Dynamic infrared aurora on Jupiter
Abstract Auroral emissions are an important diagnostic for a planet’s magnetosphere and upper atmosphere. At the outer planets, the characteristics of emission from the triatomic hydrogen ion $${{\rm{H}}}_{3}^{+}$$ H 3 + are key to understanding the auroral energy budget. We present James Webb Space...
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| Main Authors: | , , , , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Nature Portfolio
2025-05-01
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| Series: | Nature Communications |
| Online Access: | https://doi.org/10.1038/s41467-025-58984-z |
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