SDO HMI 2014-04-07 14:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.04 | 406.42 | 40.46 | 222.17 | 12.82 | 13.40 | 16.31 | 319.51 | 0.4238 | -986.6 | -390.4 | |
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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 | 0.88 | 14.11 | 15.10 | 18.00 | 318.70 | 0.4561 | 623.0 | 483.4 | |
| 0.00 | 1.67 | 0.00 | 0.92 | 14.23 | 13.81 | 16.72 | 320.96 | 0.4445 | -615.0 | -403.8 | |
| 69.72 | 383.73 | 38.09 | 209.75 | 12.72 | 13.47 | 16.38 | 319.24 | 0.4232 | -1445.9 | -436.8 | |
| 0.00 | 3.43 | 0.00 | 1.85 | 10.57 | 13.12 | 16.03 | 316.26 | 0.3942 | 838.0 | 704.8 | |
| 0.00 | 2.55 | 0.00 | 1.41 | 14.63 | 13.29 | 16.20 | 322.41 | 0.4444 | 693.0 | 498.6 | |
| 2.91 | -3.00 | 1.60 | -3.00 | 14.11 | 13.22 | 16.13 | 321.80 | 0.4374 | -828.9 | 999999 | |
| 0.00 | 1.94 | 0.00 | 1.07 | 14.62 | 12.90 | 15.81 | 323.06 | 0.4406 | 518.0 | 402.9 | |
| 0.00 | 0.44 | 0.00 | 0.24 | 14.97 | 12.74 | 15.64 | 323.84 | 0.4433 | 628.0 | 530.6 | |
| 0.00 | 1.23 | 0.00 | 0.68 | 14.80 | 12.69 | 15.60 | 323.69 | 0.4409 | 751.0 | 603.1 | |
| 0.00 | 1.85 | 0.00 | 1.02 | 14.93 | 12.54 | 15.45 | 324.13 | 0.4411 | 900.0 | 784.6 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 12.56 | 12.31 | 15.22 | 321.06 | 0.4095 | -912.0 | -794.3 | |
| 1.41 | 3.52 | 0.77 | 1.93 | 14.67 | 11.21 | 14.11 | 326.19 | 0.4257 | -970.3 | -736.8 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 11.91 | 10.50 | 13.41 | 323.55 | 0.3836 | 617.0 | 530.9 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 10.70 | 9.72 | 12.63 | 323.22 | 0.3603 | 709.0 | 560.4 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 14.59 | 9.35 | 12.26 | 329.71 | 0.4091 | 640.0 | 461.5 | |
| 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. | |