SDO HMI 2011-10-06 05:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.14 | 200.71 | 54.76 | 258.76 | -14.62 | 116.83 | -64.52 | 108.85 | 0.9235 | 88.0 | -9.1 | |
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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 |
| 7.21 | 95.43 | 8.24 | 110.55 | -14.62 | 119.99 | -61.35 | 109.64 | 0.9035 | 743.4 | 155.4 | |
| 14.76 | -1.00 | 17.19 | -1.00 | -14.26 | 119.44 | -61.91 | 109.11 | 0.9066 | 554.9 | 999999 | |
| 0.00 | 2.37 | 0.00 | 2.82 | -13.95 | 118.78 | -62.56 | 108.60 | 0.9106 | 358.0 | 277.6 | |
| 1.58 | 4.13 | 1.91 | 4.98 | -13.78 | 118.32 | -63.02 | 108.30 | 0.9134 | 328.5 | 147.4 | |
| 1.05 | 5.10 | 1.30 | 6.25 | -13.56 | 117.66 | -63.68 | 107.91 | 0.9174 | 313.2 | 317.0 | |
| 0.00 | 2.64 | 0.00 | 3.28 | -13.80 | 117.47 | -63.87 | 108.11 | 0.9190 | 405.0 | 259.3 | |
| 8.17 | 24.43 | 10.68 | 31.76 | -15.17 | 116.51 | -64.83 | 109.32 | 0.9273 | -592.6 | -467.3 | |
| 0.00 | 1.85 | 0.00 | 2.32 | -13.65 | 117.12 | -64.22 | 107.87 | 0.9211 | 108.0 | 56.2 | |
| 0.00 | 3.60 | 0.00 | 4.96 | -15.48 | 115.34 | -66.01 | 109.36 | 0.9348 | -512.0 | -282.5 | |
| 0.88 | 3.25 | 1.27 | 4.71 | -15.22 | 114.24 | -67.10 | 108.83 | 0.9407 | -437.8 | -327.7 | |
| 2.20 | 57.91 | 3.24 | 87.13 | -15.17 | 113.78 | -67.56 | 108.68 | 0.9431 | -364.3 | -89.0 | |
| 6.06 | -11.00 | 9.06 | -11.00 | -14.75 | 113.32 | -68.03 | 108.13 | 0.9451 | -466.0 | 999999 | |
| 1.23 | -11.00 | 1.87 | -11.00 | -14.81 | 113.02 | -68.32 | 108.13 | 0.9468 | 215.1 | 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. | |