Mapping Solar Wind Streams from the Sun to 1 AU: A Comparison of Techniques

[1]  V. Pizzo Interplanetary Shocks on the Large Scale: A Retrospective on the Last Decade's Theoretical Efforts , 2013 .

[2]  P. Riley The Three‐Dimensional Structure of the Inner Heliosphere , 2010 .

[3]  M. Moncuquet,et al.  TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE , 2010 .

[4]  J. Linker,et al.  Global MHD Modeling of the Solar Corona and Inner Heliosphere for the Whole Heliosphere Interval , 2008, Proceedings of the International Astronomical Union.

[5]  P. Riley CME dynamics in a structured solar wind , 2008 .

[6]  E. Cliver,et al.  A Floor in the Solar Wind Magnetic Field , 2007 .

[7]  R. Jimenez,et al.  Model Atmospheres for Irradiated Giant Stars: Implications for the Galactic Center , 2006, astro-ph/0601527.

[8]  J. Linker,et al.  Understanding the Solar Sources of In Situ Observations , 2003 .

[9]  D. Odstrcil,et al.  Improved Method for Specifying Solar Wind Speed Near the Sun , 2003 .

[10]  M. Velli,et al.  Solar Wind Ten , 2003 .

[11]  J. Linker,et al.  Merging of coronal and heliospheric numerical two‐dimensional MHD models , 2002 .

[12]  M. Dryer,et al.  Improvements to the HAF solar wind model for space weather predictions , 2001 .

[13]  J. Linker,et al.  An empirically‐driven global MHD model of the solar corona and inner heliosphere , 2001 .

[14]  J. Linker,et al.  Including the Transition Region in Models of the Large-Scale Solar Corona , 2001 .

[15]  M. Goldstein,et al.  A global MHD solar wind model with WKB Alfvén waves: Comparison with Ulysses data , 2000 .

[16]  C. Arge,et al.  Improvement in the prediction of solar wind conditions using near‐real time solar magnetic field updates , 2000 .

[17]  J. Richardson,et al.  A numerical study of the evolution of the solar wind from Ulysses to Voyager 2 , 2000 .

[18]  J. Gosling,et al.  Do coronal mass ejections implode in the solar wind? , 1998 .

[19]  G. Siscoe,et al.  Radial alignment simulation of solar wind streams observed by Pioneers 10 and 11 in 1974 , 1995 .

[20]  N. Sheeley,et al.  Solar wind speed and coronal flux-tube expansion , 1990 .

[21]  Eckart Marsch,et al.  Physics of the Inner Heliosphere II , 1990 .

[22]  R. Schwenn Large-scale structure of the interplanetary medium , 1990 .

[23]  E. Marsch,et al.  Large-scale phenomena , 1990 .

[24]  William H. Press,et al.  Numerical recipes in C. The art of scientific computing , 1987 .

[25]  Bruce T. Tsurutani,et al.  Collisionless shocks in the heliosphere: reviews of current research , 1985 .

[26]  K. Hakamada,et al.  Simulation of three-dimensional solar wind disturbances and resulting geomagnetic storms , 1982 .

[27]  V. Pizzo On the application of numerical models to the inverse mapping of solar wind flow structures , 1981 .

[28]  V. Pizzo A three-dimensional model of co-rotating streams in the solar wind. 2: Hydrodynamic streams , 1979 .

[29]  V. Pizzo A three-dimensional model of corotating streams in the solar wind. 1: Theoretical foundations , 1978 .

[30]  W. Feldman,et al.  Solar wind stream interfaces , 1978 .

[31]  E. Smith,et al.  Observations of interaction regions and corotating shocks between one and five AU - Pioneers 10 and 11. [solar wind streams] , 1976 .

[32]  E. Roelof,et al.  Large-scale structure of the interplanetary medium , 1973 .

[33]  P. Lerman Gangs, Networks, and Subcultural Delinquency , 1967, American Journal of Sociology.

[34]  M. Neugebauer,et al.  The relation of Mariner-2 plasma data to solar phenomena , 1966 .

[35]  W. I. Axford The solar wind , 1965 .

[36]  V. Sarabhai Some consequences of nonuniformity of solar wind velocity , 1963 .

[37]  E. Parker Dynamics of the Interplanetary Gas and Magnetic Fields , 1958 .