Images

GPS monitoring station P709 is located on The Promontory between the South Arm and Southeast Arm of Yellowstone Lake. It was installed in 2005 as part of the Yellowstone component of the National Science Foundation's Plate Boundary Observatory (PBO) under permit YELL-SCI-5546. Photo from UNAVCO station overview page.

The GeoGirls examined tephra (ash and pumice) deposits from Mount St. Helens’ eruptive past and learned how to create a stratigraphic column.

An Unmanned Aircraft Systems overflight of fissure 8 on Saturday afternoon (Sept. 1, 2018) showed incandescence within the cinder cone, with reports that lava had covered the 65x15 m (210x45 ft) crater floor by evening.

Southeast arm of Yellowstone Lake. Photo by Neal Herbert, Yellowstone National Park. Photo source: https://www.flickr.com/photos/yellowstonenps/15005709247/

An Unmanned Aircraft Systems overflight on Sunday afternoon (Sept. 2, 2018) showed that lava remained active within the fissure 8 cone.

This UAS oblique image of fissure 8 shows that the new lava is mostly confined to the crater floor within the cone, although a small amount extended a short distance into the spillway. HVO geologists noted that the lava activity was at a low level, with the area of incandescence decreasing to almost zero over the course of the afternoon.

Early this morning, the Unmanned Aircraft Systems team was able to conduct a brief overflight of fissure 8 between passing rain showers, which resulted in abundant steaming on the flow field.

A black sand beach blocks the boat ramp at Isaac Hale Beach Park. The beach consists of fragmented lava rock that is slowly migrating west at Pohoiki Bay.

Geologic field-trip guide of volcaniclastic sediments from snow- and ice-capped volcanoes—Mount St. Helens, Washington, and Mount Hood, Oregon: U.S. Geological Survey Scientific Investigations Report 2017–5022–F, 97 p., https://doi.org/10.3133/sir20175022F.

Another aerial view of the summit crater from this morning's overflight. Zoom in to see HVO and the Park's Jaggar Museum on the caldera rim (right side of photo).

HVO field crews carefully traverse the uneven surface of the channel levee (left of image) to make measurements of the fissure 8 lava channel. The lava is slowly cooling and contracting but the area remains warm (note the steam rising). The view is to the east, with Puu Honuaula in the distance (right of image).

Void spaces within the cooled lava channel and along the channel margins create hazardous conditions on the fissure 8 flow field. Here, part of the void is visible, but a fragile veneer of lava hides other parts of it (upper right).

The caldera floor near Halema‘uma‘u is a jumble of down-dropped blocks and surface cracks. HVO field crews hiked along the roadway to verify the location of benchmarks (lower left) and prepare for additional geophysical work to document the changes. The road provided access to the Overlook parking area, closed since 2008.

This morning, USGS scientists flying over fissure 8 noticed a change in the vent from yesterday. Gas jets were throwing spatter—fragments of glassy lava (light gray deposits)—from small incandescent areas deep within the cone. This activity is an indication that the lower East Rift Zone eruption may be paused rather than pau (over).

Data from continuous GPS stations indicate how the ground is moving over time. Station WLWY, near White Lake on the Sour Creek resurgent dome in Yellowstone caldera, has been operating since 2001. This plot shows vertical ground motion recorded at the site.

USGS and Washington State Department of Ecology scientists are geared up and ready to start a topographic survey at the mouth of the Elwha River, using handheld computers and backpack-mounted GPS equipment. From left to right are Owen Warrick (USGS Volunteer), Jon Warrick (USGS), Andy Ritchie (USGS), Heather Weiner (WA State Dept.

View from the bank of the cooling lava channel near the Leilani Estates subdivision. The height difference between the channel (right) and upper bank (left) is about 8 m (26 ft). Although lava is not flowing from fissure 8, the lava flow field includes large areas of still-hot, rugged, and unstable lava surfaces.

View from this morning's helicopter overflight of the Pohoiki boat ramp at Isaac Hale Park shows black sand, transported to the southwest by longshore currents, blocking the entrance to the small boat harbor.

Temperature record from Echinus geyser outflow channel for October 17–20, 2017. The plot captures a time when the geyser went from occasional eruptions to semi-regular eruptions (signified by temperature spikes after about 12:00 on October 18) occurring about every 2 hours.

Lava continues to ooze into the ocean at scattered entries along the Kapoho (pictured) and Ahalanui lobes.

A sand bar has built up at the end of the Pohoiki boat ramp, but the ramp itself remains intact and there has been no significant lava advance toward the ramp in recent days.