Genesis Expedition
GENESIS Expedition
R/V ROGER REVELLE
Leg 1
transit from San Diego to Talara
27 December 1996 - 8 January 1997
Leg 2
Peter Lonsdale (619) 534-2855
University of California, San Diego email: plonsdale@ucsd.edu
Marine Physical Laboratory
Scripps Institution of Oceanography
San Diego, CA 92093-0205
Talara - Punta Arenas
11 January - 19 February 1997
Leg 3
Alan Mix (541) 737-5212
College of Oceanic and Atmospheric Sciences email: mix@oce.orst.edu
Oregon State University
Corvallis, OR 97331-5503
James McManus (541) 737-3281
College of Oceanic and Atmospheric Sciences email: jmcmanus@oce.orst.edu
Oregon State University
Corvallis OR 97331-5503
Punta Arenas - Callao
23 February - 6 April 1997
Leg 4
Robert Weller (508) 548-1400 x 2508
Woods Hole Oceanographic Institution email: rweller@whoi.edu
Woods Hole, MA 02543
Callao - San Diego
09 April - 04 May 1997
SCRIPPS INSTITUTION OF OCEANOGRAPHY
CONTACTS
Robert A. Knox (619) 534-4729
Assoc. Director, Shipboard Operations and email: rknox@ucsd.edu
Marine Technical Support
Captain Tom Althouse (619) 534-1643
Marine Superintendent, Nimitz Marine Facility email: capt@mpl.ucsd.edu
Christian de Moustier (619) 534-1784
Scientific Advisor to Shipboard email: cpm@mpl.ucsd.edu
Technical Support Services
SEA BEAM information contact
Woody Sutherland (619) 534-4425
Manager, Shipboard Technical email: woodys@odf.ucsd.edu
Support Services
Stu Smith (619) 534-1898
Head, Geological Data Center email: ssmith@ucsd.edu
Ron Moe (619) 534-6054
Head, Shipboard Computer Group email: rmoe@ucsd.edu
Bob Wilson (619) 534-1632
Head, Resident Marine Technician Group email: restech@sdsioa.ucsd.edu
Rose Dufour (619) 534-2841
Elizabeth Rios email: shipsked@ucsd.edu
Ship Schedulers
Preface
On December 27, 1996 R/V Roger Revelle begins her first foreign expedition.
The expedition name Genesis has an obvious meaning of "beginning," and the added
virtue of the same spelling in English and Spanish, the language of the foreign
ports to be visited. Following a transit leg to Puntarenas, Costa Rica, SIO
and NAVSEA representatives will board the ship for a further transit to Talara,
Peru. Time en route will be devoted to identification and resolution of warranty
issues. The three scientific legs of the expedition after the Talara port call
will carry out research as described in the following pages.
This Genesis will be a demanding one, with work in high southern latitudes and
with a wide range of shipboard science activities, from long piston coring to
heavy mooring deployments. Fortunately, R/V Roger Revelle is an eminently
capable vessel, well-suited to these tasks and with every prospect of completing
them safely and efficiently. From this beginning we look forward to many years
of superior service to US oceanography by this newest member of the active
UNOLS fleet.
Leg 1
Transit from San Diego to Talara
27 December 1996 - 8 January 1997
(Intermediate port stop in Puntarenas on January 4 to take on NAVSEA personnel.)
On this leg, while underway for Talara, Peru, a number of shipbuilder warranty
issues will be reviewed by SIO personnel and NAVSEA representatives of the AGOR
program. Some warranty items have been addressed since delivery of the ship
in June, 1996, and the effectiveness of these repairs and modifications will
be reviewed and documented. Some warranty issues remain to be identified
and documented. Some have been identified but await an agreed-upon plan and
timeline for resolution or repair. These matters will be dealt with by the
SIO and NAVSEA parties aboard.
Leg 2
Peter Lonsdale
Scripps Institution of Oceanography
Talara - Punta Arenas
11 January - 19 February 1997
The purpose of this leg is to complete a survey of the conjugate pair of oceanic
rifts that initiated the northern part of the Pacific-Antarctic East Pacific Rise,
and of the Pacific-Farallon-Antarctic triple junction trace that marks the
subsequent growth of that rise. Henry Trough, the western member of the conjugate
rift pair, was surveyed by Melville in 1994; the eastern Hudson Trough and the
major structures that intersect it (Humboldt Trough and the Menard, Vacquier,
Raitt and Tula fracture zones) will be principal targets of this survey.
Equipment to be used includes the SEA BEAM 2112 sonar, magnetometer and gravimeter
(throughout the leg) plus 3.5 kHz and seismic (2X 80" water gun) profilers for
10-15 days. Sediment thickness in the survey area generally increases southward
toward Antarctica. How much profiling gets done, and how far south the survey
extends, will depend on how effective the profiling systems are in the prevailing
sea states.
Foreign clearance will be required only for the SEA BEAM/magnetics/gravity
transits across the coastal waters of Chile. The attached track chart assumes
entry into the Straits of Magellan via Cockburn Channel, rather than by the less
direct western end of the Straits.
The scientific party will number 10-12, including 3 techs and 4-5 Scripps
students, plus possible Chilean participants.
Leg 3
Alan C. Mix
James McManus
Oregon State University
Punta Arenas - Callao
23 February - 6 April 1997
This document provides a preliminary outline of field operations for an NSF-funded
program to provide site survey information prior to ODP drilling in depth
transects and a latitudinal transect in the SE Pacific Ocean.
The primary field operations will be:
1) high-resolution bathymetric mapping using SEA BEAM-2112,
2) digital single-channel seismic,
3) High resolution digital 3.5 kHz profiling with as much penetration of
the sediment as possible
4) Sediment coring (using piston- and multi-coring systems supplied
by Oregon State University)
Most of the sites are located on bathymetric highs outboard of the Peru-Chile
trench, to avoid as much as possible terrigenous turbidites and tectonic
complexities on the margin, but are close to the continents to maximize
sedimentation rates in the zone of high productivity and hemipelagic sediment
influx. A few of the sites are on the Chilean continental margin, under
coastal upwelling centers. The transects are designed to obtain hemipelagic
and pelagic sediments that monitor past changes in watermasses associated
with deep inflow and mid-depth outflow from the Pacific, latitudinal variations
in the Humboldt and Cape Horn Currents, and upwelling on the Chilean margin.
The cruise plan and tentative station areas is outlined in Table 1. Note
that each named station in Table 1 is the approximate center point of a Survey
Area. This plan notes fifteen such Survey Areas. Site names follow current
Ocean Drilling Program conventions, with a 3-letter location code (NAZ = Nazca Rise,
CBA = Chile Basin, CRI = Chile Rise) a sequential number within each area, and a
letter (B here indicates our second iteration on each site, revising the
locations noted in earlier documents submitted to the Ocean Drilling Program,
C indicates the third iteration, and so on). Each Survey area will contains
two stations for coring.
For purpose of obtaining clearance for operations in Chilean and/or Peruvian
waters, we expect operations to occur within 1 degree latitude and longitude
of sites noted in table 1, including transit tracks between sites.
TABLE 1: Cruise outline, with 15 target areas. Precise coring locations will
be modified at sea based on detailed geophysical survey. Following this
survey, we will core primary and secondary locations within each station area
with piston core and multicore (i.e., two PC and two MC at each named station.
Note that target areas close together, such as (CRI-1B & 2B), (CBA-2B & -2C),
and (NAZ-2B, -3B, & -4B) will be surveyed together, followed by coring. The
operational plan for each target area will be to begin the survey with swath
map, 3.5 kHz profiler, and digital water-gun seismic profiling. Initial survey
track lines are about 10-20 nm in length, to be crossed later by at least two
crossing lines (or more in areas of complex bathymetry or poorly known areas).
Crossing lines will run about 6 to 10 miles in length, and will be spaced about
3 miles apart. We expect that a typical geophysical survey, forming a partial
grid within about 30 nm of each proposed site, will take about 18 hours
(including deployment and recovery of seismic gear).
Following geophysical survey, we will core primary and secondary sites within
each Survey Area, using piston core and multicore gear supplied by the OSU
coring group. Coring time estimates include time for setup and deployment of
the piston core, switching the 9/16' coring wire from the starboard side
(piston coring) to the stern (multicoring), deploying the multicore, moving
the ship to a secondary location in the survey area, and repeating the PC
and MC coring operation. Estimated station times vary from area to area,
because the calculation includes variable lowering times to the sea floor
as a function of water depth (50m/min for PC, and 60m/min for MC are assumed).
We may also want to do some smaller-wire operations such as water sampling
and/or plankton towing during this station time (obviously not while coring
wire is over the side).
Note that final coring sites will be determined at sea based on the detailed
geophysical survey. This means that the shipboard party will have to maintain
some flexibility as there will be schedule changes at sea. This is typical
of coring operations. We will plan to keep the SEA BEAM-2112 system and 3.5
kHz profiler operating on the transit lines between all survey areas. In
table 1, transits that note speeds of 11 knots have no single-channel seismic
operations, while transits that note speeds of 7 knots include single-channel
seismic operations.
Special equipment needs for seismic and coring operations are:
1) Compressor, water guns, and hydrophone streamers appropriate for high-resolution
digital seismic profiling.
2) Excellent working 3.5kHz system -- we require good sub-bottom penetration and
digital recording of the 3.5 kHz data.
3) Open Rail Space - suitable for rigging piston cores with 80 feet of pipe
plus weightstand. OSU will supply the coring gear, including hinged bucket
system for safely deploying piston core head.
4) Fantail Access - suitable for launching the multicore system over the stern,
without interfering with deck-mounted gear (booms, etc.) for seismic operations.
5) 9/16' wire, traction unit, and winch in good condition. Note that the OSU
Piston Coring System is large, and heavy, with a weight on lowering of about
5000 lb. Pullouts of the piston core from the sea floor can exceed 20,000 lbs
at the shipboard tensiometer, and thus a wire in good condition that has not
been stressed beyond its elastic limit by dredging operations is essential.
6) A functioning, reasonably accurate, tensiometer with both digital and
analog readout.
7) Space and appropriate power for OSU refrigerated van.
8) Deck handling gear (articulated crane, etc.) appropriate for deploying
coring and seismic gear.
In the ship's laboratory space at sea, we expect to:
1) Analyze unsplit sediment cores with a GRAPE (Gamma Ray Attenuation Porosity
Evaluator) and magnetic susceptibility logging system. This system includes
a sealed, shielded, solid-source of gamma radiation. It has been used at sea
before, and does not create any risk of spilled radioactive materials. It may,
however, require special clearance, a certified operator, and a laboratory set
up with a small area of restricted entry. This has not been a problem on
previous cruises.
2) Split cores at sea, and analyze for reflectance spectroscopy using the
OSU Split Core Analysis Track. This system present no hazards, but requires
significant space, and access to reasonably clean electrical power.
3) Describe cores visually for normal sedimentological contents.
4) Archive the sediment cores in a refrigerated van (supplied by OSU group).
5) Start preliminary seismic processing, and produce SEA BEAM maps and seismic
plots appropriate to the survey.
As an extension to this cruise, an additional proposal (McManus et al, 1995),
will perform some analysis of pore waters from the sediment cores, and this
will require additional laboratory and refrigerator space for pore-water squeezing.
Leg 4
Robert Weller
NOAA
Callao - San Diego
09 April - 04 May 1997
As part of the Pan American Climate Study (PACS), funded by the NOAA Office
of Climate and Global Change, field studies of the links between the eastern
tropical Pacific ocean and climate over the Americas will begin in 1997.
This cruise will initiate one element of that PACS field work by deploying
moorings along 125 deg W. Dr. Robert Weller of Woods Hole Oceanographic
Institution (WHOI) will be Chief Scientist, and two WHOI surface moorings,
a joint effort between Weller and Dr. Steve Anderson of WHOI, will be deployed
as well as one from Dr. Robert Weisberg of South Florida University. The
moorings will carry complete meteorological instrumentation and oceanographic
instruments to measure upper ocean velocity, temperature, and salinity. One
mooring will be deployed south of the equator along 125 deg W to collect data
in the 'tongue' of cold water found there. The second mooring will be deployed
at the equator, and the third mooring north of the equator in the Intertropical
Convergence Zone (ITCZ). This will allow the air-sea interaction and upper
ocean processes that control the sea surface temperature of the eastern tropical
Pacific to be studied in three distinct regimes. The cruise will depart from
Callao, Peru, pick up the 125 deg W longitude line, stem north along the line
to deploy the moorings, and then return to San Diego.
Internet: shipsked@ucsd.edu
WWW: http://sio.ucsd.edu/
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