Synthetic EUV intensity variations from leaking fast sausage modes track the true wave damping only when the loop temperature is near the emission line's formation temperature, so observers should check temperature matching before deriving damping times.
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Synthetic Extreme-ultraviolet Emissions Modulated by Leaky Fast Sausage Modes in Solar Active Region Loops
Synthetic EUV intensity variations from leaking fast sausage modes track the true wave damping only when the loop temperature is near the emission line's formation temperature, so observers should check temperature matching before deriving damping times.