SDO HMI 2011-10-13 09:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.01 | 32.61 | 1.12 | 18.17 | 20.96 | 110.00 | 23.20 | 305.76 | 0.4557 | 300.8 | 530.6 | |
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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 | 2.97 | 0.00 | 1.75 | 25.45 | 113.94 | 27.14 | 309.81 | 0.5383 | 639.0 | 679.8 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 20.04 | 112.69 | 25.89 | 301.60 | 0.4836 | -725.0 | -561.8 | |
| 0.00 | 1.57 | 0.00 | 0.91 | 24.20 | 112.76 | 25.96 | 308.87 | 0.5149 | 689.0 | 541.4 | |
| 0.00 | 2.19 | 0.00 | 1.22 | 20.59 | 110.85 | 24.05 | 304.30 | 0.4637 | -1023.0 | -827.5 | |
| 1.40 | 1.66 | 0.78 | 0.93 | 20.25 | 110.69 | 23.89 | 303.82 | 0.4592 | -768.6 | -582.0 | |
| 0.61 | 1.31 | 0.34 | 0.73 | 20.13 | 110.53 | 23.73 | 303.74 | 0.4563 | -784.0 | -755.0 | |
| 0.00 | 1.92 | 0.00 | 1.11 | 25.98 | 111.33 | 24.53 | 313.17 | 0.5137 | 724.0 | 511.1 | |
| 0.00 | 0.87 | 0.00 | 0.48 | 18.42 | 109.41 | 22.61 | 301.40 | 0.4291 | 758.0 | 627.2 | |
| 0.00 | 4.11 | 0.00 | 2.26 | 19.44 | 109.35 | 22.55 | 303.56 | 0.4358 | 931.0 | 757.4 | |
| 0.00 | 1.22 | 0.00 | 0.67 | 19.61 | 108.96 | 22.16 | 304.31 | 0.4320 | 721.0 | 644.4 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 20.38 | 108.98 | 22.17 | 305.84 | 0.4382 | 583.0 | 447.2 | |
| 0.00 | 3.24 | 0.00 | 1.78 | 20.17 | 108.74 | 21.94 | 305.69 | 0.4335 | 825.0 | 724.3 | |
| 0.00 | 8.49 | 0.00 | 4.64 | 19.53 | 108.51 | 21.71 | 304.65 | 0.4255 | 1076.0 | 911.9 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 20.75 | 105.55 | 18.74 | 310.83 | 0.3989 | 700.0 | 569.6 | |
| 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. | |