Dear SN watchers, IAUC 7979 informed the spectral classification of two SNe. SN 2002fi: In [vsnet-obs 41399]: (Sept. 18) >SN2002fi 20020828.4 <190:C KAI >SN2002fi 20020913.4 185:C KAI >SN2002fi 20020917.4 183:C KAI > ># MCG -04-7-10, a host galaxy of SN 2002fi, is a distant spiral ># ((R'?)SA(s)a) galaxy. The reported magnitude is coincident with ># the expected maximum for typical SN Ia. It was indeed of type Ia. Features resembles that of 20 days after maximum on Sept. 26. SN 2002fj: In [vsnet-campaign-sn 475]: (Sept. 20) ># NGC 2642, a host galaxy of SN 2002fj, is a barred-spiral (SB(r)bc) ># galaxy in a dawn sky. SN is located at the east end of the bar, and ># just south of a foreground star (mag 13). The expected maximum for ># typical SN Ia is mag about 15.5. The reported fast decline is quite ># exceptional for SNe, so follow-up photometry and spectroscopy is ># very urged. It was revealed to be type IIn SN. Rapid decline would be consistent with this classification. Recent magnitude estimate is: >SN2002fj 020928.122 170CR MLF Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp