SDO HMI 2014-05-30 16:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.70 | 127.27 | 15.60 | 64.63 | -9.06 | 24.79 | 9.31 | 227.45 | 0.2179 | 612.3 | 454.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.45 | 0.00 | 0.23 | -6.89 | 26.91 | 11.43 | 241.82 | 0.2241 | 467.0 | 543.6 | |
| 5.69 | 24.65 | 2.90 | 12.56 | -8.91 | 26.24 | 10.76 | 232.74 | 0.2328 | 1095.8 | 650.7 | |
| 3.34 | -2.00 | 1.70 | -2.00 | -9.22 | 26.19 | 10.71 | 231.55 | 0.2352 | 929.8 | 999999 | |
| 1.99 | 76.74 | 1.01 | 38.99 | -9.31 | 25.69 | 10.21 | 229.91 | 0.2296 | 929.4 | 541.5 | |
| 16.61 | -4.00 | 8.44 | -4.00 | -9.00 | 25.40 | 9.92 | 230.17 | 0.2226 | 1353.3 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.37 | -7.50 | 24.99 | 9.51 | 234.71 | 0.2016 | -754.0 | -547.1 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -7.35 | 24.58 | 9.10 | 234.18 | 0.1944 | 820.0 | 493.2 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -8.85 | 24.18 | 8.70 | 227.03 | 0.2052 | 753.0 | 588.3 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -9.47 | 23.73 | 8.25 | 223.36 | 0.2070 | 938.0 | 819.1 | |
| 0.81 | 3.97 | 0.41 | 2.01 | -9.71 | 23.23 | 7.76 | 220.81 | 0.2045 | 1118.2 | 869.5 | |
| 2.26 | 7.13 | 1.14 | 3.61 | -9.96 | 22.87 | 7.39 | 218.66 | 0.2036 | 1193.8 | 824.1 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -9.13 | 20.71 | 5.23 | 212.04 | 0.1706 | -943.0 | -816.8 | |
| 0.00 | 1.26 | 0.00 | 0.63 | -4.67 | 20.36 | 4.88 | 231.91 | 0.1083 | -780.0 | -675.4 | |
| 0.00 | 1.99 | 0.00 | 1.00 | -8.30 | 20.09 | 4.61 | 211.52 | 0.1527 | -980.0 | -735.8 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -8.52 | 19.93 | 4.46 | 209.96 | 0.1546 | -971.0 | -723.7 | |
| 0.00 | 1.53 | 0.00 | 0.77 | -9.38 | 19.82 | 4.34 | 206.76 | 0.1667 | -902.0 | -679.8 | |
| 0.00 | 2.80 | 0.00 | 1.41 | -10.94 | 13.74 | -1.74 | 170.35 | 0.1784 | -804.0 | -607.8 | |
| 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. | |