scholarly journals Determination of copepod grazing on natural plankton communities: correcting for trophic cascade effects

2008 ◽  
Vol 357 ◽  
pp. 195-206 ◽  
Author(s):  
C Klaas ◽  
PG Verity ◽  
S Schultes
Hydrobiologia ◽  
2010 ◽  
Vol 644 (1) ◽  
pp. 325-335 ◽  
Author(s):  
Néstor Mazzeo ◽  
Carlos Iglesias ◽  
Franco Teixeira-de Mello ◽  
Ana Borthagaray ◽  
Claudia Fosalba ◽  
...  

2016 ◽  
Vol 25 (21) ◽  
pp. 5585-5602 ◽  
Author(s):  
Jessica L. Ray ◽  
Julia Althammer ◽  
Katrine S. Skaar ◽  
Paolo Simonelli ◽  
Aud Larsen ◽  
...  

Oecologia ◽  
2015 ◽  
Vol 180 (1) ◽  
pp. 293-303 ◽  
Author(s):  
Pei-Chen Wu ◽  
Pei-Jen L. Shaner

Ecosphere ◽  
2018 ◽  
Vol 9 (10) ◽  
pp. e02466 ◽  
Author(s):  
Shengjie Liu ◽  
Jing Hu ◽  
Jocelyn E. Behm ◽  
Xinxing He ◽  
Jianmin Gan ◽  
...  

1992 ◽  
Vol 49 (7) ◽  
pp. 1466-1473 ◽  
Author(s):  
Xavier Lazzaro ◽  
Ray W. Drenner ◽  
Roy A. Stein ◽  
J. Durward Smith

We quantified the effects of planktivore biomass and planktivore type in an experimental mesocosm study of factorial design in which five levels of fish biomass (0–75 g/m3) were cross-classified with two plantivore types: filter-feeding gizzard shad (Dorosoma cepedianum) and visual-feeding bluegill (Lepomis macrochims). As fish biomass increased, cladocerans, cyclopoids, particulate phosphorus (PP) > 200 μm, and chironomids declined; conversely, rotifers, primary productivity, chlorophyll a, turbidity, unicellular flagellates, colonial and unicellular green algae, pennate diatoms, total phosphorus, and 20–200 and 12–20 μm PP were enhanced. In the presence of gizzard shad, as compared with bluegill, cyclopoids, turbidity, unicellular green algae, pennate diatoms, > 200 μm PP, and chironomid tubes were higher whereas colonial green algae and < 0.2 μm PP were lower. Fish biomass operated independently of planktivore type for most variables, except copepods, colonial green algae, turbidity, and 20–200 μm PP. Although gizzard shad and bluegill have different trophic cascade pathways, fish biomass was more important than planktivore type as a regulator of plankton communities and water quality.


2016 ◽  
Vol 61 (5) ◽  
pp. 693-701 ◽  
Author(s):  
Qinghua Zhao ◽  
YinG Pan ◽  
John N. Griffin ◽  
Junzhao Sun ◽  
Shucun Sun

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1999 ◽  
Vol 190 ◽  
pp. 549-554
Author(s):  
Nino Panagia

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.


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