Whereas expensive, custom built solutions had been very
acceptable in the military systems of the 1980s, there has been
a shift towards more modestly priced hardware and, indeed,
the graphics engines offered by workstation manufacturers in
their standard configurations have become sufficient. Such
devices are required for stereoscopic viewing, unless split
screen is used, because the graphics cards supplied as standard
with most workstations either have too slow refresh rates (over
100 Hz is required) to display the left and right images
alternately on the screen in fast enough succession to please
the human eye, or because there is no convenient way of
handling two images. Helava and Intergraph led the way with
VITec-30 and VITec-50 processors and boards from companies
like 3Dlabs, Peritek and Teksource have been used too. Note
that while some of these processors have on board VRAM,
others make use of imagery held in main system RAM. So in
the case of the Creator 3D graphics of the Sun Ultra, for
example, Leica-Helava recommend at least 128 MB RAM.
These graphics sub-systems also help with image roaming,
though skilful use of their firmware is required to achieve
smooth motion at sufficient refresh rates. In many cases,
image roam is still achieved only piecewise, i.e. within the
imagery stored in the VRAM or the system RAM allocated to
graphics. Smooth roaming over an entire stereo model with
heavy graphics overlays of vector data or contours has barely
been achieved with off the shelf hardware. Naturally, the
fastest transfer of data is critical between VRAM, RAM and
hard disk. It is interesting that Sun has moved off its long
established SBus for the graphics of the higher end Ultra
models and SGI's reputation for fast graphics has been founded
to some extent in its excellent use of the PCI bus. While it is
not unreasonable for users to demand the same smooth
roaming all over the image that they have enjoyed for two
decades with APs, it is worth noting that this is a real issue
only with feature extraction - in most other digital
photogrammetric operations it is of little significance. Many
operators, too, having tried the DPW roaming and found it to
be inferior to APs, change to fixed image moving cursor mode
and become quite content.
Special hardware has also been used for compression. The
JPEG board offered as an option by Intergraph, for example,
has been very successful, though the latest workstations can
perform software compression at more than one MB/sec and
are fast enough for decompression on the fly during processing.
2.2.2 Storage and archiving. It has already been stated that
the large data volumes make heavy demands on storage. The
host computers are usually supplied with at least one internal
hard disk of 1-2 GB and, usually, one or more external hard
disks of 2-9 GB each. Thus many users take delivery of
systems with 5-10 GB per workstation and in many cases
expand on this soon after. In most cases the SCSI-2 standard is
preferred but fast and wide SCSI-2, offering 20 MB/sec, i.e.
twice as fast, is available as an option on most workstations
and is standard on some models of the Sun Ultra. Power users
sometimes opt for RAID technology, not so much to take
advantage of its data security features but to obtain high speed
and very large capacity with a single SCSI-2 device. RAIDs of
10-60 GB are quite common.
The data volumes preclude the use of floppy disks, even
modem high capacity models, for other than control files,
orientation results or vector data. QIC tapes, with capacities
typically below one GB, are also rather unsuitable. Despite
capacities currently of around 650 MB, CDs have become
quite popular, especially as a means for users of DPWs to
supply final deliverables to their customers. CD juke boxes
ameliorate the problems, but 650 MB is sufficient to contain
387
only one stereo pair of 12.5 um images. Optical disks, which
are currently increasing from 1.3 to 2.6 GB, have rather more
potential than CDs, but appear to be handicapped by a
multiplicity of standards and formats. Old fashioned reel to
reel tape drives are becoming less common but still find use as
input devices for remotely sensed data, of which they were the
standard distribution medium for many years.
The industry seems to have settled for the moment on high
capacity tape cartridge technology for off-line storage and
archiving. The popular DAT and Exabyte equipment, for
example, uses helical scan technology for writing and reading
the data. Exabyte capacities are 7 -14 GB per tape depending
on the effectiveness of in-built compression firmware. More
recently, vendors such as Sun have announced even higher
performance DLT (digital linear tape) units with 20 GB or
more per tape. In most cases juke boxes are available, but it
must not be forgotten that back up and restore are lengthy
operations: at one MB/sec peak rate, for example, it may take
several hours to read one tape.
2.3 Viewing systems
2.3.1 Monoscopic or stereoscopic? Photogrammetrists have
been preoccupied with stereoscopic viewing for decades and
this has been a big issue with DPWs too, but it is necessary to
pause to review the situation and discern the directions for the
near future. Many operations in digital photogrammetry are
not stereoscopic at all and in this respect DPWs differ from
APs: project management, image import, automated aspects of
triangulation, DTM generation, orthophoto computation and
mosaicking, perspective scenes and image map production are
all entirely possible monoscopically. Only three operations are
inherently stereoscopic: (i) measurement of ground control
points, where a single monoscopic measurement followed by
image matching for transfer to all the other images may be
satisfactory for targetted points but is likely to be a source of
error in all other cases; (ii) editing of automatically generated
DTMs; and (iii) feature extraction. The last two of these,
however, will become increasingly automated, as the
discussions in sections 3.4 and 3.6 below conclude. Moreover,
the trend towards head-up digitising on digital orthophotos
seems to be a strong one. Thus stereoscopic viewing will be
needed on a decreasing proportion of the DPWSs at each site.
2.3.2 Monitors. Whether there is stereoscopic viewing or not,
almost all DPWs have at least one monitor on which several
windows appear, one or more of them containing imagery. In
some cases this imagery may be 24 bit colour, which is best
displayed in 24 bit colour. Thus a high quality monitor with
high resolution is mandatory. The use of 640 x 480 VGA
displays is a thing of the past! Probably 1280 x 1024 is the
most popular resolution, but values around 800 x 600 are
sometimes used with entry level systems and Intergraph
showed the way with its “two megapixel" screen used from the
early days of the ImageStation at the beginning of the decade.
The systems which include a second monitor for the stereo
display almost invariably offer a high quality 1280 x 1024
unit, but note that the number of “stereo pixels” generated by
the graphics-subsystems is smaller than this. The Leica-Helava
systems, for example, have offered a range from 640 x 480 on
VITec-30 and 640 x 492 on SGI XL to 960 x 680 on Sun ZX
and Creator 3D and probably 1024 x 768 on SGI High Impact.
The floating mark is created by using of a cluster of pixels to
form a cross, circle or other preferred pattern. This moves, of
course, in single pixel increments, which can be a little
disturbing in that to an experienced AP operator movement
may appear to be jerky or insufficiently precise, though for
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B2. Vienna 1996