SDO HMI 2014-04-10 12:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.53 | 34.92 | 13.06 | 45.13 | -8.13 | 26.59 | 68.00 | 263.60 | 0.9230 | 239.8 | 279.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.15 | 11.82 | 5.80 | 16.41 | -7.17 | 28.39 | 69.80 | 264.56 | 0.9369 | 501.7 | 486.1 | |
| 3.09 | 5.38 | 4.23 | 7.38 | -8.58 | 28.03 | 69.44 | 263.08 | 0.9342 | 234.8 | 197.4 | |
| 0.00 | 0.79 | 0.00 | 1.07 | -7.74 | 27.54 | 68.95 | 264.01 | 0.9314 | 494.0 | 468.7 | |
| 0.00 | 1.76 | 0.00 | 2.34 | -7.74 | 27.20 | 68.61 | 264.03 | 0.9293 | 221.0 | 243.6 | |
| 0.00 | 3.88 | 0.00 | 5.20 | -8.72 | 27.48 | 68.89 | 262.96 | 0.9307 | 556.0 | 514.4 | |
| 2.29 | 3.97 | 3.03 | 5.24 | -8.27 | 27.14 | 68.54 | 263.47 | 0.9287 | 514.6 | 357.8 | |
| 0.00 | 0.71 | 0.00 | 0.92 | -7.06 | 26.73 | 68.13 | 264.79 | 0.9265 | -106.0 | -66.0 | |
| 0.00 | 0.53 | 0.00 | 0.69 | -8.05 | 26.89 | 68.30 | 263.72 | 0.9271 | 618.0 | 610.7 | |
| 0.00 | 0.26 | 0.00 | 0.35 | -9.75 | 27.23 | 68.64 | 261.86 | 0.9288 | 421.0 | 354.0 | |
| 0.00 | 1.41 | 0.00 | 1.73 | -8.31 | 25.38 | 66.78 | 263.52 | 0.9169 | -193.0 | -160.4 | |
| 0.00 | 0.26 | 0.00 | 0.33 | -9.40 | 25.46 | 66.86 | 262.32 | 0.9171 | -125.0 | -77.3 | |
| 0.00 | 1.06 | 0.00 | 0.90 | -10.49 | 13.24 | 54.65 | 261.35 | 0.8134 | -431.0 | -393.6 | |
| 0.00 | 1.94 | 0.00 | 1.64 | -10.65 | 13.13 | 54.53 | 261.15 | 0.8123 | -555.0 | -447.0 | |
| 0.00 | 1.15 | 0.00 | 0.93 | -11.68 | 11.32 | 52.73 | 259.83 | 0.7940 | -594.0 | -486.4 | |
| 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. | |