SDO HMI 2011-02-14 13:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.49 | 121.54 | 31.91 | 84.74 | 19.97 | 64.72 | 36.38 | 307.64 | 0.7057 | 73.8 | 335.0 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.33 | 39.06 | 13.37 | 28.55 | 19.43 | 68.23 | 39.90 | 304.50 | 0.7363 | -810.6 | -86.0 | |
| 0.00 | 1.88 | 0.00 | 1.36 | 18.97 | 67.77 | 39.44 | 304.25 | 0.7291 | -764.0 | -712.3 | |
| 0.00 | 0.77 | 0.00 | 0.55 | 19.08 | 67.51 | 39.18 | 304.55 | 0.7273 | -544.0 | -543.8 | |
| 0.00 | 0.34 | 0.00 | 0.23 | 19.10 | 63.96 | 35.63 | 307.06 | 0.6921 | 445.0 | 409.5 | |
| 2.14 | 6.25 | 1.46 | 4.27 | 19.26 | 63.85 | 35.51 | 307.33 | 0.6920 | 736.0 | 699.8 | |
| 0.00 | 1.46 | 0.00 | 0.99 | 18.92 | 63.76 | 35.43 | 306.99 | 0.6889 | 778.0 | 660.2 | |
| 0.00 | 1.03 | 0.00 | 0.70 | 19.91 | 63.32 | 34.98 | 308.52 | 0.6914 | 449.0 | 349.1 | |
| 3.00 | 3.68 | 2.10 | 2.58 | 21.80 | 63.79 | 35.46 | 310.38 | 0.7094 | -667.7 | -616.9 | |
| 0.77 | 60.90 | 0.52 | 41.28 | 19.82 | 63.03 | 34.69 | 308.64 | 0.6879 | 740.6 | 578.4 | |
| 4.80 | -9.00 | 3.25 | -9.00 | 19.77 | 62.74 | 34.41 | 308.79 | 0.6847 | 1068.4 | 999999 | |
| 13.11 | -9.00 | 8.91 | -9.00 | 20.22 | 62.67 | 34.33 | 309.40 | 0.6873 | 854.9 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.63 | 20.60 | 61.47 | 33.14 | 310.82 | 0.6785 | 675.0 | 588.3 | |
| 3.34 | 5.23 | 2.30 | 3.60 | 23.24 | 61.25 | 32.91 | 314.04 | 0.6969 | 629.6 | 535.6 | |
| 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. | |