ry
96
uk
ce,
)n.
ain
he
are
on
ng
Its,
of
lys
ng
10t
ılts
De
considered. For this purpose booklets, placards,
calendars, separate photos and brochures should
be used.
The scheme marks out three levels of
cartographic information support. They are
related first of all to the area of coverage and
namely global, regional and local. The first level
includes small-scale mapping, the second -
mapping of separate regions and the third one -
mapping of separate local sites on large scales.
Consequently we relate the creation of globes
and demonstration wall maps to the first level,
and complex mapping and surface modeling - to
the second and third ones. We consider the
scales of 1:2,000,000, 1:500,000, 1:100,000 and
1:25,000 to be the major scales. Mapping on a
scale of 1:2,000,000 provides for the updating
of the already compiled map.
It should be reminded that the updating of this
map in particular was among the tasks of the
surveys planned for the Mars Observer station.
As it is known, its flight has not provided the
expected results, however, it will be possibly
repeated in 1996. Regarding the MARS-96
mission, its information is also supposed to be
used for updating the map on a scale of
1:2,000,000. In addition these data are
considered for regional mapping on scales of
1:500,000 and 1:100,000 and for thematic
mapping as well.
The Atlas of Mars is included at every level. We
consider this publication to consist of three
parts. The first part is the review containing the
general information about the planet and small-
scale maps. The second part should be dedicated
to the information about the regions and the
third one - to separate local sites (both reference
and anomalous).
We have begun to create the Atlas of Mars, Part
I. The maps will be plotted in separate sheets
collected in a portfolio. Numbering of sections
allows adding sheets in a section as far as new
information becomes available. That is of
especial importance for the sections containing
various thematic maps. Preliminary the
following sections will be included in this Part:
479
introduction, geographical maps (surface map,
basic map for thematic mapping and
hypsometric map), geophysical, geochemical,
geological, morphological and climatological
maps, maps of the surface physical properties
and others.
The first Part of the Atlas presents various
thematic information characterizing the planet as
a whole. This data is given in a small-scale map
chosen as a unique basic map to show the entire
planetary surface in a single sheet without
breaks. The scale of 1:40,000,000 has been
specified for the basic map. Choice of this scale
is explained by the aspect that a scale of
1:20,000,000 was used for an analogous basic
map in the prepared for publication "Complex
Atlas of the Moon". Consequently comparison
of certain characteristics becomes easier,
because these maps have the same dimensions.
Additionally the scale chosen is convenient for
the reference desktop usage.
Regarding the projection, the equivalent elliptic-
al Mollweide projection was chosen. Also the
same choice as for the Atlas of the Moon.
In general to present the surface of a celestial
body as a whole in small-scale maps we usually
use classic pseudocylindrical equivalent projec-
tions. The Sanson (sinusoidal) projection and
the Mollweide (elliptical) projection are
concerned first of all. The Sanson projection
preserves length along the mean meridian and
along all parallels. The other meridians of this
projection's normal grid excluding the rectilinear
mean one, are sinusoids. For Mollweide
projection it is typical to preserve length along
the equator. The meridians at +90° from the
mean one are shown by a circle. The other
meridians are presented by ellipses with one
constant semi-axis and the other semi-axes
varying (Gazetteer..., 1988). The latter depends
on the longitude. Both projections are
symmetrical.
The Sanson sinusoidal projection and its
modification (the Ekkert projection) are
convenient for the presentation of the near-
equatorial zones. However, from the +60° lati-
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B4. Vienna 1996