Prominence science with ATST instrumentation

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.

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Copyright 2013 International Astronomical Union.


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Author Rimmele, Thomas
Berger, Thomas
Casini, Roberto
Elmore, David
Kuhn, Jeff
Lin, Haosheng
Schmidt, Wolfgang
Wöger, Friedrich
Publisher UCAR/NCAR - Library
Publication Date 2013-06-01T00:00:00
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Topic Category geoscientificInformation
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Metadata Date 2023-08-18T19:02:14.514814
Metadata Record Identifier edu.ucar.opensky::articles:18940
Metadata Language eng; USA
Suggested Citation Rimmele, Thomas, Berger, Thomas, Casini, Roberto, Elmore, David, Kuhn, Jeff, Lin, Haosheng, Schmidt, Wolfgang, Wöger, Friedrich. (2013). Prominence science with ATST instrumentation. UCAR/NCAR - Library. http://n2t.net/ark:/85065/d7vt1tss. Accessed 22 June 2025.

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