Geo-Magnetic Indices
}As we
know our Earth is protected by these solar activities by its own magnetic filed
shield. Which guards our planet from activities like solar winds and storms.
Magnetic field is the first , where these solar activities gets into contact
with our Earth’s atmosphere. Thus a deep understanding of the governing laws of
these magnetic fields of Earth and impact on it by solar activities is
required.
Below are the definitions and Real-Time Monitoring of Various Geo-magnetic Indices:-
ØDisturbance
Strom Time : The Dst index
monitors the variations of the globally symmetrical ring current, which
encircles the Earth close to the magnetic equator in the Van Allen (or
radiation) belt of the magnetosphere. The Dst is a
geomagnetic index which monitors the world wide magnetic storm level. It is
constructed by averaging the horizontal component of the geomagnetic field from
mid-latitude and equatorial magnetograms from all over the world.
ØAuroral
Electrojet : These indices describe the disturbance level recorded by auroral zone
magnetometers. Horizontal magnetic component recordings from a set of global
stations are plotted to the same time and amplitude scales relative to their
quiet-time levels and then graphically superposed. The upper and lower
envelopes of this superposition define the AU (amplitude upper) and the AL
(amplitude lower) indices, respectively. The difference between the two
envelopes determines the AE (Auroral Electrojet) index, i.e., AE = AU - AL. AO
is defined as the average value of AU and AL.
}Magnetic
A-Index-The geomagnetic A-Index represents the severity of magnetic
fluctuations occurring at local magnetic observatories. During magnetic storms,
the A-index may reach levels as high as 100. During severe storms, the A-index
may exceed 200. Great "rogue" storms may succeed in producing index
values in excess of 300, although storms associated with indices this high are
very rare indeed.
}Magnetic
K-Index- The geomagnetic K-Index is related to the A-index. K-indices are
scaled by comparing the H and D magnetometer traces (representing the
horizontal and declination magnetic components) to assumed "quiet-day
curves" for H and D. Each UT day is divided into 8 three-hour intervals,
starting at 0000 UT. The planetary 3-hour-range Index Kp is the
mean standardized K-index from 14 geomagnetic observatories between 44 degrees
and 60 degrees northern or southern geomagnetic latitude.
Daily solar-Indices:
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