Loihi Volcano (Seamount). Hawaii.

Loihi Seamount is an active submarine volcano built on the seafloor south of Kilauea about 35 km from the Hawaii Island. The seamount rises to 969 m below sea level. Loihi is the newest volcano in the Hawaiian-Emperor seamount chain, a string of volcanoes that stretches over 5,800 km northwest of this volcano.
Location: 18.92 N 155.27 W.
Volume: 660 km3.
Like the volcanoes on the Island of Hawaii, Loihi has grown from eruptions along its 31-km-long rift zone that extends northwest and southeast of the caldera.

Loihi volcano (Seamount). Video.

 

Mauna Loa Volcano, Hawaii.

Mauna Loa volcano is one of five volcanoes that form the Island of Hawaii in the Pacific Ocean. Mauna Loa has is the world’s largest subaerial, its most active giant shield volcano.
Location: 19.475 N 155.608 W.
Elevation above sea level: 4,170 m.
Area: 5,271 km2 (50.5% of Hawaii island)
Volume: 80,000 km3.

Hawaii Mauna Loa Volcano Eruption&Lava Flow. Video.

 

Impressive Piton de la Fournaise volcano Eruption. Reunion Hotspot.

The origin of the Reunion Island is commonly attributed to a mantle hotspot. According to certain scientists, this hotspot first created the Deccan Traps, a large basalt province in India, about 65 million years ago. Its trace corresponds to Chagos-Lacadive Ridge, Mascarene Plateau, and Mauritius Island (created between 18 and 28 million years ago). Reunion became active about 5 million years ago, reaching the surface about 2 million years ago, and is the youngest island originating from this hotspot.

Piton de la Fournaise is a basaltic shield volcano on the eastern side of Reunion Island in the Indian Ocean. Piton de la Fournaise is one of the most active and the biggest volcanoes on Earth, along with Kilauea in the Hawaiian Islands (Pacific Ocean), Stromboli, Etna (Italy) and Mount Erebus in Antarctica. From the ocean floor, it is over 6,600 m tall. The base of the volcano has a diameter of 220 km.
Location: 21.23 S; 55.71 E.
Elevation: 2,631 m.
The Enclos Fouque, a caldera 8 kilometers wide, occupies the top part of the volcano. High cliffs known as remparts form the caldera’s rim. The caldera is breached to the southeast into the sea. It is unstable and is in the initial stages of failure. It will eventually collapse into the Indian Ocean to form giant landslides like those in Hawaii.
Three calderas formed at about 250,000, 65,000, and less than 5000 years ago by progressive eastward slumping of the volcano. Numerous pyroclastic cones dot the floor of the calderas and their outer flanks.


3D Model Of Yellowstone Hotspot and Plume

The Yellowstone plume has been tomographically imaged as a tilted body extending from 80 km depth at the Yellowstone Plateau to 660 km depth beneath western Montana. Geodynamic modeling of the plume finds that the plume is up to 120 K hotter than the surrounding mantle, with a maximum of 2.5% melt and a small buoyancy flux of 0.25 MG/s, properties of a cool, weak plume. Mantle flow modeling is used to constrain the evolution of the hotspot: the Yellowstone plume initially ascended vertically through the mantle beneath the thin, accreted lithosphere of the Columbia Plateau and was responsible for the 17 Ma flood basalts there. At 12 Ma, the plume passed beneath the thicker North American lithosphere and became entrained in eastward upper mantle return flow, resulting in a shift of volcanic activity to the southeast and the onset of rhyolitic eruptions caused by melting in the lithosphere. As the North America plate moved southwest, hotspot volcanism propagated northeast, and the resulting tectonic and magmatic interactions produced the 700-km-long Yellowstone-Snake River Plain magmatic system.

 


Credit:
University of Utah Seismology and Active Tectonics Research Group

Earth’s Hot Spots.

Hotspot is a place in the Upper mantle of the Earth at which hot magma from the Lower mantle upwells to melt through the crust usually in the interior of a tectonic plate to form a volcanic feature.
Region of the Earth’s upper mantle that upwells to melt through the crust to form a volcanic feature. Most volcanoes that cannot be ascribed either to a subduction zone or to seafloor spreading at midocean ridges are attributed to hot spots. The 5% of known world volcanoes not closely related to such plate margins (see plate tectonics) are regarded as hot-spot volcanoes. Hawaiian volcanoes are the best examples of this type, occurring near the centre of the northern portion of the Pacific Plate. A chain of extinct volcanoes or volcanic islands (and seamounts), such as the Hawaiian chain, can form over millions of years where a lithospheric plate moves over a hot spot. The active volcanoes all lie at one end of the chain or ridge, and the ages of the islands or the ridge increase with their distance from those sites of volcanic activity.

The surface manifestations of plumes, that is, columns of hot material, that rise from deep in the Earth’s mantle. Hot spots are widely distributed around the Earth. One of their characteristics is an abundance of volcanic activity which persists for long time periods (greater than 1 million years). When the lithosphere (the rigid outer layer of the Earth) moves over a plume, a chain of volcanoes is left behind that progressively increases in age along its length. Hot spots are believed to be fixed with respect to each other and the deep mantle so that the age and orientation of these chains provide information on the absolute motions of the tectonic plates.

Most recently proposed hotspots. Some are parts of “hotlines,” and some are inferred on the basis of age progressions rather than specific volcanic features. Red triangles indicate fifty-one hotspots, black squares volcanoes, black rings hotspots underlain by seismic low-velocity anomalies that extend into the transition zone, yellow rings the plumes proposed on the basis of seismic P-wave velocity tomography, and magenta rings plumes from the core-mantle boundary proposed on the basis of five criteria expected to be associated with plumes. If tectonic context is ignored, these are the strongest plume candidates. ( Anderson, D.L. and Schramm, K.A., 2005, Global Hotspot Maps, in Plates, Plumes & Paradigms, Foulger, G.R., Natland, J.H., Presnall, D.C, and Anderson, D.L., eds., Boulder, CO, Geological Society of America, Special Paper 388, pp. 19-29.)