University of Kansas X-Ray Emission in the Solar System

(DRAFT) Temporal and Spatial Variations of Heliospheric X-Ray Emissions Associated with Charge Transfer of the Solar Wind with Interstellar Neutrals I. P. Robertson, T. E. Cravens, and S. Snowden

Image: Jovian soft X-rays from ROSAT; courtesy of J. H. Waite.

References

Cox, D. P., Modeling the Local Bubble, in The Local Bubble and Beyond, edited by D. Breitschwerdt, M. J. Freyberg, and J. Trumper, New York, Springer-Verlag, 1998, p. 121.
Cravens, T. E., Geophys. Res. Lett., 24, 105 (1997).
Cravens, T. E., Astrophys. J., 532, L153 (2000).
Cravens, T. E., Science, 296, 1042 (2002).
Cravens, T. E., Robertson, I. P., and Snowden, S. L., J. Geophys. Res., 106, 24883 (2001).
Dennerl, K., Englhauser, J., and Trumper, J., Science 277, 1625 (1997).
Fahr, H. J., Astron. Astrophys., 14, 263 (1971).
Lisse, C. M. , et al., Science, 274, 205 (1996).
Robertson, I. P., Cravens, T. E., Snowden, S., and Linde, T., Space Science Reviews, 97, 401 (2001).

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Last modified Oct. 6, 2005 Tizby Hunt-Ward tizby@ku.edu