BROKEN-RING ECLIPSES

The table shows when the Moon don't cover totally the solar disk during an eplipse. This happens when the vertex of the lunar shadow cone passes close to the surface of the Earth, but without touching it.

 
             TD of
Calendar    Greatest    DT    Luna   Saros Ecl.           Ecl.   Sun Sun Path Central
  Date      Eclipse     s     Num    Num  Type  Gamma     Mag.   Alt Azm Width Dur.
                                                                  ░   ░     ░   km
0562 Ott 14  03:07:26   5071 -17776   91   A   -0.0010  0.9992    90   8    3  00m05s
0654 Mag 22  00:02:55   4207 -16643  106   P   -1.0131  0.9990     0 345
1048 Sep 10  22:09:40   1310 -11766  119   A    0.8530  0.9995    31 214    4  00m02s
1087 Aug 01  08:58:39   1132 -11285  111   A    0.1644  0.9996    80 192    1  00m02s
1384 Aug 17  13:09:06    340  -7611  125   A    0.5354  0.9999    57 200    1  00m01s
1581 Dec 25  20:35:20    128  -5170  115   A   -0.4567  0.9993    63 343    3  00m04s
1594 Nov 12  07:34:49    121  -5011  136   A   -0.7829  0.9991    38  48    5  00m04s
1704 Nov 27  05:33:52      9  -3650  118   A    0.6716  0.9999    48 196    1  00m01s
1822 Feb 21  19:40:40     11  -2200  137   A    0.6914  0.9996    46 150    2  00m02s
1840 Mar 04  03:58:22      5  -1977  137   A    0.6728  0.9995    48 147    2  00m03s
1858 Mar 15  12:05:28      7  -1754  137   A    0.6461  0.9996    50 145    2  00m02s
1876 Mar 25  20:05:06     -4  -1531  137   A    0.6142  0.9999    52 144    1  00m01s
1927 Jan 03  20:22:53     24   -903  140   A   -0.4956  0.9995    60   0    2  00m03s
1948 May 09  02:26:04     28   -639  137   A    0.4133  0.9999    65 153    0  00m00s
1966 May 20  09:39:02     37   -416  137   A    0.3467  0.9991    70 158    3  00m05s
2146 Mar 12  15:58:15    318   1808  132   A    0.4821  0.9995    61 161    2  00m03s
2191 Apr 23  17:26:06    420   2366  151   A    0.7991  0.9993    37 130    4  00m03s
2862 Sep 15  06:23:08   3449  10670  158   A    0.5956  0.9999    53 215    0  00m01s
2931 Dec 30  06:28:24   3925  11527  166   A    0.1511  1.0000    81 182    0  00m00s

 Calendar     Calendar Date at instant of Greatest Eclipse.
   Date       Gregorian Calendar is used for dates after 1582 Oct 15.
              Julian Calendar is used for dates before 1582 Oct 04.

    TD of     Dynamical Time (TD) of Greatest Eclipse, the instant
  Greatest    when the axis of the Moon's shadow cone passes closest
  Eclipse     to Earth's center.

    DT        Delta T (?T) is the arithmetic difference between
              Dynamical Time and Universal Time. It is a measure of
              the accumulated clock error due to the variable
              rotation period of Earth.

   Luna       Lunation Number is the number of synodic months since
    Num       New Moon of 2000 Jan 06. The Brown Lunation Number
              can be determined by adding 953.

   Saros      Saros series number of eclipse.
    Num       (Each eclipse in a Saros is separated by an interval
               of 18 years 11.3 days.)

   Ecl.       Eclipse Type where:
   Type         P  = Partial Eclipse.
                A  = Annular Eclipse.
                T  = Total Eclipse.
                H  = Hybrid or Annular/Total Eclipse.

              Second character in Eclipse Type:
                "m" = Middle eclipse of Saros series.
                "n" = Central eclipse with no northern limit.
                "s" = Central eclipse with no southern limit.
                "+" = Non-central eclipse with no northern limit.
                "-" = Non-central eclipse with no southern limit.
                "2" = Hybrid path begins total and ends annular.
                "3" = Hybrid path begins annular and ends total.
                "b" = Saros series begins (first eclipse in series).
                "e" = Saros series ends (last eclipse in series).

   Gamma      Distance of the shadow cone axis from the center
              of Earth (units of equatorial radii) at the
              instant of greatest eclipse.

   Ecl.       Eclipse magnitude is the fraction of the Sun's
   Mag.       diameter obscured by the Moon. For annular, total and
              hybrid eclipses, this value is actually the diameter
              ratio of Moon/Sun.


   Lat.       Latitude where greatest eclipse is seen.

   Long.      Longitude where greatest eclipse is seen.

   Sun        Sun's altitude at greatest eclipse.
   Alt

   Sun        Sun's azimuth at greatest eclipse.
   Azm

   Path       Width of the path of totality or annularity
  Width       at greatest eclipse (kilometers).

 Central      Central Line Duration of total or annular phase
   Dur.       at greatest eclipse.