SDO HMI 2014-11-29 07:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.51 | 18.82 | 0.32 | 11.73 | -23.23 | 93.83 | -29.02 | 132.72 | 0.6085 | -116.5 | -118.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.37 | 0.00 | 0.81 | -24.00 | 101.19 | -21.66 | 141.46 | 0.5432 | 686.0 | 630.2 | |
| 0.00 | 1.37 | 0.00 | 0.82 | -22.05 | 96.92 | -25.93 | 134.02 | 0.5658 | 657.0 | 500.4 | |
| 0.00 | 0.94 | 0.00 | 0.58 | -23.76 | 94.89 | -27.96 | 134.28 | 0.6017 | 878.0 | 748.2 | |
| 0.00 | 0.68 | 0.00 | 0.42 | -23.89 | 94.79 | -28.07 | 134.35 | 0.6039 | 588.0 | 536.1 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -22.20 | 95.13 | -27.72 | 132.44 | 0.5857 | -749.0 | -583.8 | |
| 0.51 | 2.91 | 0.32 | 1.80 | -23.53 | 94.80 | -28.05 | 133.90 | 0.6007 | 862.2 | 626.0 | |
| 0.00 | 0.94 | 0.00 | 0.59 | -24.16 | 93.50 | -29.35 | 133.52 | 0.6191 | -612.0 | -547.0 | |
| 0.00 | 1.11 | 0.00 | 0.70 | -24.13 | 93.21 | -29.64 | 133.22 | 0.6217 | -556.0 | -464.0 | |
| 0.00 | 1.11 | 0.00 | 0.70 | -23.64 | 93.07 | -29.78 | 132.47 | 0.6191 | -538.0 | -495.8 | |
| 0.00 | 2.48 | 0.00 | 1.57 | -24.30 | 92.75 | -30.10 | 133.04 | 0.6277 | -700.0 | -553.4 | |
| 0.00 | 1.11 | 0.00 | 0.71 | -23.69 | 91.86 | -30.99 | 131.49 | 0.6318 | -704.0 | -573.3 | |
| 0.00 | 1.03 | 0.00 | 0.64 | -19.90 | 91.41 | -31.45 | 125.97 | 0.6084 | -455.0 | -407.8 | |
| 0.00 | 1.28 | 0.00 | 0.80 | -19.33 | 91.49 | -31.36 | 125.22 | 0.6033 | -651.0 | -589.6 | |
| 0.00 | 1.63 | 0.00 | 1.07 | -24.66 | 89.86 | -32.99 | 131.12 | 0.6592 | -651.0 | -520.4 | |
| 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. | |