SDO HMI 2014-02-27 15:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.70 | 45.86 | 4.72 | 24.51 | 7.87 | 134.93 | -15.76 | 45.55 | 0.3736 | 298.6 | 95.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.64 | 0.00 | 0.85 | 6.62 | 141.73 | -8.96 | 33.12 | 0.2843 | -871.0 | -687.0 | |
| 0.00 | 3.71 | 0.00 | 1.91 | 6.47 | 141.49 | -9.20 | 34.11 | 0.2845 | -915.0 | -834.6 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 6.29 | 141.22 | -9.47 | 35.24 | 0.2846 | -847.0 | -720.4 | |
| 0.00 | 5.60 | 0.00 | 2.91 | 6.90 | 139.94 | -10.75 | 37.52 | 0.3055 | -1163.0 | -899.4 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 5.56 | 139.90 | -10.79 | 40.46 | 0.2884 | -833.0 | -672.1 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 6.12 | 139.65 | -11.04 | 39.90 | 0.2982 | -922.0 | -840.0 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 7.90 | 134.52 | -16.17 | 47.21 | 0.3776 | 823.0 | 662.0 | |
| 0.00 | 4.05 | 0.00 | 2.17 | 7.14 | 133.48 | -17.21 | 50.51 | 0.3820 | 708.0 | 718.4 | |
| 5.08 | 8.19 | 2.75 | 4.43 | 8.76 | 132.94 | -17.75 | 48.25 | 0.4055 | 1051.1 | 901.4 | |
| 0.00 | 2.24 | 0.00 | 1.21 | 7.68 | 132.39 | -18.30 | 51.19 | 0.4010 | 952.0 | 722.8 | |
| 0.00 | 2.07 | 0.00 | 1.13 | 9.80 | 131.78 | -18.91 | 48.21 | 0.4302 | 653.0 | 578.3 | |
| 0.52 | 2.07 | 0.28 | 1.13 | 8.85 | 131.74 | -18.96 | 49.99 | 0.4209 | 849.5 | 722.9 | |
| 0.00 | 1.72 | 0.00 | 0.95 | 9.72 | 131.59 | -19.10 | 48.64 | 0.4315 | 490.0 | 376.2 | |
| 3.10 | 6.38 | 1.69 | 3.47 | 8.45 | 131.63 | -19.06 | 50.88 | 0.4182 | 1021.4 | 760.7 | |
| 0.00 | 1.21 | 0.00 | 0.66 | 8.77 | 131.33 | -19.37 | 50.74 | 0.4251 | 707.0 | 592.6 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 8.59 | 131.24 | -19.45 | 51.20 | 0.4243 | 770.0 | 660.1 | |
| 0.00 | 1.47 | 0.00 | 0.80 | 8.14 | 130.88 | -19.81 | 52.55 | 0.4244 | 632.0 | 444.4 | |
| 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. | |