| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.49 | 287.15 | 20.80 | 144.07 | 9.76 | 56.28 | 5.64 | 320.34 | 0.1593 | -563.3 | -355.5 | |
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back to the solar disc SDO HMI 2011-11-12 10:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.46 | 0.00 | 0.74 | 6.22 | 62.15 | 11.51 | 285.25 | 0.2066 | -915.0 | -808.0 | |
| 0.00 | 2.32 | 0.00 | 1.16 | 7.51 | 57.96 | 7.33 | 300.95 | 0.1481 | -879.0 | -613.5 | |
| 37.79 | 244.72 | 18.95 | 122.73 | 9.42 | 57.18 | 6.55 | 314.09 | 0.1573 | -1473.0 | -449.1 | |
| 0.43 | -3.00 | 0.22 | -3.00 | 9.36 | 56.66 | 6.03 | 316.15 | 0.1503 | -1068.6 | 999999 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 9.99 | 56.07 | 5.44 | 321.85 | 0.1518 | -954.0 | -699.7 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 9.72 | 56.01 | 5.37 | 321.04 | 0.1475 | -925.0 | -743.6 | |
| 0.00 | 0.95 | 0.00 | 0.47 | 10.77 | 55.57 | 4.94 | 327.42 | 0.1577 | -690.0 | -534.4 | |
| 0.00 | 1.46 | 0.00 | 0.74 | 12.24 | 55.26 | 4.63 | 333.43 | 0.1770 | -724.0 | -609.6 | |
| 0.00 | 6.28 | 0.00 | 3.16 | 12.24 | 55.02 | 4.38 | 334.65 | 0.1752 | 378.0 | 232.0 | |
| 0.00 | 1.03 | 0.00 | 0.52 | 9.76 | 54.80 | 4.16 | 328.02 | 0.1358 | -837.0 | -562.9 | |
| 0.00 | 1.21 | 0.00 | 0.61 | 16.76 | 53.03 | 2.39 | 350.33 | 0.2392 | 833.0 | 740.9 | |
| 0.00 | 1.29 | 0.00 | 0.66 | 17.52 | 51.20 | 0.57 | 357.81 | 0.2490 | 781.0 | 599.1 | |
| 0.00 | 1.29 | 0.00 | 0.65 | 10.96 | 51.19 | 0.55 | 356.00 | 0.1363 | -843.0 | -668.5 | |
| 0.00 | 1.29 | 0.00 | 0.65 | 13.00 | 50.25 | -0.39 | 2.21 | 0.1715 | 961.0 | 750.3 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 19.46 | 49.86 | -0.78 | 2.61 | 0.2819 | 814.0 | 619.6 | |
| 0.00 | 1.38 | 0.00 | 0.69 | 12.67 | 49.70 | -0.93 | 5.51 | 0.1664 | 968.0 | 791.6 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 19.34 | 49.64 | -1.00 | 3.38 | 0.2800 | 948.0 | 737.5 | |
| 1.81 | 2.58 | 0.90 | 1.29 | 10.75 | 47.89 | -2.74 | 19.62 | 0.1405 | -919.0 | -834.7 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 10.12 | 47.30 | -3.34 | 25.37 | 0.1344 | -920.0 | -637.3 | |
| 0.00 | 2.50 | 0.00 | 1.25 | 11.13 | 46.29 | -4.35 | 28.25 | 0.1579 | 1117.0 | 956.4 | |
| 0.00 | 0.95 | 0.00 | 0.47 | 10.80 | 46.26 | -4.37 | 29.43 | 0.1532 | 844.0 | 656.0 | |
| 1.46 | 2.67 | 0.73 | 1.34 | 10.89 | 45.99 | -4.65 | 30.64 | 0.1568 | 1053.6 | 953.5 | |
| 0.00 | 0.95 | 0.00 | 0.48 | 11.10 | 45.92 | -4.71 | 30.30 | 0.1605 | 920.0 | 717.0 | |
| 0.00 | 1.12 | 0.00 | 0.56 | 13.02 | 45.74 | -4.90 | 25.93 | 0.1911 | 797.0 | 676.2 | |
| 0.00 | 1.12 | 0.00 | 0.56 | 11.19 | 45.74 | -4.89 | 30.97 | 0.1634 | 856.0 | 523.8 | |
| 0.00 | 0.77 | 0.00 | 0.39 | 11.70 | 45.64 | -4.99 | 29.90 | 0.1719 | 728.0 | 667.3 | |
| 0.00 | 2.32 | 0.00 | 1.17 | 11.49 | 45.58 | -5.05 | 30.81 | 0.1692 | 780.0 | 623.6 | |
| 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. | |