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    | Titel | 
    A comparative study of night-time enhancement of TEC at a low latitude station on storm and quiet nights including the local time, seasonal and solar activity dependence | 
   
  
    | VerfasserIn | 
    K. Unnikrishnan, R. Balachandran Nair, C. Venugopal | 
   
  
    | Medientyp | 
    Artikel
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    | Sprache | 
    Englisch
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    | ISSN | 
    0992-7689
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    | Digitales Dokument | 
    URL | 
   
  
    | Erschienen | 
    In: Annales Geophysicae ; 20, no. 11 ; Nr. 20, no. 11, S.1843-1850 | 
   
  
    | Datensatznummer | 
    250014498
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    | Publikation (Nr.) | 
     copernicus.org/angeo-20-1843-2002.pdf | 
   
  
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        | Zusammenfassung | 
       
      
        The main characteristics
 of night-time enhancements in TEC during magnetic storms are compared with
 those during quiet nights for different seasons and solar activity conditions
 at Palehua, a low latitude station during the period 1980–1989. We find that
 the mean amplitude has both a seasonal and solar activity dependence: in
 winter, the values are higher for weak storms as compared to those during quiet
 nights and increase with an increase in solar activity. In summer, the mean
 amplitude values during weak storms and quiet nights are almost equal. But
 during equinox, the mean amplitude values for quiet nights are greater than
 those during weak storms. The mean half-amplitude duration is higher during
 weak storms as compared to that during quiet nights in summer. However, during
 winter and equinox, the durations are almost equal for both quiet and weak
 storm nights. For the mean half-amplitude duration, the quiet night values for
 all the seasons and equinoctial weak storm values increase with an increase in
 solar activity. The occurrence frequency (in percent) of TEC enhancement during
 weak storms is greater than during quiet nights for all seasons. The mean
 amplitude, the mean half-amplitude duration and the occurrence frequency (in
 percent) of TEC enhancement values are higher during major storms as compared
 to those during quiet nights. The above parameters have their highest values
 during pre-midnight hours. From the data analysed, this behaviour is true in
 the case of major storms also.
  Key words. Ionosphere (ionospheric disturbances;
 plasma convection) Magnetospheric physics (storms and substorms) | 
       
    
  
  
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