June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference SOLIS A Long, Careful Look at the Sun Jack Harvey National Solar Observatory
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference Overview Why What Drivers/design Some data samples Opportunites for German-US collaboration Summary
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference Why Study the Sun? Our only vital astronomical object It’s the astrophysics of here and now As challenging as any area of astrophysics Practical applications (space weather, climate) Often first use of new photonics AAAS Journal Science posed 125 Big Science questions for its 125 th anniversary issue of July 1, 2005; one was “What drives the solar magnetic cycle?”
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference German and US Solar Programs Long histories of observation and theory Long history of beneficial collaborations Both countries now building modern 1.5 m facilities for short-term optical observations Both interested in advanced photonics Germany ceased long-term optical (synoptic) programs US invested in SOLIS synoptic program
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference What is SOLIS? Synoptic Optical Long-term Investigations of the Sun State-of-the-art instruments designed to measure the Sun regularly for 25 years Replaces and modernizes successful NSO program started in 1973 SOLIS started regular observations 2003 Science goals aimed at solar activity Decadal Survey urges a 3-station network
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference Virtues of SOLIS VSM Regular full-disk vector magnetograms Full Stokes spectral profile information Chromospheric magnetograms High efficiency optical path (6×10 7 ph/pix/s) Low polarization telescope Long projected life (~2028) Open data archive Complements related space projects (e.g., SOHO, TRACE, Hinode, STEREO, Sunrise, SDO, Solar Orbiter, etc.)
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference Why Long-Term? Magnetic solar cycle is 22 years Many solar processes are slow Synoptic data taken since 1973 still widely used for today’s research and to address originally unforeseen questions Maximize the scientific payoff for the initial investment
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference 48 Solar Rotations
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference Why Frequent? Many basic solar processes occur rapidly Increased chance of capturing rare events Minimize observational gaps Smooth out noisy local solar processes Provide frequently updated boundary conditions for data assimilation modeling Prompt forecasting of space weather
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference SOLIS on Kitt Peak
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference Long-slit spectropolarimeter 80-cm window, 50 cm aperture Helium filled Single crystal Si secondary Ferroelectric LC modulators High reflectivity coatings All light used Vector SpectroMagnetograph German tip-tilt mount German beamsplitters
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference SOLIS VSM 10 4 Dynamic Range 2004 January 6
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference Field strengthAzimuth in sky planeInclination to line of sight SOLIS VSM Vector Magnetogram
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference SOLIS VSM – Hinode XRT
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference SOLIS Collaboration Opportunities 1.Short-term campaigns In progress (e.g. Solanki; Wilhelm) 2.Instrumental improvements 3.Long-term associations Model – Data comparisons Gregor ESA Solar Orbiter 4.Partners in building a global SOLIS network
June 12, 2007J. Harvey DFG-NSF Astrophysics Research Conference Summary Long-term study of Sun is vital Advanced photonics as used in SOLIS enable that research SOLIS provides unique data waiting to be exploited SOLIS welcomes collaborations!