CISM Allhand Meeting Yang Liu Stanford University yliusolar

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

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

Generation of the Synoptic Frames • Generation of the synoptic frames. – An example to produce a synoptic frame for the active region AR 8038 before the flare at 04: 48 UT of May 12. CISM All-hand meeting Yang Liu 3

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. CISM All-hand meeting Yang Liu 4

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

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

Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) • Instrumentation and products – – – 50 cm Vector-Spectromagnetograph (VSM) (2048 x 2048, 1. 00 by 1. 00 arcsec). › The four observing modes • Stokes I, Q, U, and V profiles in the Fe. I 630. 15 nm and 630. 25 nm lines • Stokes I and V profiles in the Ca. II 854. 2 nm line • Stokes I in the He. I 1083. 0 nm line and the near-by Si. I line › The prospective products: • photospheric vector magnetogram (Fe. I 630. 2), 3 per day. • chromospheric line-of-sight magnetogram (Ca. II 854. 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 K 3 and K 2 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. • Ca. II 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. CISM All-hand meeting Yang Liu 7

Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) • Instrumentation and products – – – 50 cm Vector-Spectromagnetograph (VSM) (2048 x 2048, 1. 00 by 1. 00 arcsec). › The four observing modes • Stokes I, Q, U, and V profiles in the Fe. I 630. 15 nm and 630. 25 nm lines • Stokes I and V profiles in the Ca. II 854. 2 nm line • Stokes I in the He. I 1083. 0 nm line and the near-by Si. I line › The prospective products: • photospheric vector magnetogram (Fe. I 630. 2), 3 per day. • chromospheric line-of-sight magnetogram (Ca. II 854. 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 K 3 and K 2 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. • Ca. II 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. CISM All-hand meeting Yang Liu 8

Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) • Instrumentation and products – – – 50 cm Vector-Spectromagnetograph (VSM) (2048 x 2048, 1. 00 by 1. 00 arcsec). › The four observing modes • Stokes I, Q, U, and V profiles in the Fe. I 630. 15 nm and 630. 25 nm lines • Stokes I and V profiles in the Ca. II 854. 2 nm line • Stokes I in the He. I 1083. 0 nm line and the near-by Si. I line › The prospective products: • photospheric vector magnetogram (Fe. I 630. 2), 3 per day. • chromospheric line-of-sight magnetogram (Ca. II 854. 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 K 3 and K 2 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. • Ca. II 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. CISM All-hand meeting Yang Liu 9

Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) • Instrumentation and products – – – 50 cm Vector-Spectromagnetograph (VSM) (2048 x 2048, 1. 00 by 1. 00 arcsec). › The four observing modes • Stokes I, Q, U, and V profiles in the Fe. I 630. 15 nm and 630. 25 nm lines • Stokes I and V profiles in the Ca. II 854. 2 nm line • Stokes I in the He. I 1083. 0 nm line and the near-by Si. I line › The prospective products: • photospheric vector magnetogram (Fe. I 630. 2), 3 per day. • chromospheric line-of-sight magnetogram (Ca. II 854. 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 K 3 and K 2 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. • Ca. II 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. CISM All-hand meeting Yang Liu 10

Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) • Instrumentation and products – – – 50 cm Vector-Spectromagnetograph (VSM) (2048 x 2048, 1. 00 by 1. 00 arcsec). › The four observing modes • Stokes I, Q, U, and V profiles in the Fe. I 630. 15 nm and 630. 25 nm lines • Stokes I and V profiles in the Ca. II 854. 2 nm line • Stokes I in the He. I 1083. 0 nm line and the near-by Si. I line › The prospective products: • photospheric vector magnetogram (Fe. I 630. 2), 3 per day. • chromospheric line-of-sight magnetogram (Ca. II 854. 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 K 3 and K 2 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. • Ca. II 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. CISM All-hand meeting Yang Liu 11

Information for SOLIS (Synoptic Optical Long-term Investigations of the Sun) • Instrumentation and products – – – 50 cm Vector-Spectromagnetograph (VSM) (2048 x 2048, 1. 00 by 1. 00 arcsec). › The four observing modes • Stokes I, Q, U, and V profiles in the Fe. I 630. 15 nm and 630. 25 nm lines • Stokes I and V profiles in the Ca. II 854. 2 nm line • Stokes I in the He. I 1083. 0 nm line and the near-by Si. I line › The prospective products: • photospheric vector magnetogram (Fe. I 630. 2), 3 per day. • chromospheric line-of-sight magnetogram (Ca. II 854. 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 K 3 and K 2 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. • Ca. II 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. CISM All-hand meeting Yang Liu 12

Data from SOLIS CISM All-hand meeting Yang Liu 13

Kinematical Properties of CMEs • Cone model. CISM All-hand meeting Yang Liu 14

Kinematical Properties of CMEs • Cone model. CISM All-hand meeting Yang Liu 15

Kinematical Properties of CMEs CISM All-hand meeting Yang Liu 16

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