@article{475c66d4774b4e739c13e4098d81157d,
title = "Mid-infrared observations of Io's volcanism from the ground in 2011 and 2012",
abstract = "We report the latest volcanic activity on Io based on our ground-based observations made in 2011 and 2012 using just a 1-m telescope, at 8.9μm where Io's thermal radiation dominates solar reflected light seen at shorter wavelengths. A particular result from these observations is that the power we detected from a bright hotspot at the longitude of 282 ± 18°, perhaps Daedalus Patera, was ~1013 (W) which is comparable to that of Loki Patera, the most powerful volcanic hotspot on Io. We conclude this hotspot is one of the most powerful volcanic hotspots on Io, but its activation is not as frequent as Loki Patera.",
keywords = "Io, Jupiter, Jupiter, satellites, Volcanism",
author = "M. Yoneda and T. Miyata and Tsang, {C. C.C.} and S. Sako and T. Kamizuka and T. Nakamura and T. Asano and M. Uchiyama and K. Okada and Y. Hayashi and Y. Yoshii and M. Kagitani and T. Sakanoi and Y. Kasaba and S. Okano",
note = "Funding Information: The authors would like to thank two anonymous reviewers. This research was supported by a special fund for education and research provided by the Ministry of Education, Culture, Sports, Science and Technology to the Planetary Plasma and Atmospheric Research Center at Tohoku University, Japan. The observatory in this research is maintained by the Institute of Astronomy, the University of Tokyo. At Tohoku University Japan, this work was supported in part by a Grant-in-Aid for Fellows of Japan Society for the Promotion of Science (K224403007).",
year = "2014",
month = jul,
day = "1",
doi = "10.1016/j.icarus.2014.01.019",
language = "English",
volume = "236",
pages = "153--156",
journal = "Icarus",
issn = "0019-1035",
publisher = "Academic Press Inc.",
}