FLOTSAM: Forward-Lobe Two-Stream Radiance Model

Contact: Robin Hogan <[email protected]>

FLOTSAM is a fast solar radiance model intended to be suitable for
assimilating solar radiances affected by clouds and aerosols into
models. Unlike models based on look-up tables, it can take as input an
arbitrary layering of clouds, aerosols and Rayleigh-scattering clear
sky. It is still under heavy development.

It is coded in C++ using the Adept array and automatic-differentiation
library to compute the Jacobian matrix.  The library presents a C
interface (see include/flotsam.h).  An example driver program is
bin/flotsam.cpp.  Many test scripts are in the test directory.

WARNING: THIS CODE IS UNDER DEVELOPMENT AND MANY OF THE SETTINGS ARE
SUBJECT TO CHANGE.  THIS VERSION HAS HAD ITS SETTINGS ADJUSTED TO BEST
REPRESENT AEROSOLS, ALTHOUGH IT IS KNOWN THAT THE WAY THE PHASE
FUNCTION IS PARAMETERIZED DOES NOT YET WORK WELL ENOUGH FOR SOME
AEROSOL PHASE FUNCTIONS.  THIS WILL BE IMPROVED IN THE NEXT VERSION.


INSTALLATION

Before compiling FLOTSAM you will need to install the Adept library
(version 2+) from http://www.met.reading.ac.uk/clouds/adept, ensuring
that it finds a working BLAS library.

Configure the compilation by running the ./configure script. If you
are using the GNU compiler then it is recommended that you run the
./configure_fast.sh script instead, as it chooses the fastest options
for this compiler.  If you installed Adept in a non-system directory
then you will need to tell configure where it is.  The easiest way to
do this is to call configure_fast.sh with the ADEPT_PREFIX environment
variable set:

ADEPT_PREFIX=/path/to/adept ./configure_fast.sh

This tells configure to look for Adept header files in
/path/to/adept/include and the Adept shared library in
/path/to/adept/lib64.

Then compile with "make".  You can the try the test scripts in the
test directory.

To install you should have called the configure or configure_fast.sh
scripts with --prefix=/path/to/flotsam argument to specify the
location where you want to install it - at this location you will then
find the header file include/flotsam.h, the executable bin/flotsam,
the static library lib64/libflotsam.a and the shared library
lib64/flotsam.so.0.0.0.


TESTING

The test directory contains a number of test scripts described in the
test/README file.  These run the bin/flotsam executable, which call
the algorithm using a fixed phase function at all heights.  Its usage
is:

flotsam [param1=value1] [param2=value2...] file1.cfg [file2.cfg...]

where at least one ascii configuration file (*.cfg) must be provided;
these files contain lists of configuration options and there are a
number of examples in the test directory.  Configuration options can
be overridden on the command line.  The scripts call this executable.
Its output (on standard output) is of the following format:

Line 1: 5 numbers:
1: Number of solar zenith angles simulated
2: Number of instrument zenith angles simulated
3: Number of azimuth angles simulated
4: Number of optical depths simulated
5: "N" = number of values reported for each geometry and optical depth

Subsequent lines: 4+N numbers:
1: Solar zenith angle (degrees)
2: Instrument zenith angle (degrees)
3: Difference in azimuth angle between sun and instrument (degrees)
4: Optical depth of particulates
5: Normalized radiance
6: (if present) Direct contribution to normalized radiance
7: (if present) Lobe contribution to normalized radiance
8: (if present) Diffuse contribution to normalized radiance
9: (if present) Surface contribution to normalized radiance
10:(if present) Two-stream estimate of TOA upwelling normalized flux

The program also reports its settings and timings on standard error.
The algorithm is designed to be run many times with the same geometry
(as would be expected in an iterative retrieval algorithm or data
assimilation system).  Therefore, the timings reported are split into
setup calculations and reflectance calculations (there are usually
many more of the latter).