The 1-meter Swedish solar telescope

By G. Scharmer, Klas Bjelksjo, T. Korhonen, B. Lindberg, B. Petterson. SPIE Astronomical Telescopes + Instrumentation, 2003

333 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Atomic and Molecular Physics, and Optics, Renewable Energy, Sustainability and the Environment

View Paper: https://www.semanticscholar.org/paper/9b17393195db63c2be0f8cbfee78e4b50ee29537

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Artificial Intelligence

1. Bart De Pontieu
2. M. Carlsson
3. J. Leenaarts
4. A. Title
5. C. Schrijver
6. L. R. V. Voort
7. Markus J. Aschwanden

In Atomic and Molecular Physics, and Optics

1. M. Carlsson
2. J. Leenaarts
3. L. R. V. Voort
4. G. Verth
5. S. Saar
6. Bart De Pontieu
7. R. Morton
8. S. Grant

In Renewable Energy, Sustainability and the Environment

1. M. Carlsson
2. E. DeLuca
3. L. R. V. Voort
4. J. Leenaarts

Citations in the corpus

• Multiwavelength Studies of MHD Waves in the Solar Chromosphere (2015, background): “…the 0.76 m Dunn Solar Telescope (DST; formerly the Vacuum Tower Telescope; Dunn 1969) in New Mexico, USA, the 1 m Swedish Solar Telescope (SST; Scharmer et al. 2003) on the island of La Palma, the 1 m New Vacuum Solar Telescope (NVST; Liu et al. 2014a) at the Fux- ian Solar Observatory,…”
• Dynamic Fibrils Are Driven by Magnetoacoustic Shocks (2006, background): “OBSERVATIONS OF DYNAMIC FIBRILS The recent advent of the Swedish 1 m Solar Telescope (SST; Scharmer et al. 2003) and advances in postprocessing techniques (van Noort et al. 2005) have allowed us to obtain an unprecedented, diffraction-limited (120 km), 78 minute long time series of the chromosphere…”
• The Interface Region Imaging Spectrograph (IRIS) (2012, background): “e spacecraft was rolled by 90 degrees for these observations. The x and y coordinates are shown to indicate the scale of the image and spectra only. et al., 2008) at the Swedish Solar Telescope (SST: Scharmer et al., 2003) indicate that to properly capture the dynamics, ne-scale structuring, and sma”
• THE FORMATION OF THE Hα LINE IN THE SOLAR CHROMOSPHERE (2012, methodology): “The seeing conditions were very good and the data quality benefited from the SST adaptive optics system (Scharmer et al. 2003b) and Multi-Object Multi-Frame Blind Deconvolution (MOMFBD, van Noort et al. 2005) image restoration.”
• ON-DISK COUNTERPARTS OF TYPE II SPICULES IN THE Ca ii 854.2 nm AND Hα LINES (2009, methodology): “The observations were obtained with the CRisp Imaging SpectroPolarimeter (CRISP, Scharmer et al. 2008) installed at the Swedish 1-m Solar Telescope (SST, Scharmer et al. 2003a) on La Palma (Spain).”