SDO HMI 2014-10-05 21:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.85 | 316.95 | 33.95 | 193.02 | -1.49 | 154.92 | 34.51 | 258.12 | 0.5809 | 834.2 | 341.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.44 | 292.52 | 22.29 | 178.69 | -1.52 | 155.48 | 35.07 | 258.30 | 0.5888 | 1198.3 | 359.7 | |
| 5.36 | -1.00 | 3.25 | -1.00 | -1.51 | 154.78 | 34.38 | 258.05 | 0.5791 | 1163.7 | 999999 | |
| 9.75 | -1.00 | 5.86 | -1.00 | -1.79 | 154.03 | 33.62 | 257.26 | 0.5696 | 921.0 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -0.03 | 153.83 | 33.42 | 260.24 | 0.5611 | 449.0 | 389.2 | |
| 3.95 | 10.10 | 2.35 | 6.01 | -0.40 | 153.47 | 33.06 | 259.45 | 0.5571 | 920.8 | 644.8 | |
| 0.00 | 2.90 | 0.00 | 1.70 | -0.19 | 152.05 | 31.64 | 259.26 | 0.5361 | 469.0 | 556.9 | |
| 0.00 | 0.97 | 0.00 | 0.56 | 0.04 | 151.77 | 31.36 | 259.57 | 0.5313 | 599.0 | 415.5 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -0.88 | 151.52 | 31.12 | 257.77 | 0.5308 | -604.0 | -499.6 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -0.99 | 151.38 | 30.98 | 257.50 | 0.5292 | -482.0 | -489.4 | |
| 0.00 | 1.49 | 0.00 | 0.87 | -1.59 | 151.25 | 30.85 | 256.34 | 0.5295 | -550.0 | -480.9 | |
| 0.35 | 4.22 | 0.20 | 2.44 | -0.60 | 150.96 | 30.56 | 258.03 | 0.5217 | -731.5 | -423.5 | |
| 0.00 | 1.32 | 0.00 | 0.76 | -0.23 | 150.20 | 29.79 | 258.39 | 0.5092 | -636.0 | -432.6 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -1.66 | 148.80 | 28.39 | 254.91 | 0.4943 | -592.0 | -506.7 | |
| 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. | |