1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
|
/***********************************************/
/**
* @file magneticField2GriddedData.cpp
*
* @brief Magentic field vector.
**
* @author Torsten Mayer-Guerr
* @date 2019-05-25
*/
/***********************************************/
// Latex documentation
#define DOCSTRING docstring
static const char *docstring = R"(
Computes x, y, z of the magentic field vector.
)";
/***********************************************/
#include "programs/program.h"
#include "files/fileGriddedData.h"
#include "classes/grid/grid.h"
#include "classes/magnetosphere/magnetosphere.h"
#include "misc/miscGriddedData.h"
/***** CLASS ***********************************/
/** @brief Magentic field vector.
* @ingroup programsGroup */
class MagneticField2GriddedData
{
public:
void run(Config &config, Parallel::CommunicatorPtr comm);
};
GROOPS_REGISTER_PROGRAM(MagneticField2GriddedData, PARALLEL, "magentic field vector", Misc, Grid)
/***********************************************/
void MagneticField2GriddedData::run(Config &config, Parallel::CommunicatorPtr comm)
{
try
{
FileName fileNameGrid;
MagnetospherePtr magnetosphere;
GridPtr grid;
Time time;
Bool useLocalFrame;
Double a, f;
readConfig(config, "outputfileGriddedData", fileNameGrid, Config::MUSTSET, "", "x, y, z [Tesla = kg/A/s**2]");
readConfig(config, "magnetosphere", magnetosphere, Config::MUSTSET, "", "");
readConfig(config, "grid", grid, Config::MUSTSET, "", "");
readConfig(config, "time", time, Config::OPTIONAL, STRING_J2000, "");
readConfig(config, "localReferenceFrame", useLocalFrame, Config::OPTIONAL, "0", "local left handed reference frame (north, east, up)");
readConfig(config, "R", a, Config::DEFAULT, STRING_DEFAULT_GRS80_a, "reference radius for ellipsoidal coordinates on output");
readConfig(config, "inverseFlattening", f, Config::DEFAULT, STRING_DEFAULT_GRS80_f, "reference flattening for ellipsoidal coordinates on output, 0: spherical coordinates");
if(isCreateSchema(config)) return;
// compute
// -------
logStatus<<"compute magnetic field"<<Log::endl;
Ellipsoid ellipsoid(a, f);
std::vector<Vector3d> points = grid->points();
std::vector<Double> areas = grid->areas();
std::vector<Vector3d> values(points.size());
Parallel::forEach(values, [&](UInt i) {return magnetosphere->magenticFieldVector(time, points.at(i));}, comm);
if(Parallel::isMaster(comm))
{
// convert
std::vector<std::vector<Double>> field(3, std::vector<Double>(points.size()));
for(UInt i=0; i<points.size(); i++)
{
if(useLocalFrame)
values.at(i) = localNorthEastUp(points.at(i), ellipsoid).inverseTransform(values.at(i));
field.at(0).at(i) = values.at(i).x();
field.at(1).at(i) = values.at(i).y();
field.at(2).at(i) = values.at(i).z();
}
// write
logStatus<<"save values to file <"<<fileNameGrid<<">"<<Log::endl;
GriddedData griddedData(ellipsoid, points, areas, field);
writeFileGriddedData(fileNameGrid, griddedData);
MiscGriddedData::printStatistics(griddedData);
}
}
catch(std::exception &e)
{
GROOPS_RETHROW(e)
}
}
/***********************************************/
|
