3D Reconstruction of Interplanetary Scintillation (IPS) Remote-Sensing Data: Global Solar Wind Boundaries for Driving 3D-MHD Models
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H.-S. Yu | D. Odstrcil | A. Buffington | A. Buffington | D. Odstrcil | J. Davies | B. Jackson | M. Tokumaru | M. Bisi | H.‐S. Yu | C.-C. Wu | M. Tokumaru | J. A. Davies | B. V. Jackson | P. P. Hick | M. M. Bisi | C.-C. Wu | P. P. Hick
[1] A. Buffington,et al. Three-dimensional reconstruction of heliospheric structure using iterative tomography: A review , 2011 .
[2] Mario M. Bisi,et al. Combined STELab, EISCAT, ESR, and MERLIN IPS observations of the solar wind , 2007, SPIE Optical Engineering + Applications.
[3] J. Gonzalez-Esparza,et al. Observations of Interplanetary Scintillation (IPS) Using the Mexican Array Radio Telescope (MEXART) , 2010 .
[4] M. Kojima,et al. Solar cycle evolution of solar wind speed structure between 1973 and 1985 observed with the interplanetary scintillation method , 1987 .
[5] Dusan Odstrcil,et al. Initial coupling of coronal and heliospheric numerical magnetohydrodynamic codes , 2004 .
[6] L. Burlaga,et al. Compound streams, magnetic clouds, and major geomagnetic storms , 1987 .
[7] D. Mccomas,et al. A high‐latitude interplanetary magnetic field enhancement at Ulysses , 2002 .
[8] A. Buffington,et al. Low-Resolution STELab IPS 3D Reconstructions of the Whole Heliosphere Interval and Comparison with in-Ecliptic Solar Wind Measurements from STEREO and Wind Instrumentation , 2009 .
[9] J. T. Hoeksema,et al. Prediction of the interplanetary magnetic field strength , 1995 .
[10] Bernard V. Jackson,et al. Inclusion of Real-Time In-Situ Measurements into the UCSD Time-Dependent Tomography and Its Use as a Forecast Algorithm , 2013 .
[11] J. Linker,et al. Dynamical evolution of the inner heliosphere approaching solar activity maximum: interpreting Ulysses observations using a global MHD model , 2003 .
[12] T. Ohmi,et al. Time‐dependent tomography of hemispheric features using interplanetary scintillation (IPS) remote‐sensing observations , 2003 .
[13] A. Hewish,et al. The sources of large-scale heliospheric disturbances , 1986 .
[14] I. Richardson. Geomagnetic activity during the rising phase of solar cycle 24 , 2013 .
[15] Dusan Odstrcil,et al. Numerical simulation of the 12 May 1997 interplanetary CME event , 2004 .
[16] M. Dryer,et al. Simulated Solar Mass Ejection Imager and “Solar Terrestrial Relations Observatory‐like” views of the solar wind following the solar flares of 27–29 May 2003 , 2008 .
[17] Tucson,et al. ULTRAVIOLET SPECTROSCOPY OF TYPE IIB SUPERNOVAE: DIVERSITY AND THE IMPACT OF CIRCUMSTELLAR MATERIAL , 2014, 1412.4767.
[18] Bernard V. Jackson,et al. Heliospheric tomography: an algorithm for the reconstruction of the 3D solar wind from remote sensing observations , 2004, SPIE Optics + Photonics.
[19] Jon A. Linker,et al. Disruption of Coronal Magnetic Field Arcades , 1994 .
[20] D. Odstrcil,et al. Three-dimensional propagation of CMEs in a structured solar wind flow: 1. CME launched within the streamer belt , 1999 .
[21] M. Tokumaru. Three-dimensional exploration of the solar wind using observations of interplanetary scintillation , 2013, Proceedings of the Japan Academy. Series B, Physical and biological sciences.
[22] J. Linker,et al. Global MHD Modeling of the Solar Corona and Inner Heliosphere for the Whole Heliosphere Interval , 2011 .
[23] C. Arge,et al. Improvement in the prediction of solar wind conditions using near‐real time solar magnetic field updates , 2000 .
[24] S. Wu,et al. Global simulation of extremely fast coronal mass ejection on 23 July 2012 , 2014 .
[25] S. Wu,et al. A HYBRID SOLAR WIND MODEL OF THE CESE+HLL METHOD WITH A YIN–YANG OVERSET GRID AND AN AMR GRID , 2011, The Astrophysical Journal.
[26] L. Burlaga,et al. MHD description of the dynamical relationships between a flux rope, streamer, coronal mass ejection, and magnetic cloud : An analysis of the January 1997 Sun-Earth connection event , 1999 .
[27] W. Liu,et al. Determination of geometrical and kinematical properties of halo coronal mass ejections using the cone model , 2002 .
[28] C. Eyles,et al. Long-Term Evolution of the Photometric Calibration of the STEREO Heliospheric Imagers: I. HI-1 , 2012 .
[29] Bernard V. Jackson,et al. The Solar Mass-Ejection Imager (SMEI) Mission , 2003 .
[30] P. K. Manoharan,et al. 3-D reconstructions of the early-November 2004 CDAW geomagnetic storms: analysis of Ooty IPS speed and density data , 2009 .
[31] C. Russell,et al. Perpendicular flow deviation in a magnetized counter-streaming plasma , 2012 .
[32] Bernard V. Jackson,et al. Heliospheric tomography using interplanetary scintillation observations: 2. Latitude and heliocentric distance dependence of solar wind structure at 0.1–1 AU , 1998 .
[33] M. Dryer,et al. A global 3-D simulation of interplanetary dynamics in June 1991 , 1995 .
[34] A. Hewish,et al. Interplanetary Scintillation of Small Diameter Radio Sources , 1964, Nature.
[35] Bernard V. Jackson,et al. Time-dependent tomography of heliospheric features using the three-dimensional reconstruction techniques developed for the solar mass ejection imager (SMEI) , 2003, SPIE Astronomical Telescopes + Instrumentation.
[36] M. Tokumaru,et al. A newly developed UHF radiotelescope for interplanetary scintillation observations: Solar Wind Imaging Facility , 2011 .
[38] P. Lamy,et al. The Large Angle Spectroscopic Coronagraph (LASCO) , 1995 .
[39] Andrew Wilson. Solar variability as an input to the Earth's environment , 2003 .
[40] E. Christian,et al. The STEREO Mission: An Introduction , 2008 .
[41] Keiji Hayashi,et al. Fast solar wind after the rapid acceleration , 2004 .
[42] N. Pogorelov,et al. MHD heliosphere with boundary conditions from a tomographic reconstruction using interplanetary scintillation data , 2014 .
[43] Bernard V. Jackson,et al. The Solar Mass Ejection Imager (Smei) , 2003 .
[44] C. Eyles,et al. Calibrating the Pointing and Optical Parameters of the STEREO Heliospheric Imagers , 2009 .
[45] J. Davies,et al. The Heliospheric Imagers Onboard the STEREO Mission , 2009 .
[46] C. J. Wolfson,et al. Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) , 2008 .
[47] P. Lamy,et al. The Large Angle Spectroscopic Coronagraph (LASCO) , 1995 .
[48] S. Wu,et al. Global three‐dimensional simulation of the interplanetary evolution of the observed geoeffective coronal mass ejection during the epoch 1–4 August 2010 , 2011 .
[49] B. Jackson,et al. Heliospheric tomography using interplanetary scintillation observations. 1. Combined Nagoya and Cambridge data , 1998 .
[50] A. T. Young. INTERPRETATION OF INTERPLANETARY SCINTILLATIONS. , 1971 .
[51] B. Jackson,et al. Three-Dimensional (3-D) Reconstructions of EISCAT IPS Velocity Data in the Declining Phase of Solar Cycle 23 , 2010 .
[52] W. Coles,et al. Microturbulence in solar wind streams , 1980 .
[53] D. Odstrcil. Modeling 3-D solar wind structure , 2003 .
[54] I. Cairns,et al. Type II solar radio bursts predicted by 3‐D MHD CME and kinetic radio emission simulations , 2013 .
[55] Z. Houminer,et al. Corotating Plasma Streams revealed by Interplanetary Scintillation , 1971 .
[56] A. Wilson,et al. Solar variability: from core to outer frontiers , 2002 .
[57] J. Phillips,et al. Geomagnetic activity associated with earth passage of interplanetary shock disturbances and coronal mass ejections , 1991 .
[58] M. Tokumaru,et al. Toroidal-shaped interplanetary disturbance associated with the halo coronal mass ejection event on 14 July 2000 , 2003 .
[59] Bernard V. Jackson,et al. Comparative Analyses of the CSSS Calculation in the UCSD Tomographic Solar Observations , 2005 .
[60] N. Lugaz,et al. Numerical Modeling of Interplanetary Coronal Mass Ejections and Comparison with Heliospheric Images , 2010, 1008.5394.
[61] S. Wu,et al. THREE-DIMENSIONAL SOLAR WIND MODELING FROM THE SUN TO EARTH BY A SIP-CESE MHD MODEL WITH A SIX-COMPONENT GRID , 2010 .
[62] J. Linker,et al. An empirically‐driven global MHD model of the solar corona and inner heliosphere , 2001 .
[63] D. D. Zeeuw,et al. Global three‐dimensional MHD simulation of a space weather event: CME formation, interplanetary propagation, and interaction with the magnetosphere , 2000 .
[64] M. Tokumaru,et al. Kinematic Properties of Slow ICMEs and an Interpretation of a Modified Drag Equation for Fast and Moderate ICMEs , 2014, 1401.1724.
[65] M. Tokumaru,et al. Radial Speed Evolution of Interplanetary Coronal Mass Ejections During Solar Cycle 23 , 2013, 1303.5154.
[66] A. Buffington,et al. Inclusion of In-Situ Velocity Measurements into the UCSD Time-Dependent Tomography to Constrain and Better-Forecast Remote-Sensing Observations , 2010 .
[67] D. Mccomas,et al. Strong interplanetary field enhancements at Ulysses—evidence of dust trails' interaction with the solar wind? , 2003 .
[68] N. Sheeley,et al. Solar wind speed and coronal flux-tube expansion , 1990 .
[69] S. Wu,et al. Evolution of fast and slow shock interactions in the inner heliosphere , 2004 .
[70] J. Linker,et al. Merging of coronal and heliospheric numerical two‐dimensional MHD models , 2002 .
[71] J. Davies,et al. First Imaging of Coronal Mass Ejections in the Heliosphere Viewed from Outside the Sun – Earth Line , 2008 .
[72] P. K. Manoharan. Ooty Interplanetary Scintillation – Remote-Sensing Observations and Analysis of Coronal Mass Ejections in the Heliosphere , 2010 .
[73] M. M. Bisi,et al. Interaction between coronal mass ejections and the solar wind , 2007 .
[74] A. Hewish,et al. Structure and evolution of compound streams at ≤1 AU , 1991 .
[75] A. Buffington,et al. A DETERMINATION OF THE NORTH–SOUTH HELIOSPHERIC MAGNETIC FIELD COMPONENT FROM INNER CORONA CLOSED-LOOP PROPAGATION , 2015 .
[76] A. Buffington,et al. A Heliospheric Imager for Deep Space: Lessons Learned from Helios, SMEI, and STEREO , 2010 .
[77] Bernard V. Jackson,et al. Three-Dimensional Tomography of Interplanetary Disturbances , 2004 .