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. 2020 Jun 28;125(7):e2019JE006369. doi: 10.1029/2019JE006369

Table 1.

Summary of Previous Observations of Waves in Jupiter's Clouds Detected at 5 μm or Shorter Wavelengths That Include Small‐Scale Waves, That Is, Those Shorter Than 1,000 km

Observing platform (year) Associated publications Range of planetocentric latitudes Range of wavelengths (km)
Voyager (1979) Hunt and Muller (1979), Flasar and Gierasch (1986) 27°S to 27°N 70–430
Galileo (1996) Bosak and Ingersoll (2002) 13°S 300
Galileo (1999) Arregi et al. (2009), Simon, Li, and Reuter (2015) 0.2°N, 3.6°N 155–205
Galileo (2001) Arregi et al. (2009) 1.8°S 195–215
New Horizons (2007) Reuter et al. (2007), Simon, Li, and Reuter (2015) 0° to 1.1°N 280–330
Juno/JIRAM (2017) Adriani, Moriconi, et al. (2018), Fletcher et al. (2018) 14° to 15°N 1,400–1,900
Juno/JunoCam (2017) Sánchez‐Lavega et al. (2018) 16°S 35
Hubble Space Telescope (2012–2018) Simon et al. (2018) 14.5° ± 2.5°N 1,220–1,340
Ground‐Based Visible Observations (2017) Simon et al. (2018) 14.5° ± 2.5°N 1,220–1,340
Ground‐Based 5‐μm Observations (2016–2017) Fletcher et al. (2018) 14.5° ± 2.5°N 1,300–1,600

Note. Some values are also displayed in Figure 16. The waves addressed by Sánchez‐Lavega et al. (2018) are associated with the Great Red Spot.