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The Picentini Mountains
The Picentini mountains have been selected because of their very articulated morphology
and structure. The area is characterized by many geological formations and structural
typologies (faults, overthrusts, klippens, and tectonic windows). The geological
analysis of
SAR
images has been carried out locally (the selected area does not exceed
400 km2)
so, for example, structural trends have not been considered. The study has been
focused on both geological details (e.g., the analysis of the limit between limestone
and dolomite of the Stella mountain) and structural lineament identification.
The Phlegrean Fields
The Phlaegrean Fields area offers the opportunity to study a morphology characterized
by several crateric rims having different ages and histories. For this area
SIR-C/X-SAR
data have been integrated by
ERS-1
and
JERS-1
data imagery (lower incidence angles and different looking directions).
The Somma-Vesuvius complex
Vesuvius a very interesting test site, which was observed during a number of spaceborne
and airborne remote sensing missions. For that reason we are able to compare the
results obtained using
SIR-C/X-SAR
data with those obtained using other
SAR
imagery
acquired by
ERS-1,
JERS-1,
and
AIRSAR
missions.
Available
SIR-C/X-SAR
data
The following data takes have been used:
The
SIR-C/X-SAR
images, generated as above mentioned, have been analyzed by using
photo-interpretation techniques and integrated with images of comparable spatial
resolution acquired by other sensors (ERS-1 ascending, descending and roll-tilt mode,
JERS-1,
AIRSAR)
. The results have been compared and/or integrated with geological sheets
and when possible with aerial photos, geological sheets and field checks.
Brightness, color, texture, shading and pattern information is used for discriminating
among geological features and lithologies. Foreshortening/layover effects, in the
case of the Picentini mounts and of the Phlaegrean Fields, have been verified by
comparing
SAR
images and geological cartographic profiles.
SIGNIFICANT RESULTS
Data Processing
Tables 1 (L-band) and 2 (C-band) show some experimental results obtained by decomposing
the normalized covariance matrices computed over 9 sample windows (11x11 pixels).
Each target (Vesuvius cone, 1944 lava flow, pine forest and sea) has been selected
at most twice in order to check about the effects of slight different looking directions
and/or incidence angles. Sea samples have been extracted from
AIRSAR
images since
on these data the incidence angle ranges from 23° to about 58°.
For each sample have been computed the ratio HH/VV (second column), the ratio VV/HH
(third column), the third eigenvalue (fourth column), the module (fifth column) and
phase (sixth column) of correlation coefficient between co-polarized channels, the
first (seventh column) and second (eighth column) normalized eigenvalues. The target "entropy",
here defined as the sum of the normalized eigenvalues, is reported in the last column.
As can be noted, if the target is constituted by sand/ash as in the case of the Vesuvius
cone, the first eigenvalue represents more than the 70% and 80% of target entropy
for L-band and C-band respectively. These values suggest that, also for L-band scattering, the surface effect dominates the volumetric effect. A comparison made with P-band
AIRSAR
data shows a probably more consistent volumetric scattering at these frequencies
(a value of 60% is typical on the Vesuvius cone).
The analysis of
3
(h in the Tables)
confirms these remarks; the L-band (5-6 %) and C-band (12-13%) values
show clearly, for the latter, a higher depolarization effect suggesting that the
pyroclastic products of the Vesuvius cone are rougher at a centimeter scale than
at a decimeter scale.
For concerns of the 1944 lava flows, the depolarization effect increases sensibly
with respect to the cone in the L-band as well as the C-band. The first eigenvalue
is now only 50-55% of target entropy while the second and third eigenvalues reach
about the 20-25%. It may be concluded that the roughness at a centimeter scale is comparable
to the roughness at a decimeter scale.
Pine Forest data confirm that trend since the entropy increases and
1
is still decreasing (40-45% in L-band and 45-50% in C-band).
This decomposition of covariance matrix can be used also in the
analysis of sea scattering.
Some investigations which have been carried out show that at
low incidence angles
(23°) the specular reflections largely dominate and
target entropy is very low especially for L-band where the sea
acts like a deterministic target and
1
constitutes about the 98% of total entropy.
As the incidence angle increases the entropy
increases as well and the
VV
return becomes
also up to three times the
HH
return
(L-band at 58°).
Geology
SIR-C/X-SAR
images, because of the high incidence angle (about 50°) clearly show the
differences between the western side of the Picentini mounts and the Avella mountains.
The first ones are characterized by a complex overlapping of structures while the
second ones are simply crossed by a normal fault.
The following classes have been easily discriminated:
1) Alluvium, pyroclastic products (ignimbrite campana), colluvium, flisch, and "melange"
of the sicilide unity;
2) Carbonatic-dolomitic rocks of the "Campano-Lucana" platform;
3) Bedded sands and conglomerate of the Altavilla unit.
At low incidence angles (i.e., about 20-25°) discrimination between conglomerates
and sands of the Altavilla unit, and the carbonatic formations is not possible. On
the investigated area, the differences between calcareous-dolomitic and alluvium/flisch
terrains are simply detected while the discrimination between flisch and alluvium is
a difficult task. On the Mai mountains (a part of Picentini mountains), some Trias-Giura
limits seems to be actually tectonic and not stratigraphic as pointed out in the
literature.
In X-SAR imagery, the morphology of the Mounts Lattari stands out clearly as well
as the boundaries among carbonatic rocks, colluvium and alluvial fan and tuff or
eruptive volcanic products less or more pedogenized. The alluvial fan presents a
very thin texture while the Vesuvius 1944 lava flows are less evident.
In the Somma-Vesuvius area, the limit between the products of pre-Mount Somma and
the undiversified pyroclastic products has been recognized by using differences of
intensity, color and texture which are due to changes of morphology, vegetation cover
and drainage pattern. Good discrimination is achieved among the characteristics of the
recent lavas, principal quarries, Mount Somma caldera rim, the drainage pattern and
the pyroclastic products of the Vesuvius cone.
A detailed analysis of the Phlegrean Fields area requires the integration of data
acquired with different incidence angles and from different looking directions in
order to achieve a good detection of the crateric morphology and, in some cases,
for the detection of zones affected by volcano-tectonic collapses. This is the case of Mount
Gauro which is characterized by eastern and western crateric slopes slightly concave
toward the exterior, with the sides higher than the center. The east and west slopes
of the Gauro are related, according to some authors, to volcano-tectonic collapses following
explosive events that occurred about 5000 years ago.
SIR-C/X-SAR
images show a more
realistic morphology and the shadow distribution allows a good identification of
the heights of this crateric edge.
HH
polarization allows a good characterization, in terms of tone and texture typologies,
of terrains and anthropic constructions while in the
HV
images, the texture is more
homogeneous.
FUTURE PLANS
Research activities are still in progress. New sub-areas included in the Campania
test-site will be considered, especially for what concerns INSAR and DINSAR data
processing. For example, 16 corner reflectors have been already installed in the
area of Sannio-Matese and new installations are planned in the next months.
Polarimetry
Further investigations both theoretical and experimental will be carried out on quad-pol
data.
In particular the following items are under study:
L-band | 1/z | z | h | (deg) | ||||
Cone 1 | 1.0003 | 0.9997 | 0.1210 | 0.8654 | -2.5208 | 1.8655 | 0.1345 | 2.1210 |
Cone 2 | 1.0405 | 0.9611 | 0.1764 | 0.8119 | -4.8326 | 1.8136 | 0.1879 | 2.1780 |
44' Lava 1 | 0.9608 | 1.0408 | 0.5562 | 0.3886 | -7.2830 | 1.3914 | 0.6102 | 2.5578 |
44' Lava 2 | 0.9775 | 1.0230 | 0.5736 | 0.4111 | -7.4226 | 1.4120 | 0.5885 | 2.5741 |
Forest 1 | 1.0956 | 0.9127 | 0.7312 | 0.2185 | 3.6549 | 1.2410 | 0.7673 | 2.7395 |
Forest 2 | 1.1336 | 0.8821 | 0.6097 | 0.2737 | -1.3037 | 1.3092 | 0.7066 | 2.6254 |
Sea (23) | 0.9580 | 1.0439 | 0.0195 | 0.9613 | -0.8334 | 1.9632 | 0.0386 | 2.0214 |
Sea (45) | 0.4371 | 2.2879 | 0.0746 | 0.8739 | 0.8260 | 2.6363 | 0.0897 | 2.7996 |
Sea (58) | 0.3176 | 3.1483 | 0.1835 | 0.7040 | 7.0143 | 3.3137 | 0.1522 | 3.6494 |
C-Band | 1/z | z | h | (deg) | ||||
Cone 1 | 1.1558 | 0.8652 | 0.2873 | 0.6742 | 3.0451 | 1.7001 | 0.3208 | 2.3083 |
Cone 2 | 1.1588 | 0.8630 | 0.3033 | 0.6022 | 3.9899 | 1.6310 | 0.3908 | 2.3251 |
44' Lava 1 | 1.0277 | 0.9731 | 0.4983 | 0.4785 | -5.0762 | 1.4796 | 0.5211 | 2.4991 |
44' Lava 2 | 0.9644 | 1.0369 | 0.4388 | 0.5211 | -7.7925 | 1.5231 | 0.4782 | 2.4401 |
Forest 1 | 1.1808 | 0.8469 | 0.6669 | 0.2561 | 7.0226 | 1.3195 | 0.7081 | 2.6946 |
Forest 2 | 1.1566 | 0.8646 | 0.7099 | 0.2500 | -8.8327 | 1.3001 | 0.7211 | 2.6002 |
Sea (23) | 0.9222 | 1.0843 | 0.0070 | 0.8966 | -13.3407 | 1.9035 | 0.1030 | 2.0135 |
Sea (45) | 0.4770 | 2.0996 | 0.2048 | 0.7164 | 2.1040 | 2.3695 | 0.4141 | 2.7814 |
Sea (58) | 0.5555 | 1.8003 | 0.5000 | 0.2681 | 0.7945 | 1.8556 | 0.5002 | 2.8558 |
Table of Contents |
Converted to HTML by Alvin Wong,
al.wong@jpl.nasa.gov
The Jet Propulsion Laboratory
4800 Oak Grove Drive
Pasadena, Cailfornia 91109