SDO HMI 2011-05-03 05:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.24 | 0.00 | 14.39 | 14.21 | 116.18 | 32.21 | 300.48 | 0.6012 | -386.7 | -247.8 | |
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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 | 0.98 | 0.00 | 0.64 | 13.23 | 121.06 | 37.08 | 295.68 | 0.6536 | -663.0 | -541.6 | |
| 0.00 | 3.30 | 0.00 | 2.12 | 13.05 | 119.67 | 35.70 | 296.24 | 0.6360 | 683.0 | 576.5 | |
| 0.00 | 1.34 | 0.00 | 0.86 | 13.33 | 119.68 | 35.71 | 296.64 | 0.6377 | 788.0 | 563.7 | |
| 0.00 | 1.61 | 0.00 | 1.03 | 12.82 | 119.56 | 35.58 | 295.98 | 0.6334 | 654.0 | 586.2 | |
| 0.00 | 1.61 | 0.00 | 1.01 | 13.38 | 117.68 | 33.71 | 297.99 | 0.6137 | -797.0 | -619.4 | |
| 0.00 | 0.54 | 0.00 | 0.34 | 14.07 | 117.57 | 33.60 | 299.09 | 0.6165 | -419.0 | -383.2 | |
| 0.00 | 1.70 | 0.00 | 1.06 | 14.21 | 117.18 | 33.21 | 299.57 | 0.6127 | -736.0 | -610.8 | |
| 0.00 | 1.61 | 0.00 | 0.99 | 15.59 | 114.83 | 30.85 | 303.38 | 0.5938 | -679.0 | -537.7 | |
| 0.00 | 0.63 | 0.00 | 0.38 | 14.76 | 114.04 | 30.06 | 302.81 | 0.5785 | -598.0 | -526.9 | |
| 0.00 | 1.34 | 0.00 | 0.81 | 14.30 | 113.68 | 29.71 | 302.41 | 0.5710 | -715.0 | -572.9 | |
| 0.00 | 1.07 | 0.00 | 0.64 | 14.25 | 113.17 | 29.20 | 302.77 | 0.5644 | -671.0 | -556.4 | |
| 0.00 | 1.79 | 0.00 | 1.06 | 13.61 | 113.05 | 29.07 | 301.89 | 0.5583 | -750.0 | -574.4 | |
| 0.00 | 2.95 | 0.00 | 1.78 | 15.85 | 113.20 | 29.22 | 305.15 | 0.5766 | -507.0 | -577.6 | |
| 0.00 | 1.34 | 0.00 | 0.81 | 15.11 | 113.01 | 29.04 | 304.21 | 0.5688 | -714.0 | -580.2 | |
| 0.00 | 1.43 | 0.00 | 0.86 | 15.97 | 112.96 | 28.99 | 305.54 | 0.5748 | -677.0 | -535.1 | |
| 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. | |