AB STRACTThe tiny ion o spheric pho tom e ter (TIP) and GPS occultation ex per i ment (GOX) onboard FORMOSAT-3/COS MIC (F3/C) are em ployed to mea sure the OI 135.6 nm in ten si ties in the na dir di rec tion and the to tal elec tron con tent (TEC) be tween the F3/C and GPS sat el lite in the ion o sphere, re spec tively. Due to its very high sen si tiv ity ~600 counts/Ray leigh and rather nar row na dir point ing 3.8° cir cu lar field-of-view, the TIP pro vides ac cu rate char ac ter iza tion of ion o spheric elec tron den sity gra di ents in the hor i zon tal di rec tion. Mean while, a tech nique of the low earth or bit (LEO) to mog ra phy is ap plied to an a lyze the GOX data ob tain ing the 3D dis tri bu tion of ion o sphere elec tron den sity. Here, we com bine the two ob ser va tions to carry out the LEO-TIP tomographic in ver sions, and dem on strate that the peak elec tron den sity (NmF 2 ) re trieved from the TIP com bined to gether with the peak al ti tude (hmF 2 ) in for ma tion from the LEO tomography profiles provides more realistic electron density.Key words: Tiny ion o spheric pho tom e ter (TIP), GPS occultation ex per i ment (GOX), FORMOSAT-3/COS MIC (F3/C), LEO to mog ra phy, LEO-TIP tomographic in ver sion, Ion o spheric elec tron density Tsai, H. F. Tsai, C. H. Lin, K. F. Dymond, C. Coker, D. H. Chua, S. A. Budzien, and C. Z. Cheng, 2009: Ion o spheric elec tron den sity con cur rently de rived by TIP and GOX of FORMOSAT-3/COS MIC. Terr. Atmos. Ocean. Sci., 20, 207-214, doi: 10.3319/ TAO.2008.04.24.02(F3C)
IN TRO DUC TIONTo im prove the global weather pre dic tion and space weather mon i tor ing, six microsatellites termed the Formosa Sat el lite 3 -Con stel la tion Ob serv ing Sys tem for Mete orology, Ion o sphere, and Cli mate (FORMOSAT-3/COS MIC; F3/C) were launched into cir cu lar low-earth or bits (LEOs) from Vandenberg Air Force Base, Cal i for nia, at 0140 UTC 15 April 2006. Each microsatellite of the joint Tai wan-US sat el lite con stel la tion mis sion has a GPS occultation experiment (GOX) pay load to op er ate the at mo spheric and ion o spheric ra dio occultation, a tiny ion o spheric pho tom e ter (TIP) to ob serve the night time ion o spheric air glow OI 135.6 nm emis sion (Fig. 1), and a tri-band bea con (TBB) to tomographically es ti mate fine struc tures of ion o spheric electron den sity on the sat el lite-to-re ceiver plane (Rocken et al. 2000;Cheng 2006). While the GOX daily ob serves about 2500 ver ti cal elec tron den sity dis tri bu tions up to the sat ellite al ti tude (Schreiner et al. 2006;Lei et al. 2007;Lin et al. 2007;Lin et al. 2009;Tsai et al. 2009), the TIP pro vides accu rate hor i zon tal gra di ents of night time elec tron den sity Coker et al. 2009;Dymond et al. 2009).The ra dio occultation tech nique was first used by the Mar i ner IV Mars ex plo ra tion mis sion in 1965 ob serv ing Mars' at mo sphere struc tures (Fjeldbo and Eshleman 1968) and later on by Mar i ner V Ve nus mis sion, other plan e tary and lu nar probes, etc. (Fjeldbo et al. 1971;...