| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.70 | 197.46 | 31.93 | 116.97 | 19.78 | 64.04 | 20.34 | 323.42 | 0.5507 | 150.5 | 199.8 | |
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back to the solar disc SDO HMI 2011-02-13 09:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.63 | 0.00 | 1.00 | 20.97 | 67.31 | 23.61 | 320.63 | 0.5919 | -557.0 | -426.4 | |
| 21.24 | 51.14 | 12.80 | 30.73 | 19.42 | 66.82 | 23.13 | 319.39 | 0.5713 | -945.1 | -548.9 | |
| 1.54 | 3.26 | 0.93 | 1.96 | 19.93 | 66.38 | 22.69 | 320.52 | 0.5726 | -637.3 | -636.0 | |
| 0.00 | 1.46 | 0.00 | 0.87 | 18.64 | 66.19 | 22.50 | 319.20 | 0.5572 | -932.0 | -739.4 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 19.56 | 66.19 | 22.50 | 320.32 | 0.5669 | -704.0 | -605.9 | |
| 3.26 | 4.54 | 1.92 | 2.68 | 18.87 | 64.74 | 21.05 | 321.33 | 0.5462 | 874.7 | 569.2 | |
| 0.00 | 1.46 | 0.00 | 0.86 | 19.30 | 64.16 | 20.47 | 322.62 | 0.5458 | -604.0 | -470.2 | |
| 2.31 | 127.20 | 1.36 | 74.88 | 19.37 | 63.60 | 19.91 | 323.46 | 0.5417 | 540.4 | 467.0 | |
| 0.00 | 3.17 | 0.00 | 1.88 | 20.36 | 63.53 | 19.84 | 324.68 | 0.5525 | 482.0 | 344.5 | |
| 1.20 | -8.00 | 0.71 | -8.00 | 19.50 | 63.39 | 19.69 | 323.90 | 0.5413 | 792.6 | 999999 | |
| 6.34 | -8.00 | 3.72 | -8.00 | 19.70 | 62.78 | 19.09 | 324.97 | 0.5385 | 1274.5 | 999999 | |
| 10.36 | -8.00 | 6.10 | -8.00 | 20.06 | 62.73 | 19.03 | 325.46 | 0.5423 | 1219.3 | 999999 | |
| 3.34 | -8.00 | 1.97 | -8.00 | 20.33 | 62.76 | 19.06 | 325.70 | 0.5457 | 729.2 | 999999 | |
| 4.11 | -8.00 | 2.42 | -8.00 | 20.21 | 62.34 | 18.65 | 326.15 | 0.5409 | 876.8 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 20.22 | 61.75 | 18.05 | 327.01 | 0.5362 | 836.0 | 663.1 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 17.93 | 60.90 | 17.21 | 325.68 | 0.5013 | 678.0 | 557.2 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 20.35 | 60.77 | 17.07 | 328.58 | 0.5301 | 786.0 | 689.2 | |
| 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. | |