SDO HMI 2014-10-10 02:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.44 | 0.00 | 12.75 | -20.98 | 74.14 | 9.27 | 198.30 | 0.4878 | 283.4 | 303.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.75 | 0.00 | 1.06 | -23.19 | 83.55 | 18.68 | 211.20 | 0.5705 | 698.0 | 490.1 | |
| 0.00 | 1.14 | 0.00 | 0.66 | -20.29 | 80.83 | 15.95 | 210.22 | 0.5143 | 684.0 | 607.8 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -21.39 | 78.65 | 13.78 | 205.69 | 0.5135 | 723.0 | 604.8 | |
| 0.00 | 1.58 | 0.00 | 0.86 | -15.15 | 77.74 | 12.87 | 210.71 | 0.4228 | 650.0 | 614.5 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -17.42 | 76.42 | 11.54 | 205.57 | 0.4442 | 653.0 | 590.2 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -25.45 | 75.38 | 10.51 | 197.46 | 0.5510 | 583.0 | 446.4 | |
| 0.00 | 3.16 | 0.00 | 1.75 | -18.82 | 74.61 | 9.74 | 200.77 | 0.4533 | 543.0 | 585.3 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -19.08 | 74.21 | 9.33 | 199.78 | 0.4548 | 689.0 | 580.6 | |
| 0.00 | 3.07 | 0.00 | 1.70 | -19.07 | 74.05 | 9.17 | 199.47 | 0.4539 | 701.0 | 582.7 | |
| 0.00 | 2.28 | 0.00 | 1.32 | -23.69 | 72.98 | 8.11 | 194.54 | 0.5164 | 625.0 | 476.1 | |
| 0.00 | 1.40 | 0.00 | 0.80 | -23.65 | 67.46 | 2.59 | 184.74 | 0.5020 | -650.0 | -587.0 | |
| 0.00 | 1.31 | 0.00 | 0.78 | -27.54 | 67.48 | 2.60 | 184.14 | 0.5595 | -537.0 | -394.9 | |
| 0.00 | 1.58 | 0.00 | 0.88 | -20.52 | 66.61 | 1.73 | 183.60 | 0.4529 | -776.0 | -586.7 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -22.69 | 66.44 | 1.56 | 182.98 | 0.4862 | -618.0 | -502.4 | |
| 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. | |