SDO HMI 2011-10-14 16:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.54 | 125.07 | 18.88 | 103.94 | -14.72 | 119.45 | 49.68 | 246.70 | 0.8049 | 346.5 | 217.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.10 | 110.58 | 1.75 | 92.76 | -14.04 | 119.97 | 50.20 | 247.72 | 0.8077 | 728.0 | 299.0 | |
| 20.00 | -1.00 | 16.80 | -1.00 | -14.64 | 119.96 | 50.19 | 247.01 | 0.8096 | 836.9 | 999999 | |
| 0.00 | 1.22 | 0.00 | 1.03 | -17.68 | 118.83 | 49.07 | 243.01 | 0.8099 | -594.0 | -486.5 | |
| 0.00 | 0.70 | 0.00 | 0.56 | -16.52 | 116.83 | 47.07 | 243.48 | 0.7867 | -276.0 | -288.0 | |
| 0.00 | 1.05 | 0.00 | 0.81 | -14.64 | 116.04 | 46.28 | 245.37 | 0.7715 | -577.0 | -529.2 | |
| 0.00 | 1.31 | 0.00 | 1.02 | -15.06 | 116.11 | 46.35 | 244.90 | 0.7739 | -659.0 | -538.0 | |
| 0.00 | 1.57 | 0.00 | 1.18 | -12.72 | 114.85 | 45.09 | 247.21 | 0.7516 | 802.0 | 641.9 | |
| 0.00 | 0.70 | 0.00 | 0.54 | -16.12 | 114.99 | 45.23 | 243.09 | 0.7671 | -709.0 | -624.4 | |
| 0.00 | 1.66 | 0.00 | 1.28 | -16.41 | 114.99 | 45.22 | 242.74 | 0.7683 | -521.0 | -390.6 | |
| 0.44 | 1.48 | 0.33 | 1.14 | -16.36 | 114.66 | 44.90 | 242.65 | 0.7648 | -734.6 | -655.6 | |
| 0.00 | 0.61 | 0.00 | 0.47 | -16.96 | 114.53 | 44.77 | 241.87 | 0.7662 | -484.0 | -417.4 | |
| 0.00 | 1.66 | 0.00 | 1.27 | -16.65 | 114.35 | 44.59 | 242.14 | 0.7630 | -672.0 | -571.7 | |
| 0.00 | 2.53 | 0.00 | 1.88 | -15.83 | 113.25 | 43.49 | 242.58 | 0.7482 | -312.0 | -294.3 | |
| 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. | |