کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
8134813 1523510 2016 10 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Spatial distribution of Io's volcanic activity from near-IR adaptive optics observations on 100 nights in 2013-2015
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم فضا و نجوم
پیش نمایش صفحه اول مقاله
Spatial distribution of Io's volcanic activity from near-IR adaptive optics observations on 100 nights in 2013-2015
چکیده انگلیسی
The preferential occurrence of bright, violent eruptions at higher latitudes supports the idea that a deeper magma source supplies these events, as has been previously hypothesized. The monotonic eastward progression of bright eruptions at southern latitudes from 300° to 200°W also suggests a possible eruption triggering mechanism operating across distances of ∼500 km. A comparison to tidal heating models finds a good correspondence between recent models incorporating a partially-fluid interior (Tyler et al. [2015] Astrophys. J., 218-222). and hot spots in the leading hemisphere as well as persistent hot spots. However, hot spots on the trailing hemisphere and bright eruptions do not match these models well, corresponding better to standard deep-mantle heating models (Segatz et al. [1988] Icarus, 75, 187-206) although this match is still imperfect.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Icarus - Volume 280, December 2016, Pages 405-414
نویسندگان
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