Variabilities of the equatorial electrojet in Brazil and Perú

DOI Web Site Web Site 被引用文献5件
  • E. B. Shume
    Aeronomy Division National Institute for Space Research São Paulo Brazil
  • C. M. Denardini
    Aeronomy Division National Institute for Space Research São Paulo Brazil
  • E. R. de Paula
    Aeronomy Division National Institute for Space Research São Paulo Brazil
  • N. B. Trivedi
    Space Geophysics Division National Institute for Space Research São Paulo Brazil

書誌事項

公開日
2010-06
権利情報
  • http://onlinelibrary.wiley.com/termsAndConditions#vor
DOI
  • 10.1029/2009ja014984
公開者
American Geophysical Union (AGU)

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説明

<jats:p>This report presents seasonal and longitudinal variabilities of the equatorial electrojet in the east (Brazil, São Luís: 2.3° S; 315.8° E; 0.5° S dip latitude) and west (Jicamarca, Perú: 11.95° S; 283.13° E; 0.6° N dip latitude) coasts of the continent of South America. Ground‐based magnetic field perturbation measurements Δ<jats:italic>H</jats:italic> for solar maximum (2001/2002) and solar minimum (2006/2007) conditions from the two equatorial stations (São Luís and Jicamarca) have been used for the study. The Δ<jats:italic>H</jats:italic> signal which is a measure of the strength of the equatorial electrojet is spectrally analyzed using wavelet analysis. The results of our analysis show that (1) the equatorial electrojet has maxima around equinoxes in Jicamarca, Perú but it has a prominent maximum during Southern Hemisphere summer (centered about December/January) in São Luís, Brazil. The observed seasonal behavior of the equatorial electrojet in São Luís is highly likely due to the large magnetic declination angle (about 20° west) there. (2) The equatorial electrojet is stronger in the west coast (Jicamarca) compared to the east coast (São Luís), irrespective of solar activity condition. (3) The magnitude of the equatorial electrojet is more variable with season and solar cycle over São Luís than over Jicamarca.</jats:p>

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