SDO HMI 2014-10-05 13:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.62 | 323.70 | 35.07 | 187.72 | -1.40 | 155.12 | 30.30 | 256.43 | 0.5209 | 1036.0 | 366.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.70 | 286.79 | 0.41 | 166.66 | -1.02 | 155.56 | 30.74 | 257.35 | 0.5259 | 776.9 | 345.8 | |
| 0.00 | 1.14 | 0.00 | 0.67 | -3.93 | 155.63 | 30.82 | 252.11 | 0.5392 | 647.0 | 490.6 | |
| 39.89 | -1.00 | 23.19 | -1.00 | -1.43 | 155.39 | 30.57 | 256.51 | 0.5250 | 1234.1 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -2.25 | 154.85 | 30.03 | 254.72 | 0.5205 | 246.0 | 198.6 | |
| 1.14 | -1.00 | 0.66 | -1.00 | -1.36 | 154.80 | 29.98 | 256.33 | 0.5162 | 1297.3 | 999999 | |
| 3.78 | -1.00 | 2.18 | -1.00 | -1.51 | 154.63 | 29.81 | 255.98 | 0.5143 | 1202.2 | 999999 | |
| 1.49 | -1.00 | 0.86 | -1.00 | -1.65 | 154.49 | 29.67 | 255.64 | 0.5129 | 993.2 | 999999 | |
| 5.89 | 15.20 | 3.38 | 8.71 | -1.83 | 154.01 | 29.19 | 255.03 | 0.5067 | 915.5 | 763.1 | |
| 0.00 | 1.23 | 0.00 | 0.70 | 0.19 | 154.00 | 29.18 | 258.94 | 0.4988 | 730.0 | 603.5 | |
| 0.00 | 1.41 | 0.00 | 0.81 | -4.02 | 154.04 | 29.22 | 250.96 | 0.5172 | 669.0 | 538.9 | |
| 7.73 | 13.97 | 4.39 | 7.94 | -0.26 | 153.45 | 28.63 | 257.79 | 0.4922 | 971.8 | 704.2 | |
| 0.00 | 1.32 | 0.00 | 0.74 | 0.59 | 152.30 | 27.48 | 258.96 | 0.4720 | 721.0 | 545.1 | |
| 0.00 | 1.41 | 0.00 | 0.78 | -0.42 | 150.82 | 26.00 | 256.06 | 0.4535 | -833.0 | -661.8 | |
| 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. | |