SDO HMI 2011-05-03 11:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.80 | 0.00 | 12.75 | 14.43 | 116.00 | 35.32 | 298.61 | 0.6393 | -468.8 | -367.4 | |
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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 | 1.96 | 0.00 | 1.35 | 13.25 | 121.33 | 40.64 | 293.80 | 0.6952 | -717.0 | -636.0 | |
| 0.00 | 1.87 | 0.00 | 1.25 | 13.01 | 119.54 | 38.85 | 294.37 | 0.6733 | 721.0 | 540.5 | |
| 0.00 | 1.61 | 0.00 | 1.08 | 13.42 | 119.50 | 38.81 | 294.96 | 0.6747 | 778.0 | 582.9 | |
| 0.00 | 1.25 | 0.00 | 0.82 | 13.17 | 117.95 | 37.26 | 295.45 | 0.6552 | -642.0 | -534.7 | |
| 0.00 | 1.07 | 0.00 | 0.70 | 13.42 | 117.95 | 37.27 | 295.81 | 0.6565 | -616.0 | -480.3 | |
| 0.00 | 0.80 | 0.00 | 0.52 | 13.32 | 117.78 | 37.09 | 295.76 | 0.6539 | -659.0 | -534.6 | |
| 0.00 | 1.16 | 0.00 | 0.73 | 14.93 | 113.94 | 33.25 | 300.55 | 0.6175 | -627.0 | -471.2 | |
| 0.00 | 1.16 | 0.00 | 0.72 | 14.21 | 113.37 | 32.68 | 299.91 | 0.6061 | -809.0 | -668.7 | |
| 0.00 | 1.61 | 0.00 | 1.00 | 14.59 | 113.39 | 32.71 | 300.45 | 0.6088 | -720.0 | -551.6 | |
| 0.00 | 0.80 | 0.00 | 0.50 | 15.13 | 113.26 | 32.58 | 301.33 | 0.6107 | -575.0 | -479.7 | |
| 0.00 | 0.80 | 0.00 | 0.50 | 14.39 | 112.92 | 32.23 | 300.50 | 0.6018 | -810.0 | -678.9 | |
| 0.00 | 3.12 | 0.00 | 1.96 | 16.02 | 113.16 | 32.48 | 302.69 | 0.6155 | -713.0 | -619.3 | |
| 0.00 | 2.59 | 0.00 | 1.62 | 16.24 | 113.05 | 32.37 | 303.09 | 0.6157 | -705.0 | -558.9 | |
| 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. | |