Autonomous volcanic plume detection on planetary bodies
详细信息 查看全文
- 作者：Yucong Lin<sup> ; sup><sup>Yucong.Lin@asu.edu" class="auth_mailsup> ; Melissa Bunte <sup>Melissa.Bunte@asu.edu" class="auth_mailsup> ; Srikanth Saripalli <sup>Srikanth.Saripalli@asu.edu" class="auth_mailsup> ; James Bell III <sup>Jim.Bell@asu.edu" class="auth_mailsup> ; Ronald Greeley<sup>1sup>
- 关键词：Spacecraft images ; Feature detection ; Volcanic plume ; Planetary body
- 刊名：Acta Astronautica
- 出版年：April-May, 2014
- 年：2014
- 卷：97
- 期：Complete
- 页码：151-163
- 全文大小：7138 K
文摘
Explosive eruptive events and outgassing have been observed at several outer solar system bodies. These events indicate a range of geophysical activity and ensure that the bodies remain targets of interest for future observations. Characterizing the events demands an inordinate fraction of spacecraft's limited resources. We have developed algorithms for onboard characterization of geophysical signatures such as eruptive events and surface features in order to facilitate rapid detection and conserve data volume. We applied supervised classification (K Nearest Neighbor) on SIFT (Scale Invariant Feature Transform) features extracted from spacecraft images where such transient events are known to exist. This method evidenced successful performance on images of Io from the Voyager. Galileo, and New Horizons missions, and images of Enceladus from the Cassini missions. It is able to detect plumes of different shapes, sizes and orientations. We show a positive detection rate of 68-96% of known plumes on Io, Enceladus. Additionally, we show that a similar technique is applicable to differentiating geologic features which exhibit similar appearances.