salp/krill interactions in the southern ocean:spatial
TRANSCRIPT
Deep-Sea Research II 49 (2002) 1881–1907
Salp/krill interactions in the Southern Ocean: spatialsegregation and implications for the carbon flux
E.A. Pakhomova,*, P.W. Fronemanb, R. Perissinottoc
a Department of Zoology, University of Fort Hare, P/Bag X1314, Alice 5700, South Africab Southern Ocean Group, Department of Zoology and Entomology, Rhodes University, P.O. Box 94, Grahamstown 6140, South Africa
c School of Life and Environmental Sciences, University of Natal, Durban 4041, South Africa
Abstract
Available data on the spatial distribution and feeding ecophysiology of Antarctic krill, Euphausia superba, and the
tunicate, Salpa thompsoni, in the Southern Ocean are summarized in this study. Antarctic krill and salps generally
display pronounced spatial segregation at all spatial scales. This appears to be the result of a clear biotopical separation
of these key species in the Antarctic pelagic food web. Krill and salps are found in different water masses or water mass
modifications, which are separated by primary or secondary frontal features. On the small-scale (o100 km), Antarctic
krill and salps are usually restricted to the specific water parcels, or are well segregated vertically. Krill and salp grazing
rates estimated using the in situ gut fluorescence technique are among the highest recorded in the Antarctic pelagic food
web. Although krill and salps at times may remove the entire daily primary production, generally their grazing impact is
moderate (p50% of primary production). The regional ecological consequences of years of high salp densities may be
dramatic. If the warming trend, which is observed around the Antarctic Peninsula and in the Southern Ocean,
continues, salps may become a more prominent player in the trophic structure of the Antarctic marine ecosystem. This
likely would be coupled with a dramatic decrease in krill productivity, because of a parallel decrease in the spatial
extension of the krill biotope. The high Antarctic regions, particularly the Marginal Ice Zone, have, however, effective
physiological mechanisms that may provide protection against the salp invasion. r 2002 Elsevier Science Ltd. All
rights reserved.
Resume
Les observations disponibles sur la distribution spatiale et l’!ecophysiologie de l’alimentation du krill antractique,
Euphausia superba, et du tunicier Salpa Thompsoni dans l’Oc!ean Austral sont synth!etis!ees dans cette !etude. Le krill et les
salpes pr!esentent une distribution qui se traduit en g!en!eral par une forte s!egr!egation spatiale, "a toutes les !echelles
d’espaces. Ceci semble #etre le r!esultat d’une s!eparation claire des niches !ecologiques de ces deux esp"eces cl!es du r!eseau
trophique antarctique. Le krill et les salpes sont observ!es dans des masses d’eau diff!erentes qui sont s!epar!ees par des
fronti"eres primaires et secondaires. A petite !echelle (o100 km), soit le krill antarctique et les salpes sont habituellement
localis!ee dans des parcelles d’eaux sp!ecifiques, ou alors ils sont s!epar!es verticalement. Les vitesses de broutage du krill et
des salpes, estim!ees en utilisant la technique de fluorescence in situ, sont parmi les plus !elev!ees rencontr!ees au sein du
r!eseau trophique p!elagique antarctique. Bien que le krill et les salpes peuvent parfois consommer l’ensemble de la
production primaire journali"ere, l’impact de leur activit!e de broutage est g!en!eralement mod!er!e (p50% de la production
primaire). Les cons!equences !ecologiques r!egionales d’ann!ees caract!eris!ees par des fortes densit!es de salpes peuvent #etre
*Corresponding author.
E-mail address: [email protected] (E.A. Pakhomov).
0967-0645/02/$ - see front matter r 2002 Elsevier Science Ltd. All rights reserved.
PII: S 0 9 6 7 - 0 6 4 5 ( 0 2 ) 0 0 0 1 7 - 6
dramatiques. Si la tendance au r!echauffement, qui est observ!ee autour de la P!eninsule Antarctique et dans l’Oc!ean
Austral, continue, les salpes pourraient jouer un r #ole plus important dans la structuration des !ecosyst"emes marins
antarctiques. A cela serait probablement associ!e une diminution dramatique de la productivit!e du krill, en raison d’une
diminution de l’extension spatiale du biotope du krill. Cependant, aux hautes latitudes, et en particulier dans la zone
marginale des glaces, il existe des m!ecanismes physiologiques effectifs qui pourraient offrir une certaine protection vis "a
vis d’une invasion par les salpes.
1. Introduction
The Antarctic krill, Euphausia superba, and thetunicate, Salpa thompsoni, are among the mostimportant filter-feeding metazoans of the SouthernOcean, ranking only after copepods in terms oftotal dry pelagic biomass (Pages, 1997; Voronina,1998). These two species are also recognized asmicrophages of key importance, as they are able toefficiently re-package small particles into large fastsinking feces, thereby playing a major role inchanneling biogenic carbon from surface watersinto the long-living pools and to the ocean’sinterior and seafloor (Huntley et al., 1989; Fortieret al., 1994; Schnack-Schiel and Mujica, 1994;Pakhomov et al., 1997; Le F"evre et al., 1998;Perissinotto and Pakhomov, 1998a). As a conse-quence, the ecological role of these two key speciesin the Antarctic pelagic food web has recentlyreceived much attention (e.g., Nishikawa et al.,1995; Siegel and Loeb, 1995; Siegel and Harm,1996; Dubischar and Bathmann, 1997; Loeb et al.,1997; Kawaguchi et al., 1998; Perissinotto andPakhomov, 1998b; Ross et al., 1998). It has beensuggested that krill and salps may be in directcompetition with one another in certain areas ofthe Antarctic Peninsula (Loeb et al., 1997) and inthe Lazarev and Cooperation Seas (Perissinottoand Pakhomov, 1998a, b). It also was tentativelypostulated that if the increase in seawater tem-perature, already observed in the Antarctic Penin-sula region, continues (Zwally, 1991; Rott et al.,1996), salps may spread into the high Antarcticregions, with important implications for theregional carbon flux and the Antarctic food webstructure (Perissinotto and Pakhomov, 1998a, b).
In the Southern Ocean, S. thompsoni is generallyrestricted to the warmer water masses (Voronina,1984; Nast, 1986; Siegel et al., 1992; Pakhomov,
1993a; Park and Wormuth, 1993; Kawamura et al.,1994; Nishikawa et al., 1995). With the exceptionof only few areas, such as Antarctic Peninsularegion, spatial exclusion between Antarctic krilland salps has been widely documented (Pakhomovet al., 1994a; Hosie, 1994; Voronina, 1998). Studieson the community structure of zooplanktonconducted in the vicinity of the Greenwichmeridian have indicated that Antarctic krill andsalps may overlap in their distribution south of theAntarctic Polar Front (Fransz and Gonzalez,1997; Pakhomov et al., 2000). Feeding studiesconducted in this region provided evidence thatthese species may at times consume the entire dailyprimary production (Dubischar and Bathmann,1997; Perissinotto et al., 1997; Perissinotto andPakhomov, 1998a; Froneman et al., 2000). Unlikefor case of krill, for which there are numerous dataon its feeding ecology, there are still large gaps inour understanding of the biology and the ecologi-cal role of salps in the Southern Ocean (Le F"evreet al., 1998). The aims of this paper are tosummarize studies on the trophic ecophysiologyof Antarctic krill and of the tunicate S. thompsoni,with particular emphasis to the tunicates, and todiscuss the phenomenon of krill/salp spatialseparation.
2. Materials and methods
Data on ingestion rates of Antarctic krill, E.
superba, and of the tunicate, S. thompsoni,estimated using the gut fluorescence techniquewere obtained mainly during the three expeditionsto the southern part of the Atlantic sector of theSouthern Ocean: (a) the second cruise of the SouthAfrican Antarctic Marine Ecosystem Study(SAAMES II) conducted aboard the mv SA
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–19071882
Agulhas along the Greenwich Meridian (WOCESR2 line) in January 1993 (Perissinotto et al., 1997;Froneman et al., 2000; Pakhomov et al., 2000); (b)the SAAMES IV aboard the mv SA Agulhas in theLazarev Sea during December 1994–January 1995(Froneman et al., 1997; Perissinotto and Pakho-mov, 1998a, b); (c) the joint Scandinavian/SouthAfrican Antarctic Research Expedition aboard themv SA Agulhas along the 61E meridian between491S and 601300S (Pakhomov, 2002; Pakhomovand Froneman, 2002a, b).
In addition, numerous published and unpub-lished sources (mentioned throughout the text) onkrill and salps ingestion rates, abundances, bio-mass and distribution in the Southern Ocean wereused for this synthesis. To convert wet weight intocarbon weight, the following conversion factorswere used: (a) S. thompsoni dry weight wasassumed to be 4% of wet weight, and carbonweight was assumed to be 4.3% of dry weight(Ikeda and Mitchell, 1982; Ikeda and Bruce, 1986;Hagen, 1988; Huntley et al., 1989; Donnelly et al.,1994); (b) E. superba dry weight was assumed to be22% of wet weight, and carbon weight assumed tobe 45% of dry weight (Ikeda and Mitchell, 1982;Ikeda and Bruce, 1986; Torres et al., 1994). Toconvert chlorophyll values into carbon values astandard chlorophyll/carbon ratio of 50 wasapplied (Booth et al., 1993).
3. Euphausia superba and Salpa thompsoni:densities and distribution
3.1. Krill/salp densities: importance in the Antarctic
pelagic ecosystem
There is a great deal of uncertainty in estimatingtotal stocks of Antarctic krill and salps in theSouthern Ocean due to their extremely patchydistribution (e.g., Miller and Hampton, 1989;Voronina, 1998). The most recent revision ofAntarctic krill biomass estimates obtained usingscientific and commercial trawls was presented byVoronina (1998, Tables 2–4). After converting wetweight into carbon, the average biomass of E.
superba throughout the Southern Ocean rangesfrom 400 to 37800 mg C m�2 (mean 595071110 mg
C m�2) and from 1 to 1200 mg C m�2 (mean2207320 mg C m�2) in the regions of dense andlow krill concentrations, respectively (Voronina,1998).
Although Southern Ocean tunicates have notbeen targeted specifically, over the past twodecades a substantial amount of data on S.
thompsoni density has been accumulated in differ-ent sectors of the Southern Ocean (Table 1). Insummary, these data indicate extreme variability insalp densities across the Southern Ocean (Table 1).Nevertheless, throughout much of the area southof 401S, S. thompsoni densities remain moderate,on average varying between o0.1 and 30 mgC m�2, or between o0.1 and 30 ind m�2. However,S. thompsoni densities in the Antarctic Peninsularegion, particularly in the Bransfield Strait andaround Elephant Island, were found to beconsistently elevated (Table 1). Furthermore, thesecondary frontal systems that demarcate low andhigh latitude water masses around the AntarcticContinent, e.g., Weddell–Scotia Confluence,Warm Counter Weddell Current in the LazarevSea, the northern part of the Ross Sea, alsoshowed enhanced densities of S. thompsoni.Foxton (1966) first mentioned this phenomenon,e.g., an increased biomass of S. thompsoni at thenorthern limit of Antarctic krill distribution. In theregions of high salp densities, average concentra-tions generally ranged from 22 to 1115 mg C m�2
and from 20 to 800 ind m�2, with a maximumbiomass level of 2.5 g C m�2 observed in thenorthern Ross Sea (Voronina et al., 1993) andabundance of ca 6000 ind m�2 off the Adelie Coast(Chiba et al., 1998). The mean S. thompsoni
biomass, estimated using average values presentedin Table 1, is 72.17189 mg C m�2 (N ¼ 54).
For comparison, mean copepod biomass in theSouthern Ocean is estimated at E1161 mg C m�2.This value was obtained from Voronina (1998) byassuming that dry weight is equivalent to 15% ofwet weight and that carbon weight accounts for43% of dry weight (Ikeda and Mitchell, 1982;Ikeda and Bruce, 1986; Donnelly et al., 1994).
From the above comparative biomass estimatesof the three large Antarctic metazoan filter-feedergroups, it is obvious that the tunicates do not playa major role in terms of total carbon biomass.
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–1907 1883
Table 1
Biomass and abundance of the tunicate Salpa thompsoni in the Southern Ocean
Location Date Sampling
depth (m)
Biomass
(mgC m�2)
Abundance
(ind m�2)
Source
Mean Range Mean Range
Elephant Island Nov 1983 0–200 nd nd 31.7 0.8–123.4 Nast (1986)
Nov 1984 0–200 nd nd 1.1 0–12.8 Nast (1986)
Mar 1985 0–200 nd nd 25.0 0.1–177.8 Nast (1986)
Mar 1989 0–200 65.3 F nd F Pakhomov (1993b)
Jan–Feb 1988 0–160 nd nd 25.6 nd Park and Wormuth (1993)
Jan–Feb 1989 0–160 nd nd 92.8 nd Park and Wormuth (1993)
Jan–Feb 1990 0–160 nd nd 801.6 nd Park and Wormuth (1993)
Jan 1992 0–160? nd nd 15.1 0–197 AMLR (1994)
Jan 1993 0–160 nd nd 194.1 1.1–2573 AMLR (1994)
Feb–Mar 1993 0–160 nd nd 253.7 0.4–2666 AMLR (1994)
Jan 1994 0–160 nd nd 149.1 1.5–765 AMLR (1994)
Feb–Mar 1994 0–160 nd nd 79.2 0.8–380 AMLR (1994)
summers 1975–95 ? nd nd nd 1.2–3489* Loeb et al. (1997)
Jan 1994 ? 570.6 0–3277 nd nd Loeb et al. (1997)
Jan 1995 ? 7.8 0–75.3 nd nd Loeb et al. (1997)
Jan 1996 ? 20.2 0–134.2 nd nd Loeb et al. (1997)
Mar–Apr 1998 0–200? 1383 nd nd nd Minkina et al. (1999)
Antarctic Peninsula Nov–Dec 1983 0–600 409.2 272.4–
591.1
nd nd Torres et al. (1984)
Feb 1982 0–300 nd nd 12.3 0–228.6 Piatkowski (1985)
Mar 1984 0–200 183.5 44–671 nd nd Huntley et al. (1989)
Mar 1993 0–120 9.8 nd nd nd Ross et al. (1998)
Jan–Feb 1994 0–120 29.5 nd nd nd Ross et al. (1998)
Drake Passage and
Bransfield Strait
Dec 1983–Jan 1984 0–200 23.8 0.04–207.7nd nd Witek et al. (1985)
Bransfield Strait Mar 1989 0–200 221.1 F nd F Pakhomov (1993b)
South Shetland Isl Dec 1990–Jan 1991 0–100 22.3 0–151.4 17.8 0–132 Nishikawa et al. (1995)
Jan–Feb 1991 0–100 9.9 0–147.3 3.2 0–30 Nishikawa et al. (1995)
South Georgia Jan 1991 0–200 0.003 F nd F Piatkowski et al. (1994)
Jan 1991 0–1000 0.02 F nd F Piatkowski et al. (1994)
APF, Scotia Sea Jan 1991 0–200 49 F nd F Piatkowski et al. (1994)
Jan 1991 0–1000 71.2 F nd F Piatkowski et al. (1994)
WSC Jan 1994 0–200 nd 115–2930 nd nd Alcaraz et al. (1998)
Northern Weddell Nov–Dec 1983 0–200 4.5 nd 17.5 nd Lancraft et al. (1989)
Southern Scotia Seas Nov–Dec 1983 0–1000 49.5 nd 145.3 nd Lancraft et al. (1989)
Mar 1986 0–200 5.9 nd 4.3 nd Lancraft et al. (1989)
Mar 1986 0–1000 6.8 nd 5.6 nd Lancraft et al. (1989)
Aug 1988 0–200 0.6 nd 0.23 nd Lancraft et al. (1991)
Aug 1988 0–1000 6.8 nd 1.0 nd Lancraft et al. (1991)
Oct–Nov 1988 0–60 0.01 nd 6.1 nd Siegel et al. (1992)
Eastern Weddell Feb 1988 0–500 11.6 nd nd nd Makarov and Solyankin
(1990)
Gyre (EWG): ACC
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–19071884
Table 1 (continued)
Location Date Sampling
depth (m)
Biomass
(mgC m�2)
Abundance
(ind m�2)
Source
Mean Range Mean Range
EWG: ACC+WW Feb 1988 0–500 124.1 nd nd nd Makarov and Solyankin
(1990)
EWG: WCWC Feb 1988 0–500 711.8 nd nd nd Makarov and Solyankin
(1990)
Weddell Sea Feb–Apr 1989 0–200 0.07 0–0.32 nd nd Pakhomov (1993b)
Southern Weddell
Sea
Feb–Mar 1983 0–300 13.2 nd 12.3 nd Boysen-Ennen and
Piatkowski (1988),
Boysen-Ennen et al. (1991)
Lazarev Sea Jan–Feb 1990 0–200 6.6 0–45.7 22.1 0–189.2 Pakhomov et al. (1994a)
Dec 1994–Jan 1995 0–300 nd nd 150.1 0–1220 Perissinotto and
Pakhomov (1998b)
AS: APF Jan–Feb 1993 0–300 4.1 nd 7.3 nd Pakhomov et al. (1994a, b)
AS: STCFAPF Dec 1979–Jan 1980 surface 0.004 nd o0.01 nd Pakhomov and McQuaid
(1996)
AS: APFF60–651S Dec 1979–Jan 1980 surface 0.03 nd 0.2 nd
AS: 01, 46–691S Jan 1993 0–300 5.97 0–45.1 41.4 0–222.6 Pakhomov et al. (2000)
AS: 61E, 49–651S Dec 1997–Jan 1998 0–300 17.5 0–126.9 44.1 0–402 Pakhomov (2002)
Kerguelen Islands Feb–Mar 1988 0–150 1.1 0–22.0 2.4 0–39.7 Pakhomov (1995)
Ob and Lena banks Nov–Dec 1986 0–500 7.3 nd nd nd Pakhomov (1993c)
Prydz Bay Region
(PBR)
Feb–Mar 1985 0–52 6.2 nd 2.15 nd Pakhomov (1991)
Dec 1985–Jan 1986 0–59 0.1 nd 0.3 nd Pakhomov (1991)
Feb–Mar 1986 0–67 7.7 nd 2.6 nd Pakhomov (1991)
Feb–Mar 1987 0–124 0.4 nd 0.33 nd Pakhomov (1991)
Dec 1987–Mar 1988 0–150 7.9 nd 7.2 nd Pakhomov (1991)
Feb–Mar 1989 0–200 0.31 nd 3.2 nd Pakhomov (1991)
PBR: OC Jan 1985 0–200 nd nd 23–98 nd Hosie (1994)
PBR: OC Mar 1987 0–200 nd nd 5.4 nd Hosie (1994)
PBR: OC Jan–Feb 1993 0–200 nd nd 0.33 nd Hosie et al. (1997)
PBR: TC Jan 1985 0–200 nd nd 1.4 nd Hosie (1994)
PBR: TC Mar 1987 0–200 nd nd 0.4 nd Hosie (1994)
PBR: NC Jan–Feb 1993 0–200 nd nd 0.06 nd Hosie et al. (1997)
PBR: south of 651S Jan–Feb 1991 0–200 0 0 0 0 Hosie and Cochran (1994)
Enderby Land Apr 1988 0–200 30.3 nd 29.3 nd Pakhomov (1991)
Cosmonaut Sea Jan–Feb 1987 0–159 0.2 nd 0.9 nd Pakhomov (1991)
Feb 1988 0–100 0.5 nd 1.6 nd Pakhomov (1991)
Feb 1989 0–200 0.1 nd 1.7 nd Pakhomov (1991)
Mar–Apr 1989 0–200 o0.01 nd o0.1 nd Pakhomov (1991)
Pacific Sector (PS) Dec 1980 0–300 26.8 0–100.0 nd nd Maruyama et al. (1982)
Feb 1981 0–250 5.7 0–24.9 nd nd Maruyama et al. (1982)
PS: APF–AD Jan–Feb 1981 surface 0.21 nd 0.22 nd Pakhomov and McQuaid
(1996)
Wilkes Land Jan–Feb 1996 0–200 8.15 0.2–44.5 nd Max 5975 Chiba et al. (1998)
East Antarctica Jan–Feb 1996 0–200 28.2 0–904 19.7 0–714 Hosie et al. (2000)
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–1907 1885
Similar results could be obtained using estimatesof the total stock for these filter-feeders in theSouthern Ocean provided by Voronina (1998).Voronina (1998) showed that in terms of freshmass, salps are the main contributors to total stockin the Southern Ocean, followed by copepods andAntarctic krill (Fig. 1). However, in terms of dryand carbon mass, copepods were identified as themost important and salps the least important(Fig. 1). The main argument of Voronina is thatAntarctic krill is neither first in total metazoanbiomass nor in production, as in both cases it issecond to the herbivorous copepods (Voronina,1998). Unlike for Antarctic copepods and krill,there are no annual production estimates for S.
thompsoni available in the literature. However, it isknown, that salps exhibit the fastest individualgrowth rates among metazoans (Heron, 1972;Heron and Benham, 1984). Although salp abun-dance maxima are short-lived, the P/B coefficientof a one-year life cycle would likely exceed one(Fraser, 1962; Foxton, 1966) and reach 3 (N.M.Voronina, personal communication). As a conse-quence, salp contribution to total filter-feederproduction should be substantial, probably rank-ing second only to that of copepods. As salps playan increasingly important role in the Antarcticecosystem, studies on the production of S.
thompsoni are urgently required.
3.2. Krill/salp distribution
3.2.1. Large-scale distribution
Despite uncertainties in the small-scale distribu-tion of Antarctic krill, the large-scale distributionof this species is relatively well documented (Millerand Hampton, 1989; Knox, 1994; Voronina,
1998). One of the most important features of themacro-scale distribution of Antarctic krill is thetypical increase in density in two different zones ofthe Southern Ocean (Makarov and Spiridonov,1993). The southern circumpolar belt of high krilldensity is restricted to the Antarctic CoastalCurrent (East Wind Drift), north of the shelf edgeand above the upper part of the continental slope.The northern belt of high krill density is associatedwith the secondary frontal zones (Maslennikov,1980, 1995), where waters of high latitudes aremixed with waters of the Antarctic Circumpolar
Table 1 (continued)
Location Date Sampling
depth (m)
Biomass
(mgC m�2)
Abundance
(ind m�2)
Source
Mean Range Mean Range
Ross Sea, 671S Feb–Mar 1992 0–200 1115 522–2547 nd nd Voronina et al. (1993)
Bellingshausen Sea Feb–Mar 1994 0–200 0.2 nd nd 0–10.2 Siegel and Harm (1996)
ACC, Antarctic Circumpolar Current waters; WW, Weddell Sea waters; WCWC, Warm Counter Weddell Current; APF, Antarctic
Polar Front; STC, Subtropical Convergence; AD, Antarctic Divergence; OC, Oceanic Community; TC, Transitional Community; NC,
Neritic Community; WSC, Weddell–Scotia Confluence; AS, Atlantic sector; nd, no data; *Fabundance expressed as ind 1000 m�3.
0%
20%
40%
60%
80%
100%
Wet
mas
s
Dry
mas
s
Car
bon
mas
s
Pro
duct
ion
Fae
cal
pelle
tpr
oduc
tion
Con
trib
utio
n
copepods Antarctic krill salps
Fig. 1. Comparative role of major metazoan filter-feeders in the
Southern Ocean. Wet and dry masses are taken from Voronina
(1998). Carbon mass calculated from dry mass assuming that
carbon accounts for 4.3%, 43% and 45% dry weight of salps,
copepods and krill, respectively (see Sections 2 and 3.1). Annual
production of copepods and krill is taken from Voronina
(1998), while production of salps was calculated assuming a P/B
coefficient of 1 (see Section 3.1 for explanation). Faecal pellet
production was calculated as follows: for copepods assuming
average daily ration of 10% of body carbon and assimilation
efficiency of 70%; for Antarctic krill assuming average egestion
rate of 8.143mg C mgDW�1 d�1 (Table 3); for S. thompsoni
assuming egestion rate of 10.2% of carbon mass per day
(Huntley et al., 1989).
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–19071886
Current. Apart from the Weddell Sea, where thenorthern belt is strongest, this area is not ascontinuous as the southern one, but it can bedistinctly identified around the Antarctic Con-tinent in the Bellingshausen, Lazarev, Riiser-Larsen, Cosmonaut, Cooperation and DumontD’Urvile Seas (e.g., Makarov and Sysoeva, 1983;Williams et al., 1983, 1986; Iganake et al., 1984;Hampton, 1985; Miller, 1986, 1987; Shirakiharaet al., 1986; Bibik et al., 1988; Miquel, 1991;Pakhomov, 1993a, b).
Unlike its southern counterpart, the northernbelt of high krill density exhibits an asymmetricalpattern in distribution (Marr, 1962; Mackintosh,1973). For instance, in the Atlantic sector, watersof high krill biomass are associated with the northbranch of the Weddell Gyre (Weddell–ScotiaConfluence), which deflects southward east ofBouvet Island (Marr, 1962; Maslennikov, 1980).Accordingly krill, which are found in the Atlanticsector as far north as 511S, are not generallyrecorded north of 59–601S in eastern Antarctica(Marr, 1962; Miller and Hampton, 1989).
A detailed map showing the spatial distributionof S. thompsoni in the Southern Ocean was firstprovided by Foxton (1966) who used a compre-hensive collection of Discovery expeditions con-ducted between 1925 and 1951 (Fig. 2). On thebasis of Foxton’s (1966) data, the northern limit ofS. thompsoni distribution appears to coincide withthe mean position of the Subtropical Convergence,while the southern limit is generally shaped by theice-edge (Foxton, 1966). At that stage, a belt ofelevated densities of S. thompsoni was restricted tothe region between 45 and 601S (Fig. 2). It isevident that S. thompsoni was absent or found invery low numbers in the waters of high latitudes,particularly in waters of Weddell Sea origin(Foxton, 1966). These data were subsequentlysupported by the addition of a data set collectedbetween 1956 and 1958 by Russian expeditionsaboard the RV Ob’ (Fig. 2, see Voronina, 1998 fordetails).
After comparing the zooplankton densitiesrecorded during the BIOMASS expeditions withthose from the Discovery results, Kawamura(1986) stated ‘‘that behavior of salp populationshould be considered very important in total
Antarctic zooplankton biomass’’. Following anincrease in the occurrence of dense salp concentra-tions around the Antarctic Peninsula and SouthGeorgia, the author tentatively hypothesized thatthe increase in population size of salps over thevast range of the Southern Ocean over the pastseveral decades may have been in response to thechange in the Antarctic marine ecosystem (Kawa-mura, 1987). As the number of publicationsdocumenting mass salp occurrences in differentregions of the high Antarctic recently has in-creased dramatically (e.g., Huntley et al., 1989;Park and Wormuth, 1993; Voronina et al., 1993;Pakhomov et al., 1994a; Nishikawa et al., 1995;Loeb et al., 1997; Perissinotto and Pakhomov,1998a, b; Chiba et al., 1998, 1999), we have tried tore-construct a similar map of S. thompsoni
distribution using all data available (publishedand unpublished) from 1980 till 1998 (Fig. 3). Thestriking difference between the recent map andthat presented by Foxton in 1966 is that S.
thompsoni is now regularly found at high latitudes,including the southern parts of the Bellingshausen,Weddell and Lazarev seas, and the belt of its denseconcentrations extends further south to E651S(Fig. 3). In our opinion, this increase in distribu-tion may underline dramatic changes in theAntarctic marine environment.
Warming trend over the past 40 years has beendemonstrated for the Antarctic Peninsula region(Gloersen and Campbell, 1991; Zwally, 1991; Rottet al., 1996). This is linked to an increase in theaverage percentage of open water in the form ofleads and polynyas, to the disintegration of ice-shelves, and to a decrease in areal and seasonalextent of sea-ice cover (Doake and Vaughan, 1991;Gammie, 1995; Vaughan and Doake, 1996;Hewitt, 1997). Furthermore, the warming trendhas shown some correlation with an increase insalp occurrence and with a decrease in krill stock(Loeb et al., 1997; Naganobu et al., 1999). There isevidence for the warming in the Arctic region andoff the Antarctic Peninsula (Johannessen et al.,1995; Vaughan and Doake, 1996) as well as atsome sub-Antarctic islands (Smith and Steen-kamp, 1990; Smith, 1991). Most recently, warmingof the World Ocean, including the SouthernOcean, has been demonstrated (Levitus et al.
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–1907 1887
2000). Although the warming signals are notmonotonic, they were found to be consistent ineach ocean basin (de la Mare, 1997; Levitus et al.,2000). Therefore, since S. thompsoni is considereda warm-water species, data presented in Fig. 3 mayindicate that large-scale warming of high Antarcticregions is in progress. If the hypothesis is correct(still remains to be proven), the change in salpdistribution may have very important implicationsfor the high Antarctic ecosystem. The occurrenceof salps in high latitudes may change the regionalcarbon flux (Perissinotto and Pakhomov,
1998a, b). More importantly, an increase in salpabundance may be coupled with a dramatic fall inkrill stock and productivity due to a decrease inthe spatial extension of the krill biotope (Pakho-mov, 2002), which in turn will affect the Antarcticmarine food web and krill resource management(Loeb et al., 1997). In light of this, it is worthnoting that the most recent Antarctic krill stockestimates, ca 61� 106–155� 106 tonnes (Nicolet al., 2000a), are about half of those previouslyestimated, ca 100� 106–600� 106 tonnes (Rossand Quetin, 1986). This, however, may be linked
WEDDELL SEA
ROSSSEA
01800150 W
012
0W
090
W0
60W
030 W 00
0150 E
0120
E0
90E
060
E
030 E
AC
STC 040 S
12345
080 S
060 S
Fig. 2. Horizontal distribution of S. thompsoni in the Southern Ocean after Foxton (1966) with addition of data sets collected during
Russian expeditions onboard the RV Ob’ in March–May 1956, February–March 1957 and March–May 1958 (after Voronina, 1998). 1,
negative; 2, 1–100 (o1); 3, 101–1000 (1–10); 4, 1001–10000 (11–100); 5, >10000 (>100) individuals per 20 min tow (gWW m�2 for
Russian data).
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–19071888
to the development of better or more accurateassessment techniques/models.
3.2.2. Meso-scale distribution
Hempel (1985) described three major zooplank-ton associations south of the Antarctic PolarFront (APF). These are: (1) ice-free oceanic West
Wind Drift assemblage, where copepods, salps andsmall euphausiids dominate; (2) the seasonal pack-ice assemblage, where Antarctic krill is the mostimportant species; and (3) the permanent pack-iceassemblage. Meso-scale community structure stu-dies conducted in different sectors of the SouthernOcean provided many of the data to support
WEDDELL SEA
ROSSSEA
01800150 W
012
0W
090
W0
60W
030 W 00
0150 E
0120
E0
90E
060
E
030 E
060 S
AC
STC040 S
080 S
12345
Fig. 3. Horizontal distribution of S. thompsoni in the Southern Ocean using published and unpublished literature sources covering
period from 1980 till 1998. 1, negative; 2, 1–10 (o1); 3, 11–100 (1–10); 4, 101–1000 (11–100); 5, >1000 (>100) ind m�2 (or gWW m�2).
Sources used: unpublished data of the Southern Ocean Group, Rhodes University (South Africa) along the transect between the Prince
Edward Islands and Madagascar, Pakhomov, unpublished along 451, 501 and 801E transects; published: Boysen-Ennen and
Piatkowski (1988), Boysen-Ennen et al. (1991), Brinton (1984), Casareto and Nemoto (1986), Chiba et al. (1998), Huntley et al. (1989)
Makarov and Solyankin (1990), Maklygin and Pakhomov (1993), Maruyama et al. (1982), Nast (1986), Nishikawa et al. (1995),
Pakhomov (1989, 1991, 1993a, b, 1995, 2002), Pakhomov and Froneman (2000, 2002a), Pakhomov and McQuaid (1996) Pakhomov
et al. (1994a, b, 2000), Park and Wormuth (1993) Perissinotto and Pakhomov (1998a, b) Piatkowski (1985, 1987) Piatkowski et al.
(1994), Ross et al. (1998), Siegel and Harm (1996), Voronina (1998), and Voronina et al. (1993).
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–1907 1889
Hempel’s subdivision. These clearly showed thatAntarctic krill and S. thompsoni are dominantspecies in different zooplankton assemblages,which belong to specific water masses or modifica-tions (Brinton, 1984; Nast, 1986; Huntley et al.,1989; Lancraft et al., 1989; Makarov and Solyan-kin, 1990; Siegel and Piatkowski, 1990; Siegel et al.,1992; Pakhomov, 1993a, b; Pakhomov et al.,1994a, 2000; Hosie, 1994; Nishikawa et al., 1995;Chiba et al., 1998; Minkina et al., 1999). There isgrowing evidence in the literature to suggest thatthe ice-edge may represent a natural boundarybetween the distribution of S. thompsoni and thatof Antarctic krill (Foxton, 1966; Brinton, 1984;Torres et al., 1984; Ainley et al., 1988; Siegel et al.,1992). The importance of the frontal zone asso-ciated with the winter northern limit of theseasonal pack ice, Antarctic Ice Boundary Front(AIBF, after Klyausov, 1993), has recently beenrecognized (Grachev, 1991; Pakhomov andMcQuaid, 1996; Pakhomov and Froneman,2002a). From an oceanographic point of view,the AIBF coincides with the disappearance of thesubsurface cold-water layer that separates the highlatitude waters from the warmer water massesaffected by the ACC (Klyausov, 1993; Pakhomovet al., 2000). Ecologically, the AIBF represents thenorthern limit of Antarctic krill distribution andthe southern limit of the mass development ofsmall gastropods of the genus Limacina (Grachev,1991). The front also coincides with the sharpdecline in S. thompsoni populations to the south(Pakhomov, 1989, 1993a; Pakhomov andMcQuaid, 1996; Pakhomov et al., 2000).
High-resolution studies, conducted in the Atlan-tic sector of the Southern Ocean along the Green-wich and the 61E meridians, have shown that thespatial overlap in distribution of Antarctic krilland S. thompsoni is minimal and occurs onlywithin the AIBF region (Fig. 4). There are,however, records showing that S. thompsoni mayoccur as far south as 681S in the Lazarev Sea(Pakhomov et al., 1994a; Perissinotto and Pakho-mov, 1998a, b) and also may be found in thesouthern parts of Bellingshausen, Weddell, Cos-monaut and Cooperation seas and off the AdelieLand (Fig. 3; Boysen-Ennen et al., 1991; Pakho-mov, 1991; Siegel and Harm, 1996; Chiba et al.,
1998; Nicol et al., 2000b). It is evident that on suchoccasions S. thompsoni populations are restrictedto the warm water intrusions or layers (Fig. 5;Boysen-Ennen and Piatkowski, 1988; Makarovand Solyankin, 1990; Pakhomov, 1991, 1993a;Pakhomov et al., 1994a). This is confirmed by thesignificant positive correlation observed betweenintegrated average seawater temperature and S.
thompsoni densities in the Lazarev Sea (Pakhomovet al., 1994a; Pakhomov and Perissinotto, unpub-lished), in the Cosmonaut Sea (Pakhomov, 1991)and in the Prydz Bay region (Hosie et al., 1997).Casareto and Nemoto (1986) were the first tosuggest that at the higher latitudes S. thompsoni
exist close to its thermo-physiological limits. Thiswas recently confirmed by Chiba et al. (1999) usinga data set collected off Adelie Land. It was
0
0.06
0.05
0.04
0.03
0.02
0.01
48 50 52 54 56 58 60 62 64 66
Latitude (˚South)
0
1.8
1.5
1.2
0.9
0.6
0.3
Euphausia superba Salpa thompsoni
1997/98AIBF
0
0.1
0.2
0.3
0.4
46 48 50 52 54 56 58 60 62 64 66 68 70
Latitude (South)
Kril
l abu
ndan
ce (
ind.
m-3
)
0
0.3
0.6
0.9
1.2
1.5Euphausia superba Salpa thompsoni
1993AIBF
Kril
l abu
ndan
ce (
ind.
m-3
)
Sal
p ab
unda
nce
(ind.
m-3
)S
alp
abun
danc
e (in
d.m
-3)
Fig. 4. Horizontal distribution pattern of E. superba and S.
thompsoni along the Greenwich Meridian during January 1993
(top, data extracted from Pakhomov et al., 2000) and along the
61E meridian during December 1997–January 1998 (bottom,
data extracted from Pakhomov, 2002) in the top 300 m layer.
AIBF: Antarctic Ice Boundary Front after Klyausov (1993).
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–19071890
observed that no solitary forms were found in thehigh latitudes and that aggregate forms werealways small in size, thus suggesting that S.
thompsoni aggregates were transported into thearea, rather than being the result of asexualreproduction in situ (Boysen-Ennen et al., 1991;Siegel and Harm, 1996; Chiba et al., 1999). Thetesting of this hypothesis certainly requires moreresearch. Unlike that of S. thompsoni, the distribu-tion of Antarctic krill is restricted to highAntarctic waters masses and its life cycle is closelylinked to the seasonal sea-ice biotope (Knox, 1994;Loeb et al., 1997).
Analyzing the macro-scale contrasting distribu-tion of Antarctic krill and S. thompsoni, Kawa-mura et al. (1994) suggested that this could not beexplained by either behavioral functions of organ-isms, such as swarm formation, or ecologicalregimes, such as competitive exclusion. Theyhypothesized that the marked inverse distributionof salps and krill might be related to the watermass structure in the areas investigated. Thisseems to be confirmed by data presented in this
study, which show that Antarctic krill and S.
thompsoni are spatially separated through most ofthe Southern Ocean (Nicol et al., 2000b). Never-theless, in the Atlantic sector, particularly in thewaters off the Antarctic Peninsula and aroundSouth Shetland Islands, Antarctic krill and salpsshow some degree of overlap in their summermacro-scale distribution (e.g., Witek et al., 1985;Piatkowski, 1987; Loeb et al., 1997; Ross et al.,1998). This is hardly surprising as this region is oneof the most complex areas of the Southern Ocean,where water masses of different origin are oftenmixed together (Maslennikov and Solyankin,1979; Maslennikov, 1980; Sahrhage, 1988). Recentanalysis of long-term data sets on krill biomass,krill spawning and recruitment, salp biomass andsea-ice cover in the vicinity of the Elephant Islandhas revealed significant correlation between theseparameters (Loeb et al., 1997). It has beenpostulated that winters characterized by poorsea-ice cover would promote extensive salp bloomsand poor krill spawning during the followingsummer and, as a consequence, poor krill
Fig. 5. Vertical distribution of temperature and S. thompsoni along 601E and 751E (Indian sector) during summer seasons of 1985 and
1986. Seawater temperature was measured down to 1500 m, while salps were sampled down to 500 m at depth strata: 0–25, 25–50, 50–
100, 100–200 and 200–500 m every degree of latitude. Redrawn from Pakhomov (1991). 1, negative; 2, 1–10; 3, 11–100; 4, 101–1000; 5,
>1000 ind m�2.
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–1907 1891
recruitment the following year. A long-termwarming trend was suggested to be responsiblefor the increased occurrence of ‘salp’ years aroundElephant Island (Loeb et al., 1997). Significantcorrelations have been obtained between lowAntarctic krill biomass and unusually high sea-water temperatures in the vicinity of the AntarcticPeninsula (Priddle et al., 1988; Loeb et al., 1997),to the extent that during some years salps (mainlyS. thompsoni) dominated total zooplankton (Mu-jica and Asencio, 1985; Witek et al., 1985; Nast,1986; Huntley et al., 1989; Siegel and Loeb, 1995;Loeb et al., 1997; Minkina et al., 1999). None-theless, despite this large-scale overlapping pat-tern, during fine-scale surveys conducted off theAntarctic Peninsula, particularly around ElephantIsland, a pronounced spatial, horizontal or verticalseparation between krill and salps has beendemonstrated in a number of studies (e.g., Nast,1986; Piatkowski, 1989; Park and Wormuth, 1993;Brinton, 1984; Maklygin and Pakhomov, 1993;Pakhomov, 1993a, b; Nishikawa et al., 1995; Rosset al., 1998; Minkina et al., 1999).
4. Krill/salp feeding dynamics
4.1. Euphausia superba: ingestion and egestion
rates
Despite the numerous attempts to estimate dailyconsumption rates in Antarctic krill (see Table 2),ingestion rates obtained using the gut fluorescencetechnique are not numerous. In situ measuredphytoplankton consumption by Antarctic krillvaries between 0.06 and 0.62 mg (pigm) ind�1 d�1,for specimens o25 mm in length, and between 0.3and 96.9 mg (pigm) ind�1 d�1 in specimens>30 mm (Drits and Semenova, 1989; Daly, 1990;Drits and Pasternak, 1993; Pakhomov et al., 1997;Perissinotto et al., 1997; Pakhomov and Frone-man, 2002b). The daily carbon rations obtainedusing the gut fluorescence method are generally inthe lower range (o5% of body carbon) ofestimates calculated employing other techniques(Table 2). When the high metabolic activity ofAntarctic krill is combined with the energetic costsfor growth, molting and reproduction, krill carbon
uptake ranges between 5% and 15% of bodycarbon (Table 2). This daily ration can be obtainedfrom phytoplankton only on occasions whenchlorophyll-a concentrations are in excess of3 mg l�1 (Table 2). It is now recognized thatAntarctic krill exhibits omnivory and carnivorythroughout most of the year and can be regardedas a truly herbivore only during the period ofspring/early summer phytoplankton blooms (Mill-er and Hampton, 1989; Perissinotto et al., 1997).As a purely phytoplankton diet often does notcover even its basic metabolic demands (e.g.,Pakhomov et al., 1997; Perissinotto et al., 1997),Antarctic krill complement its diet with hetero-trophic carbon by consuming on average up to80% of total carbon in the form of micro- andmesozooplankton (Perissinotto et al., 2000).
Grazing rates of Antarctic krill, as a function offood concentration, show different types ofresponse depending on krill physiological state,season, quality and quantity of food (Kato et al.,1982; Schnack, 1985a, b; Helbling et al., 1992). Anon-saturating linear response was obtained withchlorophyll-a concentrations of up to 20 mg l�1
(Price et al., 1988; Ross et al., 1998). A saturationtype of model has also been described on severaloccasions, particularly in experiments where het-erotrophic food is offered, with upper foodconcentration thresholds of 6–8 mg C l�1 (Samy-shev and Lushov, 1983; Krylov, 1989; Ross et al.,1998).
Egestion rates of Antarctic krill range consider-ably, between 0.3 and 55 mg C mg dry wt�1 d�1
(Table 3), and appear to correlate with the ambientchlorophyll-a concentration (Clarke et al., 1988) aswell as with the krill mass (Table 3).
4.2. Salpa thompsoni: feeding dynamics
One of the goals of this revision is to derivesimple predictive models of individual ingestionand egestion rates for S. thompsoni in the SouthernOcean. As predictor variables, salp body lengthand mass were used. Salps are believed to have anon-saturation feeding response to food concen-tration, as they are probably unable to regulatetheir filtration rates (Perissinotto and Pakhomov,1998a, b). Indeed, a positive trend between S.
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–19071892
Table 2
Estimates of the daily ration in the Antarctic krill, Euphausia superba
Daily ingestion
rate (mg
C ind�1 d�1)
% of body C Length, stage Conditions, food, method Sources
0.28–5.38 3.97–11.9 18–53 mm Energy budget Chekunova and Rynkova
(1974)
0.02–1.92 0.02–1.66 30–50 mm Ingestion rates and energy budget
after Clarke and Morris (1983)
Antezana et al. (1982)
0.18–0.22 2.9–3.9 19–35 mm In vitro filtration rates with a
culture of Dunaliella
Kato et al. (1982)
1.47–1.92 1.1–1.5 35–55 mm In vitro filtration rates with a
culture of Dunaliella
Kato et al. (1982)
4.77–5.72 5.0–6.0 40–50 mm Energy budget Clarke and Morris (1983)
0.43–1.04 0.86–5.63, mean
2.0
16–50 mm Radiocarbon method, phytoplankton
cultures and detritus as food
Samyshev and Lushov (1983)
3.6–5.04 2.3–10.0 40–50 mm In vitro filtration and ingestion
rates with net phytoplankton, furcilia
of E. superba and infusoria as food
Boyd et al. (1984)
0.38–2.05 2.6–17.1 30–35 mm In vitro ingestion rates with net
phytoplankton as food
Schnack (1985a, b)
0.42–1.37 0.8–2.4 40–45 mm In vitro ingestion rates with net
phytoplankton as food
Schnack (1985a, b)
0.74–2.6 0.9–3.2 50–55 mm In vitro ingestion rates with net
phytoplankton as food
Schnack (1985a, b)
9.5–17.9 17–28 40–50 mm Faecal pellet evacuation rates using
net phytoplankton as food
Clarke et al. (1988)
7.64 8.5 20–30 mm Energy budget Price et al. (1988)
0.41–5.07 0.53–5.81 40–55 mm Filtration rates using zooplankton
and Artemia nauplii as food
Krylov (1989)
1.1–4.4 0.75–3.09 40–55 mm In situ gut pigment contents Ponomareva and Kuznetsova
(1989)
8.1–14.4 5.0–7.3 40–55 mm In vitro gut pigment contents Ponomareva and Kuznetsova
(1989)
0.18–0.6, max 9.4 0.31–5.76 40–55 mm Gut evacuation and ingestion rates Drits and Semenova (1989)
0.003–0.067 2–52, mean 10 furcilia 3–6 Gut evacuation rates Daly (1990)
0.006–0.026 mean 19.7 calyptopis 1–2 In situ and in vitro filtration rates,
net phytoplankton as food
Huntley and Brinton (1991)
0.022–0.024 mean 4.4 furcilia 4–5 In situ and in vitro filtration rates,
net phytoplankton as food
Huntley and Brinton (1991)
0.011 0.05 38–55 mm Gut evacuation and ingestion rates Drits and Pasternak (1993)
6.72–9.12 0.8–3.67 20–40 mm Estimated by model Huntley et al. (1994)
6.12 8.66 47.3 mm In vitro ingestion rates with Salpa
thompsoni aggregates as food
Kawaguchi and Takahashi
(1996)
0.23–0.93 0.43–1.7 38–43 mm In situ gut pigment contents Pakhomov et al. (1997)
2.73 4.99 38–43 mm In situ egestion rates Pakhomov et al. (1997)
0.05–4.45 0.15–1.68, max 13 35–50 mm In situ gut pigment contents Perissinotto et al. (1997)
0.026–0.031 0.5–0.6 o25 mm In situ gut pigment contents Pakhomov and Froneman
(2002b)
0.079 0.55 25–35 mm In situ gut pigment contents Pakhomov and Froneman
(2002b)
0.178 0.38 35–50 mm In situ gut pigment contents Pakhomov and Froneman
(2002b)
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–1907 1893
thompsoni ingestion rates and ambient phyto-plankton concentration has been documented inthe chlorophyll-a range of 0.2–1.2 mg l�1 (Pakho-mov and Froneman, 2002b). A linear functionalresponse of ingestion rates versus food concentra-tion may apply only to a relatively narrow range ofparticle concentrations, as it has been shown thatat higher concentrations salp feeding can bedisrupted (Harbison et al., 1986; Zeldis et al.,1995; Perissinotto and Pakhomov, 1997). Theupper concentration threshold for S. thompsoni isnot clearly defined. However, in the Lazarev Sea2–5 cm long aggregates of S. thompsoni are unableto graze at particle concentrations >1 mg l�1
(Perissinotto and Pakhomov, 1997).To date, there are only seven literature sources
dealing with estimates of gut pigment content,filtration, ingestion and egestion rates of S.
thompsoni in the Atlantic sector of the SouthernOcean (Reinke, 1987; Drits and Semenova, 1989;Huntley et al., 1989; Drits and Pasternak, 1993;Dubischar and Bathmann, 1997; Perissinotto andPakhomov, 1998a, b; Pakhomov, 2002). Poolingthese data, a significant linear relationship betweenlog-transformed salp length and gut pigmentcontent is obtained (Fig. 6). As expected, clearancerates of S. thompsoni increase with body length(Fig. 7). Although derived from several authors,the ingestion rates of S. thompsoni are remarkablysimilar and consistent. Changes in ingestion ratesas a function of salp length are best represented bya power function. However, the global data set isbest fitted by a polynomial function, or by a linearfunction when log-transformed (Fig. 8). Whenconverted to carbon units, S. thompsoni ingestionrates increase linearly with the carbon mass of thesalp body (Fig. 9). Interestingly, daily rations of S.
Table 3
Antarctic krill Euphausia superba egestion rates. Carbon content of faecal pellets was assumed to account in average for 11% of their
dry mass (Pakhomov et al., 1997)
Mean krill mass (mg dry wt) Egestion rate (mg C mg dry wt�1 d�1) Source
243.6720.0 mean 0.287, max 2.258 Antezana et al. (1982)
144.0 4.583–43.083 Clarke et al. (1988)
154.9723.2 mean 0.298, max 0.393 Ponomareva and Kuznetsova (1989)
45.3716.6 mean 10.0, max 55.0 Nordhausen and Huntley (1990)
137.0731.4 mean 7.131 Pakhomov et al. (1997)
y = 1.7291x + 0.6089
R2 = 0.8381, N = 470
0
1
2
3
4
5
0.5 1 1.5 2 2.5
Log salp length (mm)
Log
pigm
ent c
onte
nt (
ng(p
igm
).in
d.-1
)
Fig. 6. Gut pigment content of S. thompsoni as a function of
body length. Data were extracted mainly from Dubischar and
Bathmann (1997), Perissinotto and Pakhomov (1998a, b), and
Pakhomov and Froneman (2002b).
y = 1.8603x - 1.4266
R2 = 0.8439N = 16
0
0.5
1
1.5
2
2.5
0.5 1 1.5 2 2.5
Log salp length (mm)
Log
clea
ranc
e ra
te (
I.ind
.-1 d
-1)
Fig. 7. Clearance rates of S. thompsoni as a function of body
length. Data extracted from Reinke (1987); Drits and Semenova
(1989); Huntley et al. (1989), Drits and Pasternak (1993),
Dubischar and Bathmann (1997), Perissinotto and Pakhomov
(1998a, b), and Pakhomov, 2002).
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–19071894
thompsoni do not show a distinct trend, either withincreasing body length or with body carbon mass(Fig. 10).
Overall, in situ individual ingestion and clear-ance rates of S. thompsoni are the highest of anyother primary consumer in the Antarctic pelagiccommunity (e.g., Drits and Semenova, 1989; Dritsand Pasternak, 1993; Froneman et al., 1997;Perissinotto and Pakhomov, 1998a, b; Pakhomov,2002; Pakhomov and Froneman, 2002a, b). Inges-tion rates of S. thompsoni estimated with in vitroincubations are up to one order of magnitudelower than in situ consumption rates (Fig. 11).Therefore, in vitro estimated consumption ratesare most likely erroneous due to such things assmall volume, stress during capture, short adapta-tion time, particularly when large specimens areincubated.
Unlike for Antarctic krill, there is little informa-tion available on egestion rates of S. thompsoni. Ina single experiment conducted near the AntarcticPeninsula during austral summer 1983/84, a21 mm blastozoid of S. thompsoni egested 10.2%of body carbon and 6.6% of body nitrogen perday, which accounted for 40.7% and 48.8% of thecarbon and nitrogen ingested, respectively (Hunt-ley et al., 1989). During the summer season 1997/98, in the region south of the APF and along 61E,daily egestion rates of S. thompsoni ranged from187.8 ng (pigm) ind�1 d�1 (or 9.4 mg C ind�1 d�1) in10 mm salps, to 3.57 mg (pigm) ind�1 d�1 (or178.6 mg C ind�1 d�1) in 55 mm salps (Fig. 12).Although in situ egestion rates on averageaccounted for 36% (range 22–56%) of the in situpigment consumption, they were equivalent toonly 0.9–3.5% of body carbon (Pakhomov, 2002).
4.3. Krill/salp particle selectivity
As non-selective filter-feeders, salps are able toretain efficiently particles within a wide size range,
y = 2.8795x2.3194
R2 = 0.9427N = 15
y = 13.06x2 - 34.304x - 1719.2
R2 = 0.9861, N = 32
0
20
40
60
80
140
120
100
0 20 40 60 80 100 120
Salp total length (mm)
Inge
stio
n ra
te (
µg(p
igm
).in
d-1.d
-1)
Pakhomov, in press Dubischar & Bathmann, 1997
Perissinotto & Pakhomov, 1998a,b Drits & Semenova, 1989
Huntley et al., 1989 Drits & Pasternak, 1993
y = 2.0948x + 0.7424
R2 = 0.821, N = 32
2
3
4
5
6
0.7 0.9 1.1 1.3 1.5 1.7 1.9 2.1
Log salp length (mm)
Log
inge
stio
n ra
te (
ng(p
igm
).in
d-1.d
-1)
(a)
(b)
Fig. 8. A summary of daily ingestion rates of S. thompsoni as a
function of body length.
y = 0.2167x - 118.91
R2 = 0.953, N = 32
0
7000
6000
5000
4000
3000
2000
1000
0 5000 10000 15000 20000 25000 30000 35000
Salp carbon body weight (µg)
Inge
stio
n ra
te (
µgC
.ind.
-1.d
-1)
y=1.9913x - 0.3605
R2 = 0.7978, N = 32
1
1.5
2
2.5
3
3.5
4
0.5 1 1.5 2 2.5
Log Salp length (mm)
Log
IR (
mic
rogr
am C
.ind.
-1.d
-1)
Fig. 9. Carbon daily ingestion rates of S. thompsoni as a
function of carbon body mass and body length.
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–1907 1895
ranging from 1 to 1000 mm (Drits and Semenova,1989; Fortier et al., 1994), while Antarctic krillconsumes mainly food particles >10–o50 mm(Meyer and El-Sayed, 1983; Drits and Semenova,1989; Maciejewska, 1993; Opalinski et al., 1997).
4.4. Krill/salp grazing impact: implications for
vertical carbon flux
Table 4 summarizes estimates of grazing impactfor Antarctic krill and S. thompsoni obtained usinga variety of techniques. With the exception of twoestimates obtained by Dubischar and Bathmann(1997) and by Perissinotto and Pakhomov(1998a, b), the highest impacts are derived fromindirect estimates of the energetic requirements ofkrill and salps, under the assumption that allcarbon demands are met through an herbivorousdiet (Table 4). This is incorrect since bothAntarctic krill and S. thompsoni are known toconsume a substantial proportion of heterotrophicmaterial (Foxton, 1966; Hopkins, 1985; Hopkinsand Torres, 1989; Hopkins et al., 1993; Lancraftet al., 1991; Perissinotto et al., 1997, 2000).Overall, the grazing impact of both krill and salpsis moderate through most of the Southern Ocean,and even in areas where they co-occur they usuallydo not make sufficient impact to control phyto-plankton growth (Pakhomov, 2002; Pakhomovand Froneman, 2002b). This, however, might bean underestimate as Chla/carbon ratio of 50 wasemployed in most of these studies.
Regarding the contribution of krill and salps tothe vertical carbon flux, data suggest that it isindeed extremely variable, reflecting the naturalpatchiness of food and of both species. Based ondirect (fecal pellet production) and indirect (graz-ing impact and assimilation efficiency) data,Antarctic krill may account on average for a
0
10
20
30
40
50
0 20 40 60 80 100 120
Salp body length (mm)
Dai
ly ra
tion
(% b
ody
carb
on)
N = 32
0
10
20
30
40
50
0 5000 10000 15000 20000 25000 30000 35000
Salp carbon body weight (microgram)
Dai
ly ra
tion
(% b
ody
carb
on)
N = 32
Fig. 10. Carbon daily rations as percentage of body carbon of
S. thompsoni as a function of body length and body carbon
weight.
0
10000
20000
30000
40000
50000
60000
70000
30 40 70
Salp length (mm)
Inge
stio
n ra
te (
ng(p
igm
).in
d.-1
d-1)
in situ in vitro
Fig. 11. Comparison between in situ and in vitro estimated
ingestion rates of S. thompsoni. Data extracted from Dubischar
and Bathmann (1997) and Pakhomov (2002).
y = 1.6328x + 0.6634
R2 = 0.8901
1
2
3
4
1.81.71.61.51.41.31.21.110.9
Log salp length (mm)
Log
eges
tion
rate
(ng(
pigm
).in
d.-1
d-1)
Fig. 12. Egestion rates of S. thompsoni as a function of body
length. Data extracted from Pakhomov (2002).
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–19071896
vertical flux of feces ranging from 0.01 to 15.6 mgC m�2 d�1 (Pakhomov et al., 1997; Ross et al.,1998; Pakhomov, 2002). While swarming, Antarc-
tic krill are able to contribute a vertical flux ofbetween 44.9 mg C m�2 d�1 and 1.3 gC m�2 d�1
(Clarke et al., 1988; Pakhomov et al., 1997). The
Table 4
Summary of grazing impact estimates of Antarctic krill and Salpa thompsoni
Geographical location Season Daily grazing impact Source
% Chla
stock
% daily PP
Euphausia superba
Elephant Island Summer nd 60–81 Holm-Hansen and Huntley
(1984)
Summer 1989 nd 0.1–6.7 Drits and Pasternak (1993),
Pakhomov (1991)
Autumn 1998 nd 33 Minkina et al. (1999)
Scotia Sea Summer nd 2.2–4.4 Holm-Hansen and Huntley
(1984)
Summer 1984 nd 1.2 Samyshev (1991)
Bouvet Island region Winter 1982 nd o12 Sushin et al. (1985)
South Georgia Summer 1994 0.4–1.9 9.6–59.2 Pakhomov et al. (1997)
Greewich Meridian, APF–MIZ Summer 1993 o0.1–2.7 o0.1–50.8 Perissinotto et al. (1997)
61E, 56–651S Summer 1997/98 o0.1–6.9 o0.1–22.7 Pakhomov (2002)
Bransfield Strait Spring nd 45 von Bodungen (1986)
Summer 1983/84 nd p1 Godlewska (1989)
South Shetland Islands Spring 1985 p0.2 0.1–5.5 Drits and Semenova (1989)
Antarctic Peninsula Summers 1993–95 nd p23, max 421 Ross et al. (1998)
Weddell Sea Summer 1989 nd o0.1–23.4 Pakhomov (1991)
Southern Indian Ocean Summer 1981 nd E3 Miller et al. (1985)
Prydz Bay Region Summers 1980–84 nd 10–84.5, max 190 Samyshev (1985, 1991)
Salpa thompsoni
Elephant Island Summer 1994 nd 19 Loeb et al. (1997)
Autumn 1998 nd 261 Minkina et al. (1999)
South Shetland Islands Spring 1985 1.5 44 Drits and Semenova (1989)
Summer 1990/91 nd 9 Nishikawa et al. (1995)
Bransfield Strait Summer 1989 nd 14.5–39 Drits and Pasternak (1993),
Pakhomov (1991)
Summer 1994 nd E5 Alcaraz et al. (1998)
Antarctic Peninsula Summer 1989/90 nd 1–10, max E100 Huntley et al. (1989)
Summers 1993–95 nd p37 Ross et al. (1998)
Atlantic Sector, southern ACC Spring 1992 nd >100 Dubischar and Bathmann
(1997)
61E, 49–591S Summer 1997/98 1–19.3 3.1–63.3 Pakhomov (2002)
Lazarev Sea Summer 1994/95 o0.1–21.4 o1–109 Perissinotto and Pakhomov
(1998a, b)
Weddell Sea Summer 1989 nd p2.5 Pakhomov (1991)
nd: Not determined.
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–1907 1897
above values are in the range of those obtainedfrom sediment trap collections in different regionsof the high Antarctic, where krill feces were foundto contribute up to 80% of total particle carbonflux in the top 200–300 m (Schnack, 1985a, b; vonBodungen, 1986; N .othig and von Bodungen, 1989;Bathmann et al., 1991; Gonzalez, 1992).
Although the salp contribution to the verticalcarbon flux in the Southern Ocean has yet to bemeasured through sediment trap collections, S.
thompsoni feces potentially may account for0.1–88 mg C m�2 d�1 (Huntley et al., 1989; Peri-ssinotto and Pakhomov, 1998a, b; Ross et al.,1998; Pakhomov, 2002). It is estimated thattogether Antarctic krill and S. thompsoni may re-package and remove up to 20% of phytoplanktonproduction per day from the euphotic zone(Pakhomov, 2002). As S. thompsoni has lower(Pakhomov, 2002) or similar (Huntley et al., 1989)carbon mass specific egestion rates than Antarctickrill (Fig. 13), maximum salp contribution to thevertical flux in carbon units should be substantiallylower, due to the differences in carbon densitiesbetween the two species (see Section 3.1).
Antarctic krill is known to channel a largefraction of ingested material into a long-lived (e.g.,food web transport) carbon pool (sensu Fortieret al., 1994), while salps are more important insequestering biogenic carbon, by producing large,fast sinking feces (Le F"evre et al., 1998). Indeed,Antarctic krill is a well known food source fornumerous Antarctic top predators, includingsquid, demersal and mesopelagic fish, flying birdsand penguins, seals and whales (Knox, 1994).Antarctic top predators are thought to consumebetween 166� 106 and 450� 106 tonnes of Ant-arctic krill annually (Lubimova and Shust, 1980;Laws, 1985; Miller and Hampton, 1989). Salp-mediated export to the top predators is much lessknown. It has been suggested that the export maybe both direct and indirect (Le F"evre et al., 1998).Data gathered from literature sources, show that asubstantial number of Antarctic zooplanktonspecies (13), including Antarctic krill, 8 birdspecies and 24 species of fish may consume salpsin energetically meaningful amounts (Table 5). It isbecoming obvious that salps are not a trophic cul-
de-sac in the Antarctic ecosystem and may actually
play a more important role in the ecosystembudget than previously believed.
5. Krill/salp interactions: competitive exclusion or
biotopical separation?
The increasing interest developed towards krilland salp interactions in the Southern Ocean overthe past few decades has led to the formulation ofseveral hypotheses to explain their spatial separa-tion (Nishikawa et al., 1995). Firstly, it has beensuggested that salps may prey (filter out) on eggsand early larval stages of Antarctic krill, thusaffecting krill recruitment (Huntley et al., 1989).This hypothesis was based on the occurrence ofkrill debris and larvae in food boluses of S.
thompsoni (Foxton, 1966; Hopkins, 1985; Hopkinsand Torres, 1989; Hopkins et al., 1993; Lancraftet al., 1991). However, due to the verticalsegregation of Antarctic krill eggs/early stagesand salps, direct consumption appears to benegligible (Perissinotto and Pakhomov, 1998b).Even if salps prey upon early developmental stagesof Antarctic krill, the effect will only be noticeablein later years and, as a consequence, cannotexplain the spatial segregation of salps and adultkrill during a particular season.
Secondly, salps may produce distasteful meta-bolic products, which may drive krill away(Fraser, 1962). This hypothesis cannot be dis-carded although it has never been tested. In
Fig. 13. Mass specific egestion rates of E. superba and S.
thompsoni as a function of body carbon mass. Data extracted
from Table 3 and from Pakhomov (2002).
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–19071898
Table 5
Predators of Salpa thompsoni in the Southern Ocean
Predator name Consumption rate Source
Crustaceans
Euphasuia superba 0.5 salp. krill�1 d�1 Kawaguchi and Takahashi (1996)
Vibilia antarctica nd Phleger et al. (2000), Lancraft et al. (1991)
Cyllopus licasii 19.4–30.7% FO Hopkins and Torres (1989)
Cyllopus magellanicus nd Phleger et al. (2000)
Themisto gaudichaudi 47.1% FO Hopkins (1985)
Cyphocaris richardi 5.1% FO Hopkins (1985)
Epimeriella macronyx 4.5% FO Hopkins (1985)
Eusirus microps 12.5% FO Hopkins (1985)
Orchomene plebs 28% FO Hopkins (1985)
Orchomene rossi 22.7% FO Hopkins (1985)
Parandania boecki 12.5% FO Hopkins (1985)
Antarctomysis ohlinii 1.0% FO Hopkins (1985)
Polychetes
Tomopteris carpenteri 10% FO Hopkins (1985)
Birds
Black-browed Albatross (Diomedea
melanophris)
nd Foxton (1966)
Gray-headed Albatross (Diomedea
chrysostoma)
nd Foxton (1966)
Antarctic Fulmar (Fulmarus antarcticus) 5% of FBW Ainley et al. (1991)
Blue Petrel (Halobaena coerulea) 2.7% of FBW Ainley et al. (1991)
Cape Petrel (Daption capense) 1–14.9% of FBW Ainley et al. (1991)
Antarctic Prion (Pachiptila vittata) 3.2% of FBW Ainley et al. (1991)
Wilson’s Storm Petrel (Oceanites
oceanicus)
1.8% of FBW Ainley et al. (1991)
White-chinned Petrel (Procellaria
aequinoctialis)
10–15 FO; 0.3–1.5% of PN Catard et al. (2000)
Demersal fish
Gobionotothen gibberifrons 0.2–4.3% of PN Permitin and Tarverdieva (1972)
Gobionotothen gibberifrons 10% FO Permitin and Tarverdieva (1978)
Lepidonotothen nudifrons 1.4% of PN Permitin and Tarverdieva (1972)
Lepidonotothen squamifrons 2.7–39.5% of PN Duhamel (1981), Duhamel and Pletikosic
(1983), Duhamel and Hureau (1985)
Lepidonotothen squamifrons 25.3–30.6% of FBW Pakhomov (1993c)
Lepidonotothen squamifrons 8.2–40% FO, 4–19% FBW Chechun (1984)
Lepidonothoten larseni 15% FO Permitin and Tarverdieva (1978)
Nototheniops tchizh 23–88% FO, 21–84% FBW Shandikov (1986)
Notothenia rossii rossii 4.4–18.4% of PN Duhamel (1981), Duhamel and Hureau
(1985)
Notothenia rossii marmorata 1.5–2% FO, 1.3% FBW Tarverdieva (1972)
Notothenia rossii rossii 13–40% FO, 4–20% FBW Chechun (1984)
Dissostichus eleginoides 1–6.3% FO, 0.3–2.3% FBW Chechun (1984)
Channichthys rhinoceratus 5.7% FO, 0.4% FBW Chechun (1984)
Trematomus eulepidotus 0.8% of FBW Pakhomov (1991)
Trematomus lepidorchinus 3.7% FO; 3.7% of FBW Pakhomov (1991)
Trematomus hansoni 11.2% FO; 2.1% of FBW Pakhomov (1991)
Trematomus scotti 4.2% FO; 0.8% of FBW Pakhomov (1991)
Trematomus centronotus 10.1% FO; 1.9% of FBW Pakhomov (1991)
Trematomus bernacchii 54.4% FO; 32.8% of FBW Pakhomov (1991)
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–1907 1899
contrast, recent observations have shown thatAntarctic krill is actually attracted to S. thompsoni
extracts and is able to prey successfully on salpswith a meaningful rate of up to 0.5 salps per krillper day, or E8.7% of body carbon per day (Table2; Kawaguchi and Takahashi, 1996).
Thirdly, Antarctic krill may be excluded fromthe areas of high salp densities because salps mayoutcompete other zooplankton, including krill, forfood (Fraser, 1962; Perissinotto and Pakhomov,1998b). Salps are indeed efficient at retainingparticles within a wide size range, while Antarctickrill prey selectively on specific food particles(Section 4.3). Although it is almost impossible toverify the above hypothesis in the marine environ-ment (Le F"evre et al., 1998), there is indirectevidence that competition between salps andAntarctic krill for food is negligible. No directinteractions between the proportion of green krill(intensively feeding krill) and salp density has beenobserved around the Antarctic Peninsula regionusing a comprehensive data set collected duringthe Japanese krill fishing operations (Kawaguchiet al., 1998). The authors also noticed a clearspatial and temporal mismatch between salps andgreen krill and linked this to the appearance ofwarmer waters in the region (Kawaguchi et al.,1998).
Competitive removal of food may be the majorseparating force of krill and salp concentrations(Perissinotto and Pakhomov, 1998b) when they
are found together spatially and temporally, whichdoes not seem to be the case on most occasions(Kawaguchi et al., 1998). Recently, it has beenhypothesized that food availability prior to theinteraction, rather than direct food competitionbetween different herbivores, may be responsiblefor competitive exclusion (Chiba et al., 1998). Ifthis applies to Antarctic krill and salps, it meansthat in the high Antarctic region we alwaysobserve the end result of the competition ratherthan the process itself, even despite extensiveseasonal coverage. We are of the opinion thatdirect competition for food may indeed be valid inthe long-term (Loeb et al., 1997), while this wouldnot explain the short-term inverse distributionbetween krill and salps (Chiba et al., 1998).Finally, most recently an approach comparingthe carbon budgets of major metazoan herbivoresin the Southern Ocean has been used (Le F"evreet al., 1998). According to these calculations,resource thresholds at which herbivores are ableto fulfill their basic metabolic requirements are3.5–30 mg C l�1 for S. thompsoni, 105 mg C l�1 forcopepods and 125 mg C l�1 for Antarctic krill (LeF"evre et al., 1998). This clearly implies that salpsmay survive successfully at low food concentra-tions compared, for example, to Antarctic krill.Interestingly, the empirical upper threshold of>1 mg chlorophyll-a l�1, at which salp cloggingmay occur (Perissinotto and Pakhomov, 1997),would be equal to 7100 mg C l�1, after converting
Table 5 (continued)
Predator name Consumption rate Source
Gymnodraco acuticeps 1.0% FO; 0.01% of FBW Pakhomov (1991)
Dissostichus mawsoni 0.5% FO; 0.1% of FBW Pakhomov (1991)
Lepidonotothen kempi 15.9% FO; 5.4% of FBW Pakhomov (1991)
Cygnodraco mawsoni 0.3% FO; 0.1% of FBW Pakhomov (1991)
Histiodraco velifer 14.3% FO; 1.4% of FBW Pakhomov (1991)
Mesopelagic fish
Bathylagus antarcticus 11.4% FO; 1–14% of PN Hopkins and Torres (1989), Lancraft et al.
(1991)
Electrona antarctica 0.5–22.2% FO; 0.1–1% of FBW Hopkins (1985), Hopkins and Torres
(1989), Pakhomov et al. (1996)
Electrona carlsbergi 0–14% FO, 0–7.4% FBW Kozlov and Tarverdieva (1989)
Gymnoscopelus opisthopterus 11.1% of FBW Pakhomov et al. (1996)
Gymnoscopelus braueri 7.7% FO Lancraft et al. (1991)
FO, Frequency of occurrence in stomachs; FBW, Food bolus weight; PN, prey numbers; nd, Not determined.
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–19071900
to carbon and adding a heterotrophic component(following Le F"evre et al., 1998). Therefore, ifsalps would be able to maintain low foodconcentration, this may prevent development ofcopepods and Antarctic krill (Chiba et al., 1998;Perissinotto and Pakhomov, 1998a, b). It is likely,however, that once a phytoplankton bloom devel-ops within the Marginal Ice Zone, salps woulddisappear to the advantage of other zooplanktonsuch as krill and copepods, which are moreadapted to operate in the presence of high particleconcentrations (Nishikawa et al., 1995; Perissinot-to and Pakhomov, 1998b).
Finally, the spatial separation between krill andsalp populations may be due to the advection ofdifferent water masses in the region (Kawamuraet al., 1994; Kawaguchi et al., 1998). Thishypothesis has already been discussed above(Section 3.2.2) and seems to explain the limitedspatial overlap observed in krill/salp distributionoutside the Antarctic Peninsula region (see alsoNicol et al., 2000b). Although a small-scalesynchronized pattern between salp density andelevated sea-surface temperatures has been noticedaround the Antarctic Peninsula in number ofstudies (e.g., Nast, 1986; Piatkowski, 1989; Nishi-kawa et al., 1995; Minkina et al., 1999), thedistribution patterns of both Antarctic krill and S.
thompsoni are still to be studied in detail there,with particular emphasis to environmental vari-ables characterizing this area.
It appears that Antarctic krill and S. thompsoni
are adapted to be successful in biotopes withdifferent environmental conditions (Table 6, afterLe F"evre et al., 1998). These biotopes broadlycharacterize the open-ocean and coastal environ-ments, e.g., spatially separated realms (Nicol et al.,
2000b). However, in the regions of complex andvariable oceanography (e.g., off Antarctic Penin-sula, within the Marginal Ice Zone and polynyas)spatial separation, particularly in the macro-scale,becomes unclear. As a consequence, in suchregions krill and salp may theoretically co-existover short periods of time (Le F"evre et al., 1998).Nevertheless, the physiological constrains may beof crucial importance in keeping Antarctic krilland S. thompsoni separated in the long-term.Therefore, the environmental warming may leadto the increase in degree of spatial and temporaloverlap between these two large metazoans of theSouthern Ocean (see also Section 3.2.2). Theregional ecological consequences of the salp years,as discussed above, may be dramatic, suggestingthat if the warming trend will continue in the highAntarctic, salps would probably play more pro-minent role in the trophic structure of theAntarctic marine ecosystem. This could be coupledwith the dramatic decrease in krill productivitylargely due to decrease in the spatial extension ofthe krill biotope and inter-specific salp/krill inter-actions. High Antarctic regions, particularly theMarginal Ice Zone, however, have effectiveprotective mechanisms against salp invasions,e.g., low temperatures (reproduction constrains,Chiba et al., 1999) and high particle concentra-tions associated with the ice retreat (Perissinottoand Pakhomov, 1997).
Acknowledgements
This synthesis was completed with the financialsupport of the South African Department ofEnvironmental Affairs and Tourism (Pretoria)
Table 6
Environmental conditions under which salps and krill are expected to succeed (after Le F"evre et al. (1998) with additions)
Conditions Salps Krill
Food concentration Low High
Food distribution Homogeneous Patchy
Hydrodynamic conditions Dynamic Stable
Type of algae Small, flagellates Large, diatoms
Other food items Bacteria, microzooplankton, small mesozooplankton Micro- to macro-zooplankton
E.A. Pakhomov et al. / Deep-Sea Research II 49 (2002) 1881–1907 1901
and the South African National Research Foun-dation (Pretoria).
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