SDO HMI 2014-04-08 16:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.06 | 21.66 | 0.60 | 12.05 | -8.43 | 10.03 | 27.24 | 263.41 | 0.4575 | 203.2 | 281.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.45 | -5.70 | 12.72 | 29.93 | 269.15 | 0.4985 | 609.0 | 461.0 | |
| 0.00 | 1.32 | 0.00 | 0.75 | -10.80 | 11.95 | 29.15 | 258.73 | 0.4899 | -677.0 | -588.9 | |
| 0.00 | 2.82 | 0.00 | 1.59 | -8.76 | 11.72 | 28.92 | 262.88 | 0.4837 | 726.0 | 638.3 | |
| 1.06 | 4.23 | 0.60 | 2.38 | -8.26 | 11.47 | 28.68 | 263.89 | 0.4795 | 983.4 | 756.4 | |
| 0.00 | 2.20 | 0.00 | 1.24 | -8.56 | 11.39 | 28.60 | 263.25 | 0.4786 | 801.0 | 710.9 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -8.94 | 11.01 | 28.21 | 262.40 | 0.4731 | 729.0 | 664.1 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -8.77 | 10.92 | 28.13 | 262.76 | 0.4716 | 820.0 | 646.6 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -7.88 | 9.93 | 27.14 | 264.58 | 0.4557 | 785.0 | 555.8 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -8.02 | 9.57 | 26.77 | 264.24 | 0.4502 | 882.0 | 764.4 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -10.43 | 9.42 | 26.63 | 258.85 | 0.4511 | 808.0 | 618.7 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -7.58 | 6.52 | 23.73 | 264.99 | 0.4021 | -833.0 | -635.6 | |
| 0.00 | 1.94 | 0.00 | 1.04 | -7.66 | 6.13 | 23.33 | 264.76 | 0.3959 | -900.0 | -736.2 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -7.81 | 5.38 | 22.59 | 264.28 | 0.3841 | -876.0 | -687.3 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -7.16 | 5.08 | 22.29 | 265.96 | 0.3789 | -701.0 | -541.3 | |
| 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. | |