本文中藉由中壢特高頻雷達對流星尾進行觀測，根據流星尾回波在各接收波道間所產生的相位差，並運用空間干涉定位法，我們可推算出流星尾發生的位置，流星尾受風場影響之運動所產生的都卜勒頻移，可用來近一步推估出中氣層風場及利用諧波分析可得到各潮汐的資料。低密度流星尾回波強度隨時間呈指數衰減的特性，配合空間干涉法所求得之高度可湊配出擴散係數與高度的關係。我們也近一步分析流星尾發生率的日變化，流星尾隨高度的分布及流星尾回波信號強度的分布，這些結果與日本MU雷達所得到的資料進行比較，顯示中壢特高頻雷達所觀測到的流星尾高度是略低於日本MU雷達的觀測結果。本文中也計算流星的墜落速度，並證實了流星在進入大氣層與大氣摩擦的過程中產生減速的現象。最後，我們探討中壢特高頻雷達受周遭環境電磁干擾的情形，在1998年與1999年的資料分析中，我們發現干擾情形有日益嚴重的趨勢，將使得中壢特高頻雷達的觀測和資料分析更為困難。

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