Resolution Effect in the Solar Spicules Oscillations

Physics

Scientific paper

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Scientific paper

In order to explain solar limb spicule periodic recurrence, we have adopted a simulation model based on random position of spicule on the Sun limb, we allow a set number of spicules with different physical properties (such as height, lifetime and tilt angle) randomly occur along the Z-axis and after reaching the maximum length falling back to the solar surface.
This simulation has been applied for three different resolutions of frames and then analysis spicule visibility using the wavelet time/frequency method to obtain the exact period for them.
Finally, the simulation results have been compared with observations. This investigation is prompted by observations of chromosphere from the Transition Region and Coronal Explorer (TRACE) at 1600 Ångstrom , Solar Optical Telescope (SOT) on Hinode revealing at Ca II H-line and Sac-Peak H-alpha line.

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