SDO HMI 2011-06-10 14:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.19 | 47.55 | 16.94 | 38.20 | -15.85 | 246.40 | -49.95 | 110.69 | 0.7890 | 180.4 | 152.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.99 | 11.14 | 2.32 | 8.63 | -16.05 | 248.23 | -48.12 | 111.47 | 0.7712 | 687.1 | 600.3 | |
| 1.63 | -1.00 | 1.27 | -1.00 | -15.80 | 247.93 | -48.42 | 111.06 | 0.7736 | 536.3 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.92 | -15.80 | 247.54 | -48.81 | 110.95 | 0.7776 | 568.0 | 521.8 | |
| 5.07 | 5.70 | 3.97 | 4.46 | -15.45 | 247.56 | -48.79 | 110.51 | 0.7765 | 712.1 | 556.9 | |
| 0.00 | 1.36 | 0.00 | 1.08 | -15.87 | 247.09 | -49.27 | 110.89 | 0.7824 | 590.0 | 492.5 | |
| 6.43 | 12.77 | 5.12 | 10.18 | -15.65 | 246.77 | -49.59 | 110.53 | 0.7851 | 483.6 | 248.3 | |
| 0.00 | 1.45 | 0.00 | 1.16 | -15.24 | 246.56 | -49.80 | 109.96 | 0.7862 | 566.0 | 437.3 | |
| 0.00 | 1.45 | 0.00 | 1.16 | -14.61 | 246.17 | -50.18 | 109.07 | 0.7887 | 427.0 | 396.0 | |
| 0.00 | 1.54 | 0.00 | 1.27 | -15.47 | 245.08 | -51.27 | 109.85 | 0.8015 | -569.0 | -524.9 | |
| 1.99 | 3.35 | 1.66 | 2.79 | -16.20 | 244.72 | -51.64 | 110.64 | 0.8068 | -712.0 | -636.1 | |
| 3.08 | 4.35 | 2.60 | 3.67 | -16.40 | 244.28 | -52.07 | 110.76 | 0.8114 | -683.0 | -580.9 | |
| 0.00 | 0.63 | 0.00 | 0.55 | -16.63 | 243.25 | -53.11 | 110.76 | 0.8217 | -567.0 | -493.3 | |
| 0.00 | 1.18 | 0.00 | 1.02 | -16.50 | 243.25 | -53.11 | 110.61 | 0.8214 | -543.0 | -372.5 | |
| 0.00 | 1.45 | 0.00 | 1.31 | -16.96 | 241.48 | -54.88 | 110.72 | 0.8385 | -593.0 | -484.4 | |
| 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. | |