Statistical Correlation of the Rate of Failures on Geosynchronous Satellites with Fluxes of Energetic Electrons and Protons

A statistical comparison of failures on geosynchronous satellites in the maximum and during the decline of the 22nd solar cycle (1989–1994) with space weather parameters is carried out. A positive correlation of the rate of failures with the flux of relativistic electrons on the geosynchronous orbit and with the proton flux measured before the bow shock front is revealed. The significant positive correlation of the electron flux with the rate of failures is observed during the entire considered interval. The correlation coefficient varies in the solar activity cycle in coordination with the electron flux, and the maxima of the correlation coefficient are observed on the phase of decline of the cycle. A statistically significant positive correlation between the flux of protons with energy of more than 1 MeV and the rate of failures is revealed in the maximum of the solar cycle.

[1]  D. C. Wilkinson,et al.  Penetrating electron fluctuations associated with GEO spacecraft anomalies , 2000 .

[2]  R. Thorne,et al.  Relativistic theory of wave‐particle resonant diffusion with application to electron acceleration in the magnetosphere , 1998 .

[3]  Daniel C. Wilkinson National Oceanic and Atmospheric Administration's spacecraft anomaly data base and examples of solar activity affecting spacecraft , 1994 .

[4]  J. G. Laframboise,et al.  High‐voltage differential charging of geostationary spacecraft , 1980 .

[5]  R. Hynds,et al.  Penetration of low-energy solar protons to low geomagnetic latitudes , 1970 .

[6]  D. Brautigam,et al.  CRRES in review: space weather and its effects on technology , 2002 .

[7]  D. Baker The occurrence of operational anomalies in spacecraft and their relationship to space weather , 2000 .

[8]  J. B. Blake,et al.  Highly relativistic electrons in the Earth';s outer magnetosphere: 1. Lifetimes and temporal history 1979–1984 , 1986 .

[9]  Harlan E. Spence,et al.  Coronal mass ejections, magnetic clouds, and relativistic magnetospheric electron events: ISTP , 1998 .

[10]  H. Garrett,et al.  Spacecraft charging, an update , 2000 .

[11]  Gordon L. Wrenn,et al.  Modeling the Outer Belt Enhancements of Penetrating Electrons , 2000 .

[12]  K. R. Lorentzen,et al.  Multisatellite observations of MeV ion injections during storms , 2002 .

[13]  Didier Sornette,et al.  Which magnetic storms produce relativistic electrons at geosynchronous orbit , 2001 .

[14]  Keith Ryden,et al.  A solar cycle of spacecraft anomalies due to internal charging , 2002 .

[15]  D. Baker,et al.  Are energetic electrons in the solar wind the source of the outer radiation belt? , 1997 .

[16]  Scot R. Elkington,et al.  Acceleration of relativistic electrons via drift‐resonant interaction with toroidal‐mode Pc‐5 ULF oscillations , 1999 .