SDO HMI 2014-04-22 03:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.29 | 0.00 | 11.32 | -15.63 | 163.75 | -1.32 | 176.10 | 0.2017 | -810.9 | -673.3 | |
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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 | 1.95 | 0.00 | 0.98 | -11.73 | 173.28 | 8.21 | 229.97 | 0.1834 | -935.0 | -733.5 | |
| 0.00 | 1.24 | 0.00 | 0.62 | -12.42 | 171.40 | 6.33 | 219.87 | 0.1688 | -868.0 | -610.2 | |
| 0.00 | 0.89 | 0.00 | 0.47 | -25.79 | 169.47 | 4.40 | 191.02 | 0.3628 | -41.0 | -76.6 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -20.43 | 167.75 | 2.69 | 189.39 | 0.2704 | -931.0 | -762.5 | |
| 0.00 | 4.00 | 0.00 | 1.98 | -7.39 | 165.49 | 0.43 | 190.22 | 0.0419 | -791.0 | -634.2 | |
| 0.00 | 1.15 | 0.00 | 0.57 | -9.43 | 162.78 | -2.29 | 152.79 | 0.0867 | -1003.0 | -826.6 | |
| 0.00 | 0.98 | 0.00 | 0.49 | -8.59 | 162.66 | -2.41 | 146.19 | 0.0750 | -926.0 | -720.7 | |
| 0.00 | 2.13 | 0.00 | 1.09 | -19.89 | 161.49 | -3.57 | 167.13 | 0.2643 | -745.0 | -597.3 | |
| 0.00 | 1.78 | 0.00 | 0.91 | -19.02 | 161.32 | -3.74 | 165.68 | 0.2507 | -826.0 | -562.0 | |
| 0.00 | 1.78 | 0.00 | 0.91 | -19.42 | 160.74 | -4.33 | 164.02 | 0.2598 | -883.0 | -719.3 | |
| 0.00 | 1.60 | 0.00 | 0.80 | -10.07 | 159.34 | -5.73 | 131.89 | 0.1327 | -878.0 | -740.3 | |
| 0.00 | 3.64 | 0.00 | 1.91 | -23.39 | 158.20 | -6.86 | 160.82 | 0.3354 | -904.0 | -811.1 | |
| 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. | |