**Table 1:** Results of calculations.
Model	$\Delta {\it SW}^{a}$	$\Delta$ TS (upwind)^b	$\Delta$ TS (downwind)	$\Delta$ HP (upwind)	$R(BS)_{\rm time} -R(BS)_{\rm stationary}^c$
This paper	2	14 AU	25 AU	4 AU	3 AU
Zank & Muller (2003)	2	7 AU	50 AU	6 AU	n/a
Scherer & Fahr (2003)	2.67^d	$\sim$ 16 AU	n/a^e	n/a	>15 AU

^a $\Delta {\it SW}$ notes the ratio of maximum to minimum the solar wind dynamic pressure.
^b $\Delta = R_{\max} - R_{\min}$ is the difference between maximum and minimum distances of the TS, HP and BS during the solar cycle.
^c $R(BS)_{\rm time} -R(BS)_{\rm stationary}$ is the difference between mean location of the BS during the time-dependent calculations and the stationary solution.
^d Model "Sin 800'' in Fig. 4a in Scherer & Fahr (2003b).
^e n/a means that we were unable to find the corresponding value from the results presented in the cited paper.

Source LaTeX | All tables | In the text

	1 Introduction
	2 Model
	3 Results
	4 Summary
	References
	Online Material
	Appendix A