B.V. Jackson, and P.P. Hick, A. Buffington, M.M. Bisi, J.M. Clover

Slides:

Advertisements

Similar presentations

K. Fujiki, H. Ito, M. Tokumaru Solar-Terrestrial Environment Laboratory (STELab), Nagoya University. SOLAR WIND FORECAST BY USING INTERPLANETARY SCINTILLATION.

Advertisements

H.-S. Yu Center for Astrophysics and Space Sciences, University of California at San Diego, LaJolla, CA, USA 3D-MHD Models Driven by IPS

Global Properties of Heliospheric Disturbances Observed by Interplanetary Scintillation M. Tokumaru, M. Kojima, K. Fujiki, and M. Yamashita (Solar-Terrestrial.

When will disruptive CMEs impact Earth? Coronagraph observations alone aren’t enough to make the forecast for the most geoeffective halo CMEs. In 2002,

Coronal and Heliospheric Modeling of the May 12, 1997 MURI Event MURI Project Review, NASA/GSFC, MD, August 5-6, 2003 Dusan Odstrcil University of Colorado/CIRES.

The “cone model” was originally developed by Zhao et al. ~10 (?) years ago in order to interpret the times of arrival of ICME ejecta following SOHO LASCO.

CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G H.-S. Yu, P.P. Hick, A. Buffington University of California at San Diego, LaJolla, California,

CASS/UCSD AFOSR 2014 IPS 3D Velocity and Density Analysis B.V. Jackson Center for Astrophysics and Space Sciences, University of California at San Diego,

CASS/UCSD KSSS D Analysis of Remote-sensed Heliospheric Data B.V. Jackson, H.-S. Yu, P.P. Hick, A. Buffington University of California at San Diego,

Removal of background light from SMEI white- light all-sky maps, and an all-sky imager design suitable for future deep-space missions Andrew Buffington,

Solar Mass Ejection Imager (SMEI) Analysis of the 20 January 2005 CME B.V. Jackson, P.P. Hick, A. Buffington, M.M. Bisi, and E.A. Jensen Center for Astrophysics.

Solar System Physics Group Heliospheric physics with LOFAR Andy Breen, Richard Fallows Solar System Physics Group Aberystwyth University Mario Bisi Center.

Remote Sensing of Solar Wind Velocity Applying IPS Technique using MEXART Remote Sensing of Solar Wind Velocity Applying IPS Technique using MEXART Mejía-Ambriz.

RECREATING THE THREE DIMENSIONAL STRUCTURE OF INTERPLANETARY CORONAL MASS EJECTIONS Timothy A. Howard and S. James Tappin AGU Fall Meeting, December,

CASS/UCSD AOGS D Analysis of the Heliosphere B.V. Jackson Center for Astrophysics and Space Sciences, University of California at San Diego, La Jolla,

Solar System Physics Group Heliospheric studies with LOFAR and EISCAT-3D Andy Breen, Mario Bisi & Richard Fallows Aberystwyth University.

CASS/UCSD IPS 2013 Remote Sensing Solar Wind Parameters B.V. Jackson Center for Astrophysics and Space Sciences, University of California at San Diego,

CASS/UCSD - Jeju 2015 A Jets in the Heliosphere: A Solar Wind Component B.V. Jackson, H.-S. Yu, P.P. Hick, and A. Buffington, Center for Astrophysics and.

1 University of California, San Diego, U.S.A., 2 NASA - Goddard Space Flight Center, U.S.A., 3 George Mason University, U.S.A., 4 Naval Research Laboratory,

11. Assessing the Contribution of Heliospheric Imaging, IPS and other remote sensing observations in Improving Space Weather Prediction Bernie Jackson,

Measurements of White-Light Images of Cometary Plasma as a Proxy for Solar Wind Speed J.M. Clover, M.M. Bisi, A. Buffington, B.V. Jackson, P.P. Hick Center.

Global Structure of the Inner Solar Wind and it's Dynamic in the Solar Activity Cycle from IPS Observations with Multi-Beam Radio Telescope BSA LPI Chashei.

CASS/UCSD ILWS 2009 SMEI 3D reconstructions of density behind shocks B.V. Jackson, P.P. Hick, A. Buffington, M.M. Bisi, J.M. Clover, S. Hamilton Center.

1 Center for Astrophysics and Space Sciences, University of California, San Diego 9500 Gilman Drive #0424, La Jolla, CA , U.S.A

1 Center for Astrophysics and Space Sciences, University of California, San Diego 9500 Gilman Drive #0424, La Jolla, CA , U.S.A

1 Center for Astrophysics and Space Sciences, University of California, San Diego 9500 Gilman Drive #0424, La Jolla, CA , U.S.A

1 Center for Astrophysics and Space Sciences, University of California, San Diego 9500 Gilman Drive #0424, La Jolla, CA , U.S.A

IPS 3D reconstructions and their comparison with STEREO and Wind spacecraft Mario M. Bisi 1 Bernard V. Jackson 1, John M. Clover 1,

1 Center for Astrophysics and Space Sciences, University of California, San Diego 9500 Gilman Drive #0424, La Jolla, CA , U.S.A

Center for Astrophysics and Space Sciences, University of California, San Diego 9500 Gilman Drive #0424, La Jolla, CA , U.S.A

1 Center for Astrophysics and Space Sciences, University of California, San Diego 9500 Gilman Drive #0424, La Jolla, CA , U.S.A

Bernard V. Jackson, P. Paul Hick, Mario M. Bisi, John M. Clover, Andrew Buffington Center for Astrophysics and Space Sciences, University of California,

CASS/UCSD Dusan_CCMC_2013 Heliospheric Solar Wind Forecasting Using IPS Slides For A Possible CCMC Presentation 2013 Introduction:

Analysis of 3 and 8 April 2010 Coronal Mass Ejections and their Influence on the Earth Magnetic Field Marilena Mierla and SECCHI teams at ROB, USO and.

Shocks in the IPS Wageesh Mishra Eun-kyung Joo Shih-pin Chen.

State of NOAA-SEC/CIRES STEREO Heliospheric Models STEREO SWG Meeting, NOAA/SEC, Boulder, CO, March 22, 2004 Dusan Odstrcil University of Colorado/CIRES.

1 Pruning of Ensemble CME modeling using Interplanetary Scintillation and Heliospheric Imager Observations A. Taktakishvili, M. L. Mays, L. Rastaetter,

1 CASS, University of California, San Diego, U.S.A. ; 2 STFC Rutherford Appleton Laboratory, UK; 3 George Mason University, U.S.A.; 4 NASA/GSFC,

CASS/UCSD-STELab AOGS_2009 Solar Mass Ejection Imager (SMEI) 3D-reconstructions of the Inner Heliosphere Bernard V. Jackson, P. Paul Hick, Andrew Buffington,

A 3D-MHD Model Interface Using Interplanetary Scintillation (IPS) Observations B.V. Jackson 1, H.-S. Yu 1, P.P. Hick 1, A. Buffington 1, D. Odstrcil 2,

CASS/UCSD STEL 2016 Iterated Time-dependent IPS 3D-MHD Models B.V. Jackson Center for Astrophysics and Space Sciences, University of California at San.

CASS/UCSD RSW Space Weather Forecasting from IPS Data Sets M. Tokumaru Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya ,

CASS/UCSD SWG SMEI observations and comparison with STEREO SMEI direct observations and 3D-reconstruction measurements and their comparison with.

Detecting, forecasting and modeling of the 2002/04/17 halo CME Heliophysics Summer School 1.

Solar System Physics Group Heliospheric physics with LOFAR Andy Breen, Richard Fallows Solar System Physics Group Aberystwyth University Mario Bisi Center.

H.-S. Yu 1, B.V. Jackson 1, P.P. Hick 1, A. Buffington 1, M. M. Bisi 2, D. Odstrcil 3,4, M. Tokumaru 5 1 CASS, UCSD, USA ; 2 STFC RALab, Harwell Oxford,

Using World Interplanetary Scintillation Systems

B.V. Jackson H.-S. Yu, P.P. Hick, A. Buffington,

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

Driving 3D-MHD codes Using the UCSD Tomography

Observations of Heliospheric Faraday Rotation

The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network Mario M. Bisi [1], J. Americo Gonzalez-Esparza[2][3][4],

H.-S. Yu1, B.V. Jackson1, P.P. Hick1,

Determination of the North-South Heliospheric Magnetic Field from Inner-Corona Closed-Loop Propagation B.V. Jackson Center for Astrophysics and Space Sciences,

ICME in the Solar Wind from STEL IPS Observations

The Dynamic Character of the Polar Solar Wind

Hinode X-ray Jets Observations of Polar-Region Jets and Their

2014SWW - S9 3D Reconstruction of IPS Remote-sensing Data: Global Solar Wind Boundaries for Driving 3D-MHD Models Hsiu-Shan Yu1, B.V. Jackson1, P.P. Hick1,

ST23-D2-PM2-P-013 The UCSD Kinematic Global Solar Wind Boundary for use in ENLIL 3D-MHD Forecasting Bernard JACKSON1#+, Hsiu-Shan YU1, Paul HICK1, Andrew.

IPS Heliospheric Analyses (STELab)

Bernard V. Jackson1, Hsiu-Shan Yu1, P

Exploration of Solar Magnetic Fields from Propagating GONG Magnetograms Using the CSSS Model and UCSD Time-Dependent Tomography H.-S. Yu1, B. V. Jackson1,

B.V. Jackson H.-S. Yu, P.P. Hick, A. Buffington, M. Tokumaru

Bernard V. Jackson, P. Paul Hick, Andrew Buffington, John M. Clover

D. Odstrcil1,2, V.J. Pizzo2, C.N. Arge3, B.V.Jackson4, P.P. Hick4

Miho Janvier (IAS) & Ben Lynch (UCB)

ESWW 13 – Oostende, Belgium – November 2016

B.V. Jackson H.-S. Yu, P.P. Hick, A. Buffington, M. Tokumaru

The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network: Initial Results from the October 2016 Space-Weather Campaign © 2017 RAL Space.

Investigation of Heliospheric Faraday Rotation Due to a Coronal Mass Ejection (CME) Using the LOw Frequency ARray (LOFAR) and Space-Based Imaging Techniques.

Presentation transcript:

B.V. Jackson, and P.P. Hick, A. Buffington, M.M. Bisi, J.M. Clover Center for Astrophysics and Space Sciences, University of California at San Diego, LaJolla, CA, USA http://smei.ucsd.edu/ http://ips.ucsd.edu/ Masayoshi

1 gigabyte/day; now ~3 terabytes DATA Jackson, B.V., et al., 2006, J. Geophys. Res., 111, A4, A04S91 SMEI Launch 6 January 2003 1 gigabyte/day; now ~3 terabytes  Sun C1 C2 C3 Sun | V Simultaneous images from the three SMEI cameras.

“Auroral-cleaned” lines of sight on a 3-D reconstructed sky map DATA SMEI “direct images” With Milky Way, zodiac – 0, 400 No Milky Way, zodiac – 0, 20 “Auroral-cleaned” lines of sight on a 3-D reconstructed sky map With zodiacal light – 0, 200

Heliospheric 3-D Reconstruction Jackson, B.V., et al., 2009, Adv. in Geosciences, 21, 339-366. Heliospheric 3-D Reconstruction Line of sight “crossed” components on a reference surface. Projections on the reference surface are shown. These weighted components are inverted to provide the time-dependent tomographic reconstruction.

LASCO C2 coronagraph image. SMEI 3D-reconstruction. SMEI 3D reconstruction of the 28 October (Halloween Storm) 2003 CME. LASCO C2 coronagraph image. Jackson, B.V., et al., 2006, J. Geophys. Res., 111, A4, A04S91 SMEI 3D-reconstruction.

2003 October 28 CME Jensen, E.A. et al., 2010, Solar Phys., (in press), doi:10.1007/s11207-010-9543-2 . Flux Cylinder 3-D reconstruction 2003/10/30 00 UT ^ | 1 AU “B” fit of the 28 October 2003 CME Magnetic loop analysis by T. Mulligan SMEI Sky Map image to 110º LASCO C2 CME image to 6 Rs. Jackson, B.V., et al., 2006, J. Geophys. Res., 111, A4, A04S91

28 October 2003 CME “Halloween storm” ICME Recent higher-resolution SMEI PC 3D reconstructions show the CME sheath region as well as the central dense core 28 October 2003 CME “Halloween storm” ICME shock Ecliptic cuts

Shock density enhancement volumetric mass 28 October 2003 CME/ICME shock density Volumetric rendering Meridional cuts Shock density enhancement volumetric mass The major portion of the shock density enhancement for the 28 October 2003 ICME is present over only a tiny portion of the heliosphere!

Last ~12 months Bisi, M.M., B.V. Jackson, A. Buffington, J.M. Clover, P.P. Hick, and M. Tokumaru, 2009, ‘Low-Resolution STELab IPS 3D Reconstructions of the Whole Heliosphere Interval and Comparison with in-Ecliptic Solar Wind Measurements from STEREO and Wind Instrumentation’, Solar Phys. - STEREO Science Results at Solar Minimum Topical Issue, 256, 201-217, doi:10.1007/s11207-009-9350-9. Bisi, M.M., Jackson, B.V., Clover, J.M., Manoharan, P.K., Tokumaru, M., Hick, P.P., and. Buffington, A., 2009, ‘3D reconstructions of the early-November 2004 CDAW geomagnetic storms: analysis of Ooty IPS speed and density data’, Annales Geophysicae, 27, 4479. Bisi, M.M., Jackson, B.V., Clover, J.M., Tokumaru, M., and Fujiki, K., 2009, ‘Large-Scale Heliospheric Structure during Solar-Minimum Conditions using a 3D Time-Dependent Reconstruction Solar-Wind Model and STELab IPS Observations’, American Institute of Physics (Solar Wind 12 Proceedings), 1216, 355. Bisi, M.M., Jackson, B.V., Clover, J.M., Hick, P.P., and Buffington, A., 2009, ‘3D Reconstructions of the Whole Heliosphere Interval and Comparison with in-Ecliptic Solar Wind Measurements from STEREO, ACE, and Wind Instrumentation: a Brief Summary’, XXVIIth IAU General Assembly, August 2009, Highlights of Astronomy, 15, 119. Bisi, M.M., Jackson, B.V., Breen, A.R., Dorrian, G.D., Fallows, R.A., Clover, J.M., and Hick, P.P., 2009, ‘Three-Dimensional (3-D) Reconstructions of EISCAT IPS Velocity Data in the Declining Phase of Solar Cycle 23’, Solar Phys. (in-press). Bisi, M.M., Breen, A.R., Jackson, B.V., Fallows, R.A., Walsh, A.P., Mikic, Z., Riley, P., Owen, C.J., Gonzalez-Esparza, A., Aguilar-Rodriguez, E., Morgan, H., Jensen, E.A., Wood, A.G., Tokumaru, M., Manoharan, P.K., Chashei, I.V., Giunta, A.S., Linker, J.A., Shishov, V.I., Tyul’bashev, S.A., Agalya, , G., Glubokova, S.K., Hamilton, M.S., Fujiki, K., Hick, P.P., Clover, J.M., Pinter, B., 2009, ‘From the Sun to the Earth: the 13 May 2005 Coronal Mass Ejection’, Solar Phys. (in press). Buffington, A., Bisi, M.M., Clover, J.M., Hick, P.P., Jackson, B.V., Kuchar, T.A., and Price, S.D., 2009, ‘Measurements of the Gegenschein brightness from the Solar Mass Ejection Imager (SMEI)’, Icarus, 203, 124, doi:10.1016/j.icarus.2009.04.007. Jackson, B.V., Hick, P.P., Buffington, A., Bisi, M.M., and Clover, J.M., 2009, ‘SMEI direct, 3D-reconstruction sky maps and volumetric analyses, and their comparison with SOHO and STEREO observations’, Annales Geophysicae, 27, 4097. Jackson, B.V., Hick, P.P., Buffington, A., Bisi, M.M., Clover, J.M., Tokumaru, M., and Fujiki, K., 2009, ‘3D Reconstruction of Density Enhancements Behind Interplanetary Shocks from Solar Mass Ejection Imager White-Light Observations’, American Institute of Physics (Solar Wind 12 Proceedings), 1216, 659. Jackson, B.V., Hick, P.P., Buffington, A., Bisi, M.M., Clover, J.M., and Tokumaru, M., 2008, ‘Solar Mass Ejection Imager (SMEI) and Interplanetary Scintillation (IPS) 3D-Reconstructions of the Inner Heliosphere’, Adv. in Geosciences, 21, 339-366. Jackson, B.V., Hick, P.P., Bisi, M.M., Clover, J.M., and Buffington, A., 2009, ‘Inclusion of in-situ Velocity Measurements in the UCSD Time-Dependent Tomography to Constrain and Better- Forecast Remote-Sensing Observations’, Solar Phys., in-press, doi: 10.1007/s11207-010-9529-0. Jackson, B.V., Buffington, A., Hick, P.P., Bisi, M.M., and Clover, J.M., 2009, A Heliospheric Imager for Deep Space: Lessons Learned from Helios, SMEI, and STEREO’, Solar Phys., in press, doi: 10.1007/s11207-010-9579-3. Jensen, E.A., Hick, P.P., Bisi, M.M., Jackson, B.V., Clover, J., and Mulligan, T.L., 2009, ‘Faraday Rotation Response to Coronal Mass Ejection Structure’, Solar Phys., in press, 10.1007/s11207-010-9543-2. Webb, D.F., Howard, T.A., Fry, C.D., Kuchar, T.A., Odstrcil, D., Jackson, B.V., Bisi, M.M., Harrison, R.A., Morrill, J.S., Howard, R.A., and Johnston, J.C., 2009, ‘Study of CME Propagation in the Inner Heliosphere: SMEI and STEREO HI Observations of the January 2007 Events’, Solar Phys.- STEREO Special Issue, 256, 239, doi:10.1007/s11207-009-9351-8. Webb, D. F., Howard, T. A., Fry, C. D., Kuchar, T. A., Mizuno, D. R., Johnston, J. C., and Jackson, B. V., 2009, ‘Studying Geoeffective ICMEs between the Sun and Earth: Space Weather Implications of SMEI Observations’, Space Weather, 7, S05002, doi:10.1029/2008SW000409.

Summary: The Model: (not a model but a fit to data) Allows a “limited” low-resolution 3-D reconstruction over time of most of the heliosphere. Some of the things we’ve learned: How well our data collection system works. The extent, shape, 3D mass, and energies of specific ICMEs. The latitude-longitude relationship and temporal evolution of velocity structures globally in the heliosphere, and to ICMEs. In the SMEI highest-resolution tomography, the shock density enhancements analyzed to date do not show a uniform shell-like extent. (?don’t know why).