SDO HMI 2011-10-10 15:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.37 | 140.63 | 29.41 | 73.33 | 20.01 | 111.14 | -11.94 | 38.79 | 0.3116 | -17.3 | -45.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.65 | 24.38 | 114.83 | -8.25 | 22.66 | 0.3407 | 783.0 | 494.1 | |
| 10.59 | 90.80 | 5.50 | 47.19 | 20.16 | 112.37 | -10.72 | 35.68 | 0.3006 | -1032.2 | -273.4 | |
| 14.53 | -2.00 | 7.55 | -2.00 | 19.94 | 111.99 | -11.09 | 37.06 | 0.3014 | -1156.0 | 999999 | |
| 3.24 | -2.00 | 1.68 | -2.00 | 19.69 | 111.95 | -11.14 | 37.71 | 0.2987 | -1016.4 | 999999 | |
| 0.00 | 1.75 | 0.00 | 0.92 | 22.63 | 111.69 | -11.40 | 32.63 | 0.3397 | 751.0 | 647.2 | |
| 3.06 | -2.00 | 1.59 | -2.00 | 19.68 | 111.62 | -11.46 | 38.50 | 0.3019 | -764.0 | 999999 | |
| 0.00 | 1.58 | 0.00 | 0.82 | 20.60 | 111.13 | -11.95 | 37.70 | 0.3185 | 772.0 | 652.7 | |
| 0.00 | 2.80 | 0.00 | 1.46 | 18.98 | 110.41 | -12.67 | 42.84 | 0.3065 | -841.0 | -719.3 | |
| 0.00 | 1.31 | 0.00 | 0.69 | 19.60 | 110.33 | -12.75 | 41.61 | 0.3146 | 690.0 | 501.9 | |
| 0.00 | 1.93 | 0.00 | 1.01 | 20.14 | 109.89 | -13.19 | 41.33 | 0.3259 | 739.0 | 475.4 | |
| 1.40 | 37.04 | 0.73 | 19.43 | 20.04 | 109.47 | -13.61 | 42.40 | 0.3292 | 840.1 | 768.4 | |
| 8.93 | -11.00 | 4.68 | -11.00 | 19.72 | 109.18 | -13.91 | 43.70 | 0.3290 | 1210.5 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 20.18 | 108.97 | -14.11 | 43.09 | 0.3365 | 11.0 | 45.8 | |
| 14.62 | -11.00 | 7.68 | -11.00 | 19.90 | 108.93 | -14.15 | 43.78 | 0.3338 | 879.8 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 21.55 | 107.10 | -15.98 | 43.62 | 0.3728 | 740.0 | 506.5 | |
| 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. | |