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A [[Plasma Field Storm]] is a spontaneous storm in which subspace particles manage to excite plasmatic particles into a high-energy state. This phenomenon is little understood, although it is clear that the level of excitation can vary significantly, even within a single storm front event. | A [[Plasma Field Storm]] is a spontaneous storm in which subspace particles manage to excite plasmatic particles into a high-energy state. This phenomenon is little understood, although it is clear that the level of excitation can vary significantly, even within a single storm front event. | ||
These storms seem to be unique to [[Sector 6309]] although there have been other unsubstantiated reports of such storms spawning in other regions beyond | These storms seem to be unique to [[Sector 6309]] although there have been other unsubstantiated reports of such storms spawning in other regions beyond Federation Space. In 2414, the [[USS Rosenante]] encountered one such spontaneous spawning of a Plasma Field Storm. The storm measured over 20-[[Light Year]]s long and 10-[[Light Year]]s thick. The storm front progressed rapidly at a speed exceeding Warp 9.98 | ||
The impact with the storm dealt significant damage to the ship which was forced to seek a safe port for repairs. After relaying the data to [[Starfleet Command]], the Rosenante was directed to the planets [[Kozan-Kozana|Kozan and Kozana]]. Β | The impact with the storm dealt significant damage to the ship which was forced to seek a safe port for repairs. After relaying the data to [[Starfleet Command]], the Rosenante was directed to the planets [[Kozan-Kozana|Kozan and Kozana]]. Β | ||
