SDO HMI 2011-06-07 14:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.86 | 32.20 | 13.37 | 35.17 | -20.96 | 36.86 | 60.80 | 246.21 | 0.8922 | 371.0 | 240.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.63 | 0.00 | 0.76 | -19.27 | 40.08 | 64.02 | 248.71 | 0.9124 | 183.0 | 217.1 | |
| 0.00 | 3.08 | 0.00 | 3.62 | -18.88 | 39.58 | 63.52 | 249.05 | 0.9086 | 496.0 | 334.9 | |
| 8.78 | 10.86 | 10.26 | 12.69 | -19.21 | 39.37 | 63.31 | 248.67 | 0.9076 | 571.9 | 343.8 | |
| 0.00 | 1.36 | 0.00 | 1.52 | -20.60 | 37.87 | 61.81 | 246.87 | 0.8990 | 291.0 | 223.5 | |
| 0.00 | 1.18 | 0.00 | 1.26 | -22.23 | 35.98 | 59.92 | 244.68 | 0.8880 | 417.0 | 314.8 | |
| 0.00 | 0.63 | 0.00 | 0.71 | -24.69 | 37.07 | 61.01 | 242.24 | 0.8999 | 532.0 | 384.4 | |
| 0.00 | 2.71 | 0.00 | 2.79 | -21.87 | 34.76 | 58.70 | 244.80 | 0.8783 | 696.0 | 590.7 | |
| 0.00 | 1.54 | 0.00 | 1.59 | -22.33 | 34.75 | 58.69 | 244.29 | 0.8791 | 424.0 | 385.1 | |
| 0.00 | 0.90 | 0.00 | 0.88 | -21.21 | 33.04 | 56.98 | 245.13 | 0.8636 | -364.0 | -303.4 | |
| 0.00 | 0.36 | 0.00 | 0.35 | -21.40 | 32.92 | 56.86 | 244.88 | 0.8630 | -274.0 | -371.5 | |
| 3.08 | 5.61 | 3.11 | 5.68 | -23.05 | 33.85 | 57.79 | 243.26 | 0.8737 | 471.3 | 271.7 | |
| 0.00 | 0.45 | 0.00 | 0.45 | -23.65 | 32.84 | 56.78 | 242.33 | 0.8672 | 264.0 | 238.2 | |
| 0.00 | 1.99 | 0.00 | 1.97 | -23.98 | 32.76 | 56.70 | 241.94 | 0.8674 | 21.0 | -87.2 | |
| 0.00 | 0.90 | 0.00 | 0.90 | -24.58 | 32.68 | 56.62 | 241.25 | 0.8682 | -606.0 | -526.6 | |
| 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. | |