1. 1Yang LiuCISM All-hand meeting CISM All-hand Meeting Yang Liu – Stanford University yliu@solar.stanford.edu

2. 2Yang LiuCISM All-hand meeting Data and Products Available in the Community Data availability. Corresponding products.

3. 3Yang LiuCISM All-hand meeting Generation of the Synoptic Frames Generation of the synoptic frames. –An example to produce a synoptic frame for the active region AR8038 before the flare at 04:48UT of May 12.

4. 4Yang LiuCISM All-hand meeting Challenges for Frame Generation Smoothness for the seam between the charts and the individual magnetogram. Different noise levels between the charts and the individual magnetogram. Smooth using a Gaussian function.

5. 5Yang LiuCISM All-hand meeting Challenges for Frame Generation Polar fields interpolation (also for standard synoptic charts).

6. 6Yang LiuCISM All-hand meeting Challenges for Frame Generation Differential rotation correction (also for standard synoptic charts).

7. 7Yang LiuCISM All-hand meeting Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) Instrumentation and products –50 cm Vector-Spectromagnetograph (VSM) (2048x2048, 1.00 by 1.00 arcsec). ›The four observing modes Stokes I, Q, U, and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the CaII 854.2 nm line Stokes I in the HeI 1083.0 nm line and the near-by SiI line ›The prospective products: photospheric vector magnetogram (FeI630.2), 3 per day. chromospheric line-of-sight magnetogram (CaII854.2), 3 per day. deep photospheric magnetogram, 1 per day. Helium 1083 nm (coronal proxy), 3 per day. –14 cm Full-Disk Patrol (FDP). ›The FDP will produce monochromatic images of the full disk of the sun. H-alpha core, red and blue wing (one per min). 1083 nm pseudo equivalent width and Doppler images (one per min). continuum image (one per 10 min). Ca II K3 and K2 violet and red images (one per 3 hours). photospheric Doppler images from which the p-mode oscillations may be filtered to a small amplitude (one per day). ›The prospective products: Ha core and wing intensity, velocity, 1 per minute Helium 1083 nm core intensity and velocity, 1 per minute. oscillation-free photospheric velocity, 1 per day. CaII K core and wing chromospheric intensities, 1 per 3 hours. continuum (white light), 1 per 10 minutes. –8 mm Integrated Sunlight Spectrometer (ISS). › ISS is designed to obtain both high (R = 300,000) and moderate (R = 30,000) spectral resolution observations of the Sun as a star. range of 350 nm - 1100 nm. ›The prospective products: various sun-as-a-star spectral lines, 2 per day.

8. 8Yang LiuCISM All-hand meeting Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) Instrumentation and products –50 cm Vector-Spectromagnetograph (VSM) (2048x2048, 1.00 by 1.00 arcsec). ›The four observing modes Stokes I, Q, U, and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the CaII 854.2 nm line Stokes I in the HeI 1083.0 nm line and the near-by SiI line ›The prospective products: photospheric vector magnetogram (FeI630.2), 3 per day. chromospheric line-of-sight magnetogram (CaII854.2), 3 per day. deep photospheric magnetogram, 1 per day. Helium 1083 nm (coronal proxy), 3 per day. –14 cm Full-Disk Patrol (FDP). ›The FDP will produce monochromatic images of the full disk of the sun. H-alpha core, red and blue wing (one per min). 1083 nm pseudo equivalent width and Doppler images (one per min). continuum image (one per 10 min). Ca II K3 and K2 violet and red images (one per 3 hours). photospheric Doppler images from which the p-mode oscillations may be filtered to a small amplitude (one per day). ›The prospective products: Ha core and wing intensity, velocity, 1 per minute Helium 1083 nm core intensity and velocity, 1 per minute. oscillation-free photospheric velocity, 1 per day. CaII K core and wing chromospheric intensities, 1 per 3 hours. continuum (white light), 1 per 10 minutes. –8 mm Integrated Sunlight Spectrometer (ISS). › ISS is designed to obtain both high (R = 300,000) and moderate (R = 30,000) spectral resolution observations of the Sun as a star. range of 350 nm - 1100 nm. ›The prospective products: various sun-as-a-star spectral lines, 2 per day.

9. 9Yang LiuCISM All-hand meeting Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) Instrumentation and products –50 cm Vector-Spectromagnetograph (VSM) (2048x2048, 1.00 by 1.00 arcsec). ›The four observing modes Stokes I, Q, U, and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the CaII 854.2 nm line Stokes I in the HeI 1083.0 nm line and the near-by SiI line ›The prospective products: photospheric vector magnetogram (FeI630.2), 3 per day. chromospheric line-of-sight magnetogram (CaII854.2), 3 per day. deep photospheric magnetogram, 1 per day. Helium 1083 nm (coronal proxy), 3 per day. –14 cm Full-Disk Patrol (FDP). ›The FDP will produce monochromatic images of the full disk of the sun. H-alpha core, red and blue wing (one per min). 1083 nm pseudo equivalent width and Doppler images (one per min). continuum image (one per 10 min). Ca II K3 and K2 violet and red images (one per 3 hours). photospheric Doppler images from which the p-mode oscillations may be filtered to a small amplitude (one per day). ›The prospective products: Ha core and wing intensity, velocity, 1 per minute Helium 1083 nm core intensity and velocity, 1 per minute. oscillation-free photospheric velocity, 1 per day. CaII K core and wing chromospheric intensities, 1 per 3 hours. continuum (white light), 1 per 10 minutes. –8 mm Integrated Sunlight Spectrometer (ISS). › ISS is designed to obtain both high (R = 300,000) and moderate (R = 30,000) spectral resolution observations of the Sun as a star. range of 350 nm - 1100 nm. ›The prospective products: various sun-as-a-star spectral lines, 2 per day.

10. 10Yang LiuCISM All-hand meeting Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) Instrumentation and products –50 cm Vector-Spectromagnetograph (VSM) (2048x2048, 1.00 by 1.00 arcsec). ›The four observing modes Stokes I, Q, U, and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the CaII 854.2 nm line Stokes I in the HeI 1083.0 nm line and the near-by SiI line ›The prospective products: photospheric vector magnetogram (FeI630.2), 3 per day. chromospheric line-of-sight magnetogram (CaII854.2), 3 per day. deep photospheric magnetogram, 1 per day. Helium 1083 nm (coronal proxy), 3 per day. –14 cm Full-Disk Patrol (FDP). ›The FDP will produce monochromatic images of the full disk of the sun. H-alpha core, red and blue wing (one per min). 1083 nm pseudo equivalent width and Doppler images (one per min). continuum image (one per 10 min). Ca II K3 and K2 violet and red images (one per 3 hours). photospheric Doppler images from which the p-mode oscillations may be filtered to a small amplitude (one per day). ›The prospective products: Ha core and wing intensity, velocity, 1 per minute Helium 1083 nm core intensity and velocity, 1 per minute. oscillation-free photospheric velocity, 1 per day. CaII K core and wing chromospheric intensities, 1 per 3 hours. continuum (white light), 1 per 10 minutes. –8 mm Integrated Sunlight Spectrometer (ISS). › ISS is designed to obtain both high (R = 300,000) and moderate (R = 30,000) spectral resolution observations of the Sun as a star. range of 350 nm - 1100 nm. ›The prospective products: various sun-as-a-star spectral lines, 2 per day.

11. 11Yang LiuCISM All-hand meeting Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) Instrumentation and products –50 cm Vector-Spectromagnetograph (VSM) (2048x2048, 1.00 by 1.00 arcsec). ›The four observing modes Stokes I, Q, U, and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the CaII 854.2 nm line Stokes I in the HeI 1083.0 nm line and the near-by SiI line ›The prospective products: photospheric vector magnetogram (FeI630.2), 3 per day. chromospheric line-of-sight magnetogram (CaII854.2), 3 per day. deep photospheric magnetogram, 1 per day. Helium 1083 nm (coronal proxy), 3 per day. –14 cm Full-Disk Patrol (FDP). ›The FDP will produce monochromatic images of the full disk of the sun. H-alpha core, red and blue wing (one per min). 1083 nm pseudo equivalent width and Doppler images (one per min). continuum image (one per 10 min). Ca II K3 and K2 violet and red images (one per 3 hours). photospheric Doppler images from which the p-mode oscillations may be filtered to a small amplitude (one per day). ›The prospective products: Ha core and wing intensity, velocity, 1 per minute Helium 1083 nm core intensity and velocity, 1 per minute. oscillation-free photospheric velocity, 1 per day. CaII K core and wing chromospheric intensities, 1 per 3 hours. continuum (white light), 1 per 10 minutes. –8 mm Integrated Sunlight Spectrometer (ISS). › ISS is designed to obtain both high (R = 300,000) and moderate (R = 30,000) spectral resolution observations of the Sun as a star. range of 350 nm - 1100 nm. ›The prospective products: various sun-as-a-star spectral lines, 2 per day.

12. 12Yang LiuCISM All-hand meeting Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) Instrumentation and products –50 cm Vector-Spectromagnetograph (VSM) (2048x2048, 1.00 by 1.00 arcsec). ›The four observing modes Stokes I, Q, U, and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the FeI 630.15 nm and 630.25 nm lines Stokes I and V profiles in the CaII 854.2 nm line Stokes I in the HeI 1083.0 nm line and the near-by SiI line ›The prospective products: photospheric vector magnetogram (FeI630.2), 3 per day. chromospheric line-of-sight magnetogram (CaII854.2), 3 per day. deep photospheric magnetogram, 1 per day. Helium 1083 nm (coronal proxy), 3 per day. –14 cm Full-Disk Patrol (FDP). ›The FDP will produce monochromatic images of the full disk of the sun. H-alpha core, red and blue wing (one per min). 1083 nm pseudo equivalent width and Doppler images (one per min). continuum image (one per 10 min). Ca II K3 and K2 violet and red images (one per 3 hours). photospheric Doppler images from which the p-mode oscillations may be filtered to a small amplitude (one per day). ›The prospective products: Ha core and wing intensity, velocity, 1 per minute Helium 1083 nm core intensity and velocity, 1 per minute. oscillation-free photospheric velocity, 1 per day. CaII K core and wing chromospheric intensities, 1 per 3 hours. continuum (white light), 1 per 10 minutes. –8 mm Integrated Sunlight Spectrometer (ISS). › ISS is designed to obtain both high (R = 300,000) and moderate (R = 30,000) spectral resolution observations of the Sun as a star. range of 350 nm - 1100 nm. ›The prospective products: various sun-as-a-star spectral lines, 2 per day.

13. 13Yang LiuCISM All-hand meeting Data from SOLIS

14. 14Yang LiuCISM All-hand meeting Kinematical Properties of CMEs Cone model.

15. 15Yang LiuCISM All-hand meeting Kinematical Properties of CMEs Cone model.

16. 16Yang LiuCISM All-hand meeting Kinematical Properties of CMEs

17. 17Yang LiuCISM All-hand meeting Kinematical Properties of CMEs Half of Angle Width=86±1 Longitude=-34±2 Latitude=0±0