SDO HMI 2014-09-29 19:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 167.42 | 844.62 | 165.15 | 829.17 | 15.18 | 260.94 | 60.26 | 283.70 | 0.8633 | -115.7 | -85.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.03 | 168.31 | 2.38 | 190.66 | 13.12 | 266.53 | 65.85 | 281.34 | 0.9081 | -107.2 | -219.5 | |
| 14.45 | -1.00 | 16.54 | -1.00 | 13.43 | 265.87 | 65.19 | 281.67 | 0.9033 | -586.5 | 999999 | |
| 9.08 | -1.00 | 10.18 | -1.00 | 13.86 | 265.29 | 64.60 | 282.14 | 0.8990 | -635.6 | 999999 | |
| 1.50 | -1.00 | 1.66 | -1.00 | 13.59 | 265.00 | 64.32 | 281.83 | 0.8968 | -743.1 | 999999 | |
| 2.73 | -1.00 | 3.02 | -1.00 | 13.78 | 264.88 | 64.20 | 282.05 | 0.8959 | -861.0 | 999999 | |
| 3.88 | -1.00 | 4.27 | -1.00 | 14.04 | 264.80 | 64.12 | 282.33 | 0.8953 | -862.5 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.27 | 13.57 | 262.78 | 62.09 | 281.79 | 0.8795 | -452.0 | -461.3 | |
| 0.00 | 1.32 | 0.00 | 1.36 | 13.63 | 262.54 | 61.85 | 281.85 | 0.8775 | -598.0 | -531.1 | |
| 1.32 | 271.76 | 1.35 | 271.95 | 14.85 | 262.39 | 61.71 | 283.24 | 0.8764 | -1128.3 | -400.0 | |
| 0.00 | 0.62 | 0.00 | 0.61 | 13.29 | 261.61 | 60.92 | 281.46 | 0.8699 | 128.0 | 73.6 | |
| 26.17 | -9.00 | 26.72 | -9.00 | 15.19 | 262.37 | 61.68 | 283.63 | 0.8762 | -757.5 | 999999 | |
| 3.08 | -9.00 | 3.08 | -9.00 | 14.65 | 261.58 | 60.90 | 283.02 | 0.8697 | -602.6 | 999999 | |
| 12.42 | -9.00 | 12.32 | -9.00 | 15.20 | 261.39 | 60.71 | 283.65 | 0.8682 | -1122.3 | 999999 | |
| 10.13 | -9.00 | 10.10 | -9.00 | 15.86 | 261.60 | 60.91 | 284.41 | 0.8700 | -807.1 | 999999 | |
| 11.46 | -9.00 | 11.22 | -9.00 | 14.87 | 260.98 | 60.30 | 283.28 | 0.8646 | 149.3 | 999999 | |
| 0.53 | 2.91 | 0.52 | 2.88 | 16.75 | 261.36 | 60.68 | 285.45 | 0.8682 | -541.7 | -465.1 | |
| 0.35 | 2.64 | 0.33 | 2.48 | 13.21 | 259.41 | 58.72 | 281.36 | 0.8508 | -190.2 | -6.8 | |
| 0.00 | 1.67 | 0.00 | 1.56 | 13.48 | 259.21 | 58.53 | 281.67 | 0.8490 | 518.0 | 456.1 | |
| 1.85 | 12.25 | 1.72 | 11.36 | 13.98 | 259.12 | 58.43 | 282.27 | 0.8482 | 542.4 | 287.3 | |
| 2.29 | 351.77 | 2.13 | 318.03 | 14.50 | 259.15 | 58.47 | 282.88 | 0.8486 | 566.6 | 173.4 | |
| 2.73 | -20.00 | 2.53 | -20.00 | 15.00 | 259.01 | 58.33 | 283.48 | 0.8475 | 530.2 | 999999 | |
| 0.00 | 1.32 | 0.00 | 1.21 | 14.58 | 258.65 | 57.97 | 282.99 | 0.8441 | 510.0 | 447.9 | |
| 2.29 | -20.00 | 2.10 | -20.00 | 15.51 | 258.59 | 57.90 | 284.10 | 0.8438 | 263.5 | 999999 | |
| 0.00 | 1.15 | 0.00 | 1.04 | 15.01 | 258.37 | 57.68 | 283.51 | 0.8416 | 417.0 | 402.8 | |
| 2.73 | 26.70 | 2.46 | 24.01 | 14.64 | 257.98 | 57.30 | 283.08 | 0.8380 | 853.4 | 517.8 | |
| 0.00 | 1.06 | 0.00 | 0.99 | 17.70 | 259.35 | 58.67 | 286.65 | 0.8515 | 328.0 | 249.4 | |
| 13.31 | -20.00 | 12.05 | -20.00 | 15.55 | 258.14 | 57.45 | 284.17 | 0.8397 | 785.0 | 999999 | |
| 0.26 | -20.00 | 0.24 | -20.00 | 16.00 | 258.28 | 57.60 | 284.70 | 0.8412 | -47.0 | 999999 | |
| 31.99 | -20.00 | 28.59 | -20.00 | 16.29 | 257.54 | 56.86 | 285.08 | 0.8345 | 874.0 | 999999 | |
| 4.14 | -20.00 | 3.71 | -20.00 | 17.62 | 257.59 | 56.91 | 286.67 | 0.8356 | 463.7 | 999999 | |
| 1.06 | -20.00 | 0.94 | -20.00 | 17.24 | 257.40 | 56.72 | 286.22 | 0.8337 | 649.3 | 999999 | |
| 1.76 | -20.00 | 1.57 | -20.00 | 17.43 | 257.38 | 56.69 | 286.45 | 0.8336 | 748.0 | 999999 | |
| 2.03 | -20.00 | 1.80 | -20.00 | 17.57 | 257.16 | 56.48 | 286.64 | 0.8317 | 843.2 | 999999 | |
| 1.85 | -20.00 | 1.62 | -20.00 | 17.15 | 256.68 | 55.99 | 286.17 | 0.8269 | 736.5 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.76 | 17.26 | 256.16 | 55.48 | 286.34 | 0.8221 | 552.0 | 472.1 | |
| 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. | |