K-index
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The ''K''-index quantifies disturbances in the horizontal component of
earth's magnetic field Earth's magnetic field, also known as the geomagnetic field, is the magnetic field that extends from Earth's interior out into space, where it interacts with the solar wind, a stream of charged particles emanating from the Sun. The magneti ...
with an
integer An integer is the number zero (), a positive natural number (, , , etc.) or a negative integer with a minus sign ( −1, −2, −3, etc.). The negative numbers are the additive inverses of the corresponding positive numbers. In the languag ...
in the range 0–9 with 1 being calm and 5 or more indicating a
geomagnetic storm A geomagnetic storm, also known as a magnetic storm, is a temporary disturbance of the Earth's magnetosphere caused by a solar wind shock wave and/or cloud of magnetic field that interacts with the Earth's magnetic field. The disturbance that d ...
. It is derived from the maximum fluctuations of horizontal components observed on a
magnetometer A magnetometer is a device that measures magnetic field or magnetic dipole moment. Different types of magnetometers measure the direction, strength, or relative change of a magnetic field at a particular location. A compass is one such device, ...
during a three-hour interval. The label ''K'' comes from the German word ''Kennziffer'' meaning "''characteristic digit''". The ''K''-index was introduced by
Julius Bartels Julius Bartels (17 August 1899, Magdeburg – 6 March 1964) was a German geophysicist and statistician who made notable contributions to the physics of the Sun and Moon; to geomagnetism and meteorology; and to the physics of the ionosphere. He a ...
in 1939.


Calculation of ''K''-index

The ''K''-scale is quasi-logarithmic. The conversion table from maximum fluctuation ''R'' (in units of nano teslas, nT) to ''K''-index, varies from observatory to observatory in such a way that the historical rate of occurrence of certain levels of ''K'' are about the same at all observatories. In practice this means that observatories at higher geomagnetic latitude require higher levels of fluctuation for a given ''K''-index. For example, at
Godhavn Qeqertarsuaq () is a port and town in Qeqertalik municipality, located on the south coast of Disko Island on the west coast of Greenland. Founded in 1773, the town is now home to a campus of the University of Copenhagen known as Arctic Station. ...
, Greenland, a value of ''K'' = 9 is derived with ''R'' = 1500 nT, while in
Honolulu, Hawaii Honolulu (; ) is the capital and largest city of the U.S. state of Hawaii, which is in the Pacific Ocean. It is an unincorporated county seat of the consolidated City and County of Honolulu, situated along the southeast coast of the island ...
, a fluctuation of only 300 nT is recorded as ''K'' = 9. In Kiel, Germany, ''K'' = 9 corresponds to ''R'' = 500 nT or greater. The real-time ''K''-index is determined after the end of prescribed intervals of 3 hours each: 00:00–03:00, 03:00–06:00, ..., 21:00–24:00. The maximum positive and negative deviations during the 3 hour period are added together to determine the total maximum fluctuation. These maximum deviations may occur any time during the 3 hour period.


The ''K''p-index and estimated ''K''p-index

The official planetary ''K''p-index is derived by calculating a weighted average of ''K''-indices from a network of 13 geomagnetic observatories at mid-latitude locations. Since these observatories do not report their data in real-time, various operations centers around the globe estimate the index based on data available from their local network of observatories. The ''K''p-index was introduced by Bartels in 1939.


The relationship between ''K'' and ''A''

The ''A''-index provides a daily average level for geomagnetic activity. Because of the non-linear relationship of the ''K''-scale to magnetometer fluctuations, it is not meaningful to take the average of a set of ''K''-indices. What is done instead is to convert each ''K'' back into a linear scale called the "equivalent three hourly range" ''a''-index (note the lower case "''a''"), according to the following table: The daily ''A''-index is merely the average of eight ''a''-indices. Thus, for example, if the ''K''-indices for the day were 3, 4, 6, 5, 3, 2, 2 and 1, the daily ''A''-index is the average of the equivalent amplitudes: :A = (15 + 27 + 80 + 48 + 15 + 7 + 7 + 4)/8 = 25.375 The ''A''p-index is averaged planetary ''A''-index based on data from a set of specific ''K''p stations.


G-scale

This is a description of the relationship between the NOAA G-scale and ''K''p. The ''K''p-scale is a scientific way to summarize the global level of geomagnetic activity, but it has not always been easy for those affected by the space environment to understand its significance. The NOAA G-scale was designed to correspond, in a straightforward way, to the significance of effects of
geomagnetic storm A geomagnetic storm, also known as a magnetic storm, is a temporary disturbance of the Earth's magnetosphere caused by a solar wind shock wave and/or cloud of magnetic field that interacts with the Earth's magnetic field. The disturbance that d ...
s.


Use in radio propagation studies

The ''K''p-index is used for the study and prediction of ionospheric propagation of
high frequency High frequency (HF) is the ITU designation for the range of radio frequency electromagnetic waves (radio waves) between 3 and 30 megahertz (MHz). It is also known as the decameter band or decameter wave as its wavelengths range from one to ten ...
radio signals. Geomagnetic storms, indicated by a ''K''p = 5 or higher, have no direct effect on propagation. However they disturb the F-layer of the
ionosphere The ionosphere () is the ionized part of the upper atmosphere of Earth, from about to above sea level, a region that includes the thermosphere and parts of the mesosphere and exosphere. The ionosphere is ionized by solar radiation. It plays ...
, especially at middle and high geographical latitudes, causing a so-called ''
ionospheric storm Ionospheric storms are storms which contain varying densities of energised electrons produced from the sun. They are categorised into positive and negative storms, where positive storms have a high density of electrons and negative storms contain a ...
'' which degrades radio propagation. The degradation mainly consists of a reduction of the
maximum usable frequency In radio transmission maximum usable frequency (MUF) is the highest radio frequency that can be used for transmission between two points via reflection from the ionosphere (skywave or "skip" propagation) at a specified time, independent of transm ...
(MUF) by as much as 50%. Sometimes the E-layer may be affected as well. In contrast with
sudden ionospheric disturbance A sudden ionospheric disturbance (SID) is any one of several ionospheric perturbations, resulting from abnormally high ionization/ plasma density in the D region of the ionosphere and caused by a solar flare and/or solar particle event (SPE). The S ...
s (SID), which affect high frequency radio paths mostly at mid and low latitudes, the effects of ionospheric storms are more intense high latitudes and the polar regions.


References


External links

* http://www.swpc.noaa.gov/products/planetary-k-index * https://web.archive.org/web/20061107140346/http://sec.noaa.gov/rt_plots/kp_3d.html * http://www.swpc.noaa.gov/SolarCycle/ * http://www.n3kl.org/sun/noaa.html
Comprehensive radio propagation site
{{USGovernment, url=https://www.swpc.noaa.gov/noaa-scales-explanation Geomagnetism