SDO HMI 2011-05-08 05:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.10 | 241.67 | 32.72 | 151.75 | 16.80 | 50.25 | 32.37 | 303.46 | 0.6160 | -191.6 | -302.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.98 | 0.00 | 0.68 | 19.11 | 56.09 | 38.21 | 302.45 | 0.6949 | 697.0 | 568.4 | |
| 0.00 | 0.72 | 0.00 | 0.49 | 19.57 | 56.14 | 38.26 | 303.01 | 0.6980 | 580.0 | 546.9 | |
| 6.62 | 181.28 | 4.26 | 114.83 | 16.67 | 52.38 | 34.50 | 301.61 | 0.6394 | -780.3 | -462.3 | |
| 0.27 | -3.00 | 0.17 | -3.00 | 16.79 | 52.02 | 34.14 | 302.02 | 0.6360 | -204.3 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.46 | 17.27 | 51.97 | 34.09 | 302.73 | 0.6385 | 1.0 | -45.9 | |
| 18.80 | -3.00 | 11.96 | -3.00 | 16.58 | 51.60 | 33.72 | 302.04 | 0.6298 | -939.6 | 999999 | |
| 2.24 | -3.00 | 1.41 | -3.00 | 16.18 | 51.14 | 33.26 | 301.80 | 0.6220 | -895.2 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.62 | 15.53 | 50.94 | 33.06 | 301.01 | 0.6155 | -184.0 | -256.2 | |
| 7.34 | -3.00 | 4.60 | -3.00 | 15.87 | 50.63 | 32.75 | 301.73 | 0.6140 | -1031.2 | 999999 | |
| 1.97 | -3.00 | 1.24 | -3.00 | 16.60 | 50.39 | 32.51 | 302.96 | 0.6161 | -783.7 | 999999 | |
| 2.78 | -3.00 | 1.74 | -3.00 | 16.38 | 50.31 | 32.43 | 302.69 | 0.6136 | -1036.0 | 999999 | |
| 1.34 | -3.00 | 0.84 | -3.00 | 16.11 | 50.04 | 32.16 | 302.52 | 0.6087 | -877.2 | 999999 | |
| 1.43 | -3.00 | 0.90 | -3.00 | 16.63 | 50.10 | 32.22 | 303.21 | 0.6128 | -707.1 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.78 | 16.16 | 49.56 | 31.68 | 302.95 | 0.6034 | -655.0 | -650.6 | |
| 0.00 | 1.07 | 0.00 | 0.68 | 19.29 | 50.11 | 32.24 | 306.88 | 0.6317 | 763.0 | 594.2 | |
| 0.00 | 1.43 | 0.00 | 0.91 | 19.52 | 50.09 | 32.21 | 307.21 | 0.6331 | 583.0 | 462.6 | |
| 0.00 | 1.16 | 0.00 | 0.73 | 18.17 | 48.90 | 31.02 | 306.35 | 0.6102 | -505.0 | -367.1 | |
| 1.88 | 18.98 | 1.18 | 11.96 | 19.51 | 48.92 | 31.04 | 308.17 | 0.6204 | -582.4 | -609.8 | |
| 1.52 | -18.00 | 0.96 | -18.00 | 19.93 | 48.78 | 30.91 | 308.85 | 0.6222 | -632.5 | 999999 | |
| 0.00 | 2.06 | 0.00 | 1.25 | 15.84 | 47.67 | 29.80 | 304.03 | 0.5790 | 652.0 | 552.3 | |
| 0.00 | 0.90 | 0.00 | 0.53 | 14.88 | 46.48 | 28.60 | 303.60 | 0.5576 | 778.0 | 656.6 | |
| 0.00 | 1.07 | 0.00 | 0.64 | 14.94 | 46.35 | 28.47 | 303.82 | 0.5565 | 678.0 | 603.4 | |
| 0.00 | 2.24 | 0.00 | 1.34 | 16.60 | 46.21 | 28.33 | 306.46 | 0.5676 | 708.0 | 469.4 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 16.62 | 45.74 | 27.87 | 306.92 | 0.5624 | 494.0 | 493.4 | |
| 0.00 | 1.88 | 0.00 | 1.12 | 16.60 | 45.31 | 27.44 | 307.31 | 0.5573 | 745.0 | 639.9 | |
| 0.00 | 1.07 | 0.00 | 0.64 | 17.46 | 44.81 | 26.93 | 309.07 | 0.5586 | 386.0 | 405.0 | |
| 0.00 | 3.22 | 0.00 | 1.92 | 17.33 | 44.61 | 26.73 | 309.08 | 0.5552 | 733.0 | 677.6 | |
| 0.00 | 1.25 | 0.00 | 0.74 | 16.84 | 44.43 | 26.55 | 308.54 | 0.5490 | 841.0 | 652.6 | |
| 0.00 | 1.07 | 0.00 | 0.63 | 16.16 | 44.22 | 26.34 | 307.72 | 0.5409 | 616.0 | 498.3 | |
| 0.00 | 1.07 | 0.00 | 0.63 | 16.44 | 44.05 | 26.17 | 308.32 | 0.5413 | 570.0 | 451.7 | |
| 5.91 | 11.28 | 3.46 | 6.61 | 16.27 | 43.78 | 25.90 | 308.35 | 0.5368 | 943.3 | 814.3 | |
| 0.00 | 0.98 | 0.00 | 0.58 | 17.53 | 43.86 | 25.98 | 310.15 | 0.5486 | 789.0 | 671.8 | |
| 0.00 | 1.34 | 0.00 | 0.79 | 17.51 | 43.01 | 25.13 | 311.02 | 0.5390 | 756.0 | 648.7 | |
| 0.00 | 0.98 | 0.00 | 0.58 | 20.07 | 42.15 | 24.27 | 315.59 | 0.5538 | 653.0 | 530.7 | |
| 0.00 | 0.98 | 0.00 | 0.59 | 20.26 | 42.11 | 24.23 | 315.90 | 0.5553 | 513.0 | 387.3 | |
| 0.00 | 0.81 | 0.00 | 0.48 | 20.00 | 41.96 | 24.08 | 315.71 | 0.5512 | 733.0 | 636.7 | |
| 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. | |