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The sea bottom samples were collected with
2.3 Ton gravity corer (Fig.15), the ISMAR's Mod.SW-104 water/sediment corer
[Magagnoli A. and Mengoli M. (1995)] (Fig.16) and
a 60L Van-Veen grab (Fig.17).
The sample locations are shown in Figg.7,9,
10 and 11 and are reported on Tab.5
Some of the cores were opened and described.
All the cores were analyzed for magnetic suceptibility (2cm) using the ISMAR's
automatic logger SAAS-01 by a Bartington loop sensor [Masini L. (2001)].
The volume magnetic susceptibility measures the capability of the material to
become magnetized and to produce a noise in the inducing magnetic field, and
can be used for stratigraphic correlations
between cores and in the frequency analyses of temporal series to detect
sedimentary cycles.
Knowing (adimensional) and density, is it possible to
determine the mass susceptibility.
Minerals could be
- diamagnetic ( 0),
- paramagnetic ( 0) e.g. iron and nickel,
- ironmagnetic ( 0) e.g. (a) iron oxides, like magnetite,
hematite, ilmenite, maglemite, (b) iron hydroxides like
limonite and goethite, and (c) sulfurs, such as pyrite.
The obtained data were corrected for the loop sensor diameter
(10 cm or 12,5 cm) and the sediment thickness, cleaned, filtered and
plotted against core depth.
The grabs and two core-catcher were washed, sieved and described.
figure
Figure 15:
2.3 T gravity corer.
|
figure
Figure 16:
SW-104 water/sediment corer.
|
figure
Figure 17:
Sediments recovered with the 60L. grab.
|
Table 5:
Cruise MARM05: location of the sediment samples.
STATION |
TYPE |
DATE |
TIME |
LON |
LAT |
SA-101 |
SW104 |
2005-09-13 |
05:46:55 |
26:13.68152 |
40:26.04119 |
SA-102 |
COR2 |
2005-09-13 |
06:56:52 |
26:13.69103 |
40:26.04936 |
SA-103 |
SW104 |
2005-09-13 |
08:17:33 |
26:13.67555 |
40:26.03650 |
PI-104 |
COR2 |
2005-09-16 |
06:21:49 |
29:09.54222 |
40:49.36678 |
PI-105 |
COR2 |
2005-09-16 |
07:04:32 |
29:09.54888 |
40:49.37142 |
PI-106 |
COR2 |
2005-09-16 |
08:02:38 |
29:09.55057 |
40:49.37111 |
PI-107 |
COR2 |
2005-09-16 |
11:29:59 |
28:57.92607 |
40:53.38996 |
PI-108 |
COR2 |
2005-09-16 |
12:13:49 |
28:57.93107 |
40:53.39460 |
PI-109 |
COR2 |
2005-09-16 |
13:07:02 |
28:58.29240 |
40:51.85500 |
PI-110 |
COR2 |
2005-09-16 |
14:15:47 |
29:01.42309 |
40:52.84784 |
IZ-111 |
SW104 |
2005-09-19 |
08:05:12 |
29:40.99199 |
40:43.77069 |
IZ-112 |
SW104 |
2005-09-19 |
08:48:28 |
29:41.01076 |
40:43.78409 |
IZ-113 |
SW104 |
2005-09-19 |
10:39:12 |
29:40.99589 |
40:43.77682 |
IZ-114 |
COR2 |
2005-09-19 |
11:41:50 |
29:41.00798 |
40:43.77287 |
IZ-115 |
COR2 |
2005-09-19 |
13:17:13 |
29:40.13402 |
40:43.47816 |
IZ-116 |
COR2 |
2005-09-19 |
14:09:59 |
29:40.76140 |
40:45.63010 |
01 |
GRA |
2005-09-19 |
20:25:46 |
29:36.93581 |
40:42.08339 |
02 |
GRA |
2005-09-19 |
21:46:00 |
29:27.47141 |
40:43.83069 |
03 |
GRA |
2005-09-19 |
22:03:32 |
29:27.46081 |
40:43.83149 |
04 |
GRA |
2005-09-19 |
22:35:25 |
29:27.46081 |
40:43.83149 |
05 |
GRA |
2005-09-19 |
22:54:16 |
29:27.53270 |
40:43.85649 |
06 |
GRA |
2005-09-19 |
23:26:32 |
29:27.33632 |
40:43.80858 |
07 |
GRA |
2005-09-20 |
00:15:22 |
29:27.00764 |
40:43.73295 |
IZ-117 |
COR2 |
2005-09-20 |
07:41:06 |
29:42.18165 |
40:44.99639 |
IZ-118 |
COR2 |
2005-09-20 |
08:42:56 |
29:43.30675 |
40:43.36072 |
IZ-119 |
COR2 |
2005-09-20 |
10:53:08 |
29:40.98832 |
40:43.77744 |
IZ-120 |
COR2 |
2005-09-20 |
13:32:38 |
29:29.17731 |
40:45.90078 |
IZ-121 |
COR2 |
2005-09-20 |
14:10:05 |
29:29.18850 |
40:45.89901 |
IZ-122 |
COR2 |
2005-09-20 |
15:07:26 |
29:24.25779 |
40:44.75079 |
GE-123 |
COR2 |
2005-09-24 |
06:15:21 |
29:01.98169 |
40:23.82868 |
GE-124 |
COR2 |
2005-09-24 |
06:59:14 |
29:01.99450 |
40:23.82587 |
GE-125 |
COR2 |
2005-09-24 |
07:52:23 |
29:01.67126 |
40:24.94506 |
GE-126 |
COR2 |
2005-09-24 |
08:33:37 |
29:01.65890 |
40:24.95295 |
SA-127 |
COR2 |
2005-09-29 |
05:49:16 |
26:10.34994 |
40:23.85527 |
SA-128 |
COR2 |
2005-09-29 |
10:49:58 |
26:05.28425 |
40:26.56273 |
|
Next: MULTICHANNEL REFLECTION SEISMIC
Up: MATERIALS AND METHODS
Previous: CHIRP SBP
Contents
2005-12-08