Mass distribution in the fronds of macrocystis pyrifera from New Zealand and California

Author(s):  
Melvin A. Nyman ◽  
Murray T. Brown ◽  
Michael Neushul ◽  
Bruce W. W. Harger ◽  
Jonathan A. Keogh
Hydrobiologia ◽  
1993 ◽  
Vol 260-261 (1) ◽  
pp. 57-65 ◽  
Author(s):  
Melvin A. Nyman ◽  
Murray T. Brown ◽  
Michael Neushul ◽  
Bruce W. W. Harger ◽  
Jonathan A. Keogh

1990 ◽  
Vol 2 (3) ◽  
pp. 249-257 ◽  
Author(s):  
Melvin A. Nyman ◽  
Murray T. Brown ◽  
Michael Neushul ◽  
Jonathan A. Keogh

1997 ◽  
Vol 129 (3) ◽  
pp. 417-424 ◽  
Author(s):  
M. T. Brown ◽  
M. A. Nyman ◽  
J. A. Keogh ◽  
N. K. M. Chin

2021 ◽  
Vol 8 ◽  
Author(s):  
Leigh W. Tait ◽  
François Thoral ◽  
Matthew H. Pinkerton ◽  
Mads S. Thomsen ◽  
David R. Schiel

Marine heatwaves (MHW) are becoming stronger and more frequent across the globe. MHWs affect the thermal physiology of all biological organisms, but wider ecosystem effects are particularly impactful when large habitat-forming foundation species such as kelps are affected. Many studies on impacts from MHWs on kelps have focused on temperature effects in isolation, except for a few studies that have integrated co-occurring stress from grazers, wave exposure and nutrient limitation. It is likely that many stressors act in concert with MHWs and exacerbate their effects. Here we analyzed satellite images over 60 months to assess temporal changes in abundance of surface canopies of the giant kelp Macrocystis pyrifera in the New Zealand coastal zone. The analysis encompassed the most extreme MHW on record (2017/18), across a 6° latitudinal gradient of four regions southward from the northern distributional limit of Macrocystis along mainland New Zealand. We tested the association of surface canopy cover of Macrocystis with sea surface temperature, temperature anomalies, chlorophyll-a (a proxy for nutrient availability) and water clarity (diffuse attenuation coefficient). We found a reduced cover of Macrocystis across all regions during and after the 2017/18 MHW, with least impact at the most southern region where the maximum temperatures did not exceed 18°C. There was also an important and significant interaction between temperature and water clarity, showing that temperature-induced kelp loss was greater when water clarity was poor. These results show that notable negative effects occurred across the coastal range of this foundation species and highlight the importance of studying MHW effects across latitudinal gradients and in concert with other co-occurring stressors.


1999 ◽  
Vol 190 ◽  
pp. 563-566
Author(s):  
J. D. Pritchard ◽  
W. Tobin ◽  
J. V. Clausen ◽  
E. F. Guinan ◽  
E. L. Fitzpatrick ◽  
...  

Our collaboration involves groups in Denmark, the U.S.A. Spain and of course New Zealand. Combining ground-based and satellite (IUEandHST) observations we aim to determine accurate and precise stellar fundamental parameters for the components of Magellanic Cloud Eclipsing Binaries as well as the distances to these systems and hence the parent galaxies themselves. This poster presents our latest progress.


Author(s):  
S. Golladay

The theory of multiple scattering has been worked out by Groves and comparisons have been made between predicted and observed signals for thick specimens observed in a STEM under conditions where phase contrast effects are unimportant. Independent measurements of the collection efficiencies of the two STEM detectors, calculations of the ratio σe/σi = R, where σe, σi are the total cross sections for elastic and inelastic scattering respectively, and a model of the unknown mass distribution are needed for these comparisons. In this paper an extension of this work will be described which allows the determination of the required efficiencies, R, and the unknown mass distribution from the data without additional measurements or models. Essential to the analysis is the fact that in a STEM two or more signal measurements can be made simultaneously at each image point.


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