SDO HMI 2014-03-02 23:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.79 | 111.85 | 12.34 | 60.75 | 16.35 | 102.06 | -4.70 | 11.03 | 0.4106 | -158.5 | -93.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.61 | 16.14 | 105.02 | -1.75 | 4.22 | 0.3997 | -779.0 | -655.2 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 15.92 | 104.90 | -1.87 | 4.56 | 0.3962 | -784.0 | -572.8 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 16.70 | 104.80 | -1.97 | 4.63 | 0.4088 | -736.0 | -600.3 | |
| 0.69 | 4.57 | 0.37 | 2.47 | 16.34 | 104.77 | -1.99 | 4.77 | 0.4032 | -1023.0 | -819.7 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 16.76 | 104.61 | -2.15 | 5.06 | 0.4101 | -822.0 | -736.8 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 16.73 | 104.39 | -2.37 | 5.57 | 0.4099 | -795.0 | -673.7 | |
| 0.00 | 2.85 | 0.00 | 1.55 | 17.09 | 103.99 | -2.78 | 6.42 | 0.4164 | -516.0 | -522.8 | |
| 0.00 | 1.38 | 0.00 | 0.74 | 15.38 | 103.67 | -3.10 | 7.71 | 0.3897 | -894.0 | -697.8 | |
| 0.00 | 1.55 | 0.00 | 0.83 | 14.77 | 103.62 | -3.15 | 8.07 | 0.3800 | -898.0 | -801.4 | |
| 3.28 | 5.09 | 1.77 | 2.75 | 15.80 | 103.57 | -3.20 | 7.81 | 0.3966 | -974.7 | -732.5 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 16.93 | 103.55 | -3.21 | 7.46 | 0.4147 | -840.0 | -709.4 | |
| 0.52 | 8.37 | 0.28 | 4.52 | 15.64 | 103.26 | -3.50 | 8.61 | 0.3948 | -999.3 | -748.6 | |
| 3.37 | -12.00 | 1.82 | -12.00 | 15.83 | 103.23 | -3.54 | 8.61 | 0.3979 | -954.9 | 999999 | |
| 0.00 | 3.62 | 0.00 | 1.97 | 17.00 | 103.08 | -3.68 | 8.51 | 0.4168 | -568.0 | -466.6 | |
| 14.07 | 42.38 | 7.63 | 22.97 | 16.42 | 102.94 | -3.82 | 9.06 | 0.4079 | -958.8 | -354.1 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 16.97 | 102.84 | -3.93 | 9.08 | 0.4169 | -573.0 | -436.4 | |
| 0.00 | 1.21 | 0.00 | 0.67 | 18.65 | 102.61 | -4.15 | 8.94 | 0.4436 | -710.0 | -552.1 | |
| 0.00 | 1.47 | 0.00 | 0.80 | 16.18 | 101.42 | -5.34 | 12.69 | 0.4087 | 900.0 | 781.3 | |
| 0.00 | 1.55 | 0.00 | 0.84 | 15.86 | 101.00 | -5.77 | 13.86 | 0.4053 | 865.0 | 752.9 | |
| 0.00 | 2.76 | 0.00 | 1.49 | 14.87 | 100.25 | -6.51 | 16.27 | 0.3931 | 913.0 | 727.9 | |
| 0.86 | 4.23 | 0.47 | 2.29 | 15.75 | 99.85 | -6.91 | 16.55 | 0.4084 | 942.2 | 784.6 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 15.52 | 99.86 | -6.91 | 16.70 | 0.4049 | 819.0 | 670.8 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 15.14 | 99.84 | -6.92 | 17.03 | 0.3990 | 815.0 | 643.8 | |
| 0.00 | 2.16 | 0.00 | 1.18 | 16.82 | 99.78 | -6.98 | 15.96 | 0.4250 | 725.0 | 636.6 | |
| 0.00 | 0.43 | 0.00 | 0.24 | 17.12 | 99.55 | -7.21 | 16.25 | 0.4305 | 684.0 | 587.2 | |
| 0.00 | 4.40 | 0.00 | 2.40 | 16.25 | 99.24 | -7.52 | 17.55 | 0.4187 | 710.0 | 420.7 | |
| 0.00 | 1.04 | 0.00 | 0.57 | 16.45 | 98.92 | -7.84 | 18.09 | 0.4233 | 596.0 | 536.8 | |
| 0.00 | 0.35 | 0.00 | 0.19 | 17.79 | 98.83 | -7.93 | 17.29 | 0.4438 | 407.0 | 453.0 | |
| 0.00 | 1.47 | 0.00 | 0.80 | 15.64 | 98.77 | -8.00 | 19.07 | 0.4120 | 722.0 | 645.1 | |
| 0.00 | 1.04 | 0.00 | 0.57 | 17.04 | 98.71 | -8.06 | 18.10 | 0.4332 | 822.0 | 696.8 | |
| 0.00 | 1.38 | 0.00 | 0.76 | 17.07 | 98.55 | -8.21 | 18.40 | 0.4345 | 719.0 | 491.7 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 16.23 | 98.18 | -8.59 | 19.85 | 0.4239 | 840.0 | 676.8 | |
| 0.00 | 1.55 | 0.00 | 0.85 | 16.96 | 97.83 | -8.93 | 19.98 | 0.4365 | 877.0 | 704.9 | |
| 0.00 | 1.21 | 0.00 | 0.66 | 16.80 | 97.75 | -9.02 | 20.29 | 0.4346 | 837.0 | 646.5 | |
| 0.00 | 2.59 | 0.00 | 1.43 | 17.10 | 97.20 | -9.57 | 21.15 | 0.4421 | 933.0 | 682.9 | |
| 0.00 | 2.33 | 0.00 | 1.30 | 17.81 | 96.40 | -10.37 | 22.12 | 0.4569 | 618.0 | 564.5 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |