λ=193゚Ls,
(ω=012°- 032°W,
φ=20°S),
δ=12.0",
ι=43°
Seeing: 4-5 /10.
Note:
The inside of the spc seems to show a rift in addition to the shadowy area. Margaritifer S and Aurorae S look dark, while their southern area adjacent to them is faint. Especially the area to the south of Margaritifer S is devastated to the extent of Argyre.
Notable is that the white mist along the EB is not seen. The northern area of M Acidalium shows a compact white cloud.
Instrument:
Use is made of an f /7.7 Newtonian extended to f /50 having a 25 cm speculum equipped with an ST-5C (at -5゚C).
Image data are
9 ~30 IR images each exposed with 0.1 secs
12~28 R + IR Rejection images each with 0.2 secs
10~16 G + IR Rejection images each with 0.1 secs
22~29 B + IR Rejection images each with 0.1 secs
Filters: Koh-Ei-Sha's interference RGB filter of Type 3.
The Morita Observatory is located (132.3°E, 34.3°N) at Hatsuka-ichi, Hiroshima, Japan.