Coefficient file format
-----------------------
The coefficients used in the model can be found in `pyamps/coefficients/SW_OPER_MIO_SHA_2E_00000000T000000_99999999T999999_0101.txt`.

Below is a description of the coefficient file. This information is not needed to use pyAMPS, but it can be useful if you want to do something more advanced and write new/modify the code.

The coefficient file is a .txt file with fixed width columns. It can be read with the Python pandas library by the following code: 

.. code-block:: python

    >>> coeff_fn = 'SW_OPER_MIO_SHA_2E_00000000T000000_99999999T999999_0101.txt'
    >>> names = ([x for x in open(coeff_fn).readlines() if x.startswith('#')][-1][1:]).strip().split(' ') 
    >>> coeffs = pd.read_table(coeff_fn, skipinitialspace = True, comment = '#', sep = ' ', names = names, index_col = [0, 1])

The first two columns contain the spherical harmonic wave numbers n and m. The other 76 columns are named

| ``tor_c_<param>``
| ``tor_s_<param>``
| ``pol_c_<param>``
| ``pol_s_<param>``

where ``<param>`` refers to the 19 external parameters: ``const``, ``sinca``, ``epsilon_cosca``, ``epsilon_sinca``, ``epsilon_cosca``, ``tilt``, ``tilt_sinca``, ``tilt_cosca``, ``tilt_epsilon``, ``tilt_epsilon_sinca``, ``tilt_epsilon_cosca``, ``tau``, ``tau_sinca``, ``tau_cosca``, ``tilt_tau``, ``tilt_tau_sinca``, ``tilt_tau_cosca``, or ``f107``.

Here, ``const`` refers to a constant term. ``sinca`` and ``cosca`` are *sin(IMF clock angle)* and *cos(IMF clock angle)*, respectively. ``epsilon`` is the Newell coupling function divided by 1000 with inputs in nT and km/s. ``tau`` is the Newell coupling function with *sin* replaced by *cos*. ``f107`` is the F10.7 index in standard units (sfu). ``tilt`` is the dipole tilt angle in degrees. Underscores in this list refer to multiplication, e.g.: ``tilt_tau`` is the dipole tilt angle multiplied by tau. 

The prefix of the column names (apart from ``n`` and ``m``) denote the term in a real expansion of the poloidal and toroidal parts of the ionospheric magnetic field as described in Laundal et al. (2016). ``tor`` and ``pol`` refer to toroidal and poloidal, respectively. ``_c`` and ``_s`` refer to the *cos* and *sin* terms, respectively.

To get the spherical harmonic coefficients for a given set of external parameters, the coefficients should be multiplied by the corresponding external parameter (1 in the case of ``const``), and summed so that four columns remain, one for each ``tor_c``, ``tor_s``, ``pol_c``, and ``pol_s``. 

There are several missing entries: The *(n, 0)* terms for the ``_s`` coefficients are undefined, since *sin(m\*x) = 0* for all *x* if *m = 0*. In addition, the toroidal expansion have more terms (higher spatial resolution) than the poloidal expansion, so that ``pol_c_<param>`` and ``pol_s_<param>`` are missing/undefined for *n > 45*.