空间科学学报2017，Vol.37Issue(3)：291-297,7.DOI:10.11728/cjss2017.03.291
一种NRLMSISE-00模型太阳辐射校正方法
Optimizing the NRLMSISE-00 Model by a New Solar EUV Proxy
薛炳森 1苍中亚1
作者信息
- 1. 中国气象局空间天气重点开放实验室 北京100080
- 折叠
摘要
Abstract
Solar EUV radiation is one of the sources for atmospheric density variation in thermosphere.NRLMSISE-00 model is widely used to simulate the density variation in the satellite orbit.However,this model always exhibits large density errors compared with satellite observations.In this work,the model output is compared with CHAMP satellite observation on the same position,and an ideal value of proxy for solar EUV (F*) is chosen through changing the input F10.7.Further investigation shows that F* is closely related to another solar EUV index MgII.By using of neuron network technique,the correspondence relationship between the new proxy of solar EUV (Feuv)and F10.7 and MgII.The target parameter is F*.The new proxy substitutes F10.7,and is input into NRLMSISE-00 model.The results show the difference of thermosphere density between those detected by CHAMP and GRACE-A satellite and that calculated by the NRLMSISE-00 model is dropped significantly.关键词
热层大气密度/NRLMSISE-00模式/太阳紫外辐射/代理参数Key words
Thermosphere density/NRLMSISE-00 model/Solar EUV radiation/Proxy分类
天文与地球科学引用本文复制引用
薛炳森,苍中亚..一种NRLMSISE-00模型太阳辐射校正方法[J].空间科学学报,2017,37(3):291-297,7.
