SDO HMI 2011-01-04 02:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 92.84 | 302.08 | 47.14 | 153.33 | -14.13 | 208.01 | -6.19 | 151.66 | 0.2192 | -131.3 | -18.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.10 | 0.00 | 0.56 | -15.42 | 211.39 | -2.81 | 167.29 | 0.2155 | 649.0 | 639.2 | |
| 9.51 | 63.63 | 4.81 | 32.16 | -14.49 | 211.10 | -3.10 | 164.85 | 0.2012 | 1268.9 | 580.0 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -15.93 | 211.08 | -3.12 | 166.50 | 0.2252 | 823.0 | 694.7 | |
| 25.66 | 53.10 | 12.96 | 26.83 | -13.88 | 210.07 | -4.12 | 159.12 | 0.1968 | 1157.9 | 717.2 | |
| 0.00 | 1.10 | 0.00 | 0.56 | -15.24 | 209.96 | -4.24 | 160.91 | 0.2192 | 1009.0 | 752.6 | |
| 1.95 | -4.00 | 0.99 | -4.00 | -14.21 | 209.76 | -4.44 | 158.33 | 0.2040 | 1028.7 | 999999 | |
| 1.44 | 26.08 | 0.73 | 13.22 | -14.60 | 209.69 | -4.50 | 158.75 | 0.2106 | 1035.6 | 486.9 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -13.49 | 209.44 | -4.76 | 155.43 | 0.1948 | 919.0 | 727.1 | |
| 6.46 | -7.00 | 3.27 | -7.00 | -14.75 | 209.23 | -4.97 | 157.08 | 0.2159 | 943.6 | 999999 | |
| 0.00 | 1.61 | 0.00 | 0.81 | -13.40 | 209.23 | -4.97 | 154.28 | 0.1949 | 961.0 | 796.7 | |
| 0.00 | 3.14 | 0.00 | 1.60 | -14.84 | 208.53 | -5.67 | 154.41 | 0.2222 | -1041.0 | -842.4 | |
| 0.34 | 3.06 | 0.17 | 1.55 | -12.83 | 207.94 | -6.26 | 147.21 | 0.1972 | 1053.0 | 846.2 | |
| 0.00 | 1.70 | 0.00 | 0.86 | -14.83 | 207.55 | -6.65 | 150.69 | 0.2298 | -1072.0 | -854.0 | |
| 3.91 | 41.63 | 1.99 | 21.16 | -14.47 | 207.28 | -6.92 | 148.90 | 0.2268 | -1198.2 | -665.1 | |
| 9.34 | -14.00 | 4.75 | -14.00 | -14.38 | 207.01 | -7.19 | 147.70 | 0.2279 | -1201.1 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -14.89 | 206.90 | -7.30 | 148.52 | 0.2362 | -715.0 | -466.1 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -14.77 | 206.66 | -7.54 | 147.40 | 0.2367 | -848.0 | -671.0 | |
| 0.00 | 2.80 | 0.00 | 1.43 | -14.04 | 206.22 | -7.98 | 144.12 | 0.2308 | -778.0 | -747.3 | |
| 0.00 | 4.08 | 0.00 | 2.07 | -13.26 | 205.85 | -8.35 | 140.72 | 0.2242 | -1050.0 | -912.4 | |
| 11.55 | 20.13 | 5.89 | 10.26 | -14.07 | 205.70 | -8.50 | 142.47 | 0.2364 | -1153.1 | -917.2 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -12.39 | 205.73 | -8.47 | 137.65 | 0.2146 | -900.0 | -752.3 | |
| 0.00 | 0.76 | 0.00 | 0.39 | -12.12 | 205.74 | -8.46 | 136.80 | 0.2111 | -976.0 | -731.0 | |
| 0.00 | 2.38 | 0.00 | 1.22 | -14.51 | 205.31 | -8.89 | 142.43 | 0.2463 | -867.0 | -656.7 | |
| 3.31 | 44.52 | 1.69 | 22.68 | -13.34 | 205.24 | -8.96 | 138.99 | 0.2321 | -1219.6 | -511.3 | |
| 0.00 | 2.38 | 0.00 | 1.21 | -14.09 | 204.96 | -9.24 | 140.24 | 0.2446 | -889.0 | -753.1 | |
| 6.63 | -24.00 | 3.38 | -24.00 | -13.46 | 204.86 | -9.34 | 138.19 | 0.2377 | -1178.2 | 999999 | |
| 1.36 | 12.15 | 0.69 | 6.21 | -14.06 | 204.65 | -9.54 | 139.25 | 0.2475 | -974.8 | -732.3 | |
| 5.52 | -24.00 | 2.82 | -24.00 | -13.46 | 204.52 | -9.67 | 137.18 | 0.2415 | -948.8 | 999999 | |
| 0.00 | 1.61 | 0.00 | 0.83 | -14.60 | 204.44 | -9.75 | 140.08 | 0.2566 | -832.0 | -731.7 | |
| 5.86 | -27.00 | 3.00 | -27.00 | -14.03 | 204.38 | -9.82 | 138.36 | 0.2502 | -1005.4 | 999999 | |
| 0.00 | 4.84 | 0.00 | 2.48 | -14.56 | 203.95 | -10.25 | 138.62 | 0.2616 | -639.0 | -655.5 | |
| 0.00 | 1.87 | 0.00 | 0.96 | -13.99 | 203.92 | -10.28 | 136.98 | 0.2550 | -920.0 | -641.7 | |
| 0.00 | 1.27 | 0.00 | 0.65 | -13.57 | 203.72 | -10.48 | 135.26 | 0.2523 | -790.0 | -575.5 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -12.04 | 203.54 | -10.66 | 130.07 | 0.2375 | -907.0 | -640.5 | |
| 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. | |