|

In Star Trek, a magnetic storm is a spatial phenomenon
that posed a navigational hazard in the early days of space travel. At
that time, the impulse engines were not powerful enough to resist the
effects of such storms, and a ship encountering one could be swept off
course. Around 2065, an encounter with a magnetic storm swept the SS
Valiant into the galactic barrier initiating a series of events that
led to her destruction. (TOS: "Where No Man Has Gone Before")
Magnetic storms can also occur on the surface of some
planets. On Rigel XII, they are accompanied by or cause extremely
powerful sandstorms. Such a storm nearly claimed the life of Eve
McHuron in 2266; only lithium miner Ben Childress' determined search
located her. (TOS: "Mudd's Women")
In 2267, the USS Enterprise encountered a magnetic storm
at the Halkan homeworld, while James Kirk and his landing party were on
the surface conducting negotiations. The storm was reported by Spock to
be a "standard ion type, but quite violent and unpredictable." During
the beam up to the ship, interference caused by transporting through a
magnetic storm caused the crew to transport to an alternate mirror
universe. (TOS: "Mirror, Mirror")
While attempting to extract their personnel from the
Mokra homeworld in 2372, the USS Voyager hid within a large magnetic
storm over the planet's northern magnetic pole to avoid the Mokra's
phased ion cannons. (VOY: "Resistance"). In 2373, the shuttlecraft
Sacajawea crashed due to a magnetic storm, while attempting to collect
nitrogenase compound. Captain Kathryn Janeway was severely injured.
(VOY: "Coda").
Such magnetic storms appear to be similar to the
real-life phenomena of geomagnetic storms. A geomagnetic storm is a
temporary disturbance of the Earth's magnetosphere caused by a
disturbance in space weather. Associated with solar coronal mass
ejections (CME), coronal holes, or solar flares, a geomagnetic storm is
caused by a solar wind shock wave which typically strikes the Earth's
magnetic field 24 to 36 hours after the event. This only happens if the
shock wave travels in a direction toward Earth. The solar wind pressure
on the magnetosphere will increase or decrease depending on the Sun's
activity. These solar wind pressure changes modify the electric
currents in the ionosphere. Solar wind also carries with it the
magnetic field of the Sun. This field will have either a North or South
orientation. If the solar wind has energetic bursts, contracting and
expanding the magnetosphere, or if the solar wind takes a southward
polarization, geomagnetic storms can be expected. The southward field
causes magnetic reconnection of the dayside magnetopause, rapidly
injecting magnetic and particle energy into the Earth's magnetosphere.
Magnetic storms usually last 24 to 48 hours, but some may last for many
days.
The largest recorded geomagnetic storm occurred in 1859,
when telegraph wires in both the United States and Europe shorted out,
some even causing fires. Auroras were seen as far south as Hawaii,
Mexico, Cuba, and Italy—phenomena that are usually only seen near the
poles. On 13 March 1989 a severe geomagnetic storm caused the collapse
of the Hydro-Québec power grid in a matter of seconds as
equipment protection relays tripped in a cascading sequence of events.
Six million people were left without power for nine hours, with
significant economic loss. The storm even caused auroras as far south
as Texas. In August that same year, another storm affected
microcomputer chips, leading to a halt of all trading on Toronto's
stock market.
Intense solar flares release very-high-energy particles
that can be as injurious to humans as the low-energy radiation from
nuclear blasts. Earth's atmosphere and magnetosphere allow adequate
protection at ground level, but astronauts in space elevated radiation
and aircraft flying at high altitudes are subject to potentially lethal
doses of radiation. The penetration of high-energy particles into
living cells can cause chromosome damage, cancer, and a host of other
health problems. Ionospheric storms can affect radio communication,
navigation systems, satellites and electric power networks.
|
|