SDO HMI 2014-03-01 18:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.77 | 0.00 | 13.58 | 7.17 | 135.73 | 13.03 | 318.86 | 0.3395 | 136.3 | 239.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.98 | 0.00 | 1.07 | 4.92 | 143.00 | 20.31 | 300.35 | 0.4024 | -780.0 | -699.6 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 6.76 | 142.56 | 19.87 | 304.74 | 0.4125 | -656.0 | -492.9 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 5.33 | 141.34 | 18.64 | 303.51 | 0.3834 | -897.0 | -752.4 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 6.98 | 141.34 | 18.64 | 306.96 | 0.3988 | -773.0 | -586.9 | |
| 0.00 | 1.47 | 0.00 | 0.79 | 8.26 | 141.02 | 18.32 | 309.94 | 0.4076 | -751.0 | -661.6 | |
| 0.00 | 2.24 | 0.00 | 1.19 | 4.45 | 140.59 | 17.90 | 302.65 | 0.3654 | -263.0 | -404.0 | |
| 0.00 | 2.07 | 0.00 | 1.09 | 7.57 | 136.12 | 13.43 | 317.56 | 0.3427 | 797.0 | 594.7 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 8.50 | 135.48 | 12.78 | 320.75 | 0.3475 | -615.0 | -583.2 | |
| 0.00 | 0.95 | 0.00 | 0.50 | 6.96 | 135.31 | 12.61 | 318.15 | 0.3263 | 841.0 | 708.0 | |
| 0.00 | 5.17 | 0.00 | 2.70 | 7.44 | 133.73 | 11.04 | 322.88 | 0.3159 | 872.0 | 725.8 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 7.59 | 133.37 | 10.67 | 324.08 | 0.3143 | 940.0 | 755.7 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 8.17 | 133.26 | 10.57 | 325.41 | 0.3212 | 810.0 | 587.6 | |
| 0.00 | 2.07 | 0.00 | 1.07 | 8.18 | 130.80 | 8.11 | 332.17 | 0.3003 | 836.0 | 722.7 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 7.87 | 130.37 | 7.67 | 332.96 | 0.2923 | 766.0 | 436.7 | |
| 0.00 | 3.28 | 0.00 | 1.70 | 8.24 | 130.32 | 7.62 | 333.68 | 0.2974 | 917.0 | 811.6 | |
| 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. | |