SDO HMI 2011-11-29 12:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.59 | 223.15 | 54.28 | 198.07 | 7.68 | 129.63 | -55.83 | 81.49 | 0.8302 | -179.3 | -141.4 | |
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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 | 0.68 | 0.00 | 0.56 | 5.50 | 132.40 | -53.05 | 83.96 | 0.8022 | -631.0 | -592.6 | |
| 18.80 | 113.50 | 15.71 | 94.74 | 7.49 | 132.00 | -53.46 | 81.52 | 0.8076 | -835.1 | -323.3 | |
| 1.11 | -2.00 | 0.93 | -2.00 | 7.99 | 131.80 | -53.65 | 80.92 | 0.8100 | -452.2 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.80 | 8.67 | 131.46 | -53.99 | 80.11 | 0.8140 | -151.0 | -119.9 | |
| 13.08 | 26.24 | 11.20 | 22.53 | 6.55 | 130.88 | -54.57 | 82.77 | 0.8183 | -623.7 | -58.9 | |
| 1.62 | 1.62 | 1.41 | 1.41 | 7.61 | 130.28 | -55.18 | 81.52 | 0.8249 | -268.5 | 0.0 | |
| 2.82 | 4.96 | 2.47 | 4.34 | 7.31 | 130.07 | -55.39 | 81.90 | 0.8267 | -496.8 | -298.8 | |
| 0.00 | 1.54 | 0.00 | 1.35 | 7.07 | 129.96 | -55.50 | 82.20 | 0.8277 | -123.0 | -151.7 | |
| 0.00 | 0.68 | 0.00 | 0.61 | 7.51 | 129.55 | -55.90 | 81.70 | 0.8319 | -347.0 | -257.0 | |
| 2.14 | 3.16 | 1.91 | 2.82 | 7.03 | 129.32 | -56.13 | 82.29 | 0.8338 | -306.3 | -182.3 | |
| 0.00 | 0.51 | 0.00 | 0.47 | 8.68 | 128.04 | -57.42 | 80.43 | 0.8469 | -348.0 | -277.8 | |
| 2.22 | 5.30 | 2.10 | 5.00 | 9.00 | 127.22 | -58.23 | 80.13 | 0.8545 | 545.8 | 343.6 | |
| 0.00 | 0.94 | 0.00 | 0.90 | 9.05 | 126.86 | -58.59 | 80.09 | 0.8577 | 430.0 | 395.7 | |
| 18.80 | 63.08 | 18.55 | 62.54 | 8.28 | 125.77 | -59.69 | 81.07 | 0.8668 | 643.3 | 133.8 | |
| 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. | |