SDO HMI 2011-08-29 16:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.58 | 73.18 | 16.75 | 79.60 | -20.40 | 259.44 | -57.52 | 117.32 | 0.8918 | 261.5 | 42.4 | |
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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 | 0.45 | 0.00 | 0.48 | -21.33 | 260.53 | -56.44 | 118.69 | 0.8868 | 490.0 | 470.8 | |
| 1.70 | 19.98 | 1.78 | 20.98 | -20.53 | 260.69 | -56.27 | 117.91 | 0.8833 | 812.8 | 520.8 | |
| 1.25 | -2.00 | 1.33 | -2.00 | -20.57 | 260.38 | -56.59 | 117.83 | 0.8857 | 546.2 | 999999 | |
| 0.00 | 3.40 | 0.00 | 3.72 | -21.58 | 259.71 | -57.25 | 118.66 | 0.8932 | -113.0 | -119.3 | |
| 11.91 | 26.51 | 12.84 | 28.68 | -21.05 | 259.98 | -56.99 | 118.19 | 0.8898 | 553.1 | 127.5 | |
| 0.00 | 1.07 | 0.00 | 1.16 | -20.44 | 259.74 | -57.23 | 117.46 | 0.8898 | 191.0 | 187.6 | |
| 0.00 | 1.25 | 0.00 | 1.39 | -20.62 | 258.96 | -58.01 | 117.38 | 0.8957 | 210.0 | 152.4 | |
| 0.00 | 0.72 | 0.00 | 0.75 | -18.45 | 260.00 | -56.96 | 115.43 | 0.8825 | 152.0 | 123.2 | |
| 0.72 | 1.79 | 0.80 | 2.00 | -19.61 | 258.21 | -58.76 | 116.04 | 0.8983 | -124.1 | 105.4 | |
| 0.00 | 13.08 | 0.00 | 14.73 | -19.35 | 257.86 | -59.11 | 115.65 | 0.9000 | -407.0 | -444.6 | |
| 0.00 | 1.43 | 0.00 | 1.68 | -20.18 | 256.96 | -60.00 | 116.23 | 0.9080 | -502.0 | -417.8 | |
| 0.00 | 0.63 | 0.00 | 0.69 | -17.73 | 257.90 | -59.07 | 113.95 | 0.8959 | -406.0 | -388.1 | |
| 0.00 | 0.90 | 0.00 | 1.02 | -17.78 | 257.11 | -59.85 | 113.75 | 0.9015 | -490.0 | -476.5 | |
| 0.00 | 0.90 | 0.00 | 1.05 | -18.80 | 256.52 | -60.45 | 114.64 | 0.9078 | -533.0 | -429.7 | |
| 0.00 | 1.07 | 0.00 | 1.27 | -18.99 | 256.34 | -60.63 | 114.78 | 0.9094 | -511.0 | -497.9 | |
| 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. | |