Inclusion of the CSSS magnetic field calculation into the UCSD tomographic solar wind model

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 4853, Issue , 2002, Pages 504-510

  Dunn, Tamsen ^a   Hick, P Paul ^a   Jackson, Bernard V ^a   Zhao, Xuepu ^b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b STANFORD UNIVERSITY   (United States)

Author keywords

Coronal mass ejections; Heliospheric current sheet; Interplanetary magnetic field; Kinetic solar wind model; Tomography

Indexed keywords

KINEMATICS; MAGNETIC FIELDS; MATHEMATICAL MODELS; TOMOGRAPHY; WIND;

CORONAL MASS EJECTIONS; HELIOSPHERE; HELIOSPHERIC CURRENT; INTERPLANETARY MAGNETIC FIELD; PHOTOSPHERIC MAGNETIC FIELD; SOLAR WIND;

ASTROPHYSICS;

EID: 0038192424     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.460414     Document Type: Conference Paper

References (13)

1. B. T. Tsurutani, and W. D. Gonzalez, "The Interplanetary Causes of Storms: A Review," Geophysical Monograph 98, edited by B. T. Tsurutani, W. D. Gonzalez, Y. Kamide and J. K. Arballo, pp. 77-89, AGU, Washington D.C., 1997.
2. R. L. McPherron, "The Role of Substorms in Generation of Magnetic Storms," Geophysical Monograph 98, edited by B. T. Tsurutani, W. D. Gonzalez, Y. Kamide and J. K. Arballo, pp. 131-147, AGU, Washington, D.C., 1997.
3. B.V. Jackson, P.P. Hick, M. Kojima, and A. Yokobe, "Heliospheric tomography using interplanetary scintillation observations, 1. Combined Nagoya and Cambridge observations," J. Geophys. Res., 103, p. 12049, 1998.
4. B.V. Jackson and P. Hick, "Three Dimensional Tomography of Heliospheric Features Using Global Thomson Scattering Data," Advances in Space Res. 29 (3), pp. 1875-1878, 2000.
5. B.V. Jackson, A. Buffington, and P.P. Hick, "A Heliospheric Imager for Solar Orbiter," Proceedings of Solar Encounter: The First Solar Orbiter Workshop, Puerto de la Cruz, Tenerife, Spain 14-18 May, 2001, pp. 251-255, 2001.
6. B.V. Jackson, P.P. Hick and A. Buffington, "Time-dependent tomography of heliospheric features using interplanetary scintillation (IPS) remote-sensing observations," Proceedings of Solar Wind 10, Pisa, Italy, June 17-21, 2002, submitted.
7. X.P. Zhao and J.T. Hoeksema, "Prediction of the interplanetary magnetic field strength," J. Geophys. Res. Vol. 100, No. A1, pp. 19-33, 1995.
8. T. J. Bogdan and B. C. Low, "The three dimensional structures of magnetic atmospheres, II, Modeling the large-scale corona, Astrophys J. 306, pp. 271-283, 1986.
9. X.P. Zhao, J.T. Hoeksema and N.B. Rich, "Modeling the Radial Variation of Coronal Streamer Belts During Ascending Activity Phase," Advances in Space Res. 29 (3), pp. 411-413, 2002
10. K. H. Schatten, "Current sheet magnetic model for the solar corona," Cosmic Electrodyn. 2, pp. 232-245, 1971.
11. K. Schatten, J. W. Wilcox, and N. F. Ness, "A model of the interplanetary and coronal magnetic fields," Solar Phys. 6, pp. 442-455, 1969.
12. X.P. Zhao et al., "The ambient IMF and its prediction from the observed photospheric magnetic field," J. Geophys. Res., in preparation, 2002.
13. A. J. Hundhausen, Solar Wind and Coronal Expansion, pp. 10-20, Springer-Verlag, New York, 1972.