< p > <强>一个模型是< a href = " http://sd-www.jhuapl.edu/Aurora/ovation/ " > < / > OVATION极光降水模型。< /强> < / p > < p >鼓掌< a href = " https://en.wikipedia.org/wiki/Backronym " >代表< / >椭圆变化,评估,跟踪,强度,和在线短时预测。< / p > < p > < a href = " http://www.swpc.noaa.gov/ " >美国国家海洋和大气管理局太空天气预报中心< / >使用喝彩' 30分钟的极光预测模型。他们使用一种修改版的模型< a href = " http://www.swpc.noaa.gov/products/aurora-3-day-forecast " > < / >为期3天的预测。由纽厄尔et al。(2010)约翰霍普金斯大学。< / p > < p >你可以阅读所有关于Machol et al。(2013)。< a href = " http://onlinelibrary.wiley.com/doi/10.1029/2011SW000746/full " > < / >是开放和包含几个方程和描述的方法。他们解释:< / p > < blockquote > < p >喝彩'模型来源于电子和质子通量测量SSJ4探测器的< a href = " https://en.wikipedia.org/wiki/Defense_Meteorological_Satellite_Program " > < / > DMSP卫星。< / p > < /引用> < p > SSJ4传感器,根据< a href = " http://www.ferzkopp.net/Personal/Thesis/node28.html " > < / >一个来源:< / p > < blockquote > < p > […)由一个数组的四柱,弯板,静电分析器配置到两双;一对每个测量电子和离子。每一对覆盖范围从30 eV 30 keV能量20频道间隔相等的时间间隔在能源对数刻度。< / p > < /引用> < h3 >引用< / h3 > < p > Machol, j·L。, J. C. Green, R. J. Redmon, R. A. Viereck, and P. T. Newell (2012), Evaluation of OVATION Prime as a forecast model for visible aurorae, Space Weather, 10, S03005, doi:10.1029/2011SW000746. Newell, P. T., T. Sotirelis, and S. Wing (2010a), Seasonal variations in diffuse, monoenergetic, and broadband aurora, J. Geophys. Res., 115, A03216, doi:10.1029/2009JA014805.