SDO HMI 2014-04-08 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 |
| 0.00 | 20.01 | 0.00 | 10.33 | -20.28 | 352.54 | 3.72 | 192.64 | 0.2718 | -443.5 | -307.5 | |
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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 | 1.15 | 0.00 | 0.63 | -23.39 | 9.62 | 20.79 | 227.06 | 0.4469 | 879.0 | 634.1 | |
| 0.00 | 1.67 | 0.00 | 0.86 | -16.73 | 0.25 | 11.42 | 225.55 | 0.2669 | 548.0 | 342.9 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -18.11 | 355.95 | 7.13 | 209.48 | 0.2406 | -799.0 | -681.1 | |
| 0.00 | 1.41 | 0.00 | 0.72 | -18.70 | 355.85 | 7.02 | 207.92 | 0.2484 | -833.0 | -720.3 | |
| 0.00 | 0.70 | 0.00 | 0.36 | -17.99 | 355.76 | 6.93 | 209.07 | 0.2373 | -962.0 | -817.4 | |
| 0.00 | 2.20 | 0.00 | 1.16 | -25.32 | 356.04 | 7.22 | 199.02 | 0.3501 | 1.0 | -0.8 | |
| 0.00 | 1.50 | 0.00 | 0.79 | -26.21 | 352.23 | 3.41 | 188.82 | 0.3493 | 10.0 | 0.5 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -22.39 | 352.04 | 3.21 | 190.48 | 0.2863 | -661.0 | -484.1 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -19.01 | 349.78 | 0.95 | 184.04 | 0.2246 | -828.0 | -631.3 | |
| 0.00 | 2.38 | 0.00 | 1.20 | -15.89 | 349.64 | 0.82 | 184.62 | 0.1710 | -933.0 | -744.1 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -17.48 | 349.58 | 0.76 | 183.67 | 0.1982 | -747.0 | -598.7 | |
| 0.00 | 1.41 | 0.00 | 0.71 | -13.94 | 348.83 | 0.01 | 180.06 | 0.1367 | -981.0 | -742.6 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -17.57 | 348.11 | -0.72 | 176.55 | 0.1997 | -884.0 | -696.9 | |
| 0.00 | 2.38 | 0.00 | 1.26 | -25.03 | 340.78 | -8.05 | 158.68 | 0.3505 | -19.0 | -3.9 | |
| 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. | |