CISM All-hand Meeting

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

2. Data and Products Available in the Community • Data availability. • Corresponding products.

3. 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. CR1922 CR1923

4. 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. Challenges for Frame Generation • Polar fields interpolation (also for standard synoptic charts). Cubic Spline Interpolation for Polar Field

6. Challenges for Frame Generation • Differential rotation correction (also for standard synoptic charts). effect of differential rotation included

7. 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. 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. 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. 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. 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. 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. Data from SOLIS

14. Kinematical Properties of CMEs • Cone model.

15. Kinematical Properties of CMEs • Cone model.

16. Kinematical Properties of CMEs

17. Kinematical Properties of CMEs Half of Angle Width=86±1 Longitude=-34±2 Latitude=0±0