Polar Jet Manifestation in the Inner Heliosphere from Images using the LASCO C2 and STEREO COR2 Coro...
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Polar Jet Manifestation in the Inner Heliosphere from Images using the LASCO C2 and STEREO COR2 Coronagraphs and 3D Tomographic Reconstructions from Interplanetary Scintillation (IPS) 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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H s yu b v jackson and a buffington

Polar Jet Manifestation in the Inner Heliosphere from Images using the LASCO C2 and STEREO COR2 Coronagraphs and 3D Tomographic Reconstructions from Interplanetary Scintillation (IPS) 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


Hinode x ray jets survey period sep 5 sep 22 2007

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)


Hinode jets on sep 14 2007

Hinode Jets on Sep 14, 2007

brightest


Hinode jets on sep 14 20071

Hinode Jets on Sep 14, 2007

07:14:48 07:18:48 07:22:48 07:26:48


2007 sep 14 hinode jets in lasco c2

2007 Sep 14 Hinode Jets in LASCO C2


2007 sep 14 hinode jets in lasco c21

2007 Sep 14 Hinode Jets in LASCO C2

Jet

Jet


2d cross correlation of lasco c2 coronal flow

2D Cross Correlation of LASCO C2 Coronal Flow

Jet

Jet > 400km/s


Smei pseudo coronagraph observations from the 3d reconstruction

SMEI pseudo coronagraph observations from the 3D reconstruction


Smei 3d reconstructed differenced sky map shows the jet response

SMEI 3D reconstructed differenced sky map shows the jet response


Smei 3d jet analysis 2007 sep 14 jet at different distances

SMEI 3D Jet Analysis: 2007 Sep 14 Jet at different distances


Smei 3d jet analysis 2007 sep 14 jet at 0 67au

SMEI 3D Jet Analysis: 2007 Sep 14 Jet at 0.67AU

Mass: 1.552x1014 g

Volume: 0.002 AU3

Speed: ~ 525 km/s

Energy: 4.3x1029 ergs


Hinode observing proposal hop 187

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


Sdo aia jets 17 june 2011 00 00 06 00 ut

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


Sdo aia jet 2011 jun 17

SDO/AIA Jet (2011-JUN-17)

02:35 02:49 03:04 03:18


2011 june 17 sdo aia jet lasco c2 coronal flow

2011 June 17 SDO/AIA Jet LASCO C2 Coronal Flow

Jet

LASCO C2 03:30UT

SDO AIA


Stereo cor 2a coronal flow

STEREO COR 2A Coronal Flow

Jet

COR 2A 03:39UT

SDO AIA


The height time plot jet response on the sky plane

The height-time plotJet response on the sky plane


The height time plot jet location from the sun center

The height-time plotJet location from the Sun center

~1330 kms-1


Stereo cor2 coronal flow

STEREO COR2 Coronal Flow

Overplotted Blue color: 2D cross-correlation velocity at 3.6 Rs (determined from this and the following coronagraph image.)

COR 2A

SDO AIA


Synopsis of the speed with height

Synopsis of the Speed with height

2

Jet speed > 1200 kms-1

Characteristic size of jet reponse

~1.5 Rs long, 3°wide


High speed jet response in ips

High-speed jet response in IPS

meridional cut at

85o west of the

Sun-Earth Line

Jet


Jet responses

Jet responses


Jet brightness spectrum for hinode observation in september 2007

Jet brightness spectrum for Hinode observation in September 2007

Estimated total

mass of jet ~ 1016g

~5% of solar wind

determined by Ulysses

(Sako et al., 2010)


Summary

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 2 observations 90° in longitude from each other are a good indication that these measurements are material flow.

  • The jets contribute ~5% mass of solar wind estimated by observations from Ulysses.


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