SDO HMI 2011-11-07 12:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.70 | 266.30 | 48.61 | 263.60 | 9.62 | 55.49 | -59.97 | 81.03 | 0.8648 | -379.6 | -183.7 | |
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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 |
| 25.88 | 222.30 | 24.41 | 211.86 | 9.26 | 56.94 | -58.52 | 81.41 | 0.8533 | -777.4 | -197.0 | |
| 0.00 | 1.29 | 0.00 | 1.24 | 10.66 | 56.53 | -58.93 | 79.80 | 0.8573 | -388.0 | -359.7 | |
| 4.92 | 9.32 | 4.80 | 9.11 | 12.07 | 55.87 | -59.59 | 78.18 | 0.8636 | 347.5 | -96.2 | |
| 2.33 | -1.00 | 2.24 | -1.00 | 9.35 | 56.27 | -59.19 | 81.33 | 0.8593 | -374.4 | 999999 | |
| 4.05 | -1.00 | 3.91 | -1.00 | 9.61 | 56.14 | -59.32 | 81.03 | 0.8605 | -321.9 | 999999 | |
| 1.55 | 2.07 | 1.54 | 2.06 | 11.09 | 55.18 | -60.28 | 79.34 | 0.8692 | -556.1 | -525.7 | |
| 0.00 | 0.86 | 0.00 | 0.87 | 10.83 | 54.84 | -60.62 | 79.66 | 0.8720 | -324.0 | -271.2 | |
| 0.00 | 1.21 | 0.00 | 1.19 | 7.29 | 55.41 | -60.05 | 83.73 | 0.8667 | 530.0 | 498.3 | |
| 5.43 | 17.68 | 6.38 | 20.69 | 9.51 | 50.14 | -65.32 | 81.24 | 0.9085 | -538.8 | -401.5 | |
| 0.00 | 1.47 | 0.00 | 1.73 | 9.05 | 49.94 | -65.52 | 81.75 | 0.9099 | -323.0 | -314.2 | |
| 0.00 | 2.33 | 0.00 | 3.29 | 12.24 | 45.65 | -69.81 | 78.32 | 0.9382 | 504.0 | 440.4 | |
| 0.00 | 1.04 | 0.00 | 1.48 | 12.40 | 45.37 | -70.09 | 78.15 | 0.9398 | 370.0 | 294.0 | |
| 0.00 | 2.16 | 0.00 | 3.18 | 12.73 | 44.79 | -70.67 | 77.80 | 0.9431 | 252.0 | 384.2 | |
| 2.42 | 4.57 | 3.65 | 6.90 | 12.76 | 44.30 | -71.16 | 77.78 | 0.9459 | 382.0 | 113.4 | |
| 1.12 | -14.00 | 1.68 | -14.00 | 12.59 | 44.41 | -71.05 | 77.96 | 0.9453 | 342.0 | 999999 | |
| 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. | |