SDO HMI 2011-10-10 14:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.01 | 189.25 | 19.77 | 113.05 | 23.43 | 153.99 | 30.35 | 303.87 | 0.5604 | -554.6 | -270.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.55 | 24.55 | 158.69 | 35.05 | 302.49 | 0.6216 | -571.0 | -452.6 | |
| 0.00 | 2.19 | 0.00 | 1.35 | 24.07 | 156.56 | 32.92 | 303.04 | 0.5942 | -51.0 | -131.1 | |
| 2.36 | 169.01 | 1.42 | 101.29 | 23.15 | 154.87 | 31.24 | 302.68 | 0.5688 | -908.2 | -376.8 | |
| 3.24 | -3.00 | 1.94 | -3.00 | 22.96 | 154.79 | 31.15 | 302.44 | 0.5666 | -859.7 | 999999 | |
| 27.41 | -3.00 | 16.41 | -3.00 | 23.30 | 154.42 | 30.78 | 303.24 | 0.5642 | -1231.3 | 999999 | |
| 0.00 | 2.45 | 0.00 | 1.44 | 21.82 | 153.38 | 29.75 | 301.51 | 0.5424 | 649.0 | 416.3 | |
| 0.00 | 1.58 | 0.00 | 0.93 | 22.01 | 153.24 | 29.61 | 301.94 | 0.5419 | 585.0 | 441.6 | |
| 0.00 | 0.79 | 0.00 | 0.45 | 25.28 | 148.02 | 24.39 | 311.96 | 0.5041 | 925.0 | 700.1 | |
| 0.00 | 3.77 | 0.00 | 2.16 | 25.70 | 148.04 | 24.40 | 312.61 | 0.5079 | 824.0 | 658.8 | |
| 0.00 | 1.66 | 0.00 | 0.97 | 27.22 | 148.31 | 24.68 | 314.71 | 0.5245 | 602.0 | 525.1 | |
| 0.00 | 1.05 | 0.00 | 0.61 | 26.91 | 148.02 | 24.38 | 314.54 | 0.5186 | 642.0 | 546.8 | |
| 0.00 | 2.19 | 0.00 | 1.23 | 25.82 | 144.78 | 21.15 | 316.52 | 0.4739 | 1056.0 | 815.1 | |
| 0.00 | 2.63 | 0.00 | 1.48 | 26.17 | 144.85 | 21.21 | 317.00 | 0.4781 | 692.0 | 618.7 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 26.43 | 144.72 | 21.08 | 317.57 | 0.4794 | 746.0 | 619.2 | |
| 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. | |