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Table 1.

Discontinuity events observed during February–July 2022.

Date/time (UT) Clouds (a) Wavelength (b) Observer
2022-02-04 16:55 Lower 2.26 μm IRTF/SpeX
2022-05-05 04:36 Middle > 742 nm C. Foster
06:13 Middle 820–920 nm A. Cidadão
2022-05-15 04:29 Middle > 742 nm C. Foster
08:16 Middle 820–920 nm A. Cidadão
2022-05-25 04:41 Middle > 742 nm C. Foster
07:58 Middle 820–920 nm A. Cidadão
2022-05-30 05:14 Middle > 742 nm C. Foster
09:06 Middle > 685 nm L. S. Viola
2022-06-04 05:09 Middle 820–920 nm L. Morrone
09:52 Middle 820–920 nm A. Cidadão
2022-06-13 14:05 Upper 345–380 nm VCO (c)/UVI
2022-06-14 23:05
2022-06-14 05:16 Middle 820–920 nm L. Morrone
2022-06-19 05:52 Middle 820–920 nm L. Morrone
06:48 Middle 820–920 nm A. Cidadão
2022-06-24 05:46 Middle 820–920 nm L. Morrone
07:36 Middle 820–920 nm A. Cidadão
2022-07-09 06:33 Middle 820–920 nm A. Cidadão
2022-07-13 10:33 Middle 820–920 nm A. Cidadão
2022-07-18 11:57 Middle 820–920 nm A. Cidadão
2022-07-23 06:27 Middle 820–920 nm L. Morrone
07:54 Middle 820–920 nm A. Cidadão
2022-07-28 09:21 Middle 820–920 nm A. Cidadão

Notes.

(a)

Approximate level sensed: dayside upper clouds (56.5–70 km above the surface), dayside middle clouds (50.5–56.5 km), and nightside lower clouds (47.5–50.5 km).

(b)

Filters used: contK (2.22–2.32 μm), Astronomik ProPlanet 742 IR-pass filter (> 742 nm), Baader SLOAN/SDSS z′−s′ (820–920 nm), Baader IR-Pass Filter (> 685 nm), and VCO/UVI 365 nm (345–380 nm).

(c)

Venus Climate Orbiter: Previous name of Akatsuki (Nakamura et al. 2007).

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