@inproceedings{07d5632f46da4b6495422d251d77ca31,
title = "Prominence science with ATST instrumentation",
abstract = "The 4m Advance Technology Solar Telescope (ATST) is under construction on Maui, HI. With its unprecedented resolution and photon collecting power ATST will be an ideal tool for studying prominences and filaments and their role in producing Coronal Mass Ejections that drive Space Weather. The ATST facility will provide a set of first light instruments that enable imaging and spectroscopy of the dynamic filament and prominence structure at 8 times the resolution of Hinode. Polarimeters allow high precision chromospheric and coronal magnetometry at visible and infrared (IR) wavelengths. This paper summarizes the capabilities of the ATST first-light instrumentation with focus on prominence and filament science.",
keywords = "Corona, Filaments, Instrumentation, Magnetic Fields, Prominence, Sun",
author = "Thomas Rimmele and Thomas Berger and Roberto Casini and David Elmore and Jeff Kuhn and Haosheng Lin and Wolfgang Schmidt and Friedrich W{\"o}ger",
year = "2013",
month = jun,
doi = "10.1017/S1743921313011204",
language = "English",
isbn = "9781107045194",
series = "Proceedings of the International Astronomical Union",
publisher = "Cambridge University Press",
number = "S300",
pages = "362--369",
booktitle = "Nature of Prominences and their Role in Space Weather",
address = "United Kingdom",
edition = "S300",
}