Abstract

Explosive basaltic eruptions eject a great amount of pyroclastic material into the atmosphere, forming columns rising to several kilometers above the eruptive vent and causing significant disruption to both proximal and distal communities. Here, we analyze data, collected by an X-band polarimetric weather radar and an L-band Doppler fixed-pointing radar, as well as by a thermal infrared (TIR) camera, in relation to lava fountain-fed tephra plumes at the Etna volcano in Italy. We clearly identify a jet, mainly composed of lapilli and bombs mixed with hot gas in the first portion of these volcanic plumes and here called the incandescent jet region (IJR). At Etna and due to the TIR camera configuration, the IJR typically corresponds to the region that saturates thermal images. We find that the IJR is correlated to a unique signature in polarimetric radar data as it represents a zone with a relatively high reflectivity and a low copolar correlation coefficient. Analyzing five recent Etna eruptions occurring in 2013 and 2015, we propose a jet region radar retrieval algorithm (JR3A), based on a decision-tree combining polarimetric X-band observables with L-band radar constraints, aiming at the IJR height detection during the explosive eruptions. The height of the IJR does not exactly correspond to the height of the lava fountain due to a different altitude, potentially reached by lapilli and blocks detected by the X-band weather radar. Nonetheless, it can be used as a proxy of the lava fountain height in order to obtain a first approximation of the exit velocity of the mixture and, therefore, of the mass eruption rate. The comparisons between the JR3A estimates of IJR heights with the corresponding values recovered from TIR imagery, show a fairly good agreement with differences of less than 20% in clear air conditions, whereas the difference between JR3A estimates of IJR height values and those derived from L-band radar data only are greater than 40%. The advantage of using an X-band polarimetric weather radar in an early warning system is that it provides information in all weather conditions. As a matter of fact, we show that JR3A retrievals can also be obtained in cloudy conditions when the TIR camera data cannot be processed.

Highlights

  • Explosive eruptions eject large volumes of volcanic particles having different size from micrometers to meters

  • We will demonstrate the potential of using X-band polarimetric radar observables, such as ρhv jointly with Zhh, together with L-band radar constraints, to detect and estimate the incandescent jet region (IJR) height

  • We will compare radar-based retrievals of IJR height with the estimates extracted from the thermal infrared (TIR) camera

Read more

Summary

Introduction

Explosive eruptions eject large volumes of volcanic particles (i.e., tephra) having different size from micrometers to meters. During the most intense explosive events, volcanic ash can reach the stratosphere, sometimes encircling the globe (e.g., Cordon Caulle 2011 eruption, Chile) [1]. Tephra is mixed with gas (e.g., water and CO2) that controls the dynamics of explosive eruptions [2]. This mixture rises first due to gas expansion (gas-thrust region) and to buoyancy after the sufficient entrainment of air (convective region). When the mixture eventually reaches the atmospheric density, it starts spreading horizontally (umbrella region) [2]. Tephra are deposited thousands of kilometers from the vent, affecting communities at variable temporal and spatial scales [3,4]

Methods
Results
Conclusion
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call