Synoptic Optical Long-term Investigations of the Sun (SOLIS) is a synoptic facility for solar observations over a long time frame that is funded by the National Science Foundation (NSF) and designed and built by the National Solar Observatory (NSO).[1][2][3]
It is operated by the NSO Integrated Synoptic Program (NISP).
SOLIS is a single set of three instruments mounted on a common observing platform. The instruments are the 50 cm aperture Vector Spectromagnetograph (VSM), the 8 mm aperture Integrated Sunlight Spectrometer (ISS), and the 14 cm aperture Full-Disk Patrol (FDP). The VSM telescope is a quasi-Ritchey-Chretien design with a primary mirror operating
at f/1.6. The ~ 400 W of solar light from the primary is reflected by a secondary mirror fabricated from a
single silicon crystal. The final f/6.6 full-disk solar image is focused on a spectrograph slit that is cooled
by a flow of chilled water-propylene glycol solution. The mirrors are coated with protected silver. To improve the internal seeing, the VSM is sealed by 74 cm diameter, 6 mm thick fused silica window. Originally, it was filled with helium at about ambient pressure and temperature.[4] In 2014, helium was replaced by nitrogen due to the increasing cost of helium. Due to this change, the image sharpness was slightly degraded.[5]
The VSM provides full-disk vector (strength and direction) maps of the solar magnetic field both in the photosphere and in the chromosphere on a daily basis, continuing the 40-year record of NSO magnetic field observations. The ISS obtains spectra of the Sun integrated over the solar disk, so the Sun appears as it would as a much more distant star. The combination of data from the ISS and the VSM is useful for studies of exoplanet systems as it allows the modeling of the influence of a star's magnetic field on its spectrum giving clues to the activity level that the exoplanets may be subject to. The FDP provides full-disk images of the Sun in a variety of spectral lines with a cadence as high as 10 seconds.
Crews pour concrete footings, the first step in the construction of a permanent home of the NSF’s SOLIS instrument at Big Bear Solar Observatory in California
SOLIS on the shore of Big Bear Lake, California. White dome in the background is the Goode Solar Telescope
SOLIS mount installation looking down
The vector spectromagnetograph mounted on top of the Kitt Peak Synoptic Optical Long-term Investigations of the Sun (SOLIS) Tower, formerly the vacuum telescope tower.
^Keller, C. U.; Harvey, J. W.; Giampapa, M. S. (2003). Keil, Stephen L; Avakyan, Sergey V (eds.). "SOLIS: an innovative suite of synoptic instruments". Proceedings of the SPIE. Innovative Telescopes and Instrumentation for Solar Astrophysics. 4853: 194–204. Bibcode:2003SPIE.4853..194K. doi:10.1117/12.460373. S2CID121871549.
^Balasubramaniam, K. S.; Pevtsov, A. A. (2011). Fineschi, Silvano; Fennelly, Judy (eds.). "Ground-based synoptic instrumentation for solar observations". Proceedings of the SPIE. Solar Physics and Space Weather Instrumentation IV. 8148: 194–204. Bibcode:2011SPIE.8148E..09B. doi:10.1117/12.892824. S2CID123569040.
^National Research Council; Division on Engineering and Physical Sciences; Space Studies Board; Committee on Solar and Space Physics; Solar and Space Physics Survey Committee (17 December 2003). The Sun to the Earth - and Beyond: Panel Reports. National Academies Press. p. 26. ISBN978-0-309-08972-2.