SDO HMI 2014-02-28 15:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.77 | 88.54 | 14.05 | 44.74 | -6.57 | 148.74 | 11.22 | 273.24 | 0.1951 | 320.7 | 236.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.59 | 0.00 | 1.32 | -7.87 | 150.79 | 13.27 | 266.20 | 0.2289 | -924.0 | -722.9 | |
| 5.86 | 35.09 | 2.98 | 17.81 | -7.20 | 150.31 | 12.79 | 269.17 | 0.2206 | 1104.8 | 823.9 | |
| 1.38 | -2.00 | 0.70 | -2.00 | -7.09 | 150.09 | 12.57 | 269.71 | 0.2170 | 1203.4 | 999999 | |
| 3.71 | -2.00 | 1.88 | -2.00 | -7.04 | 149.90 | 12.38 | 269.98 | 0.2138 | 1264.4 | 999999 | |
| 2.85 | 25.35 | 1.44 | 12.81 | -6.72 | 149.34 | 11.83 | 271.59 | 0.2045 | 1175.7 | 770.1 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -13.14 | 149.58 | 12.06 | 242.42 | 0.2305 | -663.0 | -488.1 | |
| 9.23 | -5.00 | 4.66 | -5.00 | -6.38 | 148.76 | 11.24 | 273.51 | 0.1950 | 1193.7 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.65 | -4.73 | 147.00 | 9.48 | 284.17 | 0.1701 | -1044.0 | -890.3 | |
| 0.69 | 15.69 | 0.35 | 7.88 | -5.14 | 146.98 | 9.46 | 281.80 | 0.1680 | -967.9 | -931.5 | |
| 1.72 | -9.00 | 0.87 | -9.00 | -5.56 | 146.86 | 9.34 | 279.47 | 0.1646 | -1033.6 | 999999 | |
| 1.21 | -9.00 | 0.61 | -9.00 | -5.29 | 146.86 | 9.34 | 281.07 | 0.1654 | -1265.4 | 999999 | |
| 1.12 | -9.00 | 0.56 | -9.00 | -5.06 | 146.86 | 9.34 | 282.47 | 0.1663 | -1211.6 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.30 | -6.18 | 146.81 | 9.29 | 275.72 | 0.1621 | 792.0 | 637.3 | |
| 0.00 | 2.24 | 0.00 | 1.12 | -6.34 | 146.33 | 8.81 | 275.06 | 0.1536 | 852.0 | 598.4 | |
| 0.00 | 1.90 | 0.00 | 0.95 | -5.89 | 145.15 | 7.63 | 279.37 | 0.1345 | -941.0 | -776.3 | |
| 0.00 | 2.93 | 0.00 | 1.46 | -5.88 | 143.28 | 5.77 | 282.61 | 0.1029 | -1111.0 | -869.2 | |
| 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. | |