Geoscience Reference
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Fig. 9. Time evolution of the signal in the Ecliptic plane during 2004 (left) and 2005
(right). Each column represent average count rates (1/s) during 1 day. The
x
-axes are
day of year, and the
y
-axes are ecliptic longitudes. Only observations by sectors look-
ingatmost6
◦
off the ecliptic plane were included. For 2004 we included all umbra
observations. The dark lines represent Earth's longitude, and the light lines the Sun's
longitude.
Fig. 10. Time evolution of the signal in the Galactic plane during 2005. Identical format
as in Fig. 9 but for the Galactic plane, and with Galactic longitude and latitude. To the
right, all observations in the hemisphere of directions centered at Mars were removed.
