SST observations schedule for 2005

• 04.05--04.16 (10d): Zakharov, MPI Lindau. Blue: PD-imaging: G-band. Spectrograph.
• 04.17--04.29: Langhans, ISP. Spectrograph: Fe I 557.6, Fe I 709.0, Fe II 614.9 nm. Blue: Imaging in Ca H, G-band, G-cont via dichroic BS.
• 04.30--05.09 (10d): Bellot Rubio, Spain. Spectrograph: Fe I 557.6, Fe I 709.0, Fe II 614.9 nm. Blue: Imaging in Ca H, G-band, G-cont via dichroic BS.
• 05.10--05.23 (14d): Oslo 3. Spectrograph: Ca II, Mg I 457.1 nm
• 05.24--05.24: Tech time. Switch tables.
• 05.25--06.07 (14d): Khomenko, Spain. Blue: G-band, G-cont. Red: SOUP: H-α, 557.6, 630.2 nm.
• 06.08--06.22 (15d): Sánchez Almeida, Spain. Blue: Ca H 0.3 nm, PD imaging in G-band, G-cont, 2×M1.6 (blue) with PD prisms 1×M4.2 (blue). Chopper. Red: SOUP: 705.7, 785 nm, 1×M1.6.
• 06.23--07.02 (10d): Berger, LMSAL. Red: SOUP: 630.25, 557.6 nm, H-α. Blue: G-band, G-cont PD, Ca H. Co-observing with DOT.
• 07.03--07.14 (12d): Katsukawa, CCI ITP. Red: SOUP 630.2 nm magnetograms. Blue: G-band, Ca H. Co-observing with DOT, VTT, SOHO.
• 07.15--08.17: ISP
• 08.18--08.21 (4d): Pasachoff, NASA. Red: SOUP.
• 08.22--08.31 (10d): Zakharov, MPI Lindau. Red: PD-imaging: TiO, SOUP magnetograms. Blue: PD in G-band, CN, continuum.
• 09.01--09.10 (10d): De Pontieu, LMSAL Blue: G-band, G-cont, Ca H. Red: SOUP magnetograms, H-α, Doppler. Co-observing with DOT
• 09.11--09.22: ISP
• 09.23--10.04 (13d): Oslo 1. Blue: 2 fixed Ca H filters + PD in Ca H continuum, 4 blue-sensitive cameras, chopper. Red: SOUP: PD between prefilter and SOUP, Sarnoff cameras, Chopper.
• 10.05--10.17 (13d): Oslo 2. See Oslo 1
• 10.18--10.31 (14d): Rybák, Opticon Spectrograph: 614.9, 630.1, 557.6 nm, 2×M1.6 (spectra) + M4.2i/10 (slit jaw). Blue: Ca H, G-band, G-cont via dichroic BS. Co-observing with DOT, TRACE, SOHO.
• 11.01--11.14: Langhans, ISP Spectrograph: Fe I 557.6, Fe I 709.0, Fe II 614.9 nm. Blue: Imaging in Ca H, G-band, G-cont via dichroic BS. Co-observing with DOT, VTT, THEMIS.

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

Abbreviations: SST=Swedish 1-m Solar Telescope; MPI=Max-Planck Institut; ISP=Institute for Solar Physics; PD=Phase Diversity; LMSAL=Lockheed Martin Solar and Astrophysics Laboratory; SOUP=Solar Optical Universal Polarimeter; VTT=Vacuum Tower Telescope; CCI=International Scientific Committee, ITP=International Time Programme, NASA=National Aeronautics and Space Administration.

You are expected to bring your own backup media for transferring the data to your home institute. Our current system is to use DVD+R.

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