**Table 2:** Mars ephemerides for the observations (from JPL Horizon server at http://ssd.jpl.nasa.gov/).
Date UT	Equatorial	Geocentric	Phase	Sub-Earth point		Sub-Solar point		Ls¹
	diameter	distance	angle	long.	lat.	long.	lat.
yyyy/mm/dd.dd	[ $^{\prime \prime }$ ]	[AU]	[ $^\circ$ ]	[ $^\circ$ ]	[ $^\circ$ ]	[ $^\circ$ ]	[ $^\circ$ ]	[ $^\circ$ ]
2003/06/14.604	14.16	0.662	40.700	150.94	-21.15	191.61	-9.74	203.14
2003/06/15.111	14.23	0.658	40.618	328.59	-21.16	9.21	-9.87	203.45
2003/06/16.611	14.44	0.649	40.366	134.25	-21.21	174.73	-10.23	204.35
2003/06/18.396	14.70	0.637	40.047	39.71	-21.25	79.99	-10.65	205.42
2003/11/02.056	14.78	0.633	38.240	105.10	-23.70	63.26	-23.69	290.84
2003/11/03.167	14.61	0.641	38.483	134.51	-23.82	92.40	-23.57	291.51
2003/11/05.611	14.24	0.658	38.984	271.16	-24.08	228.51	-23.31	293.00
2003/11/06.313	14.14	0.663	39.120	156.96	-24.15	114.16	-23.23	293.43
2003/11/08.222	13.86	0.676	39.471	106.17	-24.35	63.00	-23.01	294.59
2003/11/09.382	13.69	0.684	39.671	152.56	-24.46	109.18	-22.88	295.29

¹ Solar longitude from the vernal point of Mars (e.g. Ls = 0 $^\circ$ for the spring equinox of northern
hemisphere and Ls = 180 $^\circ$ for the beginning of spring in the southern hemisphere).

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations
	3 Data reduction
	4 Modelling of Martian atmospheric lines and results
	5 Discussion and conclusions
	References