/** @file
 * $Source: /home/cvsmanager/yodaUtility/RegistryEvent.h,v $
 * $Id: RegistryEvent.h,v 1.1 2006/06/10 07:14:29 kusanagi Exp $
 * $Author: kusanagi $
 * 
 * Header file for the RegistryEvent class.
 */
#ifndef REGISTRY_EVENT_H
#define REGISTRY_EVENT_H

#include "TObject.h"
#include "TString.h"
#include "sgp4/coord.h"
#include "YMagnGeo.h"
namespace pamela {

  /**
   * RegistryEvent data Wrapper
   */
  class RegistryEvent: public TObject {
  private:
    
  public:
    /* This is the absolute Time of the event calculated after data unpacking */
    /* representing the number of millisecond after 1 January 1970 */
    ULong64_t   absTime;

    /* Name of the unpacked file this data cames from.
     * The reason for this is beacuse if multiple data are collected from several
     * files using the same xxx.Event.root & xxx.Registry.root structure, in this way you 
     * can reconstruct from which file this data cames from.
    */
    TString   originFile;
    
    /* Unique ID of the RUN from which this data cames from.
     * Even if this ID cames from the production database it can be considered decoupled
     * from the database. It is used when many RUNs are collected in a single file.
    */
    UInt_t   IDRun;
    
    /* Because on transmission multiple copies of data could be unpacked, a special procedure 
     * collect all the event just one time each. This parameter is related to the entry relative
     * to that selected event.
    */
    unsigned int        event;

    /* 
     * Position of the satellite
     *    double m_Lat;   // Latitude,  degree (negative south)
     *    double m_Lon;   // Longitude, degree (negative west)
     *    double m_Alt;   // Altitude,  km     (above mean sea level)
     */
     float m_Lat;
     float m_Lon;
     float m_Alt;
    //cCoordGeo	coordGeo;

    /* 
     * Magnetic parameters according to the position
     */
    YMagnGeo	magnGeo;

    RegistryEvent();
    ~RegistryEvent(void){};
    ClassDef(RegistryEvent, 1)
  };
}
#endif /* REGISTRY_EVENT_H */