SDO HMI 2011-10-14 18:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.32 | 123.50 | 18.31 | 105.37 | -14.69 | 119.59 | 50.93 | 247.22 | 0.8166 | 295.1 | 217.1 | |
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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 |
| 2.01 | 110.31 | 1.72 | 94.88 | -14.04 | 119.98 | 51.32 | 248.14 | 0.8182 | 612.6 | 292.6 | |
| 0.00 | 1.57 | 0.00 | 1.29 | -10.61 | 118.96 | 50.30 | 251.85 | 0.7981 | 265.0 | 307.4 | |
| 18.87 | -1.00 | 16.25 | -1.00 | -14.67 | 119.99 | 51.33 | 247.40 | 0.8203 | 809.8 | 999999 | |
| 0.00 | 1.22 | 0.00 | 1.05 | -17.71 | 118.85 | 50.19 | 243.46 | 0.8202 | -395.0 | -288.6 | |
| 0.00 | 0.96 | 0.00 | 0.77 | -14.87 | 116.27 | 47.61 | 245.68 | 0.7856 | -491.0 | -394.5 | |
| 0.00 | 0.79 | 0.00 | 0.62 | -14.71 | 116.13 | 47.47 | 245.82 | 0.7836 | -631.0 | -490.2 | |
| 0.00 | 0.70 | 0.00 | 0.55 | -15.48 | 115.49 | 46.83 | 244.61 | 0.7803 | -581.0 | -480.6 | |
| 0.00 | 0.96 | 0.00 | 0.76 | -16.30 | 115.33 | 46.67 | 243.56 | 0.7820 | -500.0 | -371.9 | |
| 0.00 | 1.57 | 0.00 | 1.23 | -16.11 | 115.00 | 46.34 | 243.63 | 0.7780 | -641.0 | -508.3 | |
| 0.00 | 1.05 | 0.00 | 0.80 | -14.48 | 114.49 | 45.83 | 245.37 | 0.7663 | -496.0 | -451.0 | |
| 0.00 | 1.31 | 0.00 | 1.03 | -16.47 | 115.06 | 46.40 | 243.24 | 0.7801 | -527.0 | -372.2 | |
| 0.44 | 2.01 | 0.34 | 1.57 | -16.38 | 114.72 | 46.06 | 243.18 | 0.7764 | -700.8 | -603.2 | |
| 0.00 | 1.05 | 0.00 | 0.82 | -16.61 | 114.34 | 45.68 | 242.73 | 0.7736 | -628.0 | -513.3 | |
| 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. | |