Contribution to the modeling of solar spicules |
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| Authors: | E Tavabi S Koutchmy A Ajabshirizadeh |
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| Institution: | 1. Payame Noor University (PNU), 45138-69987 Zanjan, Iran;2. Research Institute for Astronomy & Astrophysics of Maragha (RIAAM), 55134-441 Maraghe, Iran;3. Institut d’Astrophysique de Paris, UMR 7095, CNRS & UPMC, 98 Bis Bd Arago, F-75014 Paris, France;4. Department of Theoretical Physics and Astrophysics, Tabriz University, 51664 Tabriz, Iran |
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| Abstract: | Solar limb and disk spicule quasi-periodic motions have been reported for a long time, strongly suggesting that they are oscillating. In order to clear up the origin and possibly explain some solar limb and disk spicule quasi-periodic recurrences produced by overlapping effects, we present a simulation model assuming quasi-random positions of spicules. We also allow a set number of spicules with different physical properties (such as: height, lifetime and tilt angle as shown by an individual spicule) occurring randomly. |
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| Keywords: | Chromosphere Spicules Oscillations Wavelet analysis Simulation |
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