SDO HMI 2011-06-07 06:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.97 | 121.22 | 19.91 | 81.48 | 17.30 | 19.85 | 39.39 | 296.16 | 0.6768 | -284.9 | -309.2 | |
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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 |
| 0.00 | 3.62 | 0.00 | 2.68 | 20.97 | 24.66 | 44.20 | 298.75 | 0.7448 | -607.0 | -546.1 | |
| 5.61 | 87.90 | 3.84 | 59.80 | 16.91 | 21.35 | 40.90 | 294.85 | 0.6926 | -726.9 | -411.6 | |
| 1.72 | -2.00 | 1.17 | -2.00 | 17.00 | 21.08 | 40.63 | 295.10 | 0.6899 | -694.0 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.83 | 20.22 | 21.82 | 41.36 | 299.09 | 0.7118 | -636.0 | -471.8 | |
| 1.00 | -2.00 | 0.68 | -2.00 | 17.06 | 20.85 | 40.39 | 295.30 | 0.6875 | -673.2 | 999999 | |
| 11.77 | -2.00 | 7.97 | -2.00 | 16.75 | 20.68 | 40.22 | 294.93 | 0.6842 | -955.0 | 999999 | |
| 1.54 | 7.69 | 0.99 | 4.97 | 17.10 | 17.14 | 36.68 | 297.19 | 0.6442 | -856.7 | -712.9 | |
| 0.00 | 1.27 | 0.00 | 0.81 | 18.47 | 15.37 | 34.91 | 300.21 | 0.6304 | 439.0 | 419.4 | |
| 6.07 | 10.05 | 3.84 | 6.36 | 18.05 | 15.19 | 34.74 | 299.72 | 0.6260 | 603.6 | 731.7 | |
| 0.00 | 2.17 | 0.00 | 1.38 | 18.34 | 15.18 | 34.72 | 300.14 | 0.6275 | 583.0 | 504.1 | |
| 1.45 | 2.53 | 0.91 | 1.59 | 17.35 | 14.92 | 34.46 | 298.85 | 0.6189 | 615.2 | 598.6 | |
| 0.81 | -9.00 | 0.51 | -9.00 | 17.83 | 14.99 | 34.53 | 299.51 | 0.6223 | 625.6 | 999999 | |
| 0.00 | 2.72 | 0.00 | 1.73 | 18.98 | 14.94 | 34.48 | 301.23 | 0.6283 | 725.0 | 662.1 | |
| 0.00 | 1.09 | 0.00 | 0.69 | 20.57 | 14.19 | 33.74 | 303.99 | 0.6294 | 669.0 | 455.9 | |
| 0.00 | 1.00 | 0.00 | 0.64 | 23.93 | 12.38 | 31.92 | 309.95 | 0.6327 | 484.0 | 438.4 | |
| 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. | |