DOT tomography of the solar atmosphere. I. Telescope summary and program definition

Details DOT tomography of the solar atmosphere. I. Telescope summary and program definition DOT tomography of the solar atmosphere. I. Telescope summary and program definition

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...413.1183r&link_type=abstract

Astronomy and Astrophysics, v.413, p.1183-1189 (2004)

Astronomy and Astrophysics

Astrophysics

44

Telescopes, Techniques: Image Processing, Sun: Photosphere, Sun: Chromosphere

Scientific paper

The Dutch Open Telescope (DOT) on La Palma is an innovative optical solar telescope capable of reaching 0.2 arcsec angular resolution over extended durations. The DOT presently progresses from technology testbed to a stable science configuration providing multi-wavelength imaging and multi-camera speckle data acquisition for tomographic mapping of the solar atmosphere. Large-volume speckle processing will soon enable frequent usage and community-wide time allocation, in particular for tandem operation with other solar telescopes pursuing spectropolarimetry and EUV imaging. We summarize the DOT hardware and software in the context of this increasing availability and outline the corresponding ``open-DOT'' program.

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