlling most of the light transmitted to the under-ice water column (Mundy et al., 2014). In fact, light attenuation is strongly dominated by snow compared to sea ice. Extensive melt pond formation at the end of the snow melt period concomitant with the early stabilization of the upper water column due to freshwater input led to UIB initiation. As phytoplankton progressively consume nutrients in the surface layers, mixing is again of major importance to tap into deeper nutrient pools to maintain phytoplankton growth. In the Canadian Archipelago or Baffin Bay, tidal energy was the main source of vertical mixing (Mundy et al., 2014) that was enhanced by the presence of complex bathymetric features such as sills and shoals (Michel et al., 2006) or “Fjord-like” systems (Oziel et al., 2019). The tidal-induced mixing controlled the magnitude and depth of the SCM (Mundy et al., 2014; Oziel et al., 2019; Randelhoff et al., 2019).

The Central Arctic Ocean

Under-ice blooms in the central Arctic have been scarcely sampled but the recent shift from a MYI to a FYI-dominated sea-ice regime increases the likelihood of UIBs to occur there (Horvat et al., 2017; Kinney et al., 2020). The first in situ evidence of UIBs in the central Arctic under FYI was recently documented (Laney et al., 2014; Boles et al., 2020). Although significant relative to background Chl a levels, these UIBs were characterized by low biomass (i.e., ∼0.5–1.4 mg Chl a m^–3), which was similar in magnitude to the UIBs documented under MYI in the central Arctic by Apollonio (1959) and English (1961) (Table 1 and Figure 1). In these regions, surface layers are clearly both light and nutrient limited (Figure 6D). It is suggested that modal eddy-induced mixing could help sustain phytoplankton growth by providing nutrients from deeper Atlantic waters (Laney et al., 2014; Boles et al., 2020; Lewis et al., 2020).

Diversity of Under-Ice Blooms: Phenology, Strategy, Assemblages

Origin and Initiation of UIBs

The initiation of an UIB requires a viable seed population of algal cells present in the euphotic zone of the water column under the ice. There are three potential seeding sources for UIBs: (a) algal cells in the water column, (b) vegetative cells or resting stages at the sediment surface, and (c) algal cells or resting stages entrapped in sea ice that are released during melt onset at the underside of the ice (Johnsen et al., 2020). Very little is known about the relative importance of these three different seeding strategies, but it likely varies strongly depending on mixing depth, bottom topography, and sea-ice conditions. In relatively shallow coastal areas, re-suspension of resting stages from sediment surfaces is considered to be an important source seeding the diatom component of the spring bloom (Hegseth et al., 2019). In deeper oceanic regions, however, pelagic and sea-ice melt seeding by vegetative cells surviving the winter in the upper part of the water column are probably the most important seeding sources. Other important taxonomic groups of UIBs such as Phaeocystis are not known to form resting stages, but they have been found in single cell state throughout the winter in surface waters (Vader et al., 2015). While taxonomic composition and maximum biomass of an UIB seems to be strongly correlated with the type and amount of nutrients available (e.g., the winter nitrate:silicate ratio; Ardyna et al., 2020), the environmental cue for bloom initialization is an increase in light intensity, often caused by snow melt onset (Oziel et al., 2019; Ardyna et al., 2020) and sloughing of the ice algal community (Mundy et al., 2014).

Winters in high latitudinal areas are characterized by the Polar night when the sun does not rise above the horizon. This leads to extended periods where ambient irradiances are not sufficient for in situ primary production in ice-free surface waters (Kvernvik et al., 2018), and even less so underneath sea-ice cover (see also the previous section “Physiological Phytoplankton Assemblage Responses to Varying Light Regimes”). Phytoplankton have adapted through various strategies to cope with these conditions, ranging from mixotrophy/heterotrophy, resting stage formation, and utilization of internal lipid stores to survival of vegetative cells with lowered metabolic activity (Johnsen et al., 2020). Phytoplankton communities during wintertime are characterized by very low cell concentrations and a predominance of small, flagellated cells, as well as heterotrophic dinoflagellates (Lovejoy et al., 2007; Błachowiak-Samołyk et al., 2015; Brown et al., 2015; Vader et al., 2015). Among the small flagellated cells, two species that periodically dominate phytoplankton assemblages in Arctic waters were found throughout the Polar night: Micromonas polaris and Phaeocystis pouchetii (Vader et al., 2015). Natural microalgal assemblages, and in particular diatoms, are able to survive extended periods of darkness from months to years (Zhang et al., 1998; McMinn and Martin, 2013), while retaining their ability to resume physiological activity quickly once light returns (Kvernvik et al., 2018; Lacour et al., 2019; Morin et al., 2020). Diatoms also seem to retain their photophysiological characteristics during extended periods of darkness relatively unchanged as compared to flagellates, which possibly enables them to utilize the returning light in early spring very efficiently (van de Poll et al., 2020). Furthermore, mixotrophy (i.e., via osmotrophic or/and phagotrophic processes) also appears to be a widespread strategy among dinoflagellates and other photosynthetic flagellate taxa, keeping them active throughout the polar night (McMinn and Martin, 2013). However, important photosynthetic flagellates (e.g., green picoeukaryotes), such as M. polaris, are likely to rely on other strategies to survive through polar winter that have not yet been identified (Vader et al., 2015; Jimenez et al., 2020). This highlights the need for further study in the field.

Variability in UIB Biomass and Community Composition

Along the continental margins of the AO, UIBs are generally dominated by pelagic centric diatoms of the genera Chaetoceros and Thalassiosira and/or the colonial stage of the haptophyte alga Phaeocystis, with UIB magnitude decreasing and the role of Phaeocystis increasing toward the Atlantic sector (Ardyna et al., 2020). This overall pattern can be primarily attributed to the larger nutrient inventory and more upwelling-favorable conditions in the Pacific sector and the low silicate relative to nitrate concentrations in the Atlantic sector, respectively (Ardyna et al., 2020). A study from Darnley Bay in the Canadian Beaufort Sea showed that upwelling favorable conditions at the ice edge of landfast FYI in combination with the snow melt onset and low ice algal biomass throughout the study period provided both ample nutrients and light, including surface stratification, to fuel a large UIB (Mundy et al., 2009) dominated by the pennate diatom Fragilariopsis oceanica (Mundy et al., 2011). Furthermore, advection of high phytoplankton biomass produced in adjacent open water likely increased primary production capacity under the sea-ice cover (Mundy et al., 2009). Moderate UIBs (max. Chl a concentration of 4.3 mg m^–3), dominated initially by Micromonas sp. and diatoms and then by solitary (non-colonial) Phaeocystis, were observed in the Canadian Basin during the SHEBA ice camp in 1997/1998 (Sherr et al., 2003). A gradient in UIB biomass can be detected within the central AO, with the Amerasian Basins, particular the Beaufort Gyre, showing lower Chl a biomass than the Eurasian Basin (Laney et al., 2014) presumably due to the stronger haline stratification in the former. While light limitation in the central AO is progressively diminished by the shift from a MYI toward a FYI regime (Nicolaus et al., 2012; Horvat et al., 2017), the strong stratification limits nutrient input from below the halocline and will set an upper limit to UIB biomass accumulation. However, phytoplankton species are able to adapt their nutrient ratios, in addition to their photosynthetic parameters as discussed in the section “Physiological Phytoplankton Assemblage Responses to Varying Light Regimes,” in response to variable in situ nutrient concentrations, as shown for Arctic phytoplankton in the Chukchi Sea (Mills et al., 2015).

A synthesis of observations (Figure 8) contrasts algal composition and succession associated with the distinct regional environmental conditions described in the section “Contrasted Regional Environmental Settings Favoring UIBs.” Two expeditions were representative of the inflowing shelves describing the upwelling system in the Pacific sector (ICESCAPE cruise 2011 in the Chukchi Sea; Figures 8B,D) and the advective system in the Atlantic sector (N-ICE2015, north of Svalbard; Figure 8A). The other two expeditions were representative of the outflow shelves (i.e., the Canadian Arctic Archipelago, Resolute Passage 2010 and 2011; Figure 8C) and the central AO (North Pole expedition 2015; Figure 8E). All studies were conducted during the last decade, are thus representative of the new FYI regime, and cover the spring and summer season. One caveat common to these studies is that they were not following a Lagrangian design, i.e., following processes in the same water mass over time, but phytoplankton compositional patterns are still representative of the pre-bloom (except ICESCAPE) and bloom conditions. The N-ICE and North Pole expeditions in 2015 are representative of ice camps on drifting sea ice during the early spring to summer season while the Resolute Passage studies in 2010 and 2011 are representative of ice camps on landfast ice covering the late spring to summer season. The ICESCAPE cruise in 2011 is based on oceanographic transects from open to ice-covered waters in the Chukchi Sea during the month of July. The ice camp studies provide information on phytoplankton community composition prior to the UIB peak while information from ICESCAPE is limited to the peak of the UIB.

FIGURE 8

All UIBs were dominated by diatoms with the exception of the N-ICE UIB which was dominated by P. pouchetii (Assmy et al., 2017; Figure 9). There is a gradual decrease in maximum phytoplankton bloom abundance from the shallower and more nutrient-rich Chukchi Sea and Resolute Passage toward the Atlantic sector and the central AO (Figure 9). Particularly, the central AO shows nearly two orders of magnitude lower peak abundances (Figure 9) as was also the case for AO production estimates and Chl a concentrations (Table 1). One common feature of all studies is that pennate diatoms and dinoflagellates dominated in the early phase of the UIB development. In particular Fragilariopsis and Pseudo-nitzschia species, but also other pennate diatoms commonly found in sea ice were prominent during the pre-bloom phase. Interestingly, pennate diatoms (Fragilariopsis) were also most abundant at the northernmost stations, deepest into the ice pack during the ICESCAPE cruise (Laney and Sosik, 2014), presumably representative of an earlier UIB stage. The switch in dominance toward pelagic diatoms, in particular species of the centric diatom genera Chaetoceros and Thalassiosira, and in the case of N-ICE, P. pouchetii, coincided with the snow melt onset and a large lead fraction, respectively, and water column stratification. The notable exception is the Resolute Passage 2011 UIB which remained dominated by pennate diatoms (Fossula arctica, Fragilariopsis cylindrus, F. oceanica, and Nitzschia frigida) throughout (see “Box 2: Other Under-Ice Bloom Scenarios”). Chaetoceros, Thalassiosira, and Phaeocystis usually dominate the spring bloom along the Arctic continental margin (Degerlund and Eilertsen, 2010). In particular, spore-forming species of the former two diatom genera [e.g., Chaetoceros gelidus (formery Chaetoceros socialis), Thalassiosira hyalina and Thalassiosira antarctica var. borealis] are important bloom formers that exhibit a boom-and-bust life cycle and can increase biomass from background to bloom levels within 2–3 weeks. The comparably low Chaetoceros and Thalassiosira abundances in the deep central AO during the North Pole expedition 2015 suggest that, in addition to the low nutrient levels, these taxa might also be limited by dispersal of resting spores from the shallow shelves. Interestingly, an “UIB” dominated by Chaetoceros and Thalassiosira species was also observed during the Russian drift station North Pole 22 from May to October 1975 (Belyaeva, 1980) following formation of melt ponds on top of the MYI, similar to that observed in the late 1950s (Figure 1, Apollonio, 1959; English, 1961). However, maximum centric diatom abundances in 1975 were two orders of magnitude lower and about one month later (late August) than during the North Pole expedition 2015. The general trend toward stronger dominance of cryopelagic and pelagic diatom species in the more recent years is also supported by a study covering the MYI to FYI transition in the central AO over the last 40 years (Hop et al., 2020).

FIGURE 9

The general patterns described above are consistent with observations of UIBs in Baffin Bay in 2015 and 2016 during the Green Edge project (Oziel et al., 2019) with dominance of pennate diatoms and dinoflagellates during the early stages of UIBs and dominance of pelagic centric diatoms during the peak of the UIB. Notable exceptions are cryopelagic species belonging to the pennate diatom genera Fragilariopsis and Pseudo-nitzschia, which thrive both in sea ice and the water column (Hop et al., 2020), but are nevertheless usually outnumbered by centric diatoms of the genera Chaetoceros and Thalassiosira during the peak UIB phase.

Fate of UIBs

Intense grazing pressure is able to decimate phytoplankton biomass during the bloom peak or post-bloom phases (Sakshaug, 2004). Such large grazing pressure observed in summer requires a copepod community dominated by stage-V copepodites or adults which are relatively low in number during the early phase of an UIB (Sakshaug, 2004; Søreide et al., 2010; Daase et al., 2013). However, the UIB development is generally preceded by an ice algal bloom on which some zooplankton species are able to feed (Tourangeau and Runge, 1991; Wassmann and Slagstad, 1993; Hirche and Kosobokova, 2003; Wassmann et al., 2006; Søreide et al., 2008). Fortier et al. (2002) demonstrated that zooplankton can also feed well on released ice algae. Still, the time period of the developing UIB is often associated with a high flux of particulate organic carbon, mostly mediated by vertical sinking of ungrazed phytoplankton and ice algal cells (Fortier et al., 2002; Arrigo et al., 2014; Lalande et al., 2014, 2019). Similarly, Tamelander et al. (2008) suggested that ice algae can be an early food source for zooplankton and that the subsequent intense phytoplankton production exceeds the zooplankton grazing capacity, inducing a tight pelagic-benthic coupling. Overall, this suggests that in the early phase of an UIB, zooplankton are swamped by the abrupt increase in concentration and vertical flux of phytoplankton biomass. Hence, UIBs may represent an important and valuable food source for zooplankton grazers, including early recruitment stages, but they are likely not being controlled by grazing. In addition, sinking of UIB biomass could be an important food source for benthic ecosystems, especially on the shallow continental shelves. Export of a Phaeocystis-dominated UIB to the seafloor of the continental shelf north of Svalbard was significantly enhanced by ballasting of Phaeocystis aggregates by gypsum minerals released from melting sea ice (Wollenburg et al., 2018). Recent observations of mass sedimentation of the mat-forming sea-ice diatom Melosira arctica to the deep-sea floor of the central AO during the record summer sea ice minimum year 2012 suggest that cryopelagic-benthic coupling might be enhanced under the new Arctic sea ice regime (Boetius et al., 2013).

Perspectives

Sea-ice loss is the most prominent manifestation of climate-driven changes in the AO. The combined effect of advanced summer sea-ice melt, MYI disappearance (in terms of extent, thickness and volume; Kwok, 2018), and increase in storm frequency and intensity (Graham et al., 2017; Rinke et al., 2017) will strengthen atmospheric forcing on surface Arctic waters. It will promote wind-induced shelf-break upwelling and mixing events (Figure 6A; Pickart et al., 2013) but will also accelerate the demise of sea ice itself (Graham et al., 2019). Thinning sea ice, reduced snow cover, increased presence of melt ponds (generally associated with FYI), and/or increased lead formation will also increase under-ice light availability which could support larger UIBs under FYI (Figures 6C,D; see also Horvat et al., 2017). Such an increase in bloom magnitude could, however, be mitigated by the still uncertain increase in snow precipitation over the Arctic (Bintanja, 2018; Webster et al., 2018) and by nutrient limitation in the central AO (Codispoti et al., 2013; Fernández-Méndez et al., 2015). In contrast, there is also potential for increased rain precipitation earlier in the season (Bintanja and Andry, 2017), that can trigger mass release of the spring ice algal community and lead to a relatively short-lived and fast-sinking pennate diatom UIBs (see “Box 2: Other Under-Ice Bloom Scenarios”). Common among all scenarios is the likely increased pelagic-benthic coupling as a result of an earlier bloom with minimal top-down influence.

Sea-ice loss has also direct influences on the hydrodynamical conditions of the AO (Figure 7). Recent studies have shown an overall intensification of AO circulation. According to altimetric-derived satellite observations, surface geostrophic currents have doubled in both the Arctic basin (2003–2014; Armitage et al., 2017) and in the European sub-Arctic area (1993–2016; Oziel et al., 2020). The increased Atlantic inflow is suspected to be mainly driven by reduced sea-ice export through the Greenland Sea, resulting in lower sea surface height and intensified cyclonic gyre activity in the Nordic Seas (Wang et al., 2020). The Atlantic inflow is also largely affected by upstream alteration in the North Atlantic such as the increased influence of the sub-tropical waters due to the weakening of the sub-polar gyre (Hátún et al., 2017), which is responsible for the reduced nutrient concentrations, especially silicates, in the Nordic Seas (Rey, 2012). The overall intensification of the surface circulation will increase the potential for advection of new nutrients and organisms (Vernet et al., 2019), especially along the topographically constrained boundary currents (see Figure 6B). In general, the AO will be more dynamic, and because it is also baroclinically unstable, more meso-scale features will be produced (e.g., eddies, meanders, fronts). Consistent with this, the expansion and shift of the Beaufort Gyre (Regan et al., 2019) due to increased freshwater accumulation (+40% since 1970, Proshutinsky et al., 2019) is accompanied by an increase in eddy activity (Zhao et al., 2014, 2016; Armitage et al., 2020) and interruptions of the transpolar drift due to accelerating sea-ice melt (Krumpen et al., 2019). Over 2001–2014, annual Bering Strait volume transport from the Pacific to the AO almost doubled as well (0.7 × 10⁶ to 1.2 × 10⁶ m³ s^–1; Woodgate, 2018).

Therefore, the rapid transformation of local water masses due to the increased addition of freshwater and Atlantic- and Pacific-derived waters will alter the large-scale AO stratification. Arctic stratification will determine to a large extent nutrient availability in the surface euphotic layer (Tremblay and Gagnon, 2009, Ardyna et al., 2011) and constrain the magnitude of UIBs (Ardyna et al., 2020). Stratification is expected to increase in the Beaufort Gyre (Toole et al., 2010; Figure 6A) but decrease in other regions (e.g., in the European sector; Polyakov et al., 2017; Lind et al., 2018; Figure 6B) for different reasons (i.e., increased advection, mesoscale activity, atmospheric forcing, and related processes such as upwelling). The fate of freshwater will ultimately depend on the atmospheric and ocean circulation, which has been mainly in an anticyclonic regime during the last two decades, allowing freshwater accumulation (Haine et al., 2015). However, if the atmospheric circulation over the AO were to shift to a cyclonic regime, freshwater export may increase and ultimately alter the UIB dynamics.

Box 1: New Technologies: More Insights on Under-Ice Biogeochemical Cycles and Blooms

Our understanding of UIBs in a changing Arctic environment is based on few year-round and multiannual observations at specific locations. Additional long-term monitoring programs are clearly required, as well as large scale and/or high spatial resolution data to study spatial variability and distribution of Arctic UIBs. In view of these requirements, it is generally recognized that autonomous observing systems are well suited to provide observations at spatio-temporal resolutions previously hard to assess in the AO (Lee et al., 2017; Smith et al., 2019; Figure 10), especially during the winter-spring and summer-fall transitions when sea ice is present.

FIGURE 10

The Argo Program, which maintains a global array of autonomous and freely drifting profiling floats, is extending its array into Arctic regions (Jayne et al., 2017; Roemmich et al., 2019). All Argo floats carry conductivity-temperature-depth (CTD) sensors to measure accurate vertical temperature and salinity profiles mostly between 1000 and 2000 m to the surface, every 5–10 days and for several years (Argo Steering Team, 1998). Several of them, called biogeochemical (BGC)-Argo floats, are equipped with additional sensors measuring other essential ocean variables (EOVs): Chl a concentration, suspended particles, oxygen concentration, nitrate concentration, pH, and/or downwelling irradiance (Biogeochemical-Argo Planning Group, 2016). These BGC-Argo core variables are quantified with operational and robust sensors, as well as with new and under development technologies (e.g., a miniaturized version of the Underwater Vision Profiler, Lombard et al., 2019; an underwater sea-ice detection sensor based on laser polarimetry, Lagunas et al., 2018). Recently, it has become possible to deploy BGC-Argo floats into seasonally ice-covered Arctic areas to study UIBs (Mayot et al., 2018; Randelhoff et al., 2020). While operating beneath the sea-ice cover, profiling floats collect vertical profiles of key biogeochemical variables, and transmit data after surfacing in open water. The presence of sea ice makes it difficult to geolocate ARGO float platforms, so under-ice trajectories are estimated using interpolation methods (Wallace et al., 2020). In order to prevent risk of colliding with sea ice, floats stop their ascent at 10 m and cannot provide near-surface information.

Other autonomous observing systems exist to study UIBs in seasonal ice zones, one of them being the Warming and Irradiance Measurements (WARM) buoy system (Hill et al., 2018; Figure 10). At deployment time in early spring, the float is placed on the surface of the ice and the cable lowered through a hole that is re-filled with ice and snow. After the sea ice melts in summer, the observing system is floating in open water until the next ice formation cycle begins in late fall. Similarly, UIBs can be studied with moorings deployed, for example, in fjords and equipped with analogous physical and bio-optical sensors (Leu et al., 2011). However, recorded data are mostly available only after the mooring is recovered.

In areas with multiyear ice, data transmission by Autonomous Underwater Vehicles (AUVs, e.g., gliders) is nearly impossible due to the lack of open water for surfacing. Ice-borne observing systems are preferentially deployed in such environments. For example, Ice-Tethered Profilers (ITPs) equipped with similar sensors as BGC-Argo floats can be used to study processes associated with UIBs (Krishfield et al., 2006; Berge et al., 2016; Laney et al., 2017; Boles et al., 2020). These platforms can provide multiannual datasets with a high-temporal resolution, as demonstrated by data collected in the Arctic Transpolar Drift and the Beaufort Sea (Laney et al., 2014). Such long-term monitoring is possible thanks to engineering efforts to improve buoy survivability in thin ice, during ridging events and seasonal freeze-up.

Other autonomous observing systems can be deployed during ice camps or ship surveys, in order to provide high temporal and/or spatial resolution datasets of UIB-related processes. AUV platforms equipped with physical and bio-optical sensors were deployed in marginal ice zones in Baffin Bay (Green Edge project with glider platforms) and north of Svalbard (Johnsen et al., 2018). Surveys of the under-ice environment have been increasingly undertaken with remotely operated vehicles (ROVs). ROVs enable remote sensing of difficult to access locations across a range of temporal and spatial resolutions and minimize the disturbance of the ice environment in contrast to traditional ice coring techniques. Observational capabilities of ROVs are manifold due to a wide variety of attached sensors performing physical, chemical, and biological measurements (Katlein et al., 2017), and deployment distances from several hundred meters to extreme tether lengths of 20 km beneath the sea-ice cover (Nereid-UI ROV, Bowen et al., 2014; McFarland et al., 2015). For the investigation of parameters driving UIBs in Arctic waters, ROVs equipped with spectral radiometers have been frequently used to map under-ice irradiance and transmittance beneath landfast sea ice and moving pack ice in the AO (Nicolaus et al., 2012; Nicolaus and Katlein, 2013; Katlein et al., 2014, 2015, 2019; Lund-Hansen et al., 2018; Matthes et al., 2020).

As an example of the efficiency of autonomous platforms in providing broad spatial coverage, recently deployed autonomous instruments all around the Arctic show the anticipated latitudinal gradient in annual Chl a accumulation (Figure 11). Because annual maximum values of measured Chl a concentrations ranged from 0.2–0.5 mg m^–3 for ITP platforms to 7–20 mg m^–3 for floats and WARM buoys, these annual time series were normalized to their local annual maximum Chl a concentration value in order to focus on the phenology of UIBs. According to these time series, accumulation of phytoplankton biomass beneath mobile sea ice first occurred at the southernmost locations (e.g., in April for the Greenland Sea, Mayot et al., 2018; end of May for the Chukchi Sea, Hill et al., 2018) and 1–2 months later at northern Arctic locations (>85°N, Beaufort Sea, Laney et al., 2014; Amundsen-Nansen Basins, Boles et al., 2020).

FIGURE 11

Moreover, such annual cycle observations by autonomous systems revealed that significant phytoplankton biomass can accumulate in late spring after the melt onset, showing values as high as 15–40% of the annual maximum value observed in summer (Figure 11). These early increases in phytoplankton biomass frequently show short-term fluctuations. Upcoming concurrent measurements of Chl a concentration, water column mixing, PAR, and nitrate concentrations over a full annual cycle from more frequently deployed autonomous sampling platforms are needed to link and quantify the contribution of each individual bottom-up process to the observed short-term fluctuation in phytoplankton biomass. As pointed out by Laney et al. (2014), the impact of ice-algal Chl a on the Chl a fluorescence signal measured in the water column needs to be evaluated. Upward-looking cameras mounted on autonomous platforms can provide qualitative pictures of the ice–water interface and detect, for example, sinking aggregates of ice algae (e.g., Katlein et al., 2015; Hill et al., 2018; Johnsen et al., 2018). Finally, the drift of autonomous sampling platforms over large distances creates difficulties in the observation of UIBs in mobile pack ice over longer time periods. Some observed short-term fluctuations may be the result of the spatial variability in measurements from the drifting observing system used. An improved ocean observational effort in the pan-AO with an increased number of autonomous observing systems might overcome this issue (Smith et al., 2019).

Box 2: Other Under-Ice Bloom Scenarios

Here we briefly outline UIB scenarios that do not follow the “classical” UIB development as defined in the introduction.

UIBs During the Pre-melt Season

Although somewhat more moderate in terms of bloom magnitude, UIBs have been reported during the pre-melt season below sea ice with thin to moderate snow cover (<15 cm) in the Chukchi Sea (Lowry et al., 2018) or sea ice with thick snow cover (>40 cm) but an extensive fraction of open leads or leads covered by thin ice with thin snow cover in the Atlantic sector north of Svalbard (Assmy et al., 2017). However, in both cases, reduced vertical mixing and initiation of surface stratification, respectively, was a prerequisite for the UIB to form while extensive lead fraction under cold spring atmospheric forcing inhibited UIB formation due to convective mixing in refreezing leads (Lowry et al., 2018). Thus, water column stability, either induced by a stable water column below ∼100% sea-ice cover (no leads) (Lowry et al., 2018) or ceased convective mixing after leads have fully refrozen, in combination with Atlantic warm water influence on under-ice mixing processes (Assmy et al., 2017) are necessary conditions for UIBs to develop during the pre-melt season. In addition, the low but variable light conditions under the heavily snow-covered sea ice, crisscrossed with leads north of Svalbard, favored P. pouchetii over diatoms, facilitated by the high photosynthetic plasticity of the former species (Assmy et al., 2017).

UIBs Triggered by Extreme Meteorological Events

Depending on the mode of ice algal bloom termination, UIBs can be dominated by ice algae that continue growing in the water column and hence differ in bloom composition from the “classical” UIBs. A study from Resolute Passage in the Canadian Arctic Archipelago conducted in 2011 showed that rainfall triggered a rapid sloughing event of ice algae, dominated by pennate diatoms, followed by a pennate diatom-dominated bloom of the same species in the under-ice water column (Galindo et al., 2014). These observations were in contrast to the slower 3-week melt progression that led to an UIB dominated by centric diatoms of the genera Thalassiosira and Chaetoceros in the same region during the previous year (Mundy et al., 2014). In 2014 during another rapid melt event in Cambridge Bay, the planktonic diatom composition at the beginning of an UIB was very close to that of the ice algal community (C.J. Mundy, unpublished data), which was dominated by the pennate diatom N. frigida and the centric diatom Attheya sp. (Campbell et al., 2017). Thus, it is possible that the onset of the bloom was seeded in part by ice algae sloughing from the ice bottom. These observations led to the hypothesis that rapid surface melt rates caused by, e.g., a rain event, can influence the dominant taxa of an UIB via sea-ice seed populations (Galindo et al., 2014). Similar observations of UIBs dominated by pennate sea-ice diatoms of the genera Nitzschia, Fragilariopsis, and Navicula were made in Resolute Passage in 1994 and 1995 after a rain event and a heat wave, respectively, which led to rapid release of ice algae into the under-ice water column (Fortier et al., 2002). These results suggest that seeding from sea ice plays a minor role for UIB development, unless mass release of ice algae into the water column is triggered by extreme meteorological events (Fortier et al., 2002; Galindo et al., 2014). This is consistent with findings by Selz et al. (2018), based on in situ observations collected in the Chukchi and Beaufort Seas, suggesting that the sloughing of ice algae into the water column can only briefly increase the phytoplankton biomass. Ice algae have a high aggregation potential due to their sticky nature and high concentrations of gelatinous extracellular polymeric substances in sea ice (Krembs et al., 2002; Riedel et al., 2006; Meiners et al., 2008) leading to much lower residence time in the water column as compared to suspended phytoplankton (Riebesell et al., 1991). Such release events could partly explain observed short-term fluctuations in Chl a concentrations measured under ice in spring by autonomous platforms (see “Box 1: New technologies: More insights on under-ice biogeochemical cycles and blooms”).

Sea-Ice Meltwater UIBs

Other UIBs are restricted to the oligotrophic meltwater layer just below the sea ice (under-ice melt ponds sensuGradinger, 1996) and usually numerically dominated by phytoflagellates belonging to the prasinophytes, prymnesiophytes, and/or chrysophytes (Gradinger, 1996; Mundy et al., 2011). Similar UIBs restricted to the upper 2 m below the sea ice and dominated by phytoflagellates, termed halocline flora, were observed by Bursa (1963) and Apollonio (1985) but characterized by a different species composition (Chlorella sp., Oocystis sp., Scenedesmus bijugatus, and Ochromonas sp.) and generally lower biomass. Although hosting an active microbial community, these under-ice melt pond assemblages are often dominated by few or even a single species and are distinctly different from the pennate diatom community dominating the bottom of sea ice (Gradinger, 1996). However, seeding from sea ice seems to play an important role in the initial stages of these UIBs until a unique community characteristic to this environment develops (Mundy et al., 2011). The vertical extent of these blooms is restricted to a few meters compared to the UIBs described above, which usually occupy tens of meters in the upper surface mixed layer. Even thinner (<1 mm) yet dense accumulations of up to 117 mg Chl a m^–3 of the phototrophic ciliate Mesodinium rubrum at the ice–water interface, reminiscent of red tides of this species in open waters of temperate to tropical seas, have been observed below newly formed sea ice with little snow cover (Olsen et al., 2019). The highly motile and phototactic behavior of this ciliate in combination with convective mixing caused by brine rejection in growing sea ice enabled M. rubrum to bloom at the ice–water interface as long as the sea ice was growing.

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