We describe the design of the Sunrise Filter Imager (SuFI) and the Image Stabilization and Light Distribution (ISLiD) unit onboard the Sunrise balloon borne solar observatory. This contribution provides the necessary information which is relevant to understand the instruments' working principles, the relevant technical data, and the necessary information about calibration issues directly related to the science data. © 2010 The Author(s)
This article is an open access article distributed under the terms and conditions of the Creative Co...
The standard value for atmospheric refraction on the horizon of 34\u27, used in all publicly availab...
<p>The total solar eclipse of August 21, 2017 offers a unique opportunity for study of the infrared ...
This paper describes the wave-front correction system developed for the Sunrise balloon telescope, a...
Sunrise is a solar telescope, successfully flown in June 2009 with a long duration balloon from the ...
S. K. Solanki et. al.©2017 The American Astronomical Society. All rights reserved.The Sunrise balloo...
SUNRISE is a balloon-borne solar telescope flown with a long-duration balloon by NASA's Columbia Sci...
International audienceA new ligthweight multichannel moderate bandwidth filter instrument designed t...
This project was to study the solar prominences of the sun, using an 8” Celestron telescope, camera,...
The turbulent atmosphere has two detrimental effects in astronomy. The phase aberration induced by ...
There are strong scientific cases and practical reasons for building ground-based solar synoptic tel...
The Liege-balloon program is intended to make high-spectral resolution observations of the sun in th...
The measurement of the stray-rejection capabilities of METIS is part of the acceptance package of th...
The SUNRISE Chromospheric Infrared spectroPolarimeter (SCIP) is a balloon-borne long-slit spectrogra...
We developed a scan mirror mechanism (SMM) that enable a slit-based spectrometer or spectropolarimet...
This article is an open access article distributed under the terms and conditions of the Creative Co...
The standard value for atmospheric refraction on the horizon of 34\u27, used in all publicly availab...
<p>The total solar eclipse of August 21, 2017 offers a unique opportunity for study of the infrared ...
This paper describes the wave-front correction system developed for the Sunrise balloon telescope, a...
Sunrise is a solar telescope, successfully flown in June 2009 with a long duration balloon from the ...
S. K. Solanki et. al.©2017 The American Astronomical Society. All rights reserved.The Sunrise balloo...
SUNRISE is a balloon-borne solar telescope flown with a long-duration balloon by NASA's Columbia Sci...
International audienceA new ligthweight multichannel moderate bandwidth filter instrument designed t...
This project was to study the solar prominences of the sun, using an 8” Celestron telescope, camera,...
The turbulent atmosphere has two detrimental effects in astronomy. The phase aberration induced by ...
There are strong scientific cases and practical reasons for building ground-based solar synoptic tel...
The Liege-balloon program is intended to make high-spectral resolution observations of the sun in th...
The measurement of the stray-rejection capabilities of METIS is part of the acceptance package of th...
The SUNRISE Chromospheric Infrared spectroPolarimeter (SCIP) is a balloon-borne long-slit spectrogra...
We developed a scan mirror mechanism (SMM) that enable a slit-based spectrometer or spectropolarimet...
This article is an open access article distributed under the terms and conditions of the Creative Co...
The standard value for atmospheric refraction on the horizon of 34\u27, used in all publicly availab...
<p>The total solar eclipse of August 21, 2017 offers a unique opportunity for study of the infrared ...