
Geomagnetic Storm ( Solar Storm )

Images Credits : today.in-24.com
A geomagnetic storm (commonly referred to as a solar 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.
Geomagnetic storm is a major disturbance of Earth's magnetosphere that occurs when there is a very efficient exchange of energy from the solar wind into the space environment surrounding the Earth. The disturbance that drives the magnetic storm may be a solar coronal mass ejection (CME) or a co-rotating interaction region (CIR), a high speed stream of solar wind originating from a coronal hole.
There're 3 phases of geomagnetic storms : initial , main and recovery. The initial phase referred to storm sudden commencement (SSC). The main phase is defined by Dst (disturbance-storm time) decreasing to less than -50nT. the selection of -5OnT define that the storm is somewhat arbitrary. The recovery phase is when Dst changes from its minimum value to its quiet time value and it may last as short as 8 hours or as long as 7days.
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The Size of a geomagnetic storm is classified as:
~ MODERATE : ( -50nT > minimum of Dst > -100nT )
~ INTENSE : ( -100nT > minimum Dst > -250nT )
~ SUPER-STORM : ( minimum of Dst < -250nT )

Technological and infrastructure affected by space weather event
Credits : NASA
Geomagnetic Storm Effects
Disruption of Electrical Systems
It would cause damage to satellites, power grids and radio communications, and could cause electrical blackouts on a massive scale that might not be repaired for weeks, months, or even years
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Mains Electricity Grid
When magnetic fields move about in the vicinity of a conductor such as a wire, a geomagnetically induced current is produced in the conductor. This happens on a grand scale during geomagnetic storms (the same mechanism also influenced telephone and telegraph lines before fiber optics, see above) on all long transmission lines. These country like China, North America and Australia especially their operators in modern high-voltage, low-resistance lines might be subject to damage by this effect. The European grid consists mainly of shorter transmission circuits, which are less vulnerable to damage. The (nearly direct) currents induced in these lines from geomagnetic storms are harmful to electrical transmission equipment, especially transformers—inducing core saturation, constraining their performance (as well as tripping various safety devices), and causing coils and cores to heat up. In extreme cases, this heat can disable or destroy them, even inducing a chain reaction that can overload transformers. For instance, internet service providers may go down during geomagnetic storms (and remain non-operational long after).
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Communications
High frequency (3–30 MHz) communication systems use the ionosphere to reflect radio signals over long distances. Ionospheric storms can affect radio communication at all latitudes. Some frequencies are absorbed and others are reflected, leading to rapidly fluctuating signals and unexpected propagation paths. TV and commercial radio stations are little affected by solar activity, but ground to air, ship to shore, shortwave broadcast and amateur radio (mostly the bands below 30 MHz) are frequently disrupted. Military detection or early warning systems operating in the high frequency range are also affected by solar activity. The over-the-horizon radar bounces signals off the ionosphere to monitor the launch of aircraft and missiles from long distances. During geomagnetic storms, this system can be severely hampered by radio clutter. Also some submarine detection systems use the magnetic signatures of submarines as one input to their locating schemes. Geomagnetic storms can mask and distort these signals.
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Navigation systems
The Global Navigation Satellite System (GNSS), and other navigation systems are adversely affected when solar activity disrupts their signal propagation. Airplanes and ships used the very low frequency signals from these transmitters to determine their positions. During solar events and geomagnetic storms, the system gave navigators information that was inaccurate by as much as several miles. If navigators had been alerted that a proton event or geomagnetic storm was in progress, they could have switched to a backup system.
GNSS signals are affected when solar activity causes sudden variations in the density of the ionosphere, causing the satellite signals to scintillate
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Satellite Hardware Damage
Geomagnetic storms and increased solar ultraviolet emission heat Earth's upper atmosphere, causing it to expand. The heated air rises, and the density at the orbit of satellites up to about 1,000 km (621 mi) increases significantly. This results in increased drag, causing satellites to slow and change orbit slightly. Low Earth Orbit satellites that are not repeatedly boosted to higher orbits slowly fall and eventually burn up. Another problem for satellite operators is differential charging. During geomagnetic storms, the number and energy of electrons and ions increase. When a satellite travels through this energized environment, the charged particles striking the spacecraft differentially charge portions of the spacecraft. Discharges can arc across spacecraft components, harming and possibly disabling them.
This discharge is potentially hazardous to the satellite's electronic systems.
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Pipelines
Rapidly fluctuating geomagnetic fields can produce geomagnetically induced currents in pipelines. This can cause multiple problems for pipeline engineers. Pipeline flow meters can transmit erroneous flow information and the corrosion rate of the pipeline can be dramatically increased.
Radiation hazards to humans
Earth's atmosphere and magnetosphere allow adequate protection at ground level, but astronauts are subject to potentially lethal radiation poisoning. The penetration of high-energy particles into living cells can cause chromosome damage, cancer and other health problems. Large doses can be immediately fatal. Solar protons with energies greater than 30 MeV are particularly hazardous.
Solar proton events can also produce elevated radiation aboard aircraft flying at high altitudes. Although these risks are small, flight crews may be exposed repeatedly, and monitoring of solar proton events by satellite instrumentation allows exposure to be monitored and evaluated.
Effect on animals
Scientists are still studying whether or not animals are affected, some suggesting solar storms induce whales to beach themselves. Some have speculated that migrating animals which use magnetoreception to navigate, such as birds and honey bees, might also be affected.
