SDO HMI 2014-01-15 11:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78.49 | 409.58 | 40.79 | 213.16 | -16.36 | 12.75 | 13.65 | 227.59 | 0.3078 | 1106.8 | 432.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.19 | 0.00 | 0.64 | -17.19 | 18.11 | 19.01 | 234.45 | 0.3841 | 820.0 | 677.8 | |
| 0.00 | 3.66 | 0.00 | 1.96 | -17.70 | 18.06 | 18.96 | 233.26 | 0.3880 | 586.0 | 614.0 | |
| 0.00 | 1.62 | 0.00 | 0.86 | -16.24 | 17.36 | 18.26 | 235.62 | 0.3661 | -731.0 | -532.7 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -18.55 | 13.67 | 14.57 | 224.36 | 0.3426 | 846.0 | 611.6 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -14.70 | 13.32 | 14.22 | 233.16 | 0.2982 | -567.0 | -464.6 | |
| 38.52 | 245.51 | 20.11 | 128.18 | -16.56 | 13.38 | 14.28 | 228.41 | 0.3176 | 1380.3 | 426.4 | |
| 4.25 | -6.00 | 2.21 | -6.00 | -16.72 | 12.73 | 13.63 | 226.73 | 0.3113 | 1192.1 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -15.32 | 12.19 | 13.09 | 229.25 | 0.2897 | 689.0 | 551.7 | |
| 0.68 | 146.35 | 0.35 | 75.68 | -15.14 | 11.96 | 12.86 | 229.25 | 0.2849 | 1058.0 | 470.6 | |
| 0.00 | 2.38 | 0.00 | 1.24 | -16.86 | 11.95 | 12.85 | 224.77 | 0.3035 | 574.0 | 478.1 | |
| 35.04 | -9.00 | 18.12 | -9.00 | -15.96 | 11.61 | 12.51 | 226.29 | 0.2893 | 1340.1 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -14.58 | 11.52 | 12.42 | 229.89 | 0.2735 | -768.0 | -498.8 | |
| 0.00 | 2.81 | 0.00 | 1.47 | -18.77 | 11.73 | 12.64 | 219.99 | 0.3237 | 726.0 | 631.5 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -17.71 | 6.28 | 7.18 | 207.62 | 0.2582 | -956.0 | -808.5 | |
| 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. | |