The seeing condition is poor (2/10), and the apparent diameter is still 4.4".
Solis L seems to show up near the evening terminator. The evening mist is visible.
MORITA uses 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
20 IR images each exposed with 0.1 secs
20 R + IR Rejection images each with 0.2 secs
10 G + IR Rejection images each with 0.5 secs
10 B + IR Rejection images each with 1 secs
From this time MORITA begins to use the Koh-Eisha RGB filter Type 3.
MORITA's observing site is located at Hatsuka-ichi, Hiroshima He is a CMO member ever since July 1992 (cf CMO #122)