Charged Particle Environemnt for NGST: Model Development

摘要

The Next Generation Space Telescope (NGST) will operate in a halo orbit about the L2 point, 1.5 million km from the Earth, where the psacecraft will periodically travel throught he magnetotail region. There are a number of tools available to calculate the high energy, ionizing radiation particle environment from galactic cosmic rays and from solar disturbances. However, space environment tools are not generally available to provide assessments of the charged particle environment and its variations in the solar wind, magnetosheath, and magnetotail at L2 distances. An engineering-level phenomenology code (LRAD) was therefore develoepd to facilitate the definition of charged particle environments in the vicinity of the L2 point in support of the NGST program. LRAD contains models tied to satellite measurement data of the solar wind and magnetotail regions. The model provides particle flux and fluence calculations necessary to predict spacecraft charging conditions and the degradation of materials used in the construction of NGST. This paper describes the LRAD environment models for the deep magnetotail (X_(GSE) < -100 Re) and solar wind, and presents predictions of the charged particle environment for NGST.