A model of a spicule in the solar corona

Heading: 
Astronomy and Astrophysics
1Ladikov-Roev, Yu.P, 1Loginov, AA, 1Maslova, NV, 1Cheremnykh, ОК
1Space Research Institute of the National Academy of Sciences of Ukraine and the State Space Agency of Ukraine, Kyiv, Ukraine
Kosm. nauka tehnol. 2004, 10 ;(5-6):128-130
https://doi.org/10.15407/knit2004.05.128
Publication Language: Russian
Abstract: 
A stationary model of spicule is considered taking into account the real conditions on the boundaries. We found the relationships between the height of eruption and other main parameters, namely, vertical and azimuthal velocity, value of magnetic field, and density. The existence time of a spicule is estimated.
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References: 
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