The ADCPs consist of three components, transducers
mount in the bottom of the ship just forward of frame
63 near frame 60, deck units located in the “gyro”
room next to the gym on deck level 2, and PC computers
located in the “Computer Lab”.
The individual transducer wells are circular with removable
lids and water tight electrical stuffing-boxes. To reduce
ringing and acoustic interference from the ship, an
acoustic dampening material, approximately 1”
thick, lines the inside of each well. Acoustic windows
consisting of approximately 2” thick “SeaBeam
Orange” urethane are mounted flush with the bottom
of the ship to protect the transducers from ice damage.
The wells are flooded by a propylene glycol (Formula
2790 PG Green) antifreeze/fresh water mix maintained
at a sufficient hydraulic head to keep sea water out
in the event of a leak between the windows and the wells.
There is also an Applied Microsystems sound velocimeter
(Model SV2000) installed in the transducer well for
the Broad Band 150kHz (BB150) ADCP.
The cables from the transducers and velocimeter are
led up two deck levels and forward to the deck units
in the gyro room at bulkhead 44. Ship heading data is
fed to the deck units through gyro synchro inputs. Discussions
with one of the ship’s ETs (Chief M. McGuire)
and a representative from Sperry (Mike Chappell) indicate
that the heading data supplied to the ADCPs can come
from three possible sources. There are two gyros and
a single attitudinal GPS (Ashtech) unit that supply
heading data to the ship’s “integrated bridge
system”. These units are all inherently digital
and the data from these units are converted to analog
synchro outputs for the ADCPs through a D/A converter.
Which of the three possible heading sources is sent
to the ADCPs is controlled by a manual switch on the
bridge. Typically, gyro #1 is used but above some latitude
(~80oN) the gyros produce poor data and the attitudinal
GPS data source will be used in preference. However,
there is no guarantee as to which data source is being
used at any given time so it must be assumed that the
choice is arbitrary. The data source is clearly subject
to change outside the control of the Healy’s science
group. Given the construction, communications and command
needs on the Healy, the only way to ensure a constant
heading data source is to install a completely separate
gyro system for science use. However, under normal conditions
the arbitrariness of the heading source should not adversely
effect the ADCP data since attitudinal GPS data output
is available for post-processing and can be used to
correct the heading data to a single stable source.
Currently, the velocimeter is not functional. The BB150
ADCP deck unit has the capability to ingest sound velocity
data directly but that is a poor option because the
sound velocity correction needs to be reviewed during
post-processing before it is applied. A better choice
is to have the sound velocity data recorded by the ship’s
Science Data Network. Since the transducers are protected
from changes in the sea water by the acoustic window
and are immersed in an antifreeze/water mixture, the
sound velocity is expected to be different from that
in seawater and to vary rather slowly. Thus, the sound
velocity corrections for the BB150 can mostly easily
be addressed during post-processing.
The deck units are connected to PCs in the computer
lab through serial RS232/RS422 cables. The PC’s
for both units run a Windows-based program called “VM-DAS”,
RD Instrument’s new data acquisition system for
vessel mounted ADCPs. Briefly, this program sends commands
to the ADCP deck unit specifying the character of the
acoustic pings to be sent by the ADCP and how the returning
signal is to be processed before it is sent to the computer.
VM-DAS then takes that data, combines it with navigation
data, adds it to the data archive and displays a summary
of the data on the screen together with ancillary information.
Navigation data on the Healy can come from either the
dedicated bridge or science system. There are P-Code
GPS units for both the bridge and the science components.
The P-Code acquired by the unit in the Computer Lab
is being sent directly to the ADCP PCs in NMEA format
through RS232 serial lines at a refresh rate of 1 Hz
and includes the GGA message. Attitudinal GPS data is
also available to the ADCP system from the ship’s
single Ashtech GPS receiver mounted on the helicopter
control officer’s shack. (The helo shack is located
over frame 114 approximately 40.8m aft of the ADCP transducers.)
According to Chief McGuire and Mike Chappell from Sperry,
the Ashtech data for the PCs come directly from the
Ashtech unit via an RS232 serial splitter box on the
bridge from which cables are led to the PCs. The refresh
rate of the NMEA Ashtech data stream was adjusted by
Chief McGuire to 1Hz during Healy cruise HY0201 and
includes both the GGA message for position as well as
the GPPAT message for Ashtech 3-D attitude. During HY0201,
both P-Code and Ashtech data were sent to the PC for
the OS75 but only one of the navigation streams was
acquired by the BB150’s PC because that PC lacked
enough serial ports. A minimum of three serial ports
are needed to connect to the ADCP deck unit plus the
two navigation sources.
There are several manuals supplied by RD Instruments
describing the details of the BB150 and OS75 ADCPs and
the operation of the VmDas data acquisition system.
Below is just a brief description of the operation of
the VmDas. VmDas is a Windows based program that operates
on essentially any Windows 97 -> XP operating system.
While it is possible to set up and run the VmDas strictly
using point and click choices in the “options”
menu, it is recommended that previously saved and edited
options files be used to control its operations as this
minimizes the risk of missing essential in the setup.
The options, or *.ini, files are flat-ASCII files typically
saved in the VmDas subdirectory (C:\Program Files\RD
Instruments\VmDas). The options file contains the path
to an ADCP definitions, or *.txt file which contains
the commands that are actually sent to the deck unit
by the PC. The text files are also saved in the VmDas
subdirectory. The options file also contains directions
about the running of VmDas itself, items such as where
the data is to be stored, the short and long term averaging
intervals, scaling of screen plots, and a long list
of other items. Both the *.txt and *.ini files can be
edited with any simple editor.
Running a pre-saved version of VmDas from the keyboard
is quite simple. Double click on the VmDas icon on the
screen or start VmDas.exe in the C:\Program Files\RD
Instruments\VmDas subdirectory. A blank VmDas screen
will appear with a few menu options available. Click
on the file menu and highlight “Collect Data”.
This will open the data acquisition portion of the program
and will probably show several empty plots and a data
table. The options (*.ini) file is chosen using the
Options/Load menu and choosing the correct options file
for the ship’s location and science needs. You
can view or edit items in the options file that effect
the data processing and presentation by VmDas using
the Options/Edit menu. After you have made changes,
save the options file before starting actual data collection.
Data collection is started by clicking on the blue right
arrow in the upper left-hand corner or by clicking the
Control/Go menu item. Stopping data collection is accomplished
by clicking the blue square or by clicking the Options/Stop
menu item.
When running, VmDas shows the file name leader and
data session number in the task bar at the top of the
screen. A number of visual real-time data presentations
are available while data is being collected. These are
controlled by the square buttons on either of the two
lines immediately under the menu. The button with the
small “R” on it will cause the results from
the individual pings to be shown. The “S”
button shows results from the short-term averages while
the “L” shows those from the long-term average.
The next three buttons choose the display of velocities,
quality indicators and/or a table of the data. The buttons
with “CFS”, LDR”, “BOT”,
“WTR”, and “NAV” bring up panels
with configuration, leader, bottom track, water track
and navigation data, respectively. Choice of any of
the display options has no effect on the data collection,
these are strictly for real-time display purposes. The
figures can be fine-tuned using the blue arrows or zoom-in/zoom-out
buttons. Right-clicking the mouse over any of the graphs
brings up other choices for the displays. It is also
possible to show the short or long-term averaged velocities
as stick vectors on track plots. However, these only
result in reasonable results if the ADCP’s heading
offset has been correctly entered in the *.txt file.
Not all types of presentation are available for each
of the three types of data presented.
The VmDas data acquisition PCs on the Healy are networked
into the Science Data Network which supplies plenty
of storage space for the voluminous files produced by
the ADCPs. A mapped drive on the network is thus the
primary data file repository. A backup subset of files
is also recorded on the PC itself. There is enough room
on the present ADCP PCs to hold about 30 days of data
before the directories need to be purged and they should
be purged at least before each cruise. The data files
are currently stored on the server under separate directories
for each instrument. The files are stored under E:\cruisename
for the BB150 and under F:\cruisename for the OS75 where
cruisename should be a unique identifier The data files
are also backed-up on each instrument’s PC in
the directory: C:\RDI\cruisename.
There are 10 files generated each time VmDas starts
a new ADCP session. They are described in the VmDas
manual (pg 73 of the User’s Manual) if you need
further information. Briefly, the files use the convention:
CRUISENAMEnnn_mmmmmm.Ext, where CRUISENAME would be
something like HY0201 which uniquely identifies a cruise.
The next three digits indicate the sequential session
number; the 6 digits after the “_” constitute
the file sequence number within each the session. Each
time VmDas is restarted the session sequence number
is increased by one. Note that VmDas will choose a session
number that is as low as possible and will fill in gaps
in the session numbers so it is important for orderly
file management to let all the files for a cruise accumulate
in the directory until the end of the cruise, if possible.
The maximum size of the files is set in the options
file (typically 10 MB). When a file reaches maximum
size, a new file is started with the same session number
but with the file sequence number increased by one.
Different file types fill up faster than others so the
file sequence numbers do not necessarily correspond
to data taken within the same time window.
The file types and extensions generated by VmDas are
the following:
.ENR - Raw binary ADCP data file which contains every
ping
.ENS - Binary ADCP data after the data has been preliminarily
screened for backscatter and correlation
.ENX - Binary ADCP data after screening and rotation
to earth coordinate
.STA - Binary ADCP ensemble data that has been averaged
into short term average
.LTA - Binary ADCP ensemble data that has been averaged
into long term averages
.N1R - Raw NMEA ASCII data from the primary navigation
source
.N2R - Raw NMEA ASCII data from the secondary navigation
source, if available, and which should include Ashtech
heading data
.NMS - Binary screened and averaged navigation data
.VMO - This ASCII file is a copy of the *.ini options
file that was used during the data collection
.LOG - ASCII file containing a log of any errors
the ADCP detected during the session
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