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Changeset 9394 for branches/2017/dev_merge_2017/DOC/tex_main – NEMO

Ignore:
Timestamp:
2018-03-13T21:21:44+01:00 (6 years ago)
Author:
nicolasmartin
Message:

Fix several typos, reverse (biblio then index) and shrink the manual backmatter (columns, font size, separator height) #1793

Location:
branches/2017/dev_merge_2017/DOC/tex_main
Files:
3 edited

Legend:

Unmodified
Added
Removed

  • branches/2017/dev_merge_2017/DOC/tex_main/NEMO_manual.bib

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    658647} 
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    678666} 
    679667 
    … …  
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    793780} 
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    824811   title = {On Antarctic Bottom Water consumption in the abyssal ocean}, 
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    828814   abstract = {In studies of ocean mixing, it is generally assumed that small-scale turbulent overturns lose 15-20 \% of their energy in eroding the background stratification. Accumulating evidence that this energy fraction, or mixing efficiency Rf, significantly varies depending on flow properties challenges this assumption, however. Here, we examine the implications of a varying mixing efficiency for ocean energetics and deep water mass transformation. Combining current parameterizations of internal wave-driven mixing with a recent model expressing Rf as a function of a turbulence intensity parameter Reb = εν/νN2, we show that accounting for reduced mixing efficiencies in regions of weak stratification or energetic turbulence (high Reb) strongly limits the ability of breaking internal waves to supply oceanic potential energy and drive abyssal upwelling. Moving from a fixed Rf = 1/6 to a variable efficiency Rf(Reb) causes Antarctic Bottom Water upwelling induced by locally-dissipating internal tides and lee waves to fall from 9 to 4 Sv, and the corresponding potential energy source to plunge from 97 to 44 GW. When adding the contribution of remotely-dissipating internal tides under idealized distributions of energy dissipation, the total rate of Antarctic Bottom Water upwelling is reduced by about a factor of 2, reaching 5-15 Sv compared to 10-33 Sv for a fixed efficiency. Our results suggest that distributed mixing, overflow-related boundary processes and geothermal heating are more effective in consuming abyssal waters than topographically-enhanced mixing by breaking internal waves. Our calculations also point to the importance of accurately constraining Rf(Reb) and including the effect in ocean models.}, 
    829815   journal = {Journal of Physical Oceanography}, 
    … …  
    836822   title = {The impact of a variable mixing efficiency on the abyssal overturning}, 
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    839824   doi = {10.1175/JPO-D-14-0259.1}, 
    840825   abstract = {In studies of ocean mixing, it is generally assumed that small-scale turbulent overturns lose 15-20 \% of their energy in eroding the background stratification. Accumulating evidence that this energy fraction, or mixing efficiency Rf, significantly varies depending on flow properties challenges this assumption, however. Here, we examine the implications of a varying mixing efficiency for ocean energetics and deep water mass transformation. Combining current parameterizations of internal wave-driven mixing with a recent model expressing Rf as a function of a turbulence intensity parameter Reb = εν/νN2, we show that accounting for reduced mixing efficiencies in regions of weak stratification or energetic turbulence (high Reb) strongly limits the ability of breaking internal waves to supply oceanic potential energy and drive abyssal upwelling. Moving from a fixed Rf = 1/6 to a variable efficiency Rf(Reb) causes Antarctic Bottom Water upwelling induced by locally-dissipating internal tides and lee waves to fall from 9 to 4 Sv, and the corresponding potential energy source to plunge from 97 to 44 GW. When adding the contribution of remotely-dissipating internal tides under idealized distributions of energy dissipation, the total rate of Antarctic Bottom Water upwelling is reduced by about a factor of 2, reaching 5-15 Sv compared to 10-33 Sv for a fixed efficiency. Our results suggest that distributed mixing, overflow-related boundary processes and geothermal heating are more effective in consuming abyssal waters than topographically-enhanced mixing by breaking internal waves. Our calculations also point to the importance of accurately constraining Rf(Reb) and including the effect in ocean models.}, 
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    12231204   abstract = {Abyssal hills, which are pervasive landforms on the seafloor of the Earth's oceans, represent a potential tectonic record of the history of mid-ocean ridge spreading. However, the most detailed global maps of the seafloor, derived from the satellite altimetry-based gravity field, cannot be used to deterministically characterize such small-scale ({\textless}10 km) morphology. Nevertheless, the small-scale variability of the gravity field can be related to the statistical properties of abyssal hill morphology using the upward continuation formulation. In this paper, I construct a global prediction of abyssal hill root-mean-square (rms) heights from the small-scale variability of the altimetric gravity field. The abyssal hill-related component of the gravity field is derived by first masking distinct features, such as seamounts, mid-ocean ridges, and continental margins, and then applying a newly designed adaptive directional filter algorithm to remove fracture zone/discontinuity fabric. A noise field is derived empirically by correlating the rms variability of the small-scale gravity field to the altimetric noise field in regions of very low relief, and the noise variance is subtracted from the small-scale gravity variance. Suites of synthetically derived, abyssal hill formed gravity fields are generated as a function of water depth, basement rms heights, and sediment thickness and used to predict abyssal hill seafloor rms heights from corrected small-scale gravity rms height. The resulting global prediction of abyssal hill rms heights is validated qualitatively by comparing against expected variations in abyssal hill morphology and quantitatively by comparing against actual measurements of rms heights. Although there is scatter, the prediction appears unbiased.}, 
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    33353276  doi = {10.1029/2007GL029275}, 
    3336   url = {http://dx.doi.org/10.1029/2007GL029275} 
    33373277} 
    33383278 

  • branches/2017/dev_merge_2017/DOC/tex_main/NEMO_manual.sty

    r9393 r9394  
    77%% ============================================================================== 
    88 
    9 \usepackage{natbib}     % bib 
    10 \usepackage{caption}    % caption 
    11 \usepackage{xcolor}     % color 
    12 \usepackage{silence}    % compilation 
    13 \usepackage{times}      % font 
    14 \usepackage{hyperref}   % hyper 
    15 \usepackage{enumitem}   % list 
    16 \usepackage{minted}     % listing 
    17 \usepackage{amsmath}    % maths 
    18 \usepackage{fancyhdr}   % page 
    19 \usepackage{minitoc}    % toc 
    20 \usepackage{subfiles}   % subdocs 
     9\usepackage{natbib}     %% bib 
     10\usepackage{caption}    %% caption 
     11\usepackage{xcolor}     %% color 
     12\usepackage{silence}    %% compilation 
     13\usepackage{times}      %% font 
     14\usepackage{hyperref}   %% hyper 
     15\usepackage{idxlayout}  %% index 
     16\usepackage{enumitem}   %% list 
     17\usepackage{minted}     %% listing 
     18\usepackage{amsmath}    %% maths 
     19\usepackage{fancyhdr}   %% page 
     20\usepackage{minitoc}    %% toc 
     21\usepackage{subfiles}   %% subdocs 
    2122 
    2223 
    … …  
    3435   colorlinks 
    3536} 
     37\idxlayout{font=footnotesize, columns=3} 
     38\renewcommand{\bibfont}{\footnotesize} 
     39\renewcommand{\bibsep}{3pt} 
    3640 
    3741 
    … …  
    4145\pagestyle{fancy} 
    4246\bibliographystyle{../tex_sub/ametsoc} 
     47 
    4348 
    4449%% Additionnal fonts 
    … …  
    121126%% New commands 
    122127 
    123 \newcommand{ \gmcomment}[1]{} 
    124 \newcommand{ \sfcomment}[1]{} 
     128\newcommand{\gmcomment}[1]{} 
     129\newcommand{\sfcomment}[1]{} 
    125130\newcommand{\sgacomment}[1]{} 
    126131 
    … …  
    161166\newcommand{\mygstrut}[2]{\rule[#1 em]{0pt}{#2 em}} 
    162167\newcommand{\mystrut}{\rule[-.9 em]{0pt}{1.79 em}} 
     168 
     169\newcommand{\doi}[1]{\href{http://dx.doi.org/#1}{full-text}} 

  • branches/2017/dev_merge_2017/DOC/tex_main/NEMO_manual.tex

    r9393 r9394  
    140140 
    141141 
     142%% Bibliography 
     143 
     144\cleardoublepage 
     145\phantomsection 
     146\addcontentsline{toc}{chapter}{Bibliography} 
     147\bibliography{../tex_main/NEMO_manual} 
     148 
     149 
    142150%% Index 
    143151 
     152\cleardoublepage 
     153\phantomsection 
    144154\addcontentsline{toc}{chapter}{Index} 
    145155\printindex 
    146156 
    147157 
    148 %% Bibliography 
    149  
    150 \addcontentsline{toc}{chapter}{Bibliography} 
    151 \bibliography{../tex_main/NEMO_manual} 
    152  
    153  
    154158\end{document} 
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