By Annie Kell
Our 3D survey has the first objective of imaging Axial volcano
is to see the details of the main and satellite magma chambers. Though we have
this idea that volcanoes hold magma in a single and simple reservoir of magma
and where there is no variation in the types of magma melt, the reality is that
volcanoes have a more complicated system! There are many arms and pathways
inside the system and there are variations of the actual chemical composition
of magma.
The magma body:
When we think volcano and magma chamber, we think of it like
a single tank underground with an opening on top, like what is illustrated in
the first figure below. In this mental picture, pressure builds and the magma
either blows or seeps out of the top of the “tank.”
In an idealized setting, the volcano is very simple with one magma chamber and one vent.
https://alchetron.com/cdn/magma-chamber-a949bbe6-88eb-4aa1-8875-1c337c7c633-resize-750.jpg
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In observations of volcanic systems, the tank that holds the magma is complicated. It can be a combination of small chambers that are connected through fractures or conduits. The chambers can be mostly vertical, called dikes, or can be more horizontal, called sills (see the next image). Because there are few examples of the “text book” magma chamber, a lot can be learned by seeing an actual system and by seeing that system in 3D. The AXIAL3D Expedition will answer the fundamental questions that cannot be answered with 2D data and that are still lingering about this system. By seeing the large and small paths that make up the magma chamber, we can see how melt is stored in reality. The magma is moving from beneath the crust, within the crust and then to the surface of the earth. We will get to see that path! And in 3D!
Some of these
magma are not like the others:
Not all magma is the same. Magma is a variable material! Some
magma is very melted, meaning it has a larger proportion of liquid. In other
systems and (as we are learning) sometimes within the same system, the magma is
more crystalized. More crystalized means the material is not as melted but
rather has some “solidus” in the melt.
Within the Axial magma chambers, there are pockets where magma is more
melt rich and where there is more crystallization. How do we tell this?!? The magma
is deep within the earth so we cannot sample it! This is where the seismic data
comes in.
As mentioned earlier, we record reflections of seismic waves
off of all the material deep underground. Depending on the material, the
amplitude of the reflected wave changes. Seismic data shows variations in the
recorded amplitudes and we can plot those variations in many different ways. In
order to distinguish areas that are more crystalline from areas that are more
melted we conduct a type of seismic analysis called Amplitude Versus Offset or
AVO. Offset is simply the distance between the seismic source to the seismic
receiver. We look at the dependencies between the amplitude of the returned
wave and the offset from the source. The cartoon image of a 2D profile below
gives a bit of a picture of how offset and amplitude change along the length of
the receiver array. AVO analysis can give a lot of details about a materials
density, fluid percentage (thus melt variation) and material porosity.
So depending on HOW we analyze the data, we can tell the
internal structure AND we can get indicators of material composition. All from
the same data collection! These 2 direct uses of the seismic data are the first
learning objective for this study. We will cover more about further objectives
later.
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