At 11:10 in the morning on November 28, 2005, the active lava delta at East Lae'apuki began to fall into the ocean. This was not a catastrophic collapse, with the entire 34-acre delta going at once, but instead occurred in a piece-meal fashion over a period of just less than 5 hours.
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At 11:10 in the morning on November 28, 2005, the active lava delta at East Lae'apuki began to fall into the ocean. This was not a catastrophic collapse, with the entire 34-acre delta going at once, but instead occurred in a piece-meal fashion over a period of just less than 5 hours.
Mount St. Helens' Crater Glacier's response to lava dome growth
Mount St. Helens' Crater Glacier's response to lava dome growthFrom 2005 to 2010, the U.S. Geological Survey-Cascades Volcano Observatory operated a remote camera on the northwest flank of Mount St. Helens. Looking into the crater, the camera captured hourly photographs of volcanic dome growth during the 2004-2008 eruption.
Mount St. Helens' Crater Glacier's response to lava dome growth
Mount St. Helens' Crater Glacier's response to lava dome growthFrom 2005 to 2010, the U.S. Geological Survey-Cascades Volcano Observatory operated a remote camera on the northwest flank of Mount St. Helens. Looking into the crater, the camera captured hourly photographs of volcanic dome growth during the 2004-2008 eruption.
Mount St. Helens: Instrumentation and Dome Growth, Sept 2005-Feb 2006
Mount St. Helens: Instrumentation and Dome Growth, Sept 2005-Feb 2006Events that occurred in the crater during the 2004–2008 eruption were recorded by a network of seven remote, telemetered digital single-lens reflex (DSLR) cameras installed on the crater floor and rim. The resulting time lapse images constitute a valuable and visually compelling record of dome growth and the resulting response of Crater Glacier.
Mount St. Helens: Instrumentation and Dome Growth, Sept 2005-Feb 2006
Mount St. Helens: Instrumentation and Dome Growth, Sept 2005-Feb 2006Events that occurred in the crater during the 2004–2008 eruption were recorded by a network of seven remote, telemetered digital single-lens reflex (DSLR) cameras installed on the crater floor and rim. The resulting time lapse images constitute a valuable and visually compelling record of dome growth and the resulting response of Crater Glacier.
Mount St. Helens: Instrumentation and Dome Growth, April - July 2005.
Mount St. Helens: Instrumentation and Dome Growth, April - July 2005.Lava spines continue to emerge onto the crater floor of Mount St. Helens in 2005. By April 2005, spine 4 is broken and pushed away by spine 5. The nearly vertical spine 5 has a smooth, gouge-covered surface, growing at an average rate of 4.3 meters per day.
Mount St. Helens: Instrumentation and Dome Growth, April - July 2005.
Mount St. Helens: Instrumentation and Dome Growth, April - July 2005.Lava spines continue to emerge onto the crater floor of Mount St. Helens in 2005. By April 2005, spine 4 is broken and pushed away by spine 5. The nearly vertical spine 5 has a smooth, gouge-covered surface, growing at an average rate of 4.3 meters per day.
Mount St. Helens: Instrumentation and Dome Growth, Feb - Mar 15, 2005
Mount St. Helens: Instrumentation and Dome Growth, Feb - Mar 15, 2005Growth and disintegration of lava spines continued at Mount St. Helens through the first 8 months of 2005. Rather than building a single dome-shaped structure, the new dome grew initially as a series of recumbent, smoothly surfaced spines that extruded to lengths of almost 500 m.
Mount St. Helens: Instrumentation and Dome Growth, Feb - Mar 15, 2005
Mount St. Helens: Instrumentation and Dome Growth, Feb - Mar 15, 2005Growth and disintegration of lava spines continued at Mount St. Helens through the first 8 months of 2005. Rather than building a single dome-shaped structure, the new dome grew initially as a series of recumbent, smoothly surfaced spines that extruded to lengths of almost 500 m.
Mount St. Helens: Instrumentation and Dome Growth, January 2005
Mount St. Helens: Instrumentation and Dome Growth, January 2005Within the crater of Mount St. Helens, the 2004–2008 lava dome grew by continuous extrusion of degassed lava spines. To track growth and anticipate what the volcano might do next, scientists installed monitoring equipment, including a camera and gas sensing instruments, and made helicopter overflights to collect the temperature (FLIR) of the growing dome.
Mount St. Helens: Instrumentation and Dome Growth, January 2005
Mount St. Helens: Instrumentation and Dome Growth, January 2005Within the crater of Mount St. Helens, the 2004–2008 lava dome grew by continuous extrusion of degassed lava spines. To track growth and anticipate what the volcano might do next, scientists installed monitoring equipment, including a camera and gas sensing instruments, and made helicopter overflights to collect the temperature (FLIR) of the growing dome.
Mount St. Helens eruption highlights: September 2004 - May 2005
Mount St. Helens eruption highlights: September 2004 - May 2005Compilation video of significant events from the dome-building eruption at Mount St. Helens, from October 1, 2004 to March 15, 2005, including steam and ash eruptions, growth of lava spines, helicopter deployment of monitoring equipment, collection of lava samples, and FLIR thermal imaging of rock collapse on lava dome.
Mount St. Helens eruption highlights: September 2004 - May 2005
Mount St. Helens eruption highlights: September 2004 - May 2005Compilation video of significant events from the dome-building eruption at Mount St. Helens, from October 1, 2004 to March 15, 2005, including steam and ash eruptions, growth of lava spines, helicopter deployment of monitoring equipment, collection of lava samples, and FLIR thermal imaging of rock collapse on lava dome.
Mount St. Helens: Instrumentation and Dome Growth, Nov-Dec 2004
Mount St. Helens: Instrumentation and Dome Growth, Nov-Dec 2004By late October 2004, a whaleback-shaped extrusion of solid lava (called a spine) emerged from Mount St. Helens' crater floor. The 2004–2008 lava dome grew by continuous extrusion of degassed lava spines that had mostly solidified at less than 1 km (0.62 mi) beneath the surface.
Mount St. Helens: Instrumentation and Dome Growth, Nov-Dec 2004
Mount St. Helens: Instrumentation and Dome Growth, Nov-Dec 2004By late October 2004, a whaleback-shaped extrusion of solid lava (called a spine) emerged from Mount St. Helens' crater floor. The 2004–2008 lava dome grew by continuous extrusion of degassed lava spines that had mostly solidified at less than 1 km (0.62 mi) beneath the surface.
Mount St. Helens: Instrumentation and Dome Growth, Oct 2004-Sept 2005
Mount St. Helens: Instrumentation and Dome Growth, Oct 2004-Sept 2005Following unrest that began on September 23, 2004 and the steam and ash eruptions in early October, extrusion of solid magma typified the 2004-2008 eruption at Mount St. Helens. The magma is unusually gas poor and crystal rich. Several meters of pulverized, variably sintered rock commonly coat the emergent lava spines, lending them a smooth appearance.
Mount St. Helens: Instrumentation and Dome Growth, Oct 2004-Sept 2005
Mount St. Helens: Instrumentation and Dome Growth, Oct 2004-Sept 2005Following unrest that began on September 23, 2004 and the steam and ash eruptions in early October, extrusion of solid magma typified the 2004-2008 eruption at Mount St. Helens. The magma is unusually gas poor and crystal rich. Several meters of pulverized, variably sintered rock commonly coat the emergent lava spines, lending them a smooth appearance.
Mount St. Helens: Instrumentation and Dome Growth, Oct-Nov, 2004
Mount St. Helens: Instrumentation and Dome Growth, Oct-Nov, 2004On October 11, 2004, spines of solid, but still hot, lava punctured the surface of the deformed glacier, initiating a new dome-building phase of activity in the crater of Mount St. Helens. By late October, a larger whaleback-shaped extrusion of solid lava (called a spine) emerged from the crater floor.
Mount St. Helens: Instrumentation and Dome Growth, Oct-Nov, 2004
Mount St. Helens: Instrumentation and Dome Growth, Oct-Nov, 2004On October 11, 2004, spines of solid, but still hot, lava punctured the surface of the deformed glacier, initiating a new dome-building phase of activity in the crater of Mount St. Helens. By late October, a larger whaleback-shaped extrusion of solid lava (called a spine) emerged from the crater floor.
Mount St. Helens: Steam, Ash Emissions and Dome Growth, October 2004
Mount St. Helens: Steam, Ash Emissions and Dome Growth, October 2004After two weeks of increasing seismicity, Mount St. Helens began erupting on October 1, 2004. The first of several explosions shot a plume of volcanic ash and gases into the atmosphere. Four additional steam and ash explosions occurred through October 5, and three produced noticeable fallout of fine ash downwind.
Mount St. Helens: Steam, Ash Emissions and Dome Growth, October 2004
Mount St. Helens: Steam, Ash Emissions and Dome Growth, October 2004After two weeks of increasing seismicity, Mount St. Helens began erupting on October 1, 2004. The first of several explosions shot a plume of volcanic ash and gases into the atmosphere. Four additional steam and ash explosions occurred through October 5, and three produced noticeable fallout of fine ash downwind.
On October 1, 2004, an explosion in the crater of Mount St. Helens sent ash and water vapor several thousand feet into the air. It was the dramatic beginning of an eruption that continued for the next 3+ years. The explosion fractured Crater Glacier and hurled rocks for at least one-half mile across the western half of the glacier and the 1980-1986 lava dome.
On October 1, 2004, an explosion in the crater of Mount St. Helens sent ash and water vapor several thousand feet into the air. It was the dramatic beginning of an eruption that continued for the next 3+ years. The explosion fractured Crater Glacier and hurled rocks for at least one-half mile across the western half of the glacier and the 1980-1986 lava dome.
Propagation of Seismic Waves, Atwood Building, Oblique View
Propagation of Seismic Waves, Atwood Building, Oblique ViewAnimation of the recorded displacements of Atwood Building, Anchorage, Alaska during the M=3.7 Point MacKenzie, Alaska earthquake of 15 Dec. 2003. Displacements are color coded in order to see the propagation of seismic waves in the building during the earthquake. Oblique view.
Propagation of Seismic Waves, Atwood Building, Oblique View
Propagation of Seismic Waves, Atwood Building, Oblique ViewAnimation of the recorded displacements of Atwood Building, Anchorage, Alaska during the M=3.7 Point MacKenzie, Alaska earthquake of 15 Dec. 2003. Displacements are color coded in order to see the propagation of seismic waves in the building during the earthquake. Oblique view.
Propagation of Seismic Waves in Atwood Building, Top View
Propagation of Seismic Waves in Atwood Building, Top ViewAnimation of the recorded displacements of Atwood Building, Anchorage, Alaska during the M=3.7 Point MacKenzie, Alaska earthquake of 15 Dec. 2003. Displacements are color coded in order to see the propagation of seismic waves in the building during the earthquake. View from top.
Propagation of Seismic Waves in Atwood Building, Top View
Propagation of Seismic Waves in Atwood Building, Top ViewAnimation of the recorded displacements of Atwood Building, Anchorage, Alaska during the M=3.7 Point MacKenzie, Alaska earthquake of 15 Dec. 2003. Displacements are color coded in order to see the propagation of seismic waves in the building during the earthquake. View from top.
Video Presentation and Discussion
Featuring the award-winning USGS video Molten Paradise-Kilaea Volcano by Stephen Wessells, introduced and discussed by Robert I. Tilling, Volcanologist
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Video Presentation and Discussion
Featuring the award-winning USGS video Molten Paradise-Kilaea Volcano by Stephen Wessells, introduced and discussed by Robert I. Tilling, Volcanologist
See-
New Estimates of Earthquake Hazard and Risk Across the Bay Region
By Michael Blanpied, Geophysicist
New Estimates of Earthquake Hazard and Risk Across the Bay Region
By Michael Blanpied, Geophysicist
Fluid lava leaks from inside crusted front of cascade
Fluid lava leaks from inside crusted front of cascadeFluid lava leaks from inside crusted front of cascade.
Fluid lava leaks from inside crusted front of cascade
Fluid lava leaks from inside crusted front of cascadeFluid lava leaks from inside crusted front of cascade.
Breaking and tumbling crust on slabby flow front.
Breaking and tumbling crust on slabby flow front.
PubTalk 12/2002 — Hawai`i's Volcanoes—Never a Dull Moment
PubTalk 12/2002 — Hawai`i's Volcanoes—Never a Dull Moment20 Years of Eruption at Kilauea and Waiting for Mauna Loa
by Don Swanson,Volcanologist, Hawaiian Volcano Observatory
PubTalk 12/2002 — Hawai`i's Volcanoes—Never a Dull Moment
PubTalk 12/2002 — Hawai`i's Volcanoes—Never a Dull Moment20 Years of Eruption at Kilauea and Waiting for Mauna Loa
by Don Swanson,Volcanologist, Hawaiian Volcano Observatory
PubTalk 10/2002 — Plumbing the Mysteries of the San Andreas Fault
PubTalk 10/2002 — Plumbing the Mysteries of the San Andreas FaultDeep Drilling to Test Fundamental Theories About Faulting and Earthquakes
By Stephen H. Hickman, Geophysicist
PubTalk 10/2002 — Plumbing the Mysteries of the San Andreas Fault
PubTalk 10/2002 — Plumbing the Mysteries of the San Andreas FaultDeep Drilling to Test Fundamental Theories About Faulting and Earthquakes
By Stephen H. Hickman, Geophysicist
PubTalk 6/2002 — Finding Elusive Earthquake Faults
PubTalk 6/2002 — Finding Elusive Earthquake FaultsNew Mapping Techniques Reveal Potential Seismic Sources Beneath Seattle
By Richard J. Blakely, Geophysicist and Ralph A. Haugerud, Geologist
PubTalk 6/2002 — Finding Elusive Earthquake Faults
PubTalk 6/2002 — Finding Elusive Earthquake FaultsNew Mapping Techniques Reveal Potential Seismic Sources Beneath Seattle
By Richard J. Blakely, Geophysicist and Ralph A. Haugerud, Geologist