SDO HMI 2011-10-04 20:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.07 | 370.75 | 44.88 | 259.39 | 23.15 | 156.10 | -43.38 | 63.55 | 0.7076 | -817.0 | -285.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.53 | 1.84 | 0.37 | 1.30 | 26.38 | 156.49 | -42.99 | 59.03 | 0.7148 | -802.3 | -673.0 | |
| 0.00 | 1.41 | 0.00 | 1.00 | 26.32 | 156.15 | -43.33 | 59.24 | 0.7181 | -469.0 | -389.1 | |
| 14.85 | 291.76 | 10.25 | 202.43 | 22.59 | 156.75 | -42.73 | 64.10 | 0.6988 | -1123.4 | -335.3 | |
| 27.15 | -3.00 | 18.88 | -3.00 | 23.11 | 156.41 | -43.07 | 63.50 | 0.7042 | -1072.3 | 999999 | |
| 1.67 | -3.00 | 1.16 | -3.00 | 22.26 | 156.48 | -43.01 | 64.65 | 0.7008 | -792.0 | 999999 | |
| 16.17 | 65.63 | 11.55 | 47.07 | 24.05 | 154.97 | -44.51 | 62.70 | 0.7228 | -919.0 | -129.4 | |
| 1.32 | -6.00 | 0.94 | -6.00 | 23.67 | 154.67 | -44.81 | 63.29 | 0.7249 | -468.8 | 999999 | |
| 0.00 | 1.84 | 0.00 | 1.31 | 22.02 | 155.04 | -44.44 | 65.42 | 0.7161 | -158.0 | -239.6 | |
| 1.41 | 2.20 | 0.98 | 1.53 | 19.93 | 155.51 | -43.97 | 68.18 | 0.7054 | 562.4 | 569.2 | |
| 0.97 | 2.37 | 0.75 | 1.84 | 24.81 | 150.45 | -49.03 | 63.02 | 0.7714 | 641.2 | 522.2 | |
| 0.00 | 0.88 | 0.00 | 0.68 | 24.42 | 150.36 | -49.13 | 63.55 | 0.7714 | 346.0 | 372.7 | |
| 0.00 | 0.97 | 0.00 | 0.78 | 26.29 | 148.78 | -50.71 | 61.60 | 0.7910 | 657.0 | 595.4 | |
| 0.00 | 0.88 | 0.00 | 0.71 | 26.21 | 148.61 | -50.87 | 61.74 | 0.7924 | 542.0 | 451.1 | |
| 0.00 | 0.97 | 0.00 | 0.74 | 22.65 | 150.29 | -49.19 | 65.81 | 0.7680 | 499.0 | 458.2 | |
| 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. | |