Current status of project SWEETS: Estimating thermospheric neutral mass densities from satellite data at various altitudes

S. Krauss, Barbara Süsser-Rechberger, S. Behzadpour, T. Mayer-Gürr, M. Temmer, Sofia Kroisz, L. Drescher
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Abstract

Within the project SWEETS (funded by the FFG Austria) it is intended to develop a forecasting model, to predict the expected impact of solar events, like coronal mass ejections (CMEs), on satellites at different altitudes between 300-800 km. For the realization, scientific data, such as kinematic orbit information and accelerometer measurements, from a wide variety of satellites are incorporated. Based on the evaluation of the impact of several hundred solar events on the thermosphere the forecasting will be realized through a joint analysis and evaluation of solar wind plasma and magnetic field data observed at the Lagrange point L1.
In this contribution we show first preliminary results of thermospheric densities estimates based on kinematic orbit information for different satellite missions (e.g., TerraSAR-X, TanDEM-X, Swarm A-C, GRACE, GRACE-FO, CHAMP). To validate the outcome, we compare the results with state-of-the-art thermospheric models as well as with densities estimated from accelerometer measurements if available. Finally, for some specific CME events we will perform a comparison between the post-processed density estimates and results from our preliminary forecasting tool.

SWEETS项目的现状:根据不同高度的卫星数据估算热层中性质量密度
在SWEETS项目(由奥地利FFG资助)中,它旨在开发一个预测模型,以预测太阳事件的预期影响,如日冕物质抛射(cme),对300-800公里之间不同高度的卫星。为了实现这一目标,结合了来自各种卫星的科学数据,如运动学轨道信息和加速度计测量结果。在对数百个太阳事件对热层影响进行评估的基础上,通过对拉格朗日点L1观测到的太阳风、等离子体和磁场数据进行联合分析和评估来实现预报。在本文中,我们展示了基于不同卫星任务(例如,TerraSAR-X、TanDEM-X、Swarm A-C、GRACE、GRACE- fo、CHAMP)的运动学轨道信息估算热层密度的初步结果。为了验证结果,我们将结果与最先进的热层模型以及加速度计测量估计的密度(如果可用)进行比较。最后,对于一些特定的日冕物质抛射事件,我们将对处理后的密度估计与我们的初步预测工具的结果进行比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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