SDO HMI 2014-10-02 01:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.98 | 288.40 | 113.87 | 598.47 | -10.90 | 245.41 | 74.43 | 256.94 | 0.9687 | 75.4 | 93.4 | |
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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 |
| 25.27 | 169.34 | 63.99 | 422.26 | -10.69 | 248.15 | 77.17 | 257.66 | 0.9817 | 105.0 | 126.6 | |
| 7.04 | -1.00 | 16.51 | -1.00 | -10.91 | 247.12 | 76.14 | 257.27 | 0.9783 | 706.7 | 999999 | |
| 1.06 | 17.79 | 2.10 | 34.63 | -10.89 | 244.82 | 73.84 | 256.90 | 0.9695 | 529.2 | 367.3 | |
| 5.11 | 14.09 | 11.56 | 32.06 | -12.93 | 246.28 | 75.30 | 255.09 | 0.9766 | 156.5 | 214.8 | |
| 0.00 | 0.53 | 0.00 | 1.22 | -13.58 | 246.51 | 75.53 | 254.47 | 0.9778 | 159.0 | 217.0 | |
| 0.70 | 2.11 | 1.56 | 4.68 | -13.61 | 245.91 | 74.93 | 254.34 | 0.9757 | -41.4 | 7.9 | |
| 0.35 | 1.94 | 0.63 | 3.48 | -11.86 | 242.91 | 71.93 | 255.57 | 0.9620 | -122.8 | -194.8 | |
| 0.00 | 0.26 | 0.00 | 0.41 | -11.35 | 240.62 | 69.65 | 255.65 | 0.9502 | 132.0 | 139.3 | |
| 0.00 | 0.62 | 0.00 | 0.88 | -14.69 | 237.94 | 66.96 | 251.61 | 0.9396 | -342.0 | -254.3 | |
| 13.83 | 72.21 | 16.77 | 87.95 | -10.71 | 234.84 | 63.86 | 255.08 | 0.9146 | -603.4 | -152.5 | |
| 0.62 | 1.85 | 0.75 | 2.25 | -11.78 | 234.64 | 63.67 | 253.89 | 0.9149 | -213.6 | -193.5 | |
| 0.00 | 1.59 | 0.00 | 1.86 | -11.11 | 233.89 | 62.91 | 254.43 | 0.9087 | -427.0 | -411.2 | |
| 0.00 | 1.06 | 0.00 | 1.17 | -9.27 | 232.73 | 61.75 | 256.14 | 0.8973 | 131.0 | 79.5 | |
| 0.00 | 0.79 | 0.00 | 0.91 | -11.23 | 233.26 | 62.28 | 254.15 | 0.9044 | -614.0 | -586.4 | |
| 0.00 | 2.55 | 0.00 | 2.87 | -10.22 | 232.84 | 61.86 | 255.14 | 0.8996 | -290.0 | -300.9 | |
| 0.00 | 1.67 | 0.00 | 1.84 | -10.11 | 232.16 | 61.18 | 255.09 | 0.8944 | -447.0 | -375.8 | |
| 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. | |