Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-27T20:54:24.189Z Has data issue: false hasContentIssue false

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
Affiliation:
Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive #0424, La Jolla, CA 92093-0424, USA email: [email protected] or [email protected]
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: [email protected] or [email protected]
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: [email protected] or [email protected]
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: [email protected] or [email protected] 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: [email protected] or [email protected]
M. Tokumaru
Affiliation:
Solar-Terrestrial Environment Laboratory (STELab), Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8601, Japan
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Contributed Papers
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