SDO HMI 2014-02-28 05:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.95 | 66.50 | 10.43 | 33.11 | -6.57 | 147.92 | 4.92 | 288.28 | 0.0899 | 87.5 | 230.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.55 | 0.00 | 0.78 | -7.27 | 150.56 | 7.57 | 269.09 | 0.1313 | -862.0 | -622.3 | |
| 0.00 | 1.81 | 0.00 | 0.90 | -7.39 | 150.38 | 7.39 | 268.14 | 0.1282 | -932.0 | -666.0 | |
| 3.36 | 8.11 | 1.68 | 4.05 | -7.01 | 149.98 | 6.99 | 271.23 | 0.1214 | 1071.3 | 802.4 | |
| 6.04 | 26.91 | 3.01 | 13.41 | -7.05 | 149.41 | 6.42 | 271.08 | 0.1115 | 1069.6 | 893.6 | |
| 1.29 | -4.00 | 0.64 | -4.00 | -6.75 | 149.29 | 6.29 | 273.82 | 0.1096 | 1034.3 | 999999 | |
| 2.50 | -4.00 | 1.25 | -4.00 | -7.00 | 148.90 | 5.91 | 271.76 | 0.1027 | 1125.1 | 999999 | |
| 0.00 | 0.78 | 0.00 | 0.39 | -7.42 | 148.48 | 5.49 | 267.52 | 0.0954 | 781.0 | 572.7 | |
| 0.95 | 4.31 | 0.47 | 2.15 | -6.29 | 148.38 | 5.39 | 279.48 | 0.0951 | 1109.5 | 736.3 | |
| 0.00 | 1.38 | 0.00 | 0.69 | -8.16 | 148.22 | 5.23 | 259.29 | 0.0922 | 946.0 | 767.4 | |
| 0.00 | 2.93 | 0.00 | 1.46 | -5.11 | 147.86 | 4.87 | 293.25 | 0.0925 | -979.0 | -799.4 | |
| 0.00 | 3.45 | 0.00 | 1.71 | -5.23 | 147.15 | 4.15 | 295.41 | 0.0802 | -801.0 | -771.0 | |
| 0.00 | 0.95 | 0.00 | 0.47 | -6.00 | 146.88 | 3.89 | 287.14 | 0.0709 | 916.0 | 772.9 | |
| 0.00 | 1.21 | 0.00 | 0.60 | -5.92 | 145.42 | 2.42 | 298.02 | 0.0479 | -1003.0 | -892.1 | |
| 0.00 | 0.86 | 0.00 | 0.43 | -6.04 | 145.27 | 2.27 | 297.24 | 0.0446 | -1040.0 | -838.0 | |
| 6.81 | 12.25 | 3.38 | 6.07 | -5.87 | 143.36 | 0.36 | 344.96 | 0.0244 | -1170.9 | -797.3 | |
| 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. | |