SDO HMI 2011-08-30 03:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.79 | 276.95 | 20.97 | 146.36 | 13.99 | 291.46 | -19.45 | 68.81 | 0.3482 | -568.7 | -331.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.85 | 258.03 | 18.89 | 136.00 | 13.81 | 291.81 | -19.10 | 68.93 | 0.3420 | -1374.0 | -418.1 | |
| 3.94 | -1.00 | 2.08 | -1.00 | 13.71 | 291.52 | -19.39 | 69.46 | 0.3459 | -1054.5 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 16.24 | 290.71 | -20.20 | 63.51 | 0.3720 | 573.0 | 495.3 | |
| 0.00 | 1.70 | 0.00 | 0.91 | 13.84 | 288.94 | -21.97 | 71.00 | 0.3858 | 738.0 | 620.4 | |
| 0.00 | 1.17 | 0.00 | 0.63 | 14.23 | 288.86 | -22.04 | 70.06 | 0.3886 | 867.0 | 758.8 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 12.01 | 288.91 | -22.00 | 75.70 | 0.3797 | 876.0 | 709.5 | |
| 0.00 | 3.50 | 0.00 | 1.88 | 14.07 | 288.64 | -22.26 | 70.61 | 0.3912 | 966.0 | 749.8 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 12.35 | 288.37 | -22.53 | 75.09 | 0.3890 | 715.0 | 457.1 | |
| 0.00 | 1.88 | 0.00 | 1.02 | 14.19 | 288.02 | -22.88 | 70.71 | 0.4011 | 811.0 | 744.5 | |
| 0.00 | 1.61 | 0.00 | 0.90 | 20.51 | 286.53 | -24.37 | 58.02 | 0.4575 | 841.0 | 606.7 | |
| 0.00 | 1.61 | 0.00 | 0.88 | 15.76 | 286.75 | -24.16 | 67.90 | 0.4269 | 800.0 | 564.4 | |
| 0.00 | 1.52 | 0.00 | 0.86 | 21.51 | 285.78 | -25.12 | 56.77 | 0.4741 | 788.0 | 609.6 | |
| 0.00 | 1.61 | 0.00 | 0.94 | 23.53 | 282.30 | -28.60 | 56.02 | 0.5314 | 742.0 | 506.2 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 18.86 | 282.91 | -27.99 | 64.01 | 0.4961 | 680.0 | 446.9 | |
| 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. | |