PDS: The Planetary Atmospheres Node
The program that generated this data was funded by NASA to monitor Jupiter in the infrared, providing a long- term temporal and spatial context that supported the encounters of several spacecraft with the planet, e.g. This dataset covers part of the gap between the Galileo Mission and arrival of the Juno spacecraft.
This dataset was obtained using the Mid-Infrared Spectrometer and Imager (MIRSI) at NASA’s Infrared Telescope Facility (IRTF). Observations were made from December 2003 to September 2011and the dataset covers wavelengths 4.9 - 24.8 μm.
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PDS recommendations for citing data sets can be found here.
Orton, G., M. Venkatesan, K. Malavika, H. Mi , P. Yanamandra-Fisher (2025), jup_supp.irtf_mirsi bundle, PDS Atmospheres (ATM) Node, https://doi.org/10.17189/8hff-1a34
This dataset was obtained using the Mid-Infrared Spectrometer and Imager (MIRSI) at NASA’s Infrared Telescope Facility (IRTF). Observations were made from December 2003 to September 2011and the dataset covers wavelengths 4.9 - 24.8 μm.
Reference
Deutsch, L., J. Hora, J. Adams, M. Kassis. 2002. MIRSI: A mid-infrared spectrometer and imager. In Astronomical Telescopes and Instrumentation. Ed. A. M. Fowler. Proc. SPIE 4841, 106. https://doi.org/10.1117/12.461436
Accessing the Data
Note Overview of collections in the User’s guide.
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Citation
PDS recommendations for citing data sets can be found here.
Orton, G., M. Venkatesan, K. Malavika, H. Mi , P. Yanamandra-Fisher (2025), jup_supp.irtf_mirsi bundle, PDS Atmospheres (ATM) Node, https://doi.org/10.17189/8hff-1a34
