Generation and Life Cycle of Solar Spicules
Hamid Saleem, Zain H.Saleem

TL;DR
This paper proposes a detailed physical model describing the formation, acceleration, and decay of solar spicules through a three-stage process involving plasma density structures and temperature gradients in the solar chromosphere and corona.
Contribution
It introduces an analytical two-fluid plasma model with explicit solutions for the spicule life cycle, highlighting the role of thermal forces and temperature gradients in their dynamics.
Findings
Density hump forms in the chromosphere due to temperature gradients.
Upward acceleration exceeds solar gravity in the transition region.
Density structures decelerate and dissipate in the corona.
Abstract
Physical mechanism for the creation of solar spicules is proposed with three stages of their life cycle. It is assumed that at stage-I, the density hump is formed locally in the xy-plane in lower chromosphere in the presence of temperature gradients of electrons and ions along z-axis (the vertical direction). In this region, the density structure of quasi-neutral plasma after taking birth is accelerated in the vertical direction due to the thermal force . The exact time-dependent analytical solution of two fluid plasma equations is presented assuming that density is maximum at the center and decays away from it gradually. The two dimensional (2D) density structure is created as a step function in time at bottom of the chromosphere and consequently the vertical plasma velocity turns out to…
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Taxonomy
TopicsSolar and Space Plasma Dynamics
