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A Summary of 3-D Reconstructions of the Whole Heliosphere Interval and Comparison with in-Ecliptic Solar Wind Measurements from STEREO, ACE, and Wind Instrumentation

Published online by Cambridge University Press:  21 October 2010

Mario M. Bisi ,
B. V. Jackson ,
J. M. Clover ,
P. P. Hick ,
A. Buffington  and
M. Tokumaru
Mario M. Bisi
Affiliation:
Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive #0424, La Jolla, CA 92093-0424, USA email: mmbisi@ucsd.edu or Mario.Bisi@gmail.com
B. V. Jackson
Affiliation:
Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive #0424, La Jolla, CA 92093-0424, USA email: mmbisi@ucsd.edu or Mario.Bisi@gmail.com
J. M. Clover
Affiliation:
Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive #0424, La Jolla, CA 92093-0424, USA email: mmbisi@ucsd.edu or Mario.Bisi@gmail.com
P. P. Hick
Affiliation:
Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive #0424, La Jolla, CA 92093-0424, USA email: mmbisi@ucsd.edu or Mario.Bisi@gmail.com San Diego Supercomputer Center, University of California, San Diego, 9500 Gilman Drive #0505, La Jolla, CA 92093-0505, USA
A. Buffington
Affiliation:
Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive #0424, La Jolla, CA 92093-0424, USA email: mmbisi@ucsd.edu or Mario.Bisi@gmail.com
M. Tokumaru
Affiliation:
Solar-Terrestrial Environment Laboratory (STELab), Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8601, Japan
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Abstract

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We present a summary of results from simultaneous Solar-Terrestrial Environment Laboratory (STELab) Interplanetary Scintillation (IPS), STEREO, ACE, and Wind observations using three-dimensional reconstructions of the Whole Heliosphere Interval – Carrington rotation 2068. This is part of the world-wide IPS community's International Heliosphysical Year (IHY) collaboration. We show the global structure of the inner heliosphere and how our 3-D reconstructions compare with in-ecliptic spacecraft measurements.

Keywords

(Sun:) solar wind(Sun:) solar-terrestrial relations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 480 - 483
Copyright
Copyright © International Astronomical Union 2010

References

Bisi, M. M., Jackson, B. V., Buffington, A., Clover, J. M., Hick, P. P., & Tokumaru, M. 2009, Solar Phys. 256, 201CrossRefGoogle Scholar
Hewish, A., Scott, P. F., & Wills, D., 1964, Nature 203, 1214CrossRefGoogle Scholar
Jackson, B. V. & Hick, P. P., 2005, in Astrophys. and Space Sci. Lib., 314, Solar and Space Weather Radiophysics: Current status and future developments, ed. Gary, D. & Keller, C. U. (Kluwer Academic Publ., Dordrecht.), 355Google Scholar
Kojima, M. & Kakinuma, T. 1987, J. Geophys. Res. 92, 7269CrossRefGoogle Scholar