SDO HMI 2014-03-15 04:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.47 | 281.78 | 92.22 | 347.23 | 5.25 | 11.23 | 65.33 | 278.97 | 0.9176 | 155.3 | 20.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.30 | 6.52 | 2.12 | 10.53 | 5.03 | 17.21 | 71.31 | 277.66 | 0.9535 | -284.7 | -322.7 | |
| 5.91 | 16.08 | 8.18 | 22.25 | 6.17 | 13.78 | 67.87 | 279.46 | 0.9352 | -373.1 | -161.1 | |
| 17.12 | 242.75 | 21.62 | 294.90 | 3.48 | 12.06 | 66.16 | 276.91 | 0.9213 | -423.5 | 30.2 | |
| 4.00 | -3.00 | 4.96 | -3.00 | 5.10 | 11.38 | 65.48 | 278.77 | 0.9186 | 171.0 | 999999 | |
| 0.00 | 1.83 | 0.00 | 2.33 | 6.73 | 11.76 | 65.86 | 280.44 | 0.9232 | -200.0 | -167.5 | |
| 0.00 | 1.30 | 0.00 | 1.66 | 6.45 | 11.69 | 65.79 | 280.15 | 0.9223 | -56.0 | -81.7 | |
| 19.99 | -3.00 | 24.37 | -3.00 | 6.03 | 10.71 | 64.81 | 279.90 | 0.9153 | 442.0 | 999999 | |
| 0.00 | 1.22 | 0.00 | 1.50 | 6.87 | 10.85 | 64.95 | 280.77 | 0.9173 | -153.0 | -141.7 | |
| 1.30 | -3.00 | 1.56 | -3.00 | 5.14 | 10.38 | 64.48 | 279.01 | 0.9118 | 260.8 | 999999 | |
| 1.56 | -3.00 | 1.85 | -3.00 | 4.54 | 10.21 | 64.30 | 278.39 | 0.9098 | -338.7 | 999999 | |
| 2.17 | -3.00 | 2.59 | -3.00 | 5.46 | 10.24 | 64.34 | 279.38 | 0.9112 | 595.6 | 999999 | |
| 5.30 | -3.00 | 6.21 | -3.00 | 4.63 | 9.94 | 64.04 | 278.54 | 0.9080 | 439.1 | 999999 | |
| 0.00 | 1.56 | 0.00 | 1.90 | 7.21 | 10.37 | 64.47 | 281.24 | 0.9145 | -176.0 | -175.5 | |
| 13.47 | -3.00 | 16.03 | -3.00 | 6.34 | 10.02 | 64.11 | 280.38 | 0.9108 | 676.1 | 999999 | |
| 2.35 | 10.52 | 2.73 | 12.16 | 4.97 | 9.73 | 63.83 | 278.96 | 0.9069 | 671.1 | 511.3 | |
| 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. | |