SDO HMI 2014-02-28 21:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.27 | 72.66 | 11.96 | 37.27 | -6.81 | 149.16 | 14.95 | 270.81 | 0.2578 | 342.8 | 294.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.50 | 44.14 | 6.45 | 22.75 | -7.35 | 150.61 | 16.40 | 268.49 | 0.2814 | 1030.1 | 684.4 | |
| 6.98 | -1.00 | 3.59 | -1.00 | -7.08 | 149.95 | 15.74 | 269.53 | 0.2704 | 1171.0 | 999999 | |
| 0.00 | 1.55 | 0.00 | 0.80 | -6.68 | 149.38 | 15.17 | 271.12 | 0.2611 | 906.0 | 680.3 | |
| 0.00 | 4.31 | 0.00 | 2.21 | -6.51 | 149.09 | 14.88 | 271.84 | 0.2565 | 974.0 | 909.3 | |
| 0.00 | 1.90 | 0.00 | 0.97 | -6.31 | 148.75 | 14.54 | 272.71 | 0.2509 | 1039.0 | 947.2 | |
| 0.00 | 1.12 | 0.00 | 0.57 | -5.88 | 148.28 | 14.06 | 274.63 | 0.2436 | 793.0 | 598.8 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -4.75 | 147.30 | 13.09 | 280.01 | 0.2302 | -678.0 | -525.2 | |
| 0.52 | 1.55 | 0.26 | 0.79 | -4.70 | 146.87 | 12.66 | 280.60 | 0.2233 | -955.5 | -775.1 | |
| 0.00 | 3.02 | 0.00 | 1.53 | -5.53 | 146.86 | 12.65 | 276.90 | 0.2205 | -702.0 | -640.4 | |
| 0.00 | 4.74 | 0.00 | 2.41 | -5.09 | 146.79 | 12.58 | 278.94 | 0.2206 | -717.0 | -810.9 | |
| 2.24 | 3.36 | 1.14 | 1.71 | -5.71 | 146.77 | 12.56 | 276.13 | 0.2186 | -1008.3 | -824.1 | |
| 0.00 | 1.72 | 0.00 | 0.88 | -5.30 | 146.73 | 12.52 | 278.04 | 0.2190 | -1134.0 | -954.0 | |
| 1.03 | 2.24 | 0.52 | 1.13 | -8.56 | 145.65 | 11.44 | 262.47 | 0.1987 | 955.5 | 761.9 | |
| 0.00 | 1.12 | 0.00 | 0.56 | -8.97 | 144.71 | 10.50 | 259.72 | 0.1838 | -820.0 | -556.6 | |
| 0.00 | 0.86 | 0.00 | 0.43 | -8.50 | 144.64 | 10.43 | 262.25 | 0.1815 | -783.0 | -645.5 | |
| 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. | |