SDO HMI 2011-08-16 04:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.62 | 246.79 | 80.61 | 447.05 | 15.48 | 60.25 | -75.11 | 75.73 | 0.9601 | -111.2 | -4.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.33 | 126.82 | 20.36 | 183.54 | 15.96 | 64.74 | -70.61 | 75.42 | 0.9386 | -725.0 | -100.8 | |
| 1.71 | -1.00 | 2.48 | -1.00 | 15.88 | 64.32 | -71.04 | 75.49 | 0.9411 | 181.6 | 999999 | |
| 0.54 | -1.00 | 0.80 | -1.00 | 15.68 | 63.89 | -71.46 | 75.70 | 0.9435 | -142.3 | 999999 | |
| 3.97 | -1.00 | 5.83 | -1.00 | 15.35 | 64.07 | -71.29 | 76.05 | 0.9426 | -224.8 | 999999 | |
| 3.06 | -1.00 | 4.53 | -1.00 | 15.58 | 63.87 | -71.48 | 75.80 | 0.9436 | 159.5 | 999999 | |
| 5.50 | 24.79 | 9.69 | 44.24 | 16.54 | 60.51 | -74.85 | 74.68 | 0.9606 | -335.5 | 122.5 | |
| 0.00 | 2.07 | 0.00 | 3.48 | 15.06 | 61.43 | -73.93 | 76.26 | 0.9565 | 476.0 | 448.5 | |
| 0.90 | 10.64 | 1.61 | 19.00 | 14.97 | 60.32 | -75.03 | 76.30 | 0.9618 | 551.4 | 539.5 | |
| 5.77 | 12.44 | 14.35 | 31.09 | 18.18 | 55.31 | -80.05 | 72.74 | 0.9808 | 393.1 | 183.3 | |
| 0.00 | 6.13 | 0.00 | 11.69 | 15.31 | 59.18 | -76.18 | 75.89 | 0.9668 | 696.0 | 492.8 | |
| 0.00 | 1.26 | 0.00 | 2.53 | 15.91 | 58.33 | -77.03 | 75.22 | 0.9703 | 350.0 | 331.1 | |
| 0.00 | 1.26 | 0.00 | 2.26 | 14.02 | 60.27 | -75.09 | 77.29 | 0.9623 | 513.0 | 455.3 | |
| 0.00 | 1.44 | 0.00 | 3.68 | 17.64 | 55.01 | -80.35 | 73.27 | 0.9819 | 106.0 | 61.1 | |
| 0.00 | 1.26 | 0.00 | 3.32 | 17.79 | 54.70 | -80.65 | 73.10 | 0.9828 | -219.0 | -191.2 | |
| 4.69 | 58.68 | 10.95 | 142.22 | 14.18 | 56.38 | -78.98 | 76.89 | 0.9781 | 388.3 | -97.8 | |
| 4.15 | -15.00 | 10.01 | -15.00 | 14.16 | 55.90 | -79.46 | 76.88 | 0.9798 | -406.9 | 999999 | |
| 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. | |