SDO HMI 2014-10-05 15:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.49 | 332.55 | 35.95 | 195.03 | -1.39 | 155.05 | 31.33 | 256.95 | 0.5356 | 970.2 | 336.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.16 | 296.89 | 21.85 | 174.58 | -1.44 | 155.41 | 31.69 | 257.03 | 0.5410 | 1275.1 | 339.6 | |
| 0.79 | -1.00 | 0.46 | -1.00 | -1.11 | 154.98 | 31.26 | 257.43 | 0.5337 | 1067.3 | 999999 | |
| 7.38 | -1.00 | 4.31 | -1.00 | -1.48 | 154.71 | 30.99 | 256.61 | 0.5312 | 1187.2 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.66 | 0.31 | 154.00 | 30.28 | 259.64 | 0.5146 | 627.0 | 446.8 | |
| 8.43 | 12.74 | 4.89 | 7.38 | -1.80 | 153.94 | 30.22 | 255.64 | 0.5214 | 940.4 | 735.9 | |
| 7.73 | 12.12 | 4.44 | 6.97 | -0.29 | 153.48 | 29.76 | 258.26 | 0.5090 | 976.0 | 765.7 | |
| 0.00 | 1.32 | 0.00 | 0.76 | -1.62 | 153.39 | 29.67 | 255.69 | 0.5126 | 700.0 | 533.6 | |
| 0.00 | 1.14 | 0.00 | 0.65 | 0.59 | 152.35 | 28.63 | 259.48 | 0.4893 | 634.0 | 551.1 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 0.04 | 151.93 | 28.22 | 258.18 | 0.4850 | 877.0 | 645.2 | |
| 0.00 | 2.46 | 0.00 | 1.38 | -0.54 | 150.88 | 27.17 | 256.47 | 0.4715 | -783.0 | -654.8 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -1.51 | 150.86 | 27.14 | 254.48 | 0.4752 | -612.0 | -532.9 | |
| 0.00 | 1.49 | 0.00 | 0.83 | -1.86 | 150.02 | 26.30 | 253.24 | 0.4645 | -661.0 | -480.7 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -1.68 | 148.39 | 24.67 | 252.47 | 0.4394 | -640.0 | -532.5 | |
| 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. | |