2020
DOI: 10.1051/swsc/2020062
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Semi-annual, annual and Universal Time variations in the magnetosphere and in geomagnetic activity: 3. Modelling

Abstract: This is the third in a series of papers that investigate the semi-annual, annual and Universal Time variations in the magnetosphere.  In this paper we use the Lin et al. (2010) empirical model of magnetopause locations, along with the assumption of pressure equilibrium and the Newtonian approximation of magnetosheath pressure.  We show that the equinoctial pattern arises in both the cross-tail current at the tail hinge point and in the total energy stored in the tail. The model allows us to study the effects… Show more

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Cited by 20 publications
(47 citation statements)
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“…(2020), Lockwood, Owens, et al. (2020), and Lockwood et al. (2021) as being the effect of p SW in squeezing the near‐Earth tail.…”
Section: Resultsmentioning
confidence: 99%
See 2 more Smart Citations
“…(2020), Lockwood, Owens, et al. (2020), and Lockwood et al. (2021) as being the effect of p SW in squeezing the near‐Earth tail.…”
Section: Resultsmentioning
confidence: 99%
“…The modeling analysis of Lockwood, Owens, et al. (2020) found the influence of p SW through both Φ N and the energy stored in the tail lobe. The results presented here show an effect of p SW on Φ PC , but that the effect is smaller than for am : this indicates that the effect of energy stored in the tail may be a larger factor for midlatitude range indices such as am .…”
Section: Discussionmentioning
confidence: 99%
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“…The factor P w (w) was modelled in Paper 3 (Lockwood et al, 2020c) using the asymmetric magnetopause location model of Lin et al (2010) by assuming that the tail is in equilibrium with a solar wind of dynamic pressure p SW . These authors modelled the magnetic shear DB across the cross tail current sheet for various values of the geoeffective southward component of the IMF [B Z ] GSM , and the solar wind dynamic pressure, p SW that are the inputs to the magnetopause model.…”
Section: 3mentioning
confidence: 99%
“…In some cases, after a maximum near local midnight, a decline in airglow brightness was followed by a substantial brightening several hours later. Insufficient data prevented us from determining if these features were the result of atmospheric airglow waves15 , energy being released from Earth's magnetospheric tail 16,17,18 , or an unknown physical process. Bottom Panel: The night airglow above the quiescent level, ΔMC-N(t) MC(t), for each site is plotted versus Julian Date (JD).…”
Section: Article (Continued)mentioning
confidence: 99%