A single localized heating event on a coronal loop can trigger prominence formation when its rate is about 10^4 times steady heating, with condensation occurring once the Field number exceeds unity.
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Conditions for Solar Prominence Formation Triggered by Single Localized Heating
A single localized heating event on a coronal loop can trigger prominence formation when its rate is about 10^4 times steady heating, with condensation occurring once the Field number exceeds unity.