SDO HMI 2011-01-04 20:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.62 | 182.30 | 21.59 | 92.29 | -14.28 | 208.58 | 4.25 | 199.76 | 0.2078 | -7.9 | -64.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.01 | 51.88 | 2.55 | 26.38 | -14.65 | 211.35 | 7.02 | 211.21 | 0.2294 | 1074.7 | 509.4 | |
| 1.10 | -1.00 | 0.56 | -1.00 | -14.35 | 211.25 | 6.92 | 211.56 | 0.2242 | 1146.9 | 999999 | |
| 1.10 | -1.00 | 0.56 | -1.00 | -14.17 | 211.18 | 6.86 | 211.75 | 0.2210 | 1100.3 | 999999 | |
| 0.00 | 1.78 | 0.00 | 0.91 | -16.55 | 211.20 | 6.87 | 206.74 | 0.2561 | 727.0 | 615.1 | |
| 0.76 | 1.95 | 0.39 | 0.99 | -15.07 | 211.00 | 6.67 | 208.98 | 0.2325 | 955.3 | 732.7 | |
| 12.74 | 32.18 | 6.46 | 16.31 | -13.90 | 210.87 | 6.54 | 211.23 | 0.2143 | 1134.3 | 800.9 | |
| 5.52 | -6.00 | 2.80 | -6.00 | -13.82 | 210.56 | 6.23 | 210.24 | 0.2104 | 1212.2 | 999999 | |
| 0.00 | 2.12 | 0.00 | 1.08 | -15.68 | 210.49 | 6.17 | 205.92 | 0.2377 | 851.0 | 702.6 | |
| 2.21 | -6.00 | 1.12 | -6.00 | -14.06 | 210.38 | 6.06 | 208.96 | 0.2124 | 946.2 | 999999 | |
| 0.00 | 2.72 | 0.00 | 1.38 | -15.38 | 210.42 | 6.10 | 206.25 | 0.2326 | 963.0 | 748.7 | |
| 0.00 | 2.04 | 0.00 | 1.04 | -14.99 | 210.32 | 5.99 | 206.65 | 0.2259 | 905.0 | 730.0 | |
| 0.00 | 1.61 | 0.00 | 0.82 | -14.33 | 209.87 | 5.55 | 206.28 | 0.2125 | 835.0 | 738.7 | |
| 0.00 | 2.38 | 0.00 | 1.20 | -13.10 | 209.81 | 5.49 | 208.92 | 0.1935 | 1050.0 | 838.1 | |
| 1.78 | 4.59 | 0.90 | 2.33 | -14.63 | 209.79 | 5.46 | 205.31 | 0.2164 | 1000.6 | 820.4 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -14.43 | 208.29 | 3.96 | 199.29 | 0.2035 | -935.0 | -745.2 | |
| 0.00 | 1.53 | 0.00 | 0.77 | -14.85 | 207.50 | 3.18 | 195.10 | 0.2064 | -883.0 | -714.4 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -14.67 | 207.25 | 2.93 | 194.20 | 0.2024 | -711.0 | -575.1 | |
| 0.00 | 0.93 | 0.00 | 0.47 | -15.06 | 207.08 | 2.75 | 192.92 | 0.2082 | -819.0 | -615.9 | |
| 4.33 | 13.67 | 2.19 | 6.90 | -14.52 | 206.76 | 2.44 | 192.07 | 0.1980 | -1103.5 | -882.6 | |
| 0.00 | 3.14 | 0.00 | 1.58 | -13.62 | 206.76 | 2.43 | 193.08 | 0.1829 | -918.0 | -782.1 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -14.13 | 206.33 | 2.01 | 190.36 | 0.1900 | -989.0 | -740.2 | |
| 0.00 | 1.27 | 0.00 | 0.64 | -12.58 | 206.08 | 1.75 | 190.63 | 0.1628 | -1013.0 | -681.9 | |
| 0.00 | 2.38 | 0.00 | 1.20 | -14.22 | 205.88 | 1.55 | 187.98 | 0.1903 | -1293.0 | -1075.8 | |
| 0.00 | 1.78 | 0.00 | 0.90 | -14.40 | 205.58 | 1.25 | 186.33 | 0.1927 | -715.0 | -632.3 | |
| 0.00 | 0.76 | 0.00 | 0.38 | -13.09 | 205.54 | 1.21 | 187.00 | 0.1701 | -913.0 | -687.0 | |
| 0.00 | 0.93 | 0.00 | 0.47 | -13.69 | 205.51 | 1.19 | 186.44 | 0.1803 | -941.0 | -768.8 | |
| 0.00 | 1.02 | 0.00 | 0.51 | -14.25 | 205.52 | 1.19 | 186.11 | 0.1900 | -1053.0 | -755.1 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -13.24 | 205.30 | 0.97 | 185.53 | 0.1722 | -1139.0 | -852.8 | |
| 0.51 | 1.70 | 0.26 | 0.86 | -14.38 | 205.27 | 0.95 | 184.81 | 0.1917 | -1115.8 | -1012.7 | |
| 1.36 | 7.30 | 0.68 | 3.68 | -13.66 | 205.27 | 0.94 | 185.14 | 0.1794 | -1087.7 | -990.4 | |
| 0.00 | 3.91 | 0.00 | 1.97 | -14.68 | 205.03 | 0.70 | 183.49 | 0.1966 | -852.0 | -739.1 | |
| 0.00 | 14.27 | 0.00 | 7.20 | -14.41 | 204.82 | 0.49 | 182.49 | 0.1917 | -552.0 | -808.7 | |
| 3.99 | 13.93 | 2.01 | 7.00 | -13.39 | 204.69 | 0.37 | 182.06 | 0.1741 | -1131.6 | -613.4 | |
| 0.00 | 4.25 | 0.00 | 2.14 | -14.17 | 204.48 | 0.16 | 180.81 | 0.1874 | -1174.0 | -972.2 | |
| 2.21 | -33.00 | 1.11 | -33.00 | -13.60 | 204.42 | 0.10 | 180.52 | 0.1776 | -961.4 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -16.15 | 202.18 | -2.14 | 170.75 | 0.2244 | -904.0 | -733.5 | |
| 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. | |