SDO HMI 2011-07-03 10:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.88 | 223.95 | 21.34 | 114.20 | 16.37 | 353.73 | -0.39 | 1.44 | 0.2347 | -285.0 | -201.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.91 | 0.00 | 1.01 | 23.42 | 359.01 | 4.89 | 347.31 | 0.3577 | 942.0 | 794.6 | |
| 0.00 | 2.09 | 0.00 | 1.07 | 16.66 | 358.64 | 4.53 | 342.15 | 0.2476 | -886.0 | -734.1 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 19.85 | 358.66 | 4.54 | 345.51 | 0.2992 | -630.0 | -396.7 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 19.60 | 357.58 | 3.47 | 348.66 | 0.2911 | -907.0 | -752.0 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 14.82 | 356.20 | 2.08 | 350.19 | 0.2072 | -871.0 | -602.6 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 17.70 | 355.98 | 1.86 | 353.01 | 0.2552 | -800.0 | -654.3 | |
| 9.81 | 154.27 | 4.99 | 78.52 | 15.88 | 355.42 | 1.30 | 354.36 | 0.2234 | -1087.5 | -448.6 | |
| 14.90 | -7.00 | 7.58 | -7.00 | 16.20 | 354.95 | 0.83 | 356.49 | 0.2281 | -1330.3 | 999999 | |
| 12.99 | -7.00 | 6.62 | -7.00 | 16.48 | 354.41 | 0.29 | 358.80 | 0.2326 | -1159.1 | 999999 | |
| 0.00 | 4.27 | 0.00 | 2.17 | 15.51 | 353.99 | -0.12 | 0.55 | 0.2160 | -1084.0 | -847.6 | |
| 0.00 | 1.82 | 0.00 | 0.92 | 13.83 | 353.93 | -0.18 | 0.96 | 0.1871 | -825.0 | -594.0 | |
| 0.00 | 2.09 | 0.00 | 1.06 | 15.73 | 353.90 | -0.22 | 0.96 | 0.2197 | -747.0 | -628.8 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 16.13 | 353.77 | -0.35 | 1.47 | 0.2267 | -664.0 | -455.2 | |
| 0.00 | 3.45 | 0.00 | 1.80 | 20.98 | 353.60 | -0.52 | 1.58 | 0.3085 | -572.0 | -534.5 | |
| 0.00 | 2.36 | 0.00 | 1.19 | 13.36 | 353.43 | -0.69 | 3.74 | 0.1795 | -947.0 | -696.3 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 15.67 | 353.36 | -0.76 | 3.34 | 0.2190 | -688.0 | -530.4 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 17.39 | 352.65 | -1.47 | 5.65 | 0.2492 | -1003.0 | -794.2 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 15.69 | 350.67 | -3.45 | 14.87 | 0.2267 | 911.0 | 710.6 | |
| 0.00 | 0.64 | 0.00 | 0.33 | 19.50 | 350.53 | -3.59 | 11.79 | 0.2899 | -752.0 | -526.1 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 15.44 | 350.01 | -4.11 | 17.90 | 0.2258 | 901.0 | 735.3 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 15.31 | 349.82 | -4.30 | 18.84 | 0.2248 | 942.0 | 712.6 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 15.41 | 349.56 | -4.55 | 19.73 | 0.2277 | 1065.0 | 740.4 | |
| 0.00 | 2.27 | 0.00 | 1.15 | 15.00 | 349.51 | -4.61 | 20.60 | 0.2216 | 958.0 | 730.6 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 15.72 | 349.43 | -4.69 | 19.78 | 0.2335 | 965.0 | 768.1 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 15.28 | 349.38 | -4.74 | 20.67 | 0.2268 | 976.0 | 789.3 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 15.44 | 349.25 | -4.87 | 20.94 | 0.2301 | 1119.0 | 861.6 | |
| 0.00 | 1.64 | 0.00 | 0.83 | 15.87 | 349.01 | -5.10 | 21.14 | 0.2384 | 1153.0 | 893.3 | |
| 0.00 | 11.99 | 0.00 | 6.14 | 16.62 | 348.93 | -5.19 | 20.31 | 0.2508 | 1062.0 | 901.2 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 15.93 | 348.63 | -5.49 | 22.46 | 0.2418 | 864.0 | 705.1 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 16.97 | 348.50 | -5.61 | 21.30 | 0.2587 | 947.0 | 712.2 | |
| 0.00 | 2.27 | 0.00 | 1.17 | 17.00 | 348.25 | -5.87 | 22.13 | 0.2608 | 864.0 | 694.6 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 17.02 | 347.57 | -6.54 | 24.33 | 0.2657 | 1071.0 | 965.5 | |
| 1.18 | 2.18 | 0.61 | 1.12 | 16.84 | 347.55 | -6.57 | 24.72 | 0.2630 | 962.5 | 992.2 | |
| 0.00 | 1.64 | 0.00 | 0.84 | 17.21 | 347.50 | -6.62 | 24.25 | 0.2691 | 979.0 | 801.5 | |
| 3.00 | 3.27 | 1.54 | 1.68 | 16.46 | 347.43 | -6.68 | 25.75 | 0.2581 | 935.5 | 777.3 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 18.03 | 346.83 | -7.29 | 25.06 | 0.2862 | 713.0 | 641.5 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 17.62 | 346.78 | -7.34 | 25.86 | 0.2803 | 897.0 | 756.8 | |
| 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. | |