SDO HMI 2014-03-02 00:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.78 | 26.24 | 0.42 | 13.88 | 7.69 | 133.51 | 14.12 | 316.67 | 0.3536 | 404.9 | 381.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.52 | 0.00 | 0.28 | 5.25 | 141.32 | 21.93 | 299.12 | 0.4275 | -390.0 | -470.8 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 7.45 | 136.36 | 16.97 | 310.61 | 0.3829 | 543.0 | 526.4 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 7.14 | 136.29 | 16.90 | 310.11 | 0.3788 | 644.0 | 585.0 | |
| 0.00 | 0.35 | 0.00 | 0.18 | 7.01 | 135.87 | 16.49 | 310.54 | 0.3723 | 572.0 | 397.0 | |
| 0.78 | 3.62 | 0.42 | 1.94 | 8.64 | 135.10 | 15.71 | 315.13 | 0.3811 | -843.3 | -636.4 | |
| 0.00 | 2.67 | 0.00 | 1.41 | 6.26 | 134.73 | 15.34 | 311.05 | 0.3503 | 11.0 | 8.7 | |
| 0.00 | 4.31 | 0.00 | 2.28 | 6.89 | 134.35 | 14.96 | 313.11 | 0.3526 | 811.0 | 640.3 | |
| 0.00 | 1.64 | 0.00 | 0.87 | 7.43 | 133.90 | 14.51 | 315.09 | 0.3535 | 810.0 | 625.1 | |
| 0.00 | 2.85 | 0.00 | 1.51 | 8.11 | 133.15 | 13.76 | 317.95 | 0.3533 | 905.0 | 768.2 | |
| 0.00 | 0.60 | 0.00 | 0.32 | 8.64 | 132.12 | 12.73 | 321.14 | 0.3489 | -10.0 | -1.4 | |
| 0.00 | 1.73 | 0.00 | 0.91 | 8.67 | 131.08 | 11.69 | 323.59 | 0.3390 | 595.0 | 428.5 | |
| 0.00 | 3.11 | 0.00 | 1.63 | 8.23 | 130.79 | 11.40 | 323.49 | 0.3303 | 833.0 | 661.3 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 8.29 | 130.55 | 11.16 | 324.19 | 0.3287 | 983.0 | 814.6 | |
| 0.00 | 1.81 | 0.00 | 0.95 | 8.01 | 130.38 | 11.00 | 324.07 | 0.3234 | 729.0 | 503.8 | |
| 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. | |