SDO HMI 2014-03-11 17:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.31 | 163.72 | 28.87 | 88.99 | 6.04 | 11.83 | 20.33 | 302.86 | 0.4128 | 156.6 | -140.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.91 | 0.00 | 1.06 | 5.27 | 15.48 | 23.99 | 296.89 | 0.4558 | -743.0 | -603.8 | |
| 0.00 | 1.47 | 0.00 | 0.82 | 5.38 | 15.26 | 23.76 | 297.34 | 0.4535 | -326.0 | -387.9 | |
| 4.59 | 6.15 | 2.55 | 3.41 | 5.19 | 15.12 | 23.63 | 297.11 | 0.4503 | -1102.0 | -784.2 | |
| 0.00 | 1.56 | 0.00 | 0.86 | 5.45 | 14.97 | 23.47 | 297.79 | 0.4501 | -1002.0 | -829.7 | |
| 0.00 | 1.47 | 0.00 | 0.81 | 5.40 | 14.51 | 23.02 | 298.17 | 0.4434 | -861.0 | -680.9 | |
| 3.73 | 26.00 | 2.06 | 14.34 | 5.85 | 14.43 | 22.94 | 299.15 | 0.4458 | -844.9 | -777.8 | |
| 1.47 | 7.89 | 0.80 | 4.31 | 4.74 | 13.42 | 21.92 | 298.03 | 0.4233 | -1079.1 | -758.6 | |
| 0.35 | 3.73 | 0.19 | 2.05 | 6.17 | 13.41 | 21.92 | 300.95 | 0.4345 | -918.5 | -703.2 | |
| 0.00 | 1.82 | 0.00 | 0.99 | 5.01 | 13.36 | 21.87 | 298.65 | 0.4246 | -912.0 | -694.0 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 4.15 | 13.17 | 21.68 | 297.06 | 0.4155 | -875.0 | -662.6 | |
| 0.00 | 1.30 | 0.00 | 0.71 | 5.89 | 13.20 | 21.71 | 300.63 | 0.4294 | -774.0 | -590.0 | |
| 0.00 | 1.56 | 0.00 | 0.85 | 5.27 | 13.15 | 21.65 | 299.45 | 0.4237 | -679.0 | -570.1 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 6.37 | 12.97 | 21.47 | 301.87 | 0.4302 | -852.0 | -672.1 | |
| 0.00 | 1.04 | 0.00 | 0.57 | 5.28 | 12.57 | 21.07 | 300.15 | 0.4158 | 382.0 | 328.6 | |
| 0.61 | 2.17 | 0.33 | 1.18 | 5.61 | 12.45 | 20.96 | 300.98 | 0.4170 | 539.4 | 443.6 | |
| 10.31 | 20.63 | 5.64 | 11.28 | 6.71 | 12.40 | 20.91 | 303.25 | 0.4256 | -1045.9 | -712.9 | |
| 0.00 | 3.81 | 0.00 | 2.08 | 6.21 | 12.32 | 20.82 | 302.38 | 0.4202 | -1059.0 | -823.2 | |
| 0.00 | 0.43 | 0.00 | 0.24 | 5.17 | 12.28 | 20.78 | 300.29 | 0.4110 | 298.0 | 296.6 | |
| 0.00 | 0.87 | 0.00 | 0.47 | 4.20 | 12.21 | 20.72 | 298.28 | 0.4023 | 532.0 | 314.9 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 5.13 | 11.99 | 20.49 | 300.56 | 0.4067 | 552.0 | 461.7 | |
| 0.52 | 1.99 | 0.28 | 1.08 | 5.43 | 11.97 | 20.47 | 301.23 | 0.4089 | 767.5 | 595.5 | |
| 0.00 | 2.43 | 0.00 | 1.31 | 4.15 | 11.80 | 20.30 | 298.68 | 0.3961 | 743.0 | 664.4 | |
| 0.00 | 1.73 | 0.00 | 0.95 | 7.02 | 11.78 | 20.28 | 304.69 | 0.4202 | -528.0 | -483.9 | |
| 0.00 | 1.13 | 0.00 | 0.61 | 6.14 | 11.23 | 19.73 | 303.66 | 0.4051 | 641.0 | 483.8 | |
| 0.00 | 1.65 | 0.00 | 0.89 | 5.45 | 10.98 | 19.49 | 302.57 | 0.3957 | 893.0 | 725.4 | |
| 0.00 | 2.34 | 0.00 | 1.26 | 5.41 | 10.79 | 19.29 | 302.76 | 0.3928 | 1001.0 | 815.3 | |
| 0.00 | 1.82 | 0.00 | 0.98 | 6.63 | 10.64 | 19.15 | 305.50 | 0.4020 | 648.0 | 423.4 | |
| 0.00 | 1.65 | 0.00 | 0.88 | 5.37 | 10.47 | 18.98 | 303.11 | 0.3882 | 1025.0 | 778.2 | |
| 0.00 | 1.39 | 0.00 | 0.75 | 6.71 | 10.43 | 18.93 | 305.99 | 0.3999 | 593.0 | 479.5 | |
| 3.73 | 21.67 | 2.01 | 11.66 | 6.55 | 10.07 | 18.58 | 306.17 | 0.3937 | 898.6 | 598.0 | |
| 2.34 | -30.00 | 1.26 | -30.00 | 6.27 | 9.96 | 18.47 | 305.75 | 0.3897 | 991.0 | 999999 | |
| 0.00 | 1.39 | 0.00 | 0.75 | 7.00 | 9.90 | 18.41 | 307.35 | 0.3959 | 664.0 | 427.1 | |
| 3.21 | -30.00 | 1.73 | -30.00 | 6.66 | 9.85 | 18.36 | 306.73 | 0.3921 | 877.8 | 999999 | |
| 1.56 | 34.15 | 0.84 | 18.29 | 6.37 | 9.53 | 18.03 | 306.64 | 0.3851 | 975.4 | 740.6 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 5.88 | 9.51 | 18.01 | 305.63 | 0.3801 | 1027.0 | 837.1 | |
| 20.89 | -34.00 | 11.18 | -34.00 | 6.36 | 9.18 | 17.69 | 307.15 | 0.3805 | 1091.1 | 999999 | |
| 0.00 | 1.47 | 0.00 | 0.79 | 6.07 | 8.73 | 17.24 | 307.26 | 0.3718 | 979.0 | 754.1 | |
| 0.00 | 1.30 | 0.00 | 0.69 | 7.73 | 7.17 | 15.67 | 313.42 | 0.3701 | 812.0 | 669.1 | |
| 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. | |