provide calculation of parameters of normal
(undisturbed) geomagnetic field in real-time mode
for any point on the Earth’s surface.
The obvious way to solve the problem is to
implement innovative information technologies
there. In particular the most expectations are about
using geoinformation systems to solve the problem.
In this paper the authors suggest an approach to
study, monitoring, analyze and visualize
geomagnetic field, its variations and anomalies,
which is based on modern Web and geoinformation
technologies.
2 GEOMAGNETIC FIELD AND
ITS VARIATIONS
The first question to be discussed is what
geomagnetic field is and why is it important to study
this subject? According to the modern science, the
Earth’s outer core is liquid and mainly iron. Its
chemical elements (such as iron and nickel)
respectively make ~85.5 % and ~5.2 % of Earth’s
core mass fraction, i.e. totally more than 90 %.
Permanent rotations of the Earth and its core cause
the constant flows inside of the core and
corresponding electric currents. According to the
laws of magnetic hydrodynamics, these flows and
currents provide the existence of geomagnetic field
(Campbell, 2003).
Geomagnetic field is a complex structured
natural matter with ambiguous field characteristics,
which is distributed in the Earth (and near-Earth)
space and interacts with both astronomical objects
and terrestrial objects / processes on the Earth’s
surface, subsoil and in near-Earth space (Mandea,
2011)(Merrill, 1996).
Because of the permanent interaction with the
magnetic fields, which are generated by the Sun, the
planets of the Solar system and other celestial bodies
and systems, the Earth’s magnetic field can be
significantly deformed. Herewith geomagnetic field
becomes some kind of protective shield, which
prevents a penetration of the Solar wind to the
geospace (the Solar wind is a flow of ionized
particles, which radially spreads from the solar
corona to the outer space). The Solar wind interacts
with this barrier, flows around the Earth and creates
a special region with the geomagnetic field inside,
which is known as the Earth’s magnetosphere with
its typical teardrop shape.
Geomagnetic variations are declinations of
observed amplitude parameters of the Earth’s
magnetosphere from the calculated values, which are
defined as a normal (or undisturbed) state of
geomagnetosphere. The events and processes, which
cause geomagnetic variations, have various and
independent origin. Besides, all local and global
deformations of geomagnetosphere significantly
differ by both their amplitude-frequency and
probabilistic estimations and characteristics. As a
result the actual picture of geomagnetic field is a
complicated superposition of probabilistic set of
geomagnetic variations, which are caused by the
number of uncoordinated events. That’s why their
estimation by traditional physical quantities
(magnetic field intensity, frequency, magnetic
induction, etc.) is useful.
Today the specialists in many scientific and
applied spheres (such as biology, medicine,
geophysics, geology, technics, sociology,
psychology and many others) consider parameters of
geomagnetic field and its variations as one of the
key factors, which can influence on systems and
objects of various origins. They pay great attention
to correlations between external geomagnetic
variations and existence and evolution of various
objects and systems.
This interest is based on idea that some
components of geomagnetic variations or their
combinations can influence on biological, technical,
geological and other objects and systems in common
and on human in particular. As a result, distorted
normal conditions of existence force these objects
and systems to either adapt to changes of magnetic
state (via deformation, mutation, etc.) or keep
existing there in stressed (or unstable) mode
(Vorobev and Shakirova, 2015).
The full vector of the Earth’s magnetic field
intensity in any geographical point with
spatiotemporal coordinates is defined as follows:
B
ge
= B
1
+ B
2
+ B
3
,
where B
1
is an intensity vector of GMF of
intraterrestrial sources; B
2
is a regular component of
intensity vector of geomagnetic field of
magnetosphere currents, which is calculated in solar-
magnetosphere coordinate system; B
3
is a
geomagnetic field intensity vector component with
technogenic origin.
The normal (or undisturbed) geomagnetic field is
supposed as a value of B
1
vector with excluding a
component, which is caused by magnetic properties
of rocks (including magnetic anomalies). So, this
component can be excluded as a geomagnetic
variation: