SDO HMI 2014-10-05 10:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.80 | 324.28 | 35.15 | 184.81 | -1.36 | 155.04 | 28.58 | 255.58 | 0.4957 | 956.5 | 368.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.02 | 284.37 | 24.01 | 162.49 | -1.39 | 155.38 | 28.92 | 255.73 | 0.5008 | 1260.1 | 364.8 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -2.50 | 154.78 | 28.32 | 253.23 | 0.4970 | 706.0 | 592.1 | |
| 4.40 | -1.00 | 2.49 | -1.00 | -1.49 | 154.59 | 28.13 | 255.08 | 0.4897 | 1206.5 | 999999 | |
| 9.23 | 15.74 | 5.21 | 8.88 | -1.76 | 153.92 | 27.45 | 254.15 | 0.4810 | 975.5 | 665.3 | |
| 0.00 | 1.32 | 0.00 | 0.74 | 0.15 | 153.84 | 27.38 | 257.99 | 0.4720 | 681.0 | 604.1 | |
| 6.15 | 11.69 | 3.44 | 6.54 | -0.22 | 153.40 | 26.94 | 257.00 | 0.4668 | 988.9 | 697.6 | |
| 0.00 | 2.64 | 0.00 | 1.48 | -1.40 | 153.41 | 26.94 | 254.57 | 0.4719 | 415.0 | 452.3 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 0.65 | 152.43 | 25.97 | 258.33 | 0.4489 | 693.0 | 609.8 | |
| 0.00 | 1.76 | 0.00 | 0.97 | 0.30 | 151.50 | 25.03 | 257.06 | 0.4360 | 804.0 | 631.9 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -1.73 | 150.29 | 23.82 | 251.73 | 0.4270 | -719.0 | -584.0 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -2.26 | 150.06 | 23.60 | 250.36 | 0.4266 | -761.0 | -603.4 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -2.07 | 149.90 | 23.43 | 250.65 | 0.4230 | -601.0 | -447.8 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -1.74 | 147.91 | 21.45 | 249.68 | 0.3914 | -733.0 | -622.6 | |
| 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. | |