_BML.dox

1/*! \page BML Bulk Surface Mixed Layer
2
3This bulk surface mixed layer scheme was designed to be used with a
4purely isopycnal model. Following \cite niiler1977, \cite oberhuber1993,
5and Hallberg (\cite muller2003) the TKE budget is used to construct a
6time-evolving homogeneous mixed layer. A buffer layer sits between
7the mixed layer and the interior ocean to mediate between the two.
8
9 The following processes are executed, in the order listed.
10
11\li 1. Undergo convective adjustment into mixed layer.
12\li 2. Apply surface heating and cooling.
13\li 3. Starting from the top, entrain whatever fluid the TKE budget
14 permits. Penetrating shortwave radiation is also applied at
15 this point.
16\li 4. If there is any unentrained fluid that was formerly in the
17 mixed layer, detrain this fluid into the buffer layer. This
18 is equivalent to the mixed layer detraining to the Monin-
19 Obukhov depth.
20\li 5. Divide the fluid in the mixed layer evenly into CS\%nkml pieces.
21\li 6. Split the buffer layer if appropriate.
22
23Layers 1 to nkml are the mixed layer, nkml+1 to nkml+nkbl are the
24buffer layers. The results of this subroutine are mathematically
25identical if there are multiple pieces of the mixed layer with
26the same density or if there is just a single layer. There is no
27stability limit on the time step.
28
29The key parameters for the mixed layer are found in the control structure.
30These include mstar, nstar, nstar2, pen\_SW\_frac, pen\_SW\_scale, and TKE\_decay.
31For the \cite oberhuber1993 and \cite kraus1967 mixed layers, the values of these are:
32
33<table>
34<caption id="table_symbols_bml">Model variables used in the bulk mixed layer</caption>
35<tr><th>Symbol <th>Value in Oberhuber (1993) <th>Value in Kraus-Turner (1967)
36<tr><td>pen\_SW\_frac <td> 0.42 <td> 0.0
37<tr><td>pen\_SW\_scale <td> 15.0 m <td> 0.0 m
38<tr><td>mstar <td> 1.25 <td> 1.25
39<tr><td>nstar <td> 1 <td> 0.4
40<tr><td>TKE\_decay <td> 2.5 <td> 0.0
41<tr><td>conv\_decay <td> 0.5 <td> 0.0
42</table>
43
44TKE\_decay is \f$1/\kappa\f$ in eq. 28 of \cite oberhuber1993, while
45conv\_decay is \f$1/\mu\f$. Conv\_decay has been eliminated in favor of
46the well-calibrated form for the efficiency of penetrating convection
47from \cite wang2003.
48
49*/