SDO HMI 2011-05-26 08:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.09 | 65.36 | 12.41 | 36.48 | -15.65 | 114.48 | -23.68 | 122.80 | 0.4615 | -5.4 | 210.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 7.12 | 0.00 | 3.91 | -15.35 | 116.64 | -21.51 | 124.50 | 0.4309 | 793.0 | 838.5 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -15.41 | 116.33 | -21.83 | 124.26 | 0.4354 | 613.0 | 564.4 | |
| 6.76 | 17.41 | 3.73 | 9.59 | -15.82 | 116.25 | -21.90 | 124.97 | 0.4398 | 986.0 | 690.9 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -16.60 | 115.34 | -22.82 | 125.41 | 0.4579 | 760.0 | 596.1 | |
| 0.00 | 1.44 | 0.00 | 0.80 | -14.71 | 115.15 | -23.01 | 121.59 | 0.4456 | 1046.0 | 774.1 | |
| 0.00 | 3.43 | 0.00 | 1.90 | -14.68 | 114.88 | -23.28 | 121.25 | 0.4490 | 811.0 | 653.6 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -16.30 | 114.20 | -23.96 | 123.66 | 0.4701 | 683.0 | 536.2 | |
| 0.00 | 1.62 | 0.00 | 0.91 | -14.77 | 113.91 | -24.25 | 120.46 | 0.4626 | 345.0 | 267.1 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -14.76 | 113.70 | -24.45 | 120.26 | 0.4653 | 593.0 | 502.0 | |
| 0.00 | 1.44 | 0.00 | 0.81 | -15.67 | 113.38 | -24.78 | 121.67 | 0.4760 | -972.0 | -776.7 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -15.98 | 113.10 | -25.06 | 121.98 | 0.4820 | -635.0 | -563.1 | |
| 5.68 | 10.19 | 3.20 | 5.73 | -15.38 | 113.07 | -25.09 | 120.85 | 0.4781 | -935.3 | -875.8 | |
| 4.87 | 5.86 | 2.76 | 3.32 | -15.63 | 112.69 | -25.47 | 120.96 | 0.4848 | -896.7 | -506.3 | |
| 4.78 | 10.82 | 2.72 | 6.14 | -16.32 | 112.56 | -25.60 | 122.09 | 0.4914 | -870.3 | -715.2 | |
| 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. | |