SDO HMI 2014-04-11 05:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.80 | 143.53 | 41.72 | 192.88 | 4.28 | 241.54 | -67.68 | 82.99 | 0.9302 | -116.8 | -36.0 | |
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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 |
| 3.35 | 81.47 | 4.07 | 99.60 | 4.95 | 244.15 | -65.08 | 81.87 | 0.9144 | -912.6 | -325.9 | |
| 3.00 | -1.00 | 3.61 | -1.00 | 4.48 | 244.23 | -65.00 | 82.36 | 0.9133 | -781.3 | 999999 | |
| 1.94 | -1.00 | 2.35 | -1.00 | 4.74 | 244.11 | -65.11 | 82.10 | 0.9144 | -964.2 | 999999 | |
| 2.21 | -1.00 | 2.73 | -1.00 | 4.87 | 243.65 | -65.58 | 82.03 | 0.9178 | -342.6 | 999999 | |
| 3.97 | -1.00 | 4.89 | -1.00 | 4.54 | 243.64 | -65.59 | 82.40 | 0.9175 | -466.3 | 999999 | |
| 3.27 | -1.00 | 4.04 | -1.00 | 4.12 | 243.56 | -65.67 | 82.86 | 0.9176 | -382.4 | 999999 | |
| 0.00 | 1.24 | 0.00 | 1.59 | 3.85 | 242.54 | -66.68 | 83.31 | 0.9242 | 230.0 | 231.9 | |
| 0.00 | 0.53 | 0.00 | 0.72 | 4.26 | 241.21 | -68.02 | 83.08 | 0.9331 | 36.0 | 6.8 | |
| 0.00 | 0.79 | 0.00 | 1.08 | 3.38 | 241.11 | -68.12 | 84.02 | 0.9330 | 280.0 | 262.4 | |
| 1.06 | 4.33 | 1.50 | 6.12 | 3.14 | 240.22 | -69.00 | 84.41 | 0.9382 | 331.6 | 258.6 | |
| 1.06 | 47.84 | 1.53 | 71.56 | 3.54 | 239.82 | -69.41 | 84.04 | 0.9409 | 609.9 | 287.2 | |
| 7.68 | -11.00 | 11.56 | -11.00 | 3.89 | 239.05 | -70.18 | 83.78 | 0.9456 | 435.1 | 999999 | |
| 1.32 | 3.80 | 2.21 | 6.34 | 5.20 | 237.23 | -71.99 | 82.67 | 0.9562 | 242.1 | 210.2 | |
| 1.94 | 3.53 | 3.23 | 5.87 | 4.77 | 237.25 | -71.98 | 83.11 | 0.9558 | 246.6 | 165.1 | |
| 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. | |