SDO HMI 2012-01-03 22:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.57 | 237.12 | 22.69 | 135.48 | -24.46 | 100.59 | 21.76 | 222.68 | 0.5000 | 436.5 | 326.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.93 | 0.00 | 0.55 | -17.58 | 109.62 | 30.79 | 242.45 | 0.5526 | -741.0 | -573.5 | |
| 0.00 | 1.19 | 0.00 | 0.69 | -15.61 | 108.45 | 29.63 | 245.14 | 0.5269 | -837.0 | -708.2 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -17.85 | 108.48 | 29.66 | 241.22 | 0.5395 | -574.0 | -522.9 | |
| 0.00 | 1.36 | 0.00 | 0.84 | -25.56 | 109.51 | 30.68 | 229.99 | 0.6032 | 768.0 | 720.8 | |
| 0.00 | 1.19 | 0.00 | 0.70 | -22.60 | 106.76 | 27.93 | 232.08 | 0.5503 | 610.0 | 484.4 | |
| 1.10 | 2.21 | 0.66 | 1.31 | -23.61 | 106.41 | 27.58 | 230.21 | 0.5543 | 799.7 | 665.2 | |
| 0.00 | 1.95 | 0.00 | 1.16 | -23.77 | 106.37 | 27.54 | 229.93 | 0.5551 | 692.0 | 609.5 | |
| 0.00 | 1.95 | 0.00 | 1.16 | -24.00 | 106.24 | 27.41 | 229.48 | 0.5555 | 750.0 | 567.0 | |
| 0.00 | 1.70 | 0.00 | 1.00 | -22.85 | 105.48 | 26.65 | 230.52 | 0.5377 | 728.0 | 560.1 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -22.38 | 105.35 | 26.52 | 231.13 | 0.5324 | 867.0 | 753.2 | |
| 0.00 | 0.93 | 0.00 | 0.55 | -24.11 | 105.65 | 26.82 | 228.76 | 0.5499 | 630.0 | 418.5 | |
| 0.00 | 0.68 | 0.00 | 0.40 | -22.92 | 105.31 | 26.49 | 230.26 | 0.5363 | 723.0 | 714.9 | |
| 0.00 | 1.53 | 0.00 | 0.89 | -23.08 | 105.03 | 26.20 | 229.73 | 0.5344 | 847.0 | 661.6 | |
| 0.00 | 0.76 | 0.00 | 0.44 | -20.85 | 104.20 | 25.38 | 232.53 | 0.5067 | -679.0 | -517.6 | |
| 0.00 | 0.93 | 0.00 | 0.53 | -20.08 | 103.03 | 24.20 | 232.67 | 0.4862 | -715.0 | -571.1 | |
| 0.00 | 0.93 | 0.00 | 0.57 | -28.88 | 104.10 | 25.27 | 220.56 | 0.5771 | 703.0 | 594.5 | |
| 0.00 | 1.44 | 0.00 | 0.80 | -18.05 | 101.57 | 22.74 | 234.81 | 0.4516 | -719.0 | -556.0 | |
| 0.00 | 0.85 | 0.00 | 0.49 | -25.33 | 102.22 | 23.39 | 223.39 | 0.5244 | -620.0 | -393.2 | |
| 5.52 | 7.64 | 3.28 | 4.54 | -28.13 | 102.55 | 23.72 | 219.90 | 0.5553 | 773.0 | 566.8 | |
| 0.00 | 1.19 | 0.00 | 0.65 | -17.72 | 100.12 | 21.29 | 233.82 | 0.4303 | -692.0 | -530.6 | |
| 0.00 | 3.06 | 0.00 | 1.73 | -22.89 | 100.85 | 22.02 | 225.50 | 0.4863 | -832.0 | -725.9 | |
| 0.00 | 1.02 | 0.00 | 0.56 | -18.24 | 100.15 | 21.32 | 232.85 | 0.4352 | -688.0 | -477.4 | |
| 0.00 | 2.04 | 0.00 | 1.18 | -26.06 | 101.12 | 22.29 | 221.09 | 0.5207 | 971.0 | 718.0 | |
| 0.00 | 0.76 | 0.00 | 0.46 | -29.55 | 101.82 | 22.99 | 217.28 | 0.5633 | -715.0 | -534.6 | |
| 0.00 | 1.02 | 0.00 | 0.59 | -26.77 | 100.77 | 21.94 | 219.68 | 0.5247 | 783.0 | 625.8 | |
| 0.00 | 1.61 | 0.00 | 0.97 | -30.09 | 101.18 | 22.35 | 215.89 | 0.5635 | 724.0 | 577.2 | |
| 32.95 | 187.32 | 18.75 | 106.58 | -24.61 | 100.01 | 21.18 | 221.81 | 0.4947 | 1300.0 | 409.5 | |
| 0.00 | 0.59 | 0.00 | 0.33 | -19.92 | 98.84 | 20.01 | 228.02 | 0.4346 | -707.0 | -481.9 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -19.59 | 96.74 | 17.91 | 225.65 | 0.4070 | -737.0 | -589.4 | |
| 0.00 | 0.93 | 0.00 | 0.53 | -26.09 | 97.66 | 18.83 | 216.60 | 0.4882 | -668.0 | -519.3 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -25.56 | 96.85 | 18.02 | 216.18 | 0.4747 | -852.0 | -653.5 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -24.90 | 96.54 | 17.71 | 216.66 | 0.4641 | -873.0 | -697.9 | |
| 0.00 | 0.51 | 0.00 | 0.28 | -23.16 | 94.79 | 15.96 | 216.48 | 0.4270 | -794.0 | -693.2 | |
| 0.00 | 1.61 | 0.00 | 0.88 | -23.35 | 94.44 | 15.62 | 215.62 | 0.4262 | -97.0 | -111.3 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -24.44 | 92.90 | 14.08 | 211.42 | 0.4266 | -821.0 | -682.3 | |
| 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. | |