ラジオ探査の昼間バイアスと20世紀後半の温暖化
Steven C Sherwood1, John R Lanzante, Cathryn L Meyer
1Department of Geology and Geophysics, Yale University, New Haven, CT 06520, USA. ssherwood@alum.mit.edu
まとめ
天気気気球の昼間の気温は夜間の気温より低温で,1970年代以降の傾向です. 太陽熱によって引き起こされるこのバイアスは,気候記録に影響を及ぼし,放射探査機と地表温度トレンドの間の不一致を説明する可能性があります.
科学分野:
- 大気科学 大気科学
- 気候学 気候学
- 気象学 気象学 気象学
背景:
- 天気気気球 (無線探査機) は大気温データにとって極めて重要です.
- 放射探査機と地表温度傾向の間には不一致がある.
- 昼間の太陽光による加熱は,計器エラーの既知の原因です.
研究 の 目的:
- ラジオ探査データにおける昼間の温度差を調査するために.
- 太陽熱の偏差がトロポスフィアの気温動向に影響するかどうかを判断する.
- このバイアスの影響が,放射探査機と表面温度のトレンド調整に与える影響を評価する.
主な方法:
- 隣接する00:00と1200UTCの無線探査レポートの分析.
- 1970年代以降,特に熱帯地域における気温の動向の調査.
- 観測された昼間の温度差の特徴の評価.
主要な成果:
- 1970年代以降,昼間と夜間の無線探査機の温度がより涼しいという一貫した傾向が観察されました.
- この傾向は,熱帯の駅ではより顕著です.
- 観測された傾向は,時間の経過とともに太陽熱の誤差が体系的に減少していることに起因する.
結論:
- ラジオ探査データにおける昼間の温度差は,おそらく人工物である.
- この人工物は,放射探査機と地表温度傾向の間の観察された差異を調和させることができます.
- 正確な気候記録は,この太陽熱のバイアスから自由でなければなりません.
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