[1] We study the source locations of 130 solar flare-type II radio burst events with the associated interplanetary shocks observed by L1 spacecraft (type A events) and 217 flare-type II events without such shocks observed at L1 (type B events) during 3) The angular distance from the flare source to the Earth (defined as Y below) also contributes to the probability of the associated shock being observed at the Earth. The shock arrival probability decreases with the increment of Y and the mean initial shock speed increases with Y for those Earth-encountered shocks. (4) The so-called ''same-opposite side effect'' of the HCS is confirmed to exist. That is, the shocks whose associated flares are located on the same side of the HCS as the Earth (called as ''same side events'') have a greater chance of reaching the Earth than those shocks with their associated flares on the opposite side (''opposite side events''). Here for the first time, a comprehensive sample of solar transient events of both arriving and nonarriving ones (at Earth) is used to testify to the same-opposite side effect. These results would be valuable in understanding the solar-terrestrial relations, and helpful for space weather prediction.Citation: Zhao, X., X. Feng, and C.-C. Wu (2007), Influence of solar flare's location and heliospheric current sheet on the associated shock's arrival at Earth,