The Glowing Avalanches: Pumice and Scoria Flows
"Fossil Fumaroles"
Kôzu observed that for more than 6 weeks after the great explosions of Komagatake, white columns of gas rose from the surface of the pumice flows, and some of them formed small ash cones, depositing sulphur, ammonium chloride, and iron chloride at their mouths. In the area covered by the pumice fall, on the other hand, even where the deposit was more than 3 meters thick, there were neither fumes nor sublimates. The surface of the pumice flows was
colored in streaks of yellow and brown, like a tiger skin, whereas that of the pumice fall was uniformly grayish white. These differences imply that the flows were much richer in gas and much hotter than the pumice fall. Measurements taken at a depth of
40 cm. below the surface showed that, in general, the temperature fell from about 350° to about 125° C. during the first 50 days. Thereafter the rate of cooling was much slower; in the next
100 days the temperature fell only from 125° to about 60° C., and during the next 640 days it fell to about that of the atmosphere. These measurements were taken on the flows where there was no special concentration of gas. But where gases were streaming off most abundantly, the temperatures were higher. At such places, temperatures of 450° and 510° C. were recorded between 8 and 11 days after the eruption, and more than 2 years later the temperatures at a depth of 40 cm. were still 99° and 60° C., respectively. Since the Komagatake pumice flows were thin and small compared with those of Mount Mazama, it cannot be doubted that the Mazama flows remained at higher temperatures for much longer periods. Being compact and almost cemented with dust, they must have been well insulated, and probably they continued to give off hot gases for many years, after the manner of the "sand flow" in the Valley of Ten Thousand Smokes.
The signs of fumarolic action within the flows are abundantly displayed near the rims of the canyons about Crater Lake. Beyond a distance of about 10 miles from the former summit of the volcano they disappear, for by the time the flows had moved that far they had lost much of their gas.
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Plate 17. Fig. 2. "Fossil fumarole" in Castle Creek canyon. Note figure at the base for scale; note also the massive, unbedded, coarse nature of the deposits on the far wall of
the canyon. (Photograph by National Park Service.) |
Visitors to Crater Lake entering along the valleys. of Annie and Sand creeks are familiar with the spectacular columns and spires that rise from the upper part of the canyon walls. These result partly from erosion of the pumice and scoria along vertical joints, and in this sense they are analogous in origin to the "earth pillars" commonly seen in "badlands." But many occur where the pumice and scoria deposits are cut by vertical cracks the walls of which are cemented by iron oxides, kaolin, and opal. These are in fact "fossil fumaroles." Brown, pink, and white streaks cut the gray scoria where the gases rose to the surface. Some of the spires are hollow inside and have irregular openings at the top. The largest of these tubular spires is 8 feet across and may be seen near Llao's Hallway, in a tributary of Castle Creek. One of them is shown in plate 17, figure 2. All occur within the upper part of the scoria layer. On Sand Creek, as many as 150 "fossil fumaroles" may be counted in a distance of 1
1/2 miles along the canyon walls.
Above the columns and spires, and within a few feet of the top of the flows, there is usually a distinct pink or brick-red zone, several feet in thickness. In places, particularly above the tubular openings mentioned, the pink color is intense. Where the color is deepest, pink and brown streaks lead from cracks below. It is not only in the canyons that this feature is to be seen, for all over the Pumice Desert and along Desert Creek the deposits are characterized by pink and brown blotches, the traces of thousands of fumaroles. Usually the discoloration is most marked where scoria predominates, but it may also be seen in flows of dacite pumice, as along the Diamond Lake highway above Union Creek. The reason is of course that the scoria contains much more iron than the dacite pumice, and it was the oxidation of iron-bearing gases, probably iron chlorides, that caused the pink color. Gases rising from the hot ejecta reacted with the air and percolating rains, and the level of oxidation depended largely on the porosity of the topmost materials. Usually the pink zone is at the top of the pumice-scoria deposits or a short distance above, in the overlying layer of ash. It follows that the ash must have fallen soon if not immediately after the flows had come to rest, and while they were still emitting gas.
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Plate 17. Fig. 3. Pumice deposits on Diamond Lake highway. At the base, 4 feet of coarse, unbedded pumice-flow deposits containing a charcoal log (near hammer). Above, bedded,
fine pumice fall. The dark band near the top is the pink zone caused by oxidation of fumarolic gases rising from the pumice flow at the base. This indicates that the fine pumice
fell on the flow while it was still hot. |
A spectacular instance of this kind may be seen near where the Diamond Lake highway crosses the Rogue River. Here the coarse, unbedded pumice flow is overlain by fine, well bedded pumice fall up to 15 feet in thickness (plate 17, figure 3). Yet the pink, fumarolic zone occurs not within the flow, but between 3 and
5 feet from the top of the overlying bedded pumice.
When one sees these extensive signs of fumarolic action, one is tempted to imagine how the slopes of Mount Mazama may have appeared at the close of the great eruptions. The glowing avalanches had converted the glacial canyons into wide, barren plains from which, for years, plumes of acid gas rose into the air. Long after the fumaroles had almost dwindled to extinction, the plains must have been hidden by dense clouds of steam when rains fell on the hot deposits. Nothing remained of the scant forests that had formerly clothed the lower slopes of the volcano. The ridges between the plains of "ten thousand smokes" were mantled by a gray-white pall of granular pumice. The summit of Mount Mazama had gone, leaving in its place a vast caldera, 6 miles wide. Of the long glaciers which had formerly covered the upper part of the cone, only three small relics survived in the valleys on the southern slope. It would
be difficult to imagine a scene of greater desolation. For an artist's reconstruction of the appearance of the mountain before and after the eruptions, see plate 18, figures 1 and 2.
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Plate 18. Fig. 1. Mount Mazama immediately before the collapse of the summit, looking north from near Union Peak. From a
painting by Paul Rockwood. Shows the general configuration of the volcano when the culminating eruptions began. Wind blowing to the northeast, carrying granular pumice.
Typical cauliflower eruption clouds such as must have formed during the opening activity. The three glaciers on the south slope of the volcano are, from left to right,
the Munson, Sun, and Kerry Valley glaciers. Below them stretch bare, U-shaped glacial canyons. The small cone near the center of the picture is the parasitic Crater
Peak. Pumice Flat in left foreground.
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Plate 18. Fig. 2. Mount Mazama immediately after the collapse of the summit. From a painting by Paul
Rockwood. Compare figure 1, above. Note that the U-shaped glacial canyons have been filled with the deposits of glowing avalanches (nuées ardentes), from which
countless fumaroles give off gas. The plains beyond the caldera are also covered with pumice-scoria flows which discharge fumaroles. Note that pumice is almost absent
on the west (left) slope of the volcano and thickens toward the east. The beheaded glaciers of Munson, Sun, and Kerr valleys are shown. The caldera floor lies
approximately 2000 to 4000 feet below the rim.
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