SDO HMI 2013-02-22 13:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.77 | 331.46 | 121.13 | 734.56 | 10.06 | 70.00 | 75.32 | 282.14 | 0.9730 | 134.3 | 49.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.68 | 135.25 | 26.98 | 403.78 | 9.79 | 74.07 | 79.39 | 281.16 | 0.9880 | 640.2 | -30.5 | |
| 15.05 | -1.00 | 42.91 | -1.00 | 9.64 | 73.13 | 78.45 | 281.16 | 0.9853 | -581.4 | 999999 | |
| 0.00 | 1.12 | 0.00 | 2.67 | 9.15 | 71.32 | 76.64 | 280.95 | 0.9793 | -539.0 | -428.2 | |
| 0.00 | 3.10 | 0.00 | 7.43 | 9.51 | 71.32 | 76.64 | 281.32 | 0.9795 | -460.0 | -428.3 | |
| 0.00 | 2.06 | 0.00 | 4.56 | 9.00 | 70.32 | 75.65 | 280.96 | 0.9757 | -398.0 | -358.9 | |
| 0.00 | 0.43 | 0.00 | 0.92 | 11.27 | 69.38 | 74.70 | 283.43 | 0.9736 | -538.0 | -485.6 | |
| 0.00 | 0.86 | 0.00 | 1.72 | 10.57 | 68.66 | 73.98 | 282.85 | 0.9702 | -116.0 | -81.2 | |
| 0.00 | 4.30 | 0.00 | 7.86 | 10.10 | 67.30 | 72.62 | 282.61 | 0.9640 | -102.0 | -211.5 | |
| 3.35 | 22.01 | 5.84 | 38.56 | 9.69 | 66.47 | 71.79 | 282.35 | 0.9598 | 413.5 | 127.3 | |
| 0.00 | 1.72 | 0.00 | 3.33 | 12.04 | 67.83 | 73.15 | 284.49 | 0.9679 | -379.0 | -306.2 | |
| 0.00 | 1.29 | 0.00 | 2.48 | 12.23 | 67.65 | 72.97 | 284.72 | 0.9674 | -213.0 | -206.6 | |
| 4.56 | 158.37 | 7.65 | 259.67 | 10.88 | 65.59 | 70.91 | 283.74 | 0.9567 | -311.2 | 213.7 | |
| 21.84 | -12.00 | 35.74 | -12.00 | 10.61 | 65.17 | 70.49 | 283.55 | 0.9543 | 726.7 | 999999 | |
| 0.00 | 0.95 | 0.00 | 1.58 | 11.96 | 65.40 | 70.72 | 284.89 | 0.9568 | 152.0 | 96.9 | |
| 1.29 | -12.00 | 2.01 | -12.00 | 10.74 | 64.16 | 69.48 | 283.88 | 0.9492 | 861.9 | 999999 | |
| 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. | |