Reply to Comment by A. G. Davies on “Io Hot Spot Distribution Detected by Juno/JIRAM”

Abstract Zambon et al. (2023, https://doi.org/10.1029/2022gl100597) presented a catalog of Io hot spots based on JIRAM M‐band images acquired in Juno orbits 10 to 33. They identified 242 hot spots, including 23 not previously reported in other catalogs, observing a higher hot spot number density in...

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Main Authors: F. Zambon, A. Mura, F. Tosi
Format: Article
Language:English
Published: Wiley 2025-01-01
Series:Geophysical Research Letters
Online Access:https://doi.org/10.1029/2024GL112921
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author F. Zambon
A. Mura
F. Tosi
author_facet F. Zambon
A. Mura
F. Tosi
author_sort F. Zambon
collection DOAJ
description Abstract Zambon et al. (2023, https://doi.org/10.1029/2022gl100597) presented a catalog of Io hot spots based on JIRAM M‐band images acquired in Juno orbits 10 to 33. They identified 242 hot spots, including 23 not previously reported in other catalogs, observing a higher hot spot number density in the northern polar region. Davies (2024) disputes location and counting of part of these hot spots, attributing the differences between the Zambon et al. (2023, https://doi.org/10.1029/2022gl100597) results and those obtained by Davies et al. (2024, https://doi.org/10.1038/s41550‐023‐02123‐5) to a misregistration of the JIRAM images. Here we reply to Davies (2024) showing that discrepancies in the results are due to the different methodologies, assumptions, and goals considered in the two works.
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institution Kabale University
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series Geophysical Research Letters
spelling doaj-art-c412ee4dc0db41d5a5026beca55a97e82025-01-20T13:05:57ZengWileyGeophysical Research Letters0094-82761944-80072025-01-01521n/an/a10.1029/2024GL112921Reply to Comment by A. G. Davies on “Io Hot Spot Distribution Detected by Juno/JIRAM”F. Zambon0A. Mura1F. Tosi2Istituto Nazionale di Astrofisica – Istituto di Astrofisica e Planetologia Spaziali (INAF‐IAPS) Rome ItalyIstituto Nazionale di Astrofisica – Istituto di Astrofisica e Planetologia Spaziali (INAF‐IAPS) Rome ItalyIstituto Nazionale di Astrofisica – Istituto di Astrofisica e Planetologia Spaziali (INAF‐IAPS) Rome ItalyAbstract Zambon et al. (2023, https://doi.org/10.1029/2022gl100597) presented a catalog of Io hot spots based on JIRAM M‐band images acquired in Juno orbits 10 to 33. They identified 242 hot spots, including 23 not previously reported in other catalogs, observing a higher hot spot number density in the northern polar region. Davies (2024) disputes location and counting of part of these hot spots, attributing the differences between the Zambon et al. (2023, https://doi.org/10.1029/2022gl100597) results and those obtained by Davies et al. (2024, https://doi.org/10.1038/s41550‐023‐02123‐5) to a misregistration of the JIRAM images. Here we reply to Davies (2024) showing that discrepancies in the results are due to the different methodologies, assumptions, and goals considered in the two works.https://doi.org/10.1029/2024GL112921
spellingShingle F. Zambon
A. Mura
F. Tosi
Reply to Comment by A. G. Davies on “Io Hot Spot Distribution Detected by Juno/JIRAM”
Geophysical Research Letters
title Reply to Comment by A. G. Davies on “Io Hot Spot Distribution Detected by Juno/JIRAM”
title_full Reply to Comment by A. G. Davies on “Io Hot Spot Distribution Detected by Juno/JIRAM”
title_fullStr Reply to Comment by A. G. Davies on “Io Hot Spot Distribution Detected by Juno/JIRAM”
title_full_unstemmed Reply to Comment by A. G. Davies on “Io Hot Spot Distribution Detected by Juno/JIRAM”
title_short Reply to Comment by A. G. Davies on “Io Hot Spot Distribution Detected by Juno/JIRAM”
title_sort reply to comment by a g davies on io hot spot distribution detected by juno jiram
url https://doi.org/10.1029/2024GL112921
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