Patel Manish R, Antoine Philippe, Mason Jonathon, Leese Mark, Hathi Brijen, Stevens Adam H, Dawson Daniel, Gow Jason, Ringrose Timothy, Holmes James, Lewis Stephen R, Beghuin Didier, van Donink Philip, Ligot Renaud, Dewandel Jean-Luc, Hu Daohua, Bates Doug, Cole Richard, Drummond Rachel, Thomas Ian R, Depiesse Cédric, Neefs Eddy, Equeter Eddy, Ristic Bojan, Berkenbosch Sophie, Bolsée David, Willame Yannick, Vandaele Ann Carine, Lesschaeve Stefan, De Vos Lieve, Van Vooren Nico, Thibert Tanguy, Mazy Emmanuel, Rodriguez-Gomez Julio, Morales Rafael, Candini Gian Paolo, Pastor-Morales M Carmen, Sanz Rosario, Aparicio Del Moral Beatriz, Jeronimo-Zafra José-Maria, Gómez-López Juan Manuel, Alonso-Rodrigo Gustavo, Pérez-Grande Isabel, Cubas Javier, Gomez-Sanjuan Alejandro M, Navarro-Medina Fermín, BenMoussa Ali, Giordanengo Boris, Gissot Samuel, Bellucci Giancarlo, Lopez-Moreno Jose Juan
Appl Opt. 2017 Apr 1;56(10):2771-2782. doi: 10.1364/AO.56.002771.
NOMAD is a spectrometer suite on board the ESA/Roscosmos ExoMars Trace Gas Orbiter, which launched in March 2016. NOMAD consists of two infrared channels and one ultraviolet and visible channel, allowing the instrument to perform observations quasi-constantly, by taking nadir measurements at the day- and night-side, and during solar occultations. Here, in part 2 of a linked study, we describe the design, manufacturing, and testing of the ultraviolet and visible spectrometer channel called UVIS. We focus upon the optical design and working principle where two telescopes are coupled to a single grating spectrometer using a selector mechanism.
NOMAD是搭载于欧洲航天局/俄罗斯联邦航天局的火星微量气体轨道飞行器上的一套光谱仪，该轨道飞行器于2016年3月发射。NOMAD由两个红外通道和一个紫外可见通道组成，通过在昼侧和夜侧进行天底测量以及在太阳掩星期间进行测量，使该仪器能够近乎持续地进行观测。在此，在一项关联研究的第2部分中，我们描述了名为UVIS的紫外可见光谱仪通道的设计、制造和测试。我们重点关注光学设计和工作原理，其中两台望远镜通过一个选择器机构与一台光栅光谱仪相连。
