SDO HMI 2011-10-19 08:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.57 | 406.10 | 50.39 | 311.55 | 27.62 | 55.17 | 46.96 | 301.91 | 0.7649 | -825.2 | -231.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.87 | 0.00 | 0.69 | 28.89 | 56.46 | 48.25 | 303.00 | 0.7813 | 290.0 | 241.4 | |
| 64.96 | 385.86 | 49.93 | 296.95 | 27.58 | 55.38 | 47.17 | 301.76 | 0.7668 | -1094.3 | -240.4 | |
| 0.00 | 5.32 | 0.00 | 3.97 | 27.29 | 53.75 | 45.55 | 301.98 | 0.7502 | -840.0 | -702.3 | |
| 0.00 | 0.35 | 0.00 | 0.27 | 30.58 | 55.63 | 47.42 | 305.36 | 0.7796 | 531.0 | 537.0 | |
| 0.00 | 0.87 | 0.00 | 0.68 | 30.63 | 55.35 | 47.15 | 305.53 | 0.7774 | 548.0 | 515.1 | |
| 0.00 | 1.83 | 0.00 | 1.42 | 30.23 | 54.79 | 46.59 | 305.25 | 0.7709 | 624.0 | 460.2 | |
| 0.61 | 2.62 | 0.46 | 1.97 | 30.94 | 52.64 | 44.44 | 307.00 | 0.7542 | -634.9 | -554.6 | |
| 0.00 | 0.70 | 0.00 | 0.50 | 27.90 | 50.40 | 42.19 | 304.13 | 0.7194 | -573.0 | -424.2 | |
| 0.00 | 1.66 | 0.00 | 1.23 | 30.90 | 51.65 | 43.44 | 307.38 | 0.7449 | -639.0 | -523.1 | |
| 0.00 | 1.13 | 0.00 | 0.74 | 27.55 | 44.56 | 36.36 | 306.66 | 0.6575 | 787.0 | 604.9 | |
| 0.00 | 1.22 | 0.00 | 0.80 | 27.24 | 44.36 | 36.16 | 306.35 | 0.6536 | 692.0 | 476.4 | |
| 0.00 | 2.01 | 0.00 | 1.28 | 25.00 | 43.44 | 35.24 | 303.71 | 0.6310 | 685.0 | 580.5 | |
| 0.00 | 0.61 | 0.00 | 0.38 | 22.23 | 42.60 | 34.39 | 300.05 | 0.6063 | 629.0 | 518.0 | |
| 0.00 | 1.05 | 0.00 | 0.67 | 30.51 | 40.79 | 32.59 | 313.15 | 0.6383 | 518.0 | 399.0 | |
| 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. | |