Provided by: gmt_4.5.11-1build1_amd64 bug

NAME

       mgd77magref - Evaluate the IGRF or CM4 magnetic field models

SYNOPSIS

       mgd77magref  [ inputfile ] [ -A[+aalt+tdate+y] ] [ -Ccm4file ] [ -DDstfile ] [ -Ef107file ] [ -Fflags ] [
       -G ] [ -H[i][nrec] ] [ -Sc|llow/high ] [ -V ]  [  -:[i|o]  ]  [  -b[i|o][s|S|d|D[ncol]|c[var1/...]]  ]  [
       -f[i|o]colinfo ] [ -m[i|o][flag] ]

DESCRIPTION

       mgd77magref will evaluate the IGRF or the CM4 geomagnetic models at the specified locations and times.

OPTIONS

       No space between the option flag and the associated arguments.

       inputfile
              Contains  the  moments  in space-time where we want to evaluate the magnetic reference field.  The
              first two columns must contain longitude and latitude (however, see -: for latitude and  longitude
              instead).   Normally,  the  third  and  fourth  columns  must  contain  altitude (in km) and time,
              respectively, but if one or both of these are constant for all records they can  be  supplied  via
              the  -A  option  instead and are thus not expected in the input file. If no input file is given we
              read stdin.  A note about the CM4 validity domain. The core field of CM4 is valid from 1960-2002.5
              but the ionospheric and magnetospheric fields are computed after the  Dst  and  F10.7  coefficient
              files.  We  extended  here  those  coefficient  files up to 2007, which means that one can compute
              external contributions up until 2007 but the Secular Variation will be biased (non reliable).  New
              indices files may be retrieved from:ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/DST/ (the
              Dst  coefficients)  and  ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SOLAR_RADIO/FLUX/ (The F10.7 index
              file is a MONTHPLT.ABS).  NOTE: since the Dst files in the .../DST/ directory are still only up to
              2007, for GMT4.5.3 we extended  the  Dst  until  April  2010  by  reformatting  the  data  in  the
              preliminary          file          Est_Ist_index_0_mean.pli,          which          is         at
              ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/EST_IST/

       -A     Adjusts how the input record is interpreted.  Append +a to set  a  fixed  altitude  (in  km)  that
              should  apply  to  all  data  records  [Default  expects  altitude  to be in the 3rd column of all
              records].  Append +t to set a fixed time that should apply to all data  records  [Default  expects
              time  to  be in the 4th column of all records].  Finally, append +y to indicate that all times are
              specified as decimal years [Default is ISO dateTcolck format].

       -C     Specify an alternate CM4 coefficient file [umdl.CM4].

       -D     Specify  an  alternate  file  with  hourly  means  of  the  Dst  index  for   CM4   [Dst_all.wdc].
              Alternatively, simply specify a single index to apply for all records.

       -E     Specify  an  alternate  file  with  monthly  means  of  absolute  F10.7  solar  radio flux for CM4
              [F107_mon.plt].  Alternatively, simply specify a single flux to apply for all records.

       -F     Selects output items; flags is a string made up of one or more of these characters:
              r means output all input columns before adding the items below
              t means list total field (nT).
              h means list horizontal field (nT).
              x means list X component (nT, positive north).
              y means list Y component (nT, positive east).
              z means list Z component (nT, positive down).
              d means list declination (deg, clockwise from north).
              i means list inclination (deg, positive down).
              Append one or more number to indicate the requested field contribution(s):
              0 means IGRF field (no combinations allowed)
              1 means CM4 Core field
              2 means CM4 Lithospheric field
              3 means CM4 Primary Magnetospheric field
              4 means CM4 Induced Magnetospheric field
              5 means CM4 Primary ionospheric field
              6 means CM4 Induced ionospheric field
              7 means CM4 Toroidal field
              9 means Core field from IGRF and other contributions from CM4. DO NOT USE BOTH 1 AND 9.
              Appending several numbers (1-7) will add  up  the  different  contributions.  For  example  -Ft/12
              computes  the  total  field  due to Core and Lithospheric sources.  Two special cases are allowed,
              which mix which Core field from IGRF and other sources from CM4.  -Ft/934 computes Core field  due
              to  IGRF  plus  terms  3  and  4 from CM4 (but you can add others).  -Ft/934 the same as above but
              output the field components.  The data is written out in the order they appear in  flags  [Default
              is -Frthxyzdi/1].

       -G     Specifies that coordinates are geocentric [geodetic].

       -H     Input  file(s)  has  header  record(s).   If  used,  the  default  number  of  header  records  is
              N_HEADER_RECS.  Use -Hi if only input data should have header  records  [Default  will  write  out
              header  records  if  the  input  data have them]. Blank lines and lines starting with # are always
              skipped.

       -L     Computes J field vectors from certain external sources.
              r means output all input columns before adding the items below (all in Ampers/m).
              t means list magnitude field.
              x means list X component.
              y means list Y component.
              z means list Z or current function Psi.
              Append a number to indicate the requested J contribution:
              1 means Induced Magnetospheric field.
              2 means Primary ionospheric field.
              3 means Induced ionospheric field.
              4 means Poloidal field.

       -Sc    Limits the wavelengths of the core field contribution to the band indicated by the  low  and  high
              spherical harmonic order [1/13].

       -Sl    Limits  the wavelengths of the lithosphere field contribution to the band indicated by the low and
              high spherical harmonic order [14/65].

       -V     Selects verbose mode, which will send progress reports to stderr [Default runs "silently"].

       -:     Toggles between (longitude,latitude) and (latitude,longitude) input and/or  output.   [Default  is
              (longitude,latitude)].   Append  i  to  select  input  only  or o to select output only.  [Default
              affects both].

       -bi    Selects binary input.  Append s for single precision [Default is d (double)].  Uppercase  S  or  D
              will  force  byte-swapping.   Optionally,  append ncol, the number of columns in your binary input
              file if it exceeds the columns needed by the program.  Or append c if the input  file  is  netCDF.
              Optionally, append var1/var2/... to specify the variables to be read.  [Default is 4 input columns
              unless -A is used].

       -bo    Selects  binary  output.  Append s for single precision [Default is d (double)].  Uppercase S or D
              will force byte-swapping.  Optionally, append ncol, the number of desired columns in  your  binary
              output file.  [Default is reflected by -F].

       -m     Multiple  segment file(s).  Segments are separated by a special record.  For ASCII files the first
              character must be flag [Default is '>'].  For binary files all fields must be NaN and -b must  set
              the  number  of  output  columns  explicitly.  By default the -m setting applies to both input and
              output.  Use -mi and -mo to give separate settings to input and output.

TIME SETTINGS

       If binary input files are used then absolute time are stored as time  relative  to  the  selected  epoch.
       However,  since the epoch used is not stored in the data files there can be problems decoding the correct
       time.  The mgd77 supplement uses the Unix time system as its default; thus  you  should  make  sure  that
       binary data files with time uses the same system (see the GMT default TIME_SYSTEM).

EXAMPLES

       To get the CM4 Total field, Declination and Inclination due to all but lithospheric and toroidal field at
       a one point location and decimal time 2000.0, try

       echo -28 38 0 2000.0 | mgd77magref -A+y -F tdi/13456

       To do the same as above but at noon (Universal Time) of first May 2001, try

       echo -28 38 0 2001-05-01T12:00:00 | mgd77magref -F tdi/13456

SEE ALSO

       GMT(1) mgd77info(1) mgd77list(1) mgd77manage(1) mgd77track(1)

REFERENCES

       Wessel,  P., and W. H. F. Smith, 2013, The Generic Mapping Tools (GMT) version 4.5.11 Technical Reference
       & Cookbook, SOEST/NOAA.
       Wessel, P., and W. H. F. Smith, 1998, New, Improved  Version  of  Generic  Mapping  Tools  Released,  EOS
       Trans., AGU, 79 (47), p. 579.
       Wessel, P., and W. H. F. Smith, 1995, New Version of the Generic Mapping Tools Released, EOS Trans., AGU,
       76 (33), p. 329.
       Wessel,   P.,   and  W.  H.  F.  Smith,  1995,  New  Version  of  the  Generic  Mapping  Tools  Released,
       http://www.agu.org/eos_elec/95154e.html, Copyright 1995 by the American Geophysical Union.
       Wessel, P., and W. H. F. Smith, 1991, Free Software Helps Map and Display Data, EOS Trans., AGU, 72 (41),
       p. 441.
       "Comprehensive Modeling of the Geomagnetic Field", see http://denali.gsfc.nasa.gov/cm/.
       "The        International        Geomagnetic         Reference         Field         (IGRF)",         see
       http://www.iugg.org/IAGA/iaga_pages/pubs_prods/igrf.htm.

GMT 4.5.11                                         5 Nov 2013                                  MGD77MAGREF(1gmt)