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- W2023643823 abstract "view Abstract Citations (57) References (27) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Rebound Shock Model for Solar Spicules: Dynamics at Long Times Sterling, Alphonse C. ; Hollweg, Joseph V. Abstract The spicule model due to Hollweg is extended and developed. The dynamics is emphasized here; radiative and ionization losses, heat conduction, and nonshock heat input, are not included. In the model, a series of rebound shocks results in chromospheric material with spicule-like properties below a raised transition region. The shocks result from a single quasi-impulsive source in the photosphere. It is found that at long times, the model approaches a new hydrostatic equilibrium with the transition region remaining raised, and with a region of shock-heated chromosphere below it. Attention is given to the variation of the properties of the model in response to different values for the magnitude and location of the source, and to different initial transition region heights. It is concluded that the model is capable of generating structures with properties consistent with observations of spicules (with the exception of temperature) when only the dynamics is considered. Publication: The Astrophysical Journal Pub Date: April 1988 DOI: 10.1086/166252 Bibcode: 1988ApJ...327..950S Keywords: Magnetohydrodynamic Waves; Shock Waves; Solar Atmosphere; Spicules; Stellar Models; Chromosphere; Long Term Effects; Magnetohydrodynamic Stability; Solar Physics; HYDRODYNAMICS; SHOCK WAVES; SUN: ATMOSPHERE; SUN: TRANSITION REGION full text sources ADS |" @default.
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- W2023643823 title "The rebound shock model for solar spicules - Dynamics at long times" @default.
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