SDO HMI 2011-09-03 13:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.63 | 231.16 | 35.46 | 128.89 | -19.51 | 258.07 | 5.49 | 191.31 | 0.4601 | 71.7 | 49.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.06 | 0.00 | 1.19 | -22.01 | 262.44 | 9.86 | 198.08 | 0.5137 | 679.0 | 481.4 | |
| 0.00 | 1.25 | 0.00 | 0.72 | -21.18 | 262.18 | 9.60 | 198.18 | 0.5006 | 871.0 | 677.4 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -18.18 | 260.01 | 7.43 | 196.02 | 0.4469 | 350.0 | 388.7 | |
| 0.00 | 1.07 | 0.00 | 0.60 | -20.04 | 259.90 | 7.32 | 194.68 | 0.4742 | 620.0 | 479.8 | |
| 1.25 | 1.61 | 0.70 | 0.90 | -19.86 | 259.76 | 7.18 | 194.51 | 0.4711 | 756.6 | 675.0 | |
| 11.17 | 14.04 | 6.27 | 7.88 | -20.09 | 259.19 | 6.61 | 193.28 | 0.4724 | 829.3 | 533.3 | |
| 0.00 | 1.16 | 0.00 | 0.69 | -25.95 | 259.21 | 6.63 | 190.77 | 0.5581 | 624.0 | 436.2 | |
| 0.00 | 1.34 | 0.00 | 0.76 | -20.57 | 258.85 | 6.27 | 192.40 | 0.4783 | 579.0 | 471.6 | |
| 23.51 | 112.91 | 13.14 | 63.07 | -19.71 | 258.72 | 6.14 | 192.56 | 0.4650 | 1044.5 | 327.2 | |
| 3.84 | -9.00 | 2.14 | -9.00 | -19.27 | 258.70 | 6.12 | 192.74 | 0.4583 | 935.9 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.49 | -17.59 | 258.19 | 5.62 | 192.56 | 0.4308 | -731.0 | -634.5 | |
| 0.00 | 2.06 | 0.00 | 1.13 | -17.89 | 258.14 | 5.56 | 192.29 | 0.4353 | -833.0 | -674.0 | |
| 0.00 | 1.34 | 0.00 | 0.77 | -23.15 | 258.24 | 5.66 | 190.18 | 0.5150 | 794.0 | 631.4 | |
| 0.00 | 2.77 | 0.00 | 1.53 | -18.35 | 258.03 | 5.45 | 191.81 | 0.4421 | 591.0 | 460.8 | |
| 0.00 | 1.25 | 0.00 | 0.69 | -18.18 | 257.64 | 5.06 | 191.07 | 0.4382 | -632.0 | -458.9 | |
| 0.00 | 1.88 | 0.00 | 1.08 | -22.83 | 257.76 | 5.18 | 189.45 | 0.5091 | 828.0 | 615.9 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -18.31 | 257.42 | 4.84 | 190.54 | 0.4396 | -778.0 | -641.9 | |
| 0.00 | 10.37 | 0.00 | 5.78 | -19.56 | 257.42 | 4.84 | 190.03 | 0.4588 | 163.0 | 184.0 | |
| 0.63 | 11.26 | 0.35 | 6.23 | -18.85 | 257.27 | 4.69 | 190.01 | 0.4475 | -735.6 | -377.7 | |
| 4.11 | 5.63 | 2.28 | 3.13 | -19.18 | 257.15 | 4.58 | 189.63 | 0.4523 | -682.9 | -509.0 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -18.41 | 257.07 | 4.49 | 189.76 | 0.4402 | -871.0 | -703.8 | |
| 0.00 | 5.18 | 0.00 | 2.84 | -17.74 | 257.02 | 4.44 | 189.93 | 0.4296 | -674.0 | -691.7 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -18.95 | 256.99 | 4.41 | 189.37 | 0.4483 | -833.0 | -632.3 | |
| 0.00 | 0.89 | 0.00 | 0.49 | -18.17 | 256.90 | 4.32 | 189.50 | 0.4361 | -727.0 | -614.1 | |
| 0.00 | 1.16 | 0.00 | 0.65 | -19.25 | 256.90 | 4.32 | 189.08 | 0.4527 | -676.0 | -551.1 | |
| 2.86 | 40.59 | 1.59 | 22.47 | -19.15 | 256.67 | 4.09 | 188.64 | 0.4506 | -793.0 | -628.3 | |
| 2.23 | -26.00 | 1.23 | -26.00 | -18.50 | 256.46 | 3.89 | 188.43 | 0.4401 | -895.4 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.50 | -20.09 | 256.47 | 3.89 | 187.92 | 0.4647 | -657.0 | -515.0 | |
| 11.17 | -26.00 | 6.17 | -26.00 | -18.81 | 256.38 | 3.80 | 188.14 | 0.4446 | -1006.1 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -20.23 | 256.34 | 3.77 | 187.62 | 0.4665 | -677.0 | -505.2 | |
| 2.86 | -26.00 | 1.59 | -26.00 | -19.51 | 256.26 | 3.68 | 187.68 | 0.4554 | -738.8 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.60 | -19.44 | 255.94 | 3.36 | 187.03 | 0.4536 | -681.0 | -614.8 | |
| 0.00 | 1.70 | 0.00 | 0.94 | -19.61 | 255.72 | 3.14 | 186.53 | 0.4558 | -801.0 | -700.0 | |
| 0.00 | 1.16 | 0.00 | 0.65 | -20.05 | 255.47 | 2.89 | 185.91 | 0.4622 | -590.0 | -451.0 | |
| 0.00 | 0.89 | 0.00 | 0.50 | -20.15 | 254.89 | 2.31 | 184.71 | 0.4629 | -693.0 | -534.6 | |
| 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. | |