| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 116.08 | 451.37 | 77.81 | 306.70 | -10.39 | 264.12 | -39.38 | 113.64 | 0.6808 | 239.9 | 45.6 | |
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back to the solar disc SDO HMI 2014-09-22 00:00:34 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.89 | 0.00 | 0.50 | -3.47 | 276.44 | -27.06 | 110.48 | 0.4867 | 785.0 | 689.6 | |
| 0.00 | 1.15 | 0.00 | 0.69 | -8.95 | 273.24 | -30.27 | 117.52 | 0.5636 | 786.0 | 663.5 | |
| 0.00 | 1.33 | 0.00 | 0.81 | -7.12 | 271.19 | -32.31 | 113.11 | 0.5789 | 697.0 | 564.7 | |
| 0.00 | 0.97 | 0.00 | 0.60 | -9.84 | 270.56 | -32.94 | 116.87 | 0.6029 | 756.0 | 625.9 | |
| 31.70 | 197.55 | 19.95 | 124.45 | -8.87 | 268.79 | -34.71 | 114.22 | 0.6192 | 1087.0 | 356.8 | |
| 15.58 | -5.00 | 9.85 | -5.00 | -8.65 | 268.37 | -35.13 | 113.63 | 0.6232 | 909.2 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.72 | -5.77 | 267.96 | -35.54 | 109.03 | 0.6140 | 600.0 | 530.3 | |
| 0.00 | 1.68 | 0.00 | 1.06 | -5.63 | 267.79 | -35.71 | 108.72 | 0.6156 | 748.0 | 539.8 | |
| 0.00 | 0.97 | 0.00 | 0.61 | -5.36 | 267.62 | -35.88 | 108.22 | 0.6166 | 676.0 | 530.6 | |
| 0.53 | 1.51 | 0.34 | 0.96 | -8.31 | 267.13 | -36.37 | 112.37 | 0.6368 | 797.7 | 734.4 | |
| 3.28 | 5.14 | 2.10 | 3.29 | -8.03 | 267.08 | -36.42 | 111.94 | 0.6360 | 947.5 | 710.9 | |
| 22.40 | 27.72 | 14.46 | 17.89 | -8.38 | 266.63 | -36.87 | 112.18 | 0.6434 | 811.9 | 418.9 | |
| 0.00 | 2.66 | 0.00 | 1.73 | -8.78 | 266.24 | -37.26 | 112.54 | 0.6502 | 599.0 | 475.8 | |
| 0.00 | 0.80 | 0.00 | 0.52 | -8.38 | 266.17 | -37.33 | 111.93 | 0.6491 | 519.0 | 380.8 | |
| 0.53 | 2.13 | 0.34 | 1.38 | -7.73 | 266.13 | -37.38 | 110.97 | 0.6465 | 658.0 | 504.8 | |
| 0.00 | 1.77 | 0.00 | 1.15 | -7.95 | 266.10 | -37.40 | 111.27 | 0.6478 | 629.0 | 497.1 | |
| 2.04 | 4.96 | 1.33 | 3.24 | -8.61 | 265.95 | -37.55 | 112.14 | 0.6529 | 668.0 | 396.5 | |
| 0.00 | 0.89 | 0.00 | 0.57 | -6.24 | 266.12 | -37.39 | 108.78 | 0.6398 | 546.0 | 379.4 | |
| 0.00 | 1.77 | 0.00 | 1.16 | -8.25 | 265.80 | -37.70 | 111.54 | 0.6530 | 531.0 | 407.7 | |
| 1.06 | 2.66 | 0.71 | 1.76 | -8.62 | 264.67 | -38.83 | 111.45 | 0.6685 | 602.9 | 436.9 | |
| 0.00 | 0.89 | 0.00 | 0.60 | -8.50 | 263.81 | -39.69 | 110.84 | 0.6781 | -755.0 | -625.4 | |
| 0.53 | 2.13 | 0.37 | 1.47 | -10.35 | 262.67 | -40.83 | 112.76 | 0.6999 | -807.2 | -543.7 | |
| 2.39 | 17.62 | 1.67 | 12.31 | -10.33 | 262.14 | -41.36 | 112.47 | 0.7058 | -784.9 | -642.5 | |
| 0.00 | 1.06 | 0.00 | 0.75 | -10.67 | 261.84 | -41.66 | 112.76 | 0.7108 | -613.0 | -551.8 | |
| 3.36 | -23.00 | 2.36 | -23.00 | -10.08 | 261.77 | -41.73 | 111.95 | 0.7089 | -866.5 | 999999 | |
| 0.00 | 1.51 | 0.00 | 1.06 | -10.75 | 261.62 | -41.88 | 112.76 | 0.7136 | -663.0 | -589.5 | |
| 0.00 | 0.71 | 0.00 | 0.50 | -11.02 | 261.36 | -42.14 | 112.99 | 0.7177 | -599.0 | -406.4 | |
| 0.00 | 1.68 | 0.00 | 1.20 | -10.86 | 261.06 | -42.44 | 112.63 | 0.7203 | -593.0 | -525.6 | |
| 0.00 | 0.71 | 0.00 | 0.51 | -11.12 | 260.89 | -42.62 | 112.89 | 0.7234 | -593.0 | -414.2 | |
| 2.04 | 5.67 | 1.46 | 4.05 | -10.67 | 260.72 | -42.78 | 112.21 | 0.7233 | 181.8 | -90.5 | |
| 1.77 | 4.43 | 1.28 | 3.20 | -11.21 | 260.24 | -43.26 | 112.68 | 0.7309 | -721.8 | -634.0 | |
| 0.00 | 1.06 | 0.00 | 0.77 | -10.77 | 259.94 | -43.56 | 111.97 | 0.7323 | 553.0 | 459.8 | |
| 0.00 | 0.89 | 0.00 | 0.65 | -11.82 | 259.48 | -44.02 | 113.08 | 0.7417 | -740.0 | -566.3 | |
| 5.49 | 155.31 | 4.08 | 116.54 | -12.29 | 259.12 | -44.38 | 113.51 | 0.7475 | -1016.1 | -243.9 | |
| 23.38 | -34.00 | 17.51 | -34.00 | -12.94 | 258.93 | -44.57 | 114.23 | 0.7523 | -1031.0 | 999999 | |
| 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. | |