SDO HMI 2011-11-29 07:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.15 | 213.35 | 58.90 | 204.55 | 7.77 | 129.51 | -58.68 | 81.59 | 0.8567 | -121.4 | -126.7 | |
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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 |
| 2.57 | 110.91 | 2.31 | 99.52 | 8.65 | 131.86 | -56.33 | 80.38 | 0.8367 | 392.2 | -287.2 | |
| 20.87 | -1.00 | 18.72 | -1.00 | 7.54 | 131.82 | -56.37 | 81.70 | 0.8363 | -811.7 | 999999 | |
| 0.00 | 1.37 | 0.00 | 1.25 | 8.85 | 131.32 | -56.87 | 80.19 | 0.8419 | -168.0 | -61.2 | |
| 10.18 | 20.95 | 9.40 | 19.40 | 6.51 | 130.70 | -57.49 | 83.01 | 0.8463 | -532.1 | -378.1 | |
| 0.00 | 1.62 | 0.00 | 1.51 | 7.05 | 130.60 | -57.59 | 82.38 | 0.8474 | -533.0 | -479.2 | |
| 0.00 | 1.11 | 0.00 | 1.04 | 7.73 | 130.23 | -57.96 | 81.60 | 0.8512 | -294.0 | -220.2 | |
| 1.88 | -4.00 | 1.76 | -4.00 | 7.07 | 130.26 | -57.93 | 82.37 | 0.8506 | -117.8 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.97 | 7.75 | 129.83 | -58.36 | 81.60 | 0.8548 | 369.0 | 263.2 | |
| 2.99 | 4.96 | 2.84 | 4.71 | 7.36 | 129.80 | -58.39 | 82.06 | 0.8549 | -398.0 | -191.4 | |
| 0.34 | 3.51 | 0.33 | 3.38 | 7.00 | 129.30 | -58.89 | 82.52 | 0.8592 | 53.2 | -160.9 | |
| 2.22 | -10.00 | 2.14 | -10.00 | 7.00 | 129.24 | -58.95 | 82.52 | 0.8597 | -266.6 | 999999 | |
| 3.85 | 8.12 | 3.94 | 8.30 | 8.94 | 127.32 | -60.87 | 80.41 | 0.8771 | 563.5 | 461.9 | |
| 0.00 | 2.05 | 0.00 | 2.13 | 9.14 | 126.95 | -61.24 | 80.21 | 0.8803 | -88.0 | 32.6 | |
| 16.25 | 57.72 | 17.46 | 62.34 | 8.19 | 125.75 | -62.44 | 81.36 | 0.8894 | 672.5 | 142.4 | |
| 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. | |