# Source code for pygmt.src.project

```
"""
project - Project data onto lines or great circles, or generate tracks.
"""
import pandas as pd
from pygmt.clib import Session
from pygmt.exceptions import GMTInvalidInput
from pygmt.helpers import (
GMTTempFile,
build_arg_string,
fmt_docstring,
kwargs_to_strings,
use_alias,
)
[docs]@fmt_docstring
@use_alias(
A="azimuth",
C="center",
E="endpoint",
F="convention",
G="generate",
L="length",
N="flat_earth",
Q="unit",
S="sort",
T="pole",
V="verbose",
W="width",
Z="ellipse",
f="coltypes",
)
@kwargs_to_strings(E="sequence", L="sequence", T="sequence", W="sequence", C="sequence")
def project(data=None, x=None, y=None, z=None, outfile=None, **kwargs):
r"""
Project data onto lines or great circles, or generate tracks.
Project reads arbitrary :math:`(x, y [, z])` data and returns any
combination of :math:`(x, y, z, p, q, r, s)`, where :math:`(p, q)` are the
coordinates in the projection, :math:`(r, s)` is the position in the
:math:`(x, y)` coordinate system of the point on the profile (:math:`q = 0`
path) closest to :math:`(x, y)`, and :math:`z` is all remaining columns in
the input (beyond the required :math:`x` and :math:`y` columns).
Alternatively, ``project`` may be used to generate
:math:`(r, s, p)` triplets at equal increments along a profile using the
``generate`` parameter. In this case, the value of ``data`` is ignored
(you can use, e.g., ``data=None``).
Projections are defined in any (but only) one of three ways:
1. By a ``center`` and an ``azimuth`` in degrees clockwise from North.
2. By a ``center`` and ``endpoint`` of the projection path.
3. By a ``center`` and a ``pole`` position.
To spherically project data along a great circle path, an oblique
coordinate system is created which has its equator along that path, and the
zero meridian through the Center. Then the oblique longitude (:math:`p`)
corresponds to the distance from the Center along the great circle, and the
oblique latitude (:math:`q`) corresponds to the distance perpendicular to
the great circle path. When moving in the increasing (:math:`p`) direction,
(toward B or in the azimuth direction), the positive (:math:`q`) direction
is to your left. If a Pole has been specified, then the positive
(:math:`q`) direction is toward the pole.
To specify an oblique projection, use the ``pole`` parameter to set
the pole. Then the equator of the projection is already determined and the
``center`` parameter is used to locate the :math:`p = 0` meridian. The
center *cx/cy* will be taken as a point through which the :math:`p = 0`
meridian passes. If you do not care to choose a particular point, use the
South pole (*cx* = 0, *cy* = -90).
Data can be selectively windowed by using the ``length`` and ``width``
parameters. If ``width`` is used, the projection width is set to use only
data with :math:`w_{{min}} < q < w_{{max}}`. If ``length`` is set, then
the length is set to use only those data with
:math:`l_{{min}} < p < l_{{max}}`. If the ``endpoint`` parameter
has been used to define the projection, then ``length="w"`` may be used to
window the length of the projection to exactly the span from O to B.
Flat Earth (Cartesian) coordinate transformations can also be made. Set
``flat_earth=True`` and remember that azimuth is clockwise from North (the
y axis), NOT the usual cartesian theta, which is counterclockwise from the
x axis. azimuth = 90 - theta.
No assumptions are made regarding the units for
:math:`x, y, r, s, p, q, dist, l_{{min}}, l_{{max}}, w_{{min}}, w_{{max}}`.
If ``unit`` is selected, map units are assumed and :math:`x, y, r, s` must
be in degrees and
:math:`p, q, dist, l_{{min}}, l_{{max}}, w_{{min}}, w_{{max}}`
will be in km.
Calculations of specific great-circle and geodesic distances or for
back-azimuths or azimuths are better done using :gmt-docs:`mapproject` as
project is strictly spherical.
Full option list at :gmt-docs:`project.html`
{aliases}
Parameters
----------
data : str or {table-like}
Pass in (x, y, z) or (longitude, latitude, elevation) values by
providing a file name to an ASCII data table, a 2-D
{table-classes}.
center : str or list
*cx*/*cy*.
Set the origin of the projection, in Definition 1 or 2. If
Definition 3 is used, then *cx/cy* are the coordinates of a
point through which the oblique zero meridian (:math:`p = 0`) should
pass. The *cx/cy* is not required to be 90 degrees from the pole.
azimuth : float or str
Define the azimuth of the projection (Definition 1).
endpoint : str or list
*bx*/*by*.
Define the end point of the projection path (Definition 2).
convention : str
Specify the desired output using any combination of **xyzpqrs**, in
any order [Default is **xypqrsz**]. Do not space between the letters.
Use lower case. The output will be columns of values corresponding to
your ``convention``. The **z** flag is special and refers to all
numerical columns beyond the leading **x** and **y** in your input
record. The **z** flag also includes any trailing text (which is
placed at the end of the record regardless of the order of **z** in
``convention``). **Note**: If ``generate`` is True, then the output
order is hardwired to be **rsp** and ``convention`` is not allowed.
generate : str
*dist* [/*colat*][**+c**\|\ **h**].
Create :math:`(r, s, p)` output data every *dist* units of :math:`p`
(See ``unit`` parameter). Alternatively, append */colat* for a small
circle instead [Default is a colatitude of 90, i.e., a great circle].
If setting a pole with ``pole`` and you want the small circle to go
through *cx*/*cy*, append **+c** to compute the required colatitude.
Use ``center`` and ``endpoint`` to generate a circle that goes
through the center and end point. Note, in this case the center and
end point cannot be farther apart than :math:`2|\mbox{{colat}}|`.
Finally, if you append **+h** then we will report the position of
the pole as part of the segment header [Default is no header].
**Note**: No input is read and the value of ``data``, ``x``, ``y``,
and ``z`` is ignored if ``generate`` is used.
length : str or list
[**w**\|\ *l_min*/*l_max*].
Project only those data whose *p* coordinate is
within :math:`l_{{min}} < p < l_{{max}}`. If ``endpoint`` has been set,
then you may alternatively use **w** to stay within the distance from
``center`` to ``endpoint``.
flat_earth : bool
Make a Cartesian coordinate transformation in the plane.
[Default is ``False``; plane created with spherical trigonometry.]
unit : bool
Set units for :math:`x, y, r, s` to degrees and
:math:`p, q, dist, l_{{min}}, l_{{max}}, w_{{min}}, w_{{max}}` to km.
[Default is ``False``; all arguments use the same units]
sort : bool
Sort the output into increasing :math:`p` order. Useful when projecting
random data into a sequential profile.
pole : str or list
*px*/*py*.
Set the position of the rotation pole of the projection.
(Definition 3).
{verbose}
width : str or list
*w_min*/*w_max*.
Project only those data whose :math:`q` coordinate is
within :math:`w_{{min}} < q < w_{{max}}`.
ellipse : str
*major*/*minor*/*azimuth* [**+e**\|\ **n**].
Used in conjunction with ``center`` (sets its center) and ``generate``
(sets the distance increment) to create the coordinates of an ellipse
with *major* and *minor* axes given in km (unless ``flat_earth`` is
given for a Cartesian ellipse) and the *azimuth* of the major axis in
degrees. Append **+e** to adjust the increment set via ``generate`` so
that the the ellipse has equal distance increments [Default uses the
given increment and closes the ellipse]. Instead, append **+n** to set
a specific number of unique equidistant data via ``generate``. For
degenerate ellipses you can just supply a single *diameter* instead. A
geographic diameter may be specified in any desired unit other than km
by appending the unit (e.g., 3-D for degrees) [Default is km];
the increment is assumed to be in the same unit. **Note**:
For the Cartesian ellipse (which requires ``flat_earth``), the
*direction* is counter-clockwise from the horizontal instead of an
*azimuth*.
outfile : str
The file name for the output ASCII file.
{coltypes}
Returns
-------
track: pandas.DataFrame or None
Return type depends on whether the ``outfile`` parameter is set:
- :class:`pandas.DataFrame` table with (x, y, ..., newcolname) if
``outfile`` is not set
- None if ``outfile`` is set (output will be stored in file set
by ``outfile``)
"""
if kwargs.get("C") is None:
raise GMTInvalidInput("The `center` parameter must be specified.")
if kwargs.get("G") is None and data is None:
raise GMTInvalidInput(
"The `data` parameter must be specified unless `generate` is used."
)
if kwargs.get("G") is not None and kwargs.get("F") is not None:
raise GMTInvalidInput(
"The `convention` parameter is not allowed with `generate`."
)
with GMTTempFile(suffix=".csv") as tmpfile:
if outfile is None: # Output to tmpfile if outfile is not set
outfile = tmpfile.name
with Session() as lib:
if kwargs.get("G") is None:
# Choose how data will be passed into the module
table_context = lib.virtualfile_from_data(
check_kind="vector", data=data, x=x, y=y, z=z, required_z=False
)
# Run project on the temporary (csv) data table
with table_context as infile:
arg_str = build_arg_string(kwargs, infile=infile, outfile=outfile)
else:
arg_str = build_arg_string(kwargs, outfile=outfile)
lib.call_module(module="project", args=arg_str)
# if user did not set outfile, return pd.DataFrame
if outfile == tmpfile.name:
if kwargs.get("G") is not None:
column_names = list("rsp")
result = pd.read_csv(tmpfile.name, sep="\t", names=column_names)
else:
result = pd.read_csv(tmpfile.name, sep="\t", header=None, comment=">")
# return None if outfile set, output in outfile
elif outfile != tmpfile.name:
result = None
return result
```