SDO HMI 2014-03-01 23:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.47 | 22.36 | 0.78 | 11.88 | 7.57 | 134.83 | 14.89 | 315.38 | 0.3634 | 240.9 | 302.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.21 | 0.00 | 0.67 | 4.77 | 143.14 | 23.20 | 296.74 | 0.4414 | -638.0 | -554.4 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 5.29 | 141.38 | 21.45 | 299.76 | 0.4212 | -794.0 | -668.8 | |
| 0.00 | 1.29 | 0.00 | 0.73 | 11.20 | 141.38 | 21.44 | 310.64 | 0.4745 | -703.0 | -450.1 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 1.83 | 138.26 | 18.32 | 295.70 | 0.3502 | -9.0 | 3.0 | |
| 0.00 | 0.78 | 0.00 | 0.41 | 7.13 | 136.30 | 16.36 | 311.00 | 0.3720 | 661.0 | 590.4 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 7.05 | 135.86 | 15.93 | 311.62 | 0.3659 | 800.0 | 665.5 | |
| 1.47 | 2.59 | 0.78 | 1.38 | 8.62 | 134.99 | 15.05 | 316.32 | 0.3735 | -791.0 | -593.6 | |
| 0.00 | 1.47 | 0.00 | 0.78 | 8.31 | 134.89 | 14.95 | 315.94 | 0.3686 | -710.0 | -492.6 | |
| 0.00 | 1.47 | 0.00 | 0.77 | 6.91 | 134.40 | 14.46 | 314.12 | 0.3469 | 809.0 | 672.1 | |
| 0.00 | 1.47 | 0.00 | 0.77 | 7.38 | 133.86 | 13.92 | 316.19 | 0.3462 | 856.0 | 720.5 | |
| 0.00 | 2.07 | 0.00 | 1.09 | 8.13 | 133.12 | 13.18 | 319.23 | 0.3471 | 906.0 | 761.1 | |
| 0.00 | 3.02 | 0.00 | 1.58 | 8.22 | 130.76 | 10.82 | 324.90 | 0.3245 | 914.0 | 723.5 | |
| 0.00 | 2.42 | 0.00 | 1.26 | 8.34 | 130.55 | 10.61 | 325.64 | 0.3242 | 886.0 | 789.5 | |
| 0.00 | 1.29 | 0.00 | 0.68 | 8.03 | 130.41 | 10.48 | 325.42 | 0.3187 | 959.0 | 759.1 | |
| 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. | |