SDO HMI 2014-03-15 15:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.56 | 17.36 | 3.50 | 16.09 | -10.34 | 358.04 | 58.17 | 262.10 | 0.8443 | 173.8 | 185.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.13 | 0.00 | 1.16 | -7.41 | 1.46 | 61.58 | 265.47 | 0.8769 | 372.0 | 342.5 | |
| 0.00 | 0.43 | 0.00 | 0.44 | -6.67 | 1.04 | 61.16 | 266.34 | 0.8738 | 233.0 | 249.0 | |
| 0.00 | 1.39 | 0.00 | 1.41 | -7.06 | 1.06 | 61.18 | 265.90 | 0.8738 | 464.0 | 433.6 | |
| 0.00 | 0.35 | 0.00 | 0.35 | -7.44 | 1.15 | 61.27 | 265.45 | 0.8743 | 441.0 | 395.2 | |
| 0.00 | 0.43 | 0.00 | 0.43 | -7.21 | 0.78 | 60.90 | 265.75 | 0.8713 | 558.0 | 471.6 | |
| 0.00 | 1.04 | 0.00 | 1.04 | -6.89 | 0.71 | 60.83 | 266.12 | 0.8709 | 493.0 | 485.5 | |
| 3.56 | 6.08 | 3.50 | 5.96 | -9.68 | 0.25 | 60.37 | 262.94 | 0.8655 | 556.7 | 502.2 | |
| 0.00 | 1.04 | 0.00 | 0.95 | -15.30 | 357.65 | 57.78 | 256.37 | 0.8418 | 589.0 | 541.1 | |
| 0.00 | 0.78 | 0.00 | 0.68 | -11.29 | 356.08 | 56.21 | 261.18 | 0.8269 | 319.0 | 331.6 | |
| 0.00 | 0.52 | 0.00 | 0.41 | -11.13 | 351.87 | 51.99 | 261.44 | 0.7841 | -476.0 | -437.8 | |
| 0.00 | 0.96 | 0.00 | 0.76 | -10.87 | 351.75 | 51.88 | 261.77 | 0.7829 | -664.0 | -551.2 | |
| 0.00 | 1.56 | 0.00 | 1.26 | -16.82 | 352.23 | 52.35 | 254.21 | 0.7899 | -561.0 | -417.8 | |
| 0.00 | 0.78 | 0.00 | 0.62 | -17.26 | 351.79 | 51.91 | 253.61 | 0.7857 | -252.0 | -244.9 | |
| 0.00 | 0.87 | 0.00 | 0.62 | -12.01 | 345.96 | 46.08 | 260.18 | 0.7174 | -597.0 | -532.9 | |
| 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. | |