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A module for calculation of the geomagnetic K-Index from horizontal geomagnetic components.

This module uses the Finnish Meteorological Institute (FMI) method, details of which can be found here:

In a nutshell, this module takes horizontal geomagnetic components like this:

... and calculates the K-Index:

Assuming you have 4 days of geomagnetic data in the following format:

Times = array of datetime objects in second bins.

Bx, By, Bz = arrays of geomagnetic data in second bins.

First, convert the Times array into second floats:

>>> Times_float = Time2Float(Times)

Now convert all of the data to minute bins:

>>> minute_time, minute_bx, minute_by, minute_bz = MinuteBin(Times_float, Bx, By, Bz)

To get the K-Index for these 4 days:

>>> k_index, k_time, order = KIndexSuperCalc(minute_time, minute_bx, minute_by, n)

where n is the maximum threshold for a K9 event (dependent on latitude).

NOTE: The first few values in the array k_index are likely to be inaccurate. This is because of the way the K-Index is calculated. It is safest to dismiss the first 8 calculated K-Index values.

To plot the K-Index:

>>> KIndexPlotter(k_index[8:], k_time[8:], m)

where m is the figure number.

To install, type

pip install k_index_calculator

Written by Sean Blake in Trinity College Dublin, 2014-2016

Email: blakese@tcd.ie

GITHUB: https://github.com/TerminusEst

Uses the MIT license.

Assuming you have 4 days of geomagnetic data in the following format:

minute_time = array of datetime objects in minute bins.

minute_bx, minute_by, minute_bz = arrays of geomagnetic data in minute bins.

Step 1

For each 3-hour block in the horizontal geomagnetic components, the max variation is found. This is then compared to the following table to get an initial K-index:

where n is the maximum threshold for a K9 event (this is dependent on geomagnetic latitude). This is calculated using the KIndex function.

Step 2

An estimation for the solar quiet or solar regular curve is calculated. This is calculated using the FMISmooth function, which is dependent on the preliminary K-Index.

Step 3 This solar quiet estimation is smoothed (SrSmooth), and subtracted from both horizontal components (Subtracted). "Bx Component and Sr Curve"

Step 4 Steps 1-2 are repeated twice more with the reduced data to get a second and then final K-Index.

All of these steps can be combined in one call of KIndexSuperCalc. ##Functions List

KIndexSuperCalc

• Calculates the K-index using the FMI method.

KIndexPlotter

• Plots K-Index values in a nice Bar Plot

Time2Float

• Converts datetime object or array of datetime objects to floats.

Float2Time

• Converts float or array of floats to datetime objects.

MinuteBin

• Bin second data into minutes.

KIndex

• Calculate K-Index according to the FMI Method.

FMISmooth

• Calculates the Solar Regular (Sr) curve according to the FMI Method.

SrSmooth

• Smooths the solar regular curves.

Subtracted

• Subtracts the smoothed solar regular curves from the minute binned data.

KIndexBarColor -Colours K-index bar plot so it looks nice.