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H.-S. Yu, B.V. Jackson, and A. Buffington

Tracing the Polar Jets into the Inner Heliosphere by Using Images from LASCO C2 and STEREO COR2 Coronagraphs and 3D Tomographic Reconstructions from Interplanetary Scintillation and the Solar Mass Ejection Imager (SMEI). H.-S. Yu, B.V. Jackson, and A. Buffington

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H.-S. Yu, B.V. Jackson, and A. Buffington

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  1. Tracing the Polar Jets into the Inner Heliosphere by Using Images from LASCO C2 and STEREO COR2 Coronagraphs and 3D Tomographic Reconstructions from Interplanetary Scintillation and the Solar Mass Ejection Imager (SMEI) H.-S. Yu, B.V. Jackson, and A. Buffington Center for Astrophysics and Space Sciences, University of California, San Diego

  2. Hinode X-ray Jets: (Survey Period: Sep 5 – Sep 22, 2007) Nearly 850 jets over a three-week period about 60 jets per day (Sako et al. 2010)

  3. Hinode Jets on Sep 14, 2007 brightest

  4. Hinode Jets on Sep 14, 2007 07:14:48 07:18:48 07:22:48 07:26:48

  5. 2007 Sep 14 Hinode Jets in LASCO C2 09:06UT 08:54UT 08:30UT 08:06UT ~420 kms-1 Jet Jet

  6. 2D Cross Correlation of LASCO C2 Coronal Flow 2007 SEP 14 08:30:04 – 08:06:04 Jet Jet > 400km/s

  7. SMEI pseudo coronagraph observations from the 3D reconstruction

  8. SMEI 3D Jet Analysis: 2007 Sep 14 Jet 2007/09/17 06 UT Mass: 1.552x1014 g Volume: 0.002 AU3 Speed: ~ 525 km/s SMEI observations of the Jet at different distances

  9. Hinode Observing Proposal (HOP-187) “Jets from the solar surface to interplanetary space” (2011/06/17 00:00 - 06:00 UT 2011/08/22 00:00 - 08:00 UT) Observational Data: Spacecraft, ground-based input –Hinode, SDO, SOHO LASCO, STEREO, SMEI, IPS 2D Correlation Technique: Measurement of jet speeds and durations in LASCO C2 and STEREO COR2 3D Analysis Technique: Tracking jet responses into the heliosphere

  10. SDO/AIA Jets: 17 June 2011 00:00 - 06:00 UT

  11. SDO/AIA Jet (2011-JUN-17) 02:35 02:49 03:04 03:18

  12. 2011 June 17 SDO/AIA Jet LASCO C2 Coronal Flow Jet LASCO C2 03:30UT SDO AIA

  13. STEREO COR2 Coronal Flow Jet COR 2 03:39UT SDO AIA

  14. The height-time plotJet response on the sky plane

  15. The height-time plotJet location from the Sun center ~1330 kms-1

  16. STEREO COR2 Coronal Flow Overplotted Blue color: 2D cross-correlation velocity at 3.6 Rs (determined from this and the following coronagraph image.) COR 2 SDO AIA

  17. Synopsis of the Speed with height 2 Jet speed > 1200 kms-1 Characteristic size of Jet ~1.5 Rs long, 3°wide

  18. High-speed jet response in IPS meridional cut 85o west of the Sun-Earth Line Jet

  19. Summary • The high speed responses measured in LASCO C2 and STEREO COR2 coronagraph images show an association with Hinode and SDO/AIA jets. • Jet responses measured in C2/COR2 can also be observed in the Solar Mass Ejection Imager (SMEI) and Interplanetary Scintillation (IPS) analysis. • We can determine the mass contained in a jet, the volume of a jet, and its speed by tracing its density in the 3D SMEI analysis. • Observations of the same high speed response (at 2011 June 17 02:50 UT by the SDO/AIA ) in both LASCO C2 and COR II observations 90° in longitude from each other are a good indication that these measurements are material flow. • The characteristic size of the main jet response of the 2011 June 17 jet seen in coronagraph images is about 1.5 Rs long and 3° wide.

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