{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,3,4]],"date-time":"2026-03-04T02:30:56Z","timestamp":1772591456942,"version":"3.50.1"},"reference-count":47,"publisher":"MDPI AG","issue":"21","license":[{"start":{"date-parts":[[2020,11,5]],"date-time":"2020-11-05T00:00:00Z","timestamp":1604534400000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Remote Sensing"],"abstract":"<jats:p>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.<\/jats:p>","DOI":"10.3390\/rs12213629","type":"journal-article","created":{"date-parts":[[2020,11,5]],"date-time":"2020-11-05T09:04:34Z","timestamp":1604567074000},"page":"3629","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":19,"title":["Multisensor Characterization of the Incandescent Jet Region of Lava Fountain-Fed Tephra Plumes"],"prefix":"10.3390","volume":"12","author":[{"ORCID":"https:\/\/orcid.org\/0000-0003-0303-1171","authenticated-orcid":false,"given":"Luigi","family":"Mereu","sequence":"first","affiliation":[{"name":"Department of Information Engineering, Sapienza University of Rome, 00184 Rome, Italy"},{"name":"Center of Excellence CETEMPS, 67100 L\u2019Aquila, Italy"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-8704-8629","authenticated-orcid":false,"given":"Simona","family":"Scollo","sequence":"additional","affiliation":[{"name":"Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Etneo, 95125 Catania, Italy"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-2368-2193","authenticated-orcid":false,"given":"Costanza","family":"Bonadonna","sequence":"additional","affiliation":[{"name":"Department of Earth Sciences, University of Geneva, 1205 Geneva, Switzerland"}]},{"given":"Valentin","family":"Freret-Lorgeril","sequence":"additional","affiliation":[{"name":"Department of Earth Sciences, University of Geneva, 1205 Geneva, Switzerland"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-5873-204X","authenticated-orcid":false,"given":"Frank Silvio","family":"Marzano","sequence":"additional","affiliation":[{"name":"Department of Information Engineering, Sapienza University of Rome, 00184 Rome, Italy"},{"name":"Center of Excellence CETEMPS, 67100 L\u2019Aquila, Italy"}]}],"member":"1968","published-online":{"date-parts":[[2020,11,5]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","unstructured":"Du Preez, D.V., Bencherif, H., B\u00e8gue, N., Clarisse, L., Hoffman, R.F., and Wright, C.Y. 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