SST observations schedule for 2006

• ...--03.28 : Pre-season TECHNICAL TIME.
• 03.29--04.10 (13d): Hillberg (ISP), Lites (HAO). Spectroscopy.
• 04.11--04.26 (16d): Rybak (OPTICON). Spectroscopy. Co-observing with DOT.
• 04.27--05.10 (14d): (Oslo). Spectroscopy. Co-observing with DOT.
• 05.11--05.21 (11d): Kiselman, Langhans, van Noort (ISP). Spectroscopy.
• 05.22--05.31 (10d): Zakharov (MPS). Spectroscopy.
• 06.01--06.02 (2d): TECHNICAL TIME. Switch from spectroscopy to imaging.
• 06.03--06.09 (7d): Berger (LMSAL). Imaging.
• 06.10--06.22 (13d): (Oslo). Imaging.
• 06.23--07.10 (18d): Narayan, Scharmer (ISP). Imaging.
• 07.11--07.14 (4d): Pasachoff (NASA). Imaging.
• 07.15--07.26 (12d): Moreno Insertis (Spain). Imaging.
• 07.27--08.07 (12d): Domingo (Spain). Imaging.
• 08.08--08.17 (10d): Hirzberger (MPS). Imaging.
• 08.18--08.19 (2d): TECHNICAL TIME. Telescope polarization measurements.
• 08.20--08.29 (10d): Snik (Utrecht). Imaging. Polarimetry with their own instrument. Co-observing with DOT.
• 08.30--09.13 (15d): Löfdahl, van Noort (ISP). Imaging.
• 09.14--09.26 (13d): (Oslo) Imaging.
• 09.27--10.06 (10d): De Pontieu (LMSAL). Imaging. Co-observing with DOT.
• 10.07--10.24 (18d): Berdyugina (Spain). Imaging. Polarimetry with their own instrument.
• 10.25--10.31 (7d): Berger (LMSAL). Canceled.
• 11.01--... : Post-season TECHNICAL TIME.

Date ranges are given in the format MM.DD--MM.DD.

Observers are expected to bring your own backup media for transferring the data to your home institute. See the instructions page. Observers are also expected to arrive one or two days early for their scheduled time slots in order to settle down and get (re-)acquainted with the telescope before the observations start for real.

Other instructions for observers are available at http://www.solarphysics.kva.se/LaPalma/.

Abbreviations: SST=Swedish 1-m Solar Telescope; MPS=Max-Planck; ISP=Institute for Solar Physics; LMSAL=Lockheed Martin Solar and Astrophysics Laboratory; NASA=National Aeronautics and Space Administration.