• Considering a single observer for a lot
of epochs with a constant mask angle,
or a masking changing versus azimuth
in order to simulate a real environment.
• Considering a grid of observers
evenly distributed on Earth or
on a part of it for a fixed epoch
with an average mask angle.
In the first mode VSN and GDOP
evolutions versus time are plotted; in the
second one VSN and GDOP maps are
obtained for a certain area at a fixed epoch.
In order to obtain more significant plots,
global and regional grids of GDOP and
VSN values are generated every 15 min for
24h, producing a 3D matrix of data (Fig.6).
Regional results
To analyse the global coverage of GPS
and its space-based augmentations,
we consider a grid of observers placed
evenly on Earth surface, with a step
of 5° in latitude and longitude; VSN
and GDOP are computed w.r.t. every
observer at observation epoch. Mask
angle values of 15°, 30° or 40° are
adopted to represent different visibility
conditions. To obtain a complete scenario
for a fixed mask angle, probability of
VSN>6 and GDOP<4.5 are estimated
using a time step of 15 min for 24 hours.
Thresholds VSN>6 and GDOP<4.5 are
adopted as conservative conditions.
With a mask angle 15° the GPS standalone
provides a probability to have a
VSN>6 of about 100% at polar zones
and 80-90 elsewhere and provides
a GDOP<4.5 probability near to
90% worldwide. Geostationary and
geosynchronous augmentations in this
case improve the visibility and GDOP in similar ways and the super-constellation
enhances further the situation.

Fig.6: Plot of 3D-grid
The simultaneous use of EGNOS and
S-QZSS satellites with GPS constellation
provides of course the best results: VSN>6
probability is 100% and GDOP<4.5
probabilities almost 100% over Europe.
At low mask angle (~15°) the standalone
GPS is sufficient to guarantee good
coverage performances w.r.t. availability
and continuity; in this scenario, which
certainly doesn’t represents the worst case,
EGNOS and S-QZSS could be useful
for upgrade accuracy and integrity.
A mask angle 30° is a good approximation
of a quite adverse but not prohibitive
environment for signal propagation and
PVT solution. In these conditions the VSN

Fig.7: VSN>6 Probability ( mask angle 30°)
of GPS constellation
is rather poor, the
probability to have a
VSN greater than 6 is
about 10-20% almost
everywhere, while over
polar zones is 35-40%
(Fig.7). The GPS
coverage situation is
quite critical, in fact the
GDOP<4.5 probability
is about 20-30% almost
everywhere and near
to 0% at high latitudes where it’s
impossible a precise positioning (Fig.8).
The GPS+EGNOS constellation provides
a considerable visibility improvement
above all on the area defined by footprints
intersection of 3 EGNOS SV; this area
includes Southern Europe and has a
VSN>6 probability about 85-95%. In
this area GDOP<4.5 probability is about
50-70%. Also by the sides of this area
we note a VSN between 40% and 70%,
and a GDOP between 25% and 45%.
Comparing with previous case the
GPS+S-QZSS constellation improves
the visibility in different way; a wider
area takes advantages, but with worse
performances. VSN>6 probability is
70-80% in Africa, 60-70% in Europe and
the benefits of S-QZSS augmentation are
clear at higher latitudes too. A similar

Fig.8: GDOP<4.5 Probability (mask angle 30°)
improvement is obtained for GDOP;
GDOP<4.5 probability is 50-70% in
Africa and 50-55% in Europe. The superconstellation
improves the visibility in
both ways: a wide area is well covered
with good performances. In this case the
VSN>6 probability is 100% in Africa and
Southern Europe. Good GDOP coverage
is also obtained; GDOP<4.5 probability
is between 65% and 90% in Africa and
between 60% and 70% over Europe.

Fig.9: VSN>6 Probability (mask angle 30°)
By the examination of Figures 9-10,
which represent coverage performances
over Europe with a constant mask angle
30°, we can see that in this condition GPS
constellation is insufficient to provide
precise positioning. The integration of GEO
SVs produces a coverage improvement
only over Southern Europe; on the rest
of the Europe the coverage remains
insufficient, owing to geostationary
satellites problems to cover high latitudes.
S-QZSS integration produces a good
improvement in visibility and GDOP
(55-70% and 40-50% respectively), but
we can see some continuity issue. The
GPS+EGNOS+S-QZSS super-constellation
provides a full coverage on Middle and
Southern Europe with a VSN>6 probability
near to 100% and a GDOP<4.5 probability
about 65-80%. Northern Europe is served
by at least 6 SVs 60-70% of time, with
a good observation geometry about
50% of time; the aforesaid coverage
shortage could be overcome, handling
geosynchronous orbital parameters.
A common urban environment can be
simply represented considering an average
mask angle 30°; in this condition the superconstellation
is suitable to offer good
performances with reference to availabilityand continuity thanks to the visibility
improvements. The coverage quality is
enhanced thanks to GDOP improvement,
which causes a more accurate positioning.
If S-QZSS is able to broadcast EGNOSlike
signals, accuracy will be further
enhanced; it should give more probability
to receive SBAS correction and integrity
message also in urban environment.

Fig.10: GDOP<4.5 Probability (mask angle 30°)
GPS constellation with a mask angle 40°,
is inadequate to provide a continuous
and precise positioning; both VSN>6 and
GDOP<4.5 probabilities are near to 0%.
The super-constellation allows a good
visibility enhancement on Africa, but with
a GDOP very poor. On Europe such a
masking makes impossible a continuous
and accurate positioning service; the
super-constellation provides a coverageimprovement only
at low latitudes.

Fig.11: Naples coverage evolution
(mask angle 30°)
Local results
The developed
software is able to
analyse the coverage
evolution for a certain
period, considering
a single observer;
this application is
useful to study in detail the
behaviour of a navigation constellation
over a not wide zone. Now we want to
examine deeply the behaviour of GPS
constellation and its augmentations over
Europe; for this purpose we have selected
Naples centre area to test the coverage
evolutions of the considered constellations.
A first analysis is made considering mask
angles 15°, 30°, 40° which represent
masking conditions of growing difficulty;
for a fixed observer VSN and GDOP
were computed every 60 seconds in a
whole day and a statistical analysis with
VSN>5 and GDOP<6 probability is carry
out. The observer is placed at Naples at
coordinates (φ: 40°50’ N; λ: 14°15’ E).
With a mask angle 15° GPS standalone
constellation provides good
performances: VSN>5 and GDOP<6
probabilities are 100%. For the superconstellation
GPS+EGNOS+S-QZSS,
VSN is between 11 and 16 and the
GDOP value is ever below 3.7.
With a mask angle 30° (Fig.11) sometimes
the only GPS has a VSN<4, so it’s
impossible the determination of 3D fix;
VSN>5 probability is about 40% and
GDOP<6 probability is about 45%. Instead
w.r.t. super-constellation, VSN is between
7 and 13, and GDOP between 2.5 and 8;
GDOP<6 probability is about 95% and so
a continuous good geometry is guaranteed.