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Recent advances in understanding MJO propagation dynamics
理解 MJO 传播动力学的最新进展
MJO伝播ダイナミクスの理解における最近の進歩
MJO 전파 역학 이해의 최근 발전
Avances recientes en la comprensión de la dinámica de propagación de la MJO
Avancées récentes dans la compréhension de la dynamique de propagation des MJO
Последние достижения в понимании динамики распространения MJO
Tim Li 李天明 ¹ ², Lu Wang 王璐 ¹, Feng Hu 胡枫 ³
¹ Key Laboratory of Meteorological Disaster, Ministry of Education/Joint International Research Laboratory of Climate and Environmental Change/Collaborative Innovation Center on Forecast and Evaluation of Meteorological Disasters, Nanjing University of Information Science and Technology, Nanjing 210044, China 南京信息工程大学 气候与环境变化国际合作联合实验室 气象灾害教育部重点实验室 气象灾害预报预警与评估协同创新中心
² International Pacific Research Center and Department of Atmospheric Sciences, School of Ocean and Earth Science and Technology, University of Hawaii at Manoa, Honolulu, Hawaii, 96822, United States
³ School of Geography and Tourism, Chuzhou University, Chuzhou 239000, China 滁州学院 地理信息与旅游学院
Science Bulletin, 10 August 2021
Perspective

The Madden–Julian Oscillation (MJO) is the most prominent intraseasonal mode in the tropics and is characterized by a slow eastward phase speed, a planetary zonal scale and a period of 30–60 d. Although the main convection of the MJO is confined to the tropics, it can exert a large remote impact on weather and climate around the globe. The MJO is the major source of predictability for sub-seasonal forecasts. It is therefore important to understand the fundamental dynamics of the MJO.
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