Introduction
The Okhotsk Sea coast of Hokkaido, the northernmost island of Japan, is covered with sea ice approximately from the beginning of January to the end of March. The maximum thickness of flat, shore-fast ice in this area is about 50 cm. The height of hummocked ice sometimes reaches more than three metres above sea-level.
In order to observe in detail the distribution of pack ice off the coast of the Okhotsk Sea and to carry out basic research on its movement, the author constructed a radar network during 1967-69 (Reference Tabata and KarlssonTabata, 1969, Reference Tabata and Karlsson1972[a], Reference Tabata[b], Reference Tabata and Ōi[c])· It consists of three radar stations, installed on the mountain tops along the coast in Esashi, Mombetsu, and Abashiri; the radar stations are called by the names of these locations for instance, Esashi radar. The heights of antennas are 440 m, 300 m, and 200 m above sea-level and the radii of actual coverage are approximately 80, 70, and 60 km respectively. The sea area covered by the total system is about 70 km in width and 250 km in length along the north-eastern coast of Hokkaido. The radar stations are remotely controlled by radio from the Sea Ice Research Laboratory (SIRL) in downtown Mombetsu, part of the Institute of Low Temperature Science, and the information obtained is transmitted back by radio to SIRL.
This land-based radar network has the shortcoming of affording only a limited coverage. However, it has the fully compensating advantage of being able to provide continuous observations of ice distribution or movement.
Specification of radar
When pack ice is distributed over a wider area than the spread of antenna beams, and the cross-section σ of a target increases in proportion to the distance R, the receiver power P2 . will be expressed by the so-called radar equation:
where P1 is the transmitted power of the radar, G the power gain of the antenna, λ the wavelength, R the distance to the target, σo the scattering cross-section of the target at the distance Ro, H1 and h2 the heights of the antenna and target from sea-level respectively.
The frequency of the radar wave used was 5 540 MHz; this frequency is nearly the same as that of a normal weather radar. Considering the maintenance benefit, we chose a relatively small output, 40 kW, and a high antenna gain, 39 dB. The antenna is the cage type, 4.0 m in diameter and 1.3 m in height. The actual beam width was 1º in horizontal and 3º in vertical. Because the height of sea ice is very small as compared with that of the radar antenna, the effective distance mainly depends upon the height of the antenna. As the theoretically expected maximum coverage for park ice of our radar network is about 90 km. the repeating frequency was fixed as I kHz for a pulse width of 1.0 μS. The radar had two pulse widths, 1.0 and 0.2 μs. The pulse width has a close relationship with the sensitivity and effective coverage. As seen in Figure 1, we could have a more detailed picture with a narrow pulse width than with a wide one. However, because the repeating frequency of the former was 2 kHz, its effective coverage was reduced to less than half of the latter. The minimum receiver power of the radar system was — 100 dB m. Observed σ0 at R0 = 10 km was 0.24 0.76 m2.
For remote control a VHF radio signal in the 70 MHz band was used; the radar information obtained was transmitted back to SIRL by a radar relay system in the 7 GHz band.
Each unmanned radar station on a mountain had a monitor with a 10 inch (25 cm) screen. Observations were usually made using the two screens of the main indicator at SIRL. It was constructed as a console table incorporating a inch (40cm) screen. The two screens showed the same picture. Since the two screens of the main indicator pick up only one radar station, they were switched to the desired station whenever necessary so as to obtain the pack ice information from that station. Λ 35 mm still camera and a 16 mm movie camera were used to photograph a radar screen. The cameras were operated automatically or manually to take successive pictures of a screen at a desired time interval. The sketching of an ice-water boundary on a translucent sheet of paper attached to the screen was another effective method.
A small electronic computer was introduced in 1972 to process the radar information so that an interpretation of the surface topography of ice was provided.
Observation of the movement
In the radar image of pack ice, several distinctive features were always seen. They were, for instance, black spots (polynyas), bright spots (very high pressure ridges) and special features of the ice-water boundaries, etc. Some of these features conserved their characteristics for a considerable time interval, sometimes several days, so well that we could easily identify them in successive photographs of the radar screens taken at suitable time intervals. Hence, using these features as landmarks, we could easily study the movement of an ice field.
From observations of this movement on calm days when wind effects were negligible, it was estimated that in this area a sea current generally runs from north-west to south-east in winter, that is, parallel to the coast line, with an average speed of about 0.5 km/h (Reference TabataTabata, 1970).
The prevailing seasonal wind in winter is north-westerly; hence the ice fields generally move from north-west to south-east along the coastal line. The drift speed was 0.5-2.5 km/h, giving a wind factor of 0.01-0.08. Though the wind factor varied through such a wide range, it was found that changes of the drift speed were rather sensitive to changes of wind speed (Tabata, 1970).
Figure 2 shows an ice pattern observed by Mombetsu radar at 05.20 h, 25 February 1973. The white pattern in the upper right portion is pack ice and the black area is open water or polynyas. It is clear from the picture that the ice undergoes a turbulent movement.
Seven landmarks as seen in the figure were selected for a movement study. Their positions were traced every 30 min during 10 h; they are shown in Figure 3. As seen in the figure, as a whole, ice was drifting south-eastward along the coast line; this is the average pattern of drift in this area. However, the velocity of movement of each landmark was different from the others, showing that the ice field underwent internal deformation during its drift. The average speed of all landmarks was 1.7 km/h. The minimum and the maximum drift speeds were observed in landmarks A and D and were 1.1 and 2.3 km/h respectively. During the measurement, the wind velocity observed at the Mombetsu meteorological observatory was 1.0 to 4.8 m/s, the direction was SW before 01.00 h, W before 06.00 h and S until 10.00 h.
The deformation of an ice field could be studied with the aid of a set of three landmarks (Reference TabataTabata, 1971). Six triangles, as seen in Figure 3, were made by connecting the landmarks with each other. Applying the theory of homogeneous strain, we can obtain the strain of an ice field from the movement of a set of three landmarks. The obtained strain of an ice field other each set, that, is for each triangle seen in Figure 3, showed little correlation with each other. The time sequence of dilatation of triangle ABC (initial area: 75 km2) calculated from the data obtained every hour, and the changes of area of pentagon ABEFCA (initial area: 210 km2) and a hexagon (600 km2) were plotted in Figure 4 along with the wind speed. Though each dilatation (change of area) especially that of the hexagon, shows some correlation with the wind speed, correlations among the dilatations are rather poor, showing that the internal deformation of an ice field varies from place to place and also from time to time and that we must be careful in interpreting the strains obtained from the deformation of triangles.
The movement of pack ice shown in Figure 3 is rather simple as compared with that shown in Figure 5, which was observed 10 to 15 March 1973.
The complex movement and violent internal deformation of an ice field are best, and only vividly, seen in time-lapse movies of a radar screen. In 1974, four movies were made: they covered from 8 January to 31 March at Mombetsu radar; from 8 January to 13 March at Abashiri radar; from 21 to 27 February at both Mombetsu and Abashiri radars.
Computer processing of radar information
The complex pattern of deformation of an ice field is probably caused by the local differences of the surface and bottom features of ice-floes as well as by the wind and current patterns. As to the surface features, analyses of an A-scope image seem to give some information on them (Reference Ishida and OnoIshida and Ono, 1969; Reference IshidaIshida, 1971). A small computer was installed in 1972 to provide topographical information on ice by processing the A-scope images (Tabata and Ōi, 1972)·
Figure 6 represents an ice distribution off Abashiri observed on 5 March 1974 at 10.00 h; Figure 7 is a computer processed chart, where the intensity of echo signals is classified into eight steps from 1 to 8. These numbers have some correlations with the ice topography. The solid line is the coast line and the total coverage is 30 nautical miles (56 km). The radar station, represented by a "star", is in the center.
Figure 8, these eight numbers are replaced by eight kinds of graded shade to make the figure more vivid. To show the differences of ice patterns during six hours the pattern obtained at 16.80 h the same day is also shown in the figure. In these figures, the bigger the number, i.e. the darker the shade, the rougher the ice surface.
The movement of ice during these six hours will be obtained from the calculation of the two-dimensional cross-correlation of these patterns (Ishida, 1974). The rectangular part surrounded with a solid line is taken for this calculation; the area is 68 km X 42 km. As a preliminary test and also to avoid a difficulty in calculating the two-dimensional cross-correlation, we calculated the cross-correlation of a horizontal line of the two rectangles from Figure 8. The lag which shows the maximum value of correlation may be assumed to be the displacement of ice along this line. Such a displacement was calculated along each line. Next, in the vertical direction to the line, the displacement along each column was calculated.
The vector summation made at each intersection shows the movement of the ice field during six hours and is seen in Figure 9(a). The movement of ice in the following period from [6.08 to 20.57 h obtained in the same way is shown in Figure 9(b). This is just a preliminary test to calculate the movement of an ice field from the digitized radar information. Although much elaboration is necessary, the method of two-dimensional cross-correlation may be one of the most useful for obtaining ice movement.
Acknowledgements
The author would like to express his heartiest thanks to Professors T. Ishida and N. Ono for their advice and support. Thanks are also due to Messrs M. Aota, M. Ōi, M. Ishikawa, and H. Fukushi for their help in obtaining radar information as well as in data analyses.
Discussion
W. F. WEEKS: Please comment on your present understanding of the appreciable coastal current near your radar stations. How does it affect your analysis of the drift information as collected by the radar array?
T. TABATA: Analysis of ice movement on a calm day shows the existence of a current running south-eastward at 0.3-0.5 knots (0.6-0.7 km h-1). This current is limited to 10-20 km off the coast. It is believed to be a principal cause of anti-clockwise ice movement. However, much more information about the current is required for a full understanding of this point.
T. HUGHES: Were the clouds in your film low enough for cloud velocity vectors to be used to calculate a wind-stress field over the sea ice that could be compared with ice deformation?
TABATA: In our film the cloud movement is usually one-dimensional, while ice movement is usually two-dimensional. Therefore the cloud velocity vector could only be useful in special cases.