/* ======================================================================== *\ ! ! * ! * This file is part of MARS, the MAGIC Analysis and Reconstruction ! * Software. It is distributed to you in the hope that it can be a useful ! * and timesaving tool in analysing Data of imaging Cerenkov telescopes. ! * It is distributed WITHOUT ANY WARRANTY. ! * ! * Permission to use, copy, modify and distribute this software and its ! * documentation for any purpose is hereby granted without fee, ! * provided that the above copyright notice appear in all copies and ! * that both that copyright notice and this permission notice appear ! * in supporting documentation. It is provided "as is" without express ! * or implied warranty. ! * ! ! ! Author(s): Thomas Bretz 12/2000 ! ! Copyright: MAGIC Software Development, 2000-2003 ! ! \* ======================================================================== */ ///////////////////////////////////////////////////////////////////////////// // // MTime // // A generalized MARS time stamp. // // // We do not use floating point values here, because of several reasons: // - having the times stored in integers only is more accurate and // more reliable in comparison conditions // - storing only integers gives similar bit-pattern for similar times // which makes compression (eg gzip algorithm in TFile) more // successfull // // Note, that there are many conversion function converting the day time // into a readable string. Also a direct interface to SQL time strings // is available. // // If you are using MTime containers as axis lables in root histograms // use GetAxisTime(). Make sure that you use the correct TimeFormat // on your TAxis (see GetAxisTime()) // // // WARNING: Be carefull changing this class. It is also used in the // MAGIC drive software cosy! // // Remarke: If you encounter strange behaviour, check the casting. // Note, that on Linux machines ULong_t and UInt_t is the same. // // // Version 1: // ---------- // - first version // // Version 2: // ---------- // - removed fTimeStamp[2] // // Version 3: // ---------- // - removed fDurtaion - we may put it back when it is needed // - complete rewrite of the data members (old ones completely replaced) // ///////////////////////////////////////////////////////////////////////////// #include "MTime.h" #include #include // struct tm #include // struct timeval #include #include "MLog.h" #include "MAstro.h" ClassImp(MTime); using namespace std; const UInt_t MTime::kHour = 3600000; // [ms] one hour const UInt_t MTime::kDay = MTime::kHour*24; // [ms] one day // -------------------------------------------------------------------------- // // Constructor. Calls SetMjd(d) for d>0 in all other cases the time // is set to the current UTC time. // MTime::MTime(Double_t d) { Init(0, 0); if (d<=0) Now(); else SetMjd(d); } // -------------------------------------------------------------------------- // // Return date as year(y), month(m), day(d) // void MTime::GetDate(UShort_t &y, Byte_t &m, Byte_t &d) const { MAstro::Mjd2Ymd((Long_t)fTime<0?fMjd-1:fMjd, y, m, d); } // -------------------------------------------------------------------------- // // Return the time in the range [0h, 24h) = [0h0m0.000s - 23h59m59.999s] // void MTime::GetTime(Byte_t &h, Byte_t &m, Byte_t &s, UShort_t &ms) const { Long_t tm = GetTime24(); ms = tm%1000; // [ms] tm /= 1000; // [s] s = tm%60; // [s] tm /= 60; // [m] m = tm%60; // [m] tm /= 60; // [h] h = tm; // [h] } // -------------------------------------------------------------------------- // // Return time as MJD (=JD-24000000.5) // Double_t MTime::GetMjd() const { return fMjd+(Double_t)(fNanoSec/1e6+(Long_t)fTime)/kDay; } // -------------------------------------------------------------------------- // // Return a time which is expressed in milliseconds since 01/01/1995 0:00h // This is compatible with root's definition used in gSystem->Now() // and TTime. // Note, gSystem->Now() returns local time, such that it may differ // from GetRootTime() (if you previously called MTime::Now()) // TTime MTime::GetRootTime() const { return (ULong_t)((GetMjd()-49718)*kDay); } // -------------------------------------------------------------------------- // // Return a time which is expressed in seconds since 01/01/1995 0:00h // This is compatible with root's definition used in TAxis. // Note, a TAxis always displayes (automatically) given times in // local time (while here we return UTC) such, that you may encounter // strange offsets. You can get rid of this by calling: // TAxis::SetTimeFormat("[your-format] %F1995-01-01 00:00:00"); // Double_t MTime::GetAxisTime() const { return (GetMjd()-49718)*kDay/1000; } // -------------------------------------------------------------------------- // // Set a time expressed in MJD, Time of Day (eg. 23:12.779h expressed // in milliseconds) and a nanosecond part. // Bool_t MTime::Set(UInt_t mjd, ULong_t ms, UInt_t ns) { // [d] mjd (eg. 52320) // [ms] time (eg. 17h expressed in ms) // [ns] time (ns part of time) if (ms>kDay-1 || ns>999999) return kFALSE; const Bool_t am = ms23 || min>59 || s>59 || ms>999 || ns>999999) return kFALSE; const Int_t mjd = MAstro::Ymd2Mjd(y, m, d); if (mjd<0) return kFALSE; const ULong_t tm = ((((h*60+min)*60)+s)*1000)+ms; return Set(mjd, tm, ns); } // -------------------------------------------------------------------------- // // Set MTime to time expressed in a 'struct timeval' // void MTime::Set(const struct timeval &tv) { const UInt_t mjd = 1000*tv.tv_sec/kDay + 40587; const Long_t tm = tv.tv_sec%(24*3600)*1000 + tv.tv_usec/1000; const UInt_t ms = tv.tv_usec%1000; Set(mjd, tm, ms*1000); } // -------------------------------------------------------------------------- // // Return contents as a TString of the form: // "dd.mm.yyyy hh:mm:ss.fff" // Bool_t MTime::SetString(const char *str) { if (!str) return kFALSE; UInt_t y, mon, d, h, m, s, ms; const Int_t n = sscanf(str, "%02u.%02u.%04u %02u:%02u:%02u.%03u", &d, &mon, &y, &h, &m, &s, &ms); return n==7 ? Set(y, mon, d, h, m, s, ms) : kFALSE; } // -------------------------------------------------------------------------- // // Return contents as a TString of the form: // "yyyy-mm-dd hh:mm:ss" // Bool_t MTime::SetSqlDateTime(const char *str) { if (!str) return kFALSE; UInt_t y, mon, d, h, m, s; const Int_t n = sscanf(str, "%04u-%02u-%02u %02u:%02u:%02u", &y, &mon, &d, &h, &m, &s); return n==6 ? Set(y, mon, d, h, m, s) : kFALSE; } // -------------------------------------------------------------------------- // // Return contents as a TString of the form: // "yyyymmddhhmmss" // Bool_t MTime::SetSqlTimeStamp(const char *str) { if (!str) return kFALSE; UInt_t y, mon, d, h, m, s; const Int_t n = sscanf(str, "%04u%02u%02u%02u%02u%02u", &y, &mon, &d, &h, &m, &s); return n==6 ? Set(y, mon, d, h, m, s) : kFALSE; } // -------------------------------------------------------------------------- // // Set MTime to time expressed as in CT1 PreProc files // void MTime::SetCT1Time(UInt_t mjd, UInt_t t1, UInt_t t0) { // int isecs_since_midday; // seconds passed since midday before sunset (JD of run start) // int isecfrac_200ns; // fractional part of isecs_since_midday // fTime->SetTime(isecfrac_200ns, isecs_since_midday); fNanoSec = (200*t1)%1000000; const ULong_t ms = (200*t1)/1000000 + t0+12*kHour; fTime = (Long_t)(ms<13*kHour ? ms : ms-kDay); fMjd = mjd+1; } // -------------------------------------------------------------------------- // // Update the magic time. Make sure, that the MJD is set correctly. // It must be the MJD of the corresponding night. You can set it // by Set(2003, 12, 24); // // It is highly important, that the time correspoding to the night is // between 13:00:00.0 (day of dawning) and 12:59:59.999 (day of sunrise) // Bool_t MTime::UpdMagicTime(Byte_t h, Byte_t m, Byte_t s, UInt_t ns) { if (h>23 || m>59 || s>59 || ns>999999999) return kFALSE; const ULong_t tm = ((((h*60+m)*60)+s)*1000)+ns/1000000; fTime = (Long_t)(tm