SDO HMI 2013-02-20 20:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 176.73 | 776.58 | 153.15 | 678.65 | 10.08 | 70.09 | 52.93 | 287.50 | 0.8243 | -42.0 | -4.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.58 | 392.71 | 2.49 | 370.65 | 10.24 | 73.91 | 56.75 | 286.42 | 0.8601 | 141.6 | -224.9 | |
| 77.89 | -1.00 | 73.53 | -1.00 | 10.01 | 73.19 | 56.03 | 286.38 | 0.8534 | -908.6 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.91 | 9.76 | 70.46 | 53.30 | 286.93 | 0.8281 | 218.0 | 163.4 | |
| 0.00 | 1.37 | 0.00 | 1.22 | 10.72 | 70.54 | 53.38 | 288.02 | 0.8315 | -512.0 | -399.8 | |
| 0.00 | 0.86 | 0.00 | 0.75 | 9.83 | 70.22 | 53.06 | 287.09 | 0.8261 | 251.0 | 177.6 | |
| 0.00 | 1.03 | 0.00 | 0.90 | 10.60 | 69.91 | 52.75 | 288.09 | 0.8253 | -440.0 | -376.5 | |
| 0.00 | 1.12 | 0.00 | 0.96 | 10.01 | 69.61 | 52.45 | 287.50 | 0.8209 | -410.0 | -407.0 | |
| 0.00 | 1.12 | 0.00 | 0.96 | 9.82 | 69.52 | 52.36 | 287.31 | 0.8195 | -391.0 | -363.6 | |
| 5.93 | 8.33 | 5.06 | 7.12 | 9.53 | 69.36 | 52.20 | 287.01 | 0.8171 | 414.8 | 150.3 | |
| 0.00 | 1.20 | 0.00 | 1.03 | 9.98 | 69.31 | 52.15 | 287.57 | 0.8179 | -307.0 | -259.6 | |
| 0.00 | 4.55 | 0.00 | 3.93 | 10.94 | 69.35 | 52.19 | 288.68 | 0.8210 | -643.0 | -519.6 | |
| 0.00 | 2.83 | 0.00 | 2.42 | 10.33 | 69.10 | 51.94 | 288.05 | 0.8169 | -268.0 | -177.5 | |
| 0.00 | 3.61 | 0.00 | 3.05 | 9.57 | 68.87 | 51.71 | 287.23 | 0.8126 | -677.0 | -583.0 | |
| 0.00 | 0.69 | 0.00 | 0.58 | 10.16 | 68.91 | 51.75 | 287.91 | 0.8146 | 89.0 | 110.5 | |
| 0.00 | 0.94 | 0.00 | 0.79 | 9.38 | 68.21 | 51.04 | 287.23 | 0.8055 | -375.0 | -307.6 | |
| 0.00 | 3.95 | 0.00 | 3.34 | 10.86 | 68.54 | 51.38 | 288.87 | 0.8131 | -389.0 | -312.3 | |
| 1.46 | 333.63 | 1.21 | 265.86 | 10.01 | 68.05 | 50.89 | 288.03 | 0.8059 | 220.5 | 333.9 | |
| 0.94 | -17.00 | 0.78 | -17.00 | 10.03 | 67.63 | 50.47 | 288.21 | 0.8018 | 351.4 | 999999 | |
| 16.57 | -17.00 | 13.51 | -17.00 | 10.05 | 67.11 | 49.95 | 288.41 | 0.7967 | 527.3 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.57 | 11.88 | 67.50 | 50.33 | 290.45 | 0.8062 | 306.0 | 289.5 | |
| 0.94 | -17.00 | 0.77 | -17.00 | 9.82 | 67.02 | 49.85 | 288.17 | 0.7950 | -246.8 | 999999 | |
| 0.00 | 1.37 | 0.00 | 1.15 | 12.06 | 67.50 | 50.34 | 290.67 | 0.8068 | 434.0 | 321.2 | |
| 1.29 | 3.18 | 1.06 | 2.62 | 11.47 | 67.11 | 49.95 | 290.11 | 0.8011 | 414.3 | 309.6 | |
| 4.64 | -17.00 | 3.72 | -17.00 | 9.58 | 66.45 | 49.29 | 288.09 | 0.7886 | 662.9 | 999999 | |
| 0.00 | 1.72 | 0.00 | 1.40 | 11.22 | 66.76 | 49.60 | 289.94 | 0.7970 | 479.0 | 408.5 | |
| 12.80 | -17.00 | 10.17 | -17.00 | 9.46 | 66.11 | 48.95 | 288.06 | 0.7847 | 861.7 | 999999 | |
| 0.00 | 1.29 | 0.00 | 1.02 | 8.58 | 65.94 | 48.78 | 287.05 | 0.7803 | 587.0 | 501.9 | |
| 1.46 | -17.00 | 1.15 | -17.00 | 8.95 | 65.96 | 48.80 | 287.49 | 0.7816 | 644.4 | 999999 | |
| 0.00 | 1.37 | 0.00 | 1.11 | 11.18 | 66.38 | 49.22 | 290.05 | 0.7931 | 511.0 | 436.4 | |
| 0.00 | 1.72 | 0.00 | 1.39 | 11.35 | 66.24 | 49.08 | 290.31 | 0.7922 | 339.0 | 258.6 | |
| 0.00 | 0.69 | 0.00 | 0.56 | 11.57 | 66.19 | 49.03 | 290.58 | 0.7925 | 240.0 | 168.6 | |
| 0.00 | 2.23 | 0.00 | 1.75 | 9.18 | 65.46 | 48.30 | 287.96 | 0.7771 | 713.0 | 615.3 | |
| 0.77 | -17.00 | 0.62 | -17.00 | 11.28 | 65.76 | 48.60 | 290.41 | 0.7871 | 434.0 | 999999 | |
| 45.08 | -17.00 | 35.61 | -17.00 | 10.38 | 65.47 | 48.31 | 289.43 | 0.7812 | 963.1 | 999999 | |
| 0.00 | 3.35 | 0.00 | 2.61 | 9.18 | 65.14 | 47.98 | 288.08 | 0.7738 | 655.0 | 628.8 | |
| 4.38 | -17.00 | 3.47 | -17.00 | 11.11 | 65.35 | 48.19 | 290.37 | 0.7825 | 618.4 | 999999 | |
| 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. | |