SDO HMI 2014-10-06 09:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.49 | 0.00 | 14.33 | 13.74 | 60.64 | -53.17 | 77.59 | 0.7979 | -230.3 | -206.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.58 | 0.00 | 1.16 | 14.77 | 66.34 | -47.47 | 75.82 | 0.7373 | -456.0 | -389.3 | |
| 0.00 | 1.23 | 0.00 | 0.96 | 14.02 | 62.85 | -50.97 | 77.12 | 0.7753 | -619.0 | -470.4 | |
| 0.00 | 1.58 | 0.00 | 1.24 | 14.05 | 62.45 | -51.37 | 77.12 | 0.7797 | -553.0 | -392.8 | |
| 0.00 | 0.88 | 0.00 | 0.72 | 16.73 | 61.04 | -52.77 | 73.84 | 0.7962 | -381.0 | -237.8 | |
| 0.00 | 1.49 | 0.00 | 1.22 | 15.13 | 60.71 | -53.11 | 75.87 | 0.7984 | -262.0 | -323.3 | |
| 0.00 | 1.49 | 0.00 | 1.21 | 11.94 | 61.00 | -52.81 | 79.87 | 0.7940 | -482.0 | -361.8 | |
| 0.00 | 1.32 | 0.00 | 1.09 | 13.22 | 60.21 | -53.60 | 78.29 | 0.8025 | -518.0 | -401.3 | |
| 0.00 | 0.97 | 0.00 | 0.80 | 13.61 | 59.87 | -53.94 | 77.81 | 0.8061 | -330.0 | -313.8 | |
| 0.00 | 2.20 | 0.00 | 1.84 | 13.11 | 59.67 | -54.15 | 78.45 | 0.8079 | -371.0 | -287.2 | |
| 0.00 | 1.05 | 0.00 | 0.89 | 13.30 | 59.45 | -54.37 | 78.22 | 0.8102 | -158.0 | -115.9 | |
| 0.00 | 0.97 | 0.00 | 0.84 | 14.32 | 58.22 | -55.59 | 77.01 | 0.8226 | -550.0 | -433.1 | |
| 0.00 | 1.76 | 0.00 | 1.51 | 12.85 | 58.52 | -55.30 | 78.80 | 0.8193 | 609.0 | 502.4 | |
| 0.00 | 0.62 | 0.00 | 0.53 | 12.94 | 58.16 | -55.65 | 78.70 | 0.8228 | 469.0 | 402.3 | |
| 0.00 | 0.35 | 0.00 | 0.32 | 13.61 | 56.75 | -57.07 | 77.93 | 0.8363 | 378.0 | 464.8 | |
| 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. | |