论文标题

宽带软X射线偏光仪的小型卫星版本

A Small Satellite Version of a Broad-band Soft X-ray Polarimeter

论文作者

Marshall, Herman L., Heine, Sarah N. T., Garner, Alan, Gullikson, Eric M., Günther, H. Moritz, Leitz, Christopher, Masterson, Rebecca, Miller, Eric D., Zhang, William, Boissay-Malaquin, Rozenn, Caiazzo, Ilaria, Chakrabarty, Deepto, Davidson, Rosemary, Gallo, Luigi C., Heilmann, Ralf K., Heyl, Jeremy, Kara, Erin, Marscher, Alan, Schulz, Norbert S.

论文摘要

我们描述了广泛的X射线偏光仪的新实现,这基本上基于先前的设计。这种实现,先锋X射线偏光仪(PISOX)是一个小型,专为NASA呼吁天体物理先驱呼吁,可以是Cubesats,气球实验或Smallsats的小型任务。与RedSox极性计中一样,光栅布置的设计最佳是为了极化的目的,通过将光谱仪通道的分散匹配到横向分级的多层(LGML),通过宽带聚焦光学器件设计。该系统可以实现超过90%的极化调制因子。对于PISOX,光学器件是单弹抛物线配置中的轻质Si镜。来自相对部门的高效率,燃烧的光栅是分散到LGML的,形成了覆盖35至75埃75埃埃斯特罗姆(165-350 eV)的波长范围的通道。卫星旋转后,分散光谱的强度,在反射和通过LGML偏振之后,提供了确定源的线性极化分数和方向所需的三个Stokes参数。随着LGML的进一步发展,该设计可以扩展到更高的能量。我们描述了基于此设计的工具中潜在的科学回报的示例。

We describe a new implementation of a broad-band soft X-ray polarimeter, substantially based on a previous design. This implementation, the Pioneer Soft X-ray Polarimeter (PiSoX) is a SmallSat, designed for NASA's call for Astrophysics Pioneers, small missions that could be CubeSats, balloon experiments, or SmallSats. As in the REDSoX Polarimeter, the grating arrangement is designed optimally for the purpose of polarimetry with broad-band focussing optics by matching the dispersion of the spectrometer channels to laterally graded multilayers (LGMLs). The system can achieve polarization modulation factors over 90%. For PiSoX, the optics are lightweight Si mirrors in a one-bounce parabolic configuration. High efficiency, blazed gratings from opposite sectors are oriented to disperse to a LGML forming a channel covering the wavelength range from 35 to 75 Angstroms (165 - 350 eV). Upon satellite rotation, the intensities of the dispersed spectra, after reflection and polarizing by the LGMLs, give the three Stokes parameters needed to determine a source's linear polarization fraction and orientation. The design can be extended to higher energies as LGMLs are developed further. We describe examples of the potential scientific return from instruments based on this design.

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