SDO HMI 2014-03-21 18:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.99 | 351.50 | 53.58 | 269.50 | -13.58 | 168.95 | -50.17 | 101.93 | 0.7648 | 561.3 | 252.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.60 | 204.73 | 24.21 | 152.46 | -14.40 | 170.60 | -48.53 | 103.09 | 0.7474 | 1049.2 | 309.7 | |
| 0.70 | -1.00 | 0.52 | -1.00 | -14.70 | 170.23 | -48.90 | 103.46 | 0.7518 | 268.9 | 999999 | |
| 9.06 | -1.00 | 6.82 | -1.00 | -14.25 | 169.89 | -49.23 | 102.83 | 0.7552 | 571.6 | 999999 | |
| 0.00 | 0.78 | 0.00 | 0.58 | -11.93 | 170.43 | -48.70 | 99.76 | 0.7482 | 644.0 | 545.7 | |
| 1.66 | -1.00 | 1.26 | -1.00 | -14.57 | 169.41 | -49.71 | 103.22 | 0.7607 | 286.4 | 999999 | |
| 0.00 | 0.78 | 0.00 | 0.59 | -11.72 | 170.20 | -48.93 | 99.48 | 0.7508 | 715.0 | 666.9 | |
| 0.00 | 1.05 | 0.00 | 0.78 | -12.13 | 170.05 | -49.08 | 100.03 | 0.7525 | 458.0 | 414.7 | |
| 0.00 | 1.39 | 0.00 | 1.04 | -11.47 | 170.12 | -49.01 | 99.15 | 0.7516 | 651.0 | 424.5 | |
| 0.00 | 0.61 | 0.00 | 0.47 | -15.52 | 168.86 | -50.27 | 104.43 | 0.7674 | 524.0 | 396.9 | |
| 0.00 | 1.31 | 0.00 | 0.98 | -11.49 | 169.97 | -49.16 | 99.17 | 0.7533 | 625.0 | 560.3 | |
| 0.00 | 0.61 | 0.00 | 0.46 | -11.96 | 169.81 | -49.32 | 99.79 | 0.7552 | 423.0 | 340.7 | |
| 0.44 | 2.61 | 0.33 | 2.01 | -14.46 | 168.96 | -50.16 | 103.05 | 0.7656 | 381.8 | 257.3 | |
| 0.00 | 0.96 | 0.00 | 0.75 | -15.37 | 168.18 | -50.95 | 104.17 | 0.7746 | 546.0 | 401.4 | |
| 17.17 | 96.31 | 13.37 | 75.12 | -12.41 | 168.11 | -51.02 | 100.33 | 0.7740 | 975.3 | 295.9 | |
| 0.00 | 1.13 | 0.00 | 0.89 | -13.50 | 167.75 | -51.38 | 101.73 | 0.7782 | -226.0 | -189.8 | |
| 0.00 | 0.96 | 0.00 | 0.76 | -14.11 | 167.41 | -51.72 | 102.49 | 0.7821 | -759.0 | -586.9 | |
| 0.00 | 0.96 | 0.00 | 0.76 | -14.16 | 167.04 | -52.09 | 102.55 | 0.7860 | -622.0 | -537.3 | |
| 0.61 | 2.09 | 0.49 | 1.66 | -13.68 | 167.09 | -52.04 | 101.93 | 0.7852 | 310.7 | 333.0 | |
| 0.00 | 0.44 | 0.00 | 0.35 | -12.14 | 167.20 | -51.93 | 99.97 | 0.7837 | -44.0 | -89.6 | |
| 0.00 | 2.44 | 0.00 | 1.96 | -13.18 | 166.59 | -52.54 | 101.28 | 0.7903 | -698.0 | -573.4 | |
| 0.00 | 2.44 | 0.00 | 1.97 | -12.74 | 166.52 | -52.61 | 100.73 | 0.7910 | 491.0 | 289.5 | |
| 0.00 | 0.70 | 0.00 | 0.57 | -13.32 | 165.57 | -53.56 | 101.43 | 0.8009 | -556.0 | -504.6 | |
| 2.70 | 6.19 | 2.25 | 5.14 | -13.62 | 165.16 | -53.97 | 101.79 | 0.8051 | -772.2 | -655.0 | |
| 0.00 | 2.35 | 0.00 | 1.97 | -13.70 | 164.81 | -54.32 | 101.89 | 0.8086 | -303.0 | -396.6 | |
| 0.00 | 1.39 | 0.00 | 1.17 | -9.90 | 164.72 | -54.41 | 97.17 | 0.8096 | 500.0 | 501.1 | |
| 0.00 | 1.92 | 0.00 | 1.64 | -12.48 | 163.83 | -55.30 | 100.36 | 0.8182 | -427.0 | -334.9 | |
| 0.00 | 1.39 | 0.00 | 1.18 | -9.88 | 164.47 | -54.66 | 97.15 | 0.8122 | 504.0 | 474.2 | |
| 0.96 | 4.53 | 0.82 | 3.89 | -11.42 | 163.89 | -55.24 | 99.07 | 0.8177 | -710.1 | -552.0 | |
| 1.13 | -28.00 | 0.98 | -28.00 | -11.49 | 163.65 | -55.48 | 99.15 | 0.8200 | -479.1 | 999999 | |
| 2.96 | 6.28 | 2.53 | 5.35 | -10.04 | 164.00 | -55.13 | 97.37 | 0.8168 | 463.4 | 442.9 | |
| 0.00 | 1.05 | 0.00 | 0.90 | -8.00 | 163.78 | -55.35 | 94.88 | 0.8198 | 423.0 | 377.0 | |
| 0.00 | 0.70 | 0.00 | 0.61 | -10.13 | 162.78 | -56.35 | 97.52 | 0.8287 | 390.0 | 368.4 | |
| 0.00 | 0.78 | 0.00 | 0.74 | -15.60 | 159.91 | -59.22 | 104.03 | 0.8551 | -445.0 | -444.6 | |
| 0.00 | 0.70 | 0.00 | 0.75 | -20.85 | 155.64 | -63.49 | 109.88 | 0.8912 | -139.0 | -107.9 | |
| 0.00 | 1.92 | 0.00 | 2.00 | -18.36 | 156.70 | -62.43 | 107.11 | 0.8823 | -196.0 | -232.1 | |
| 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. | |