SDO HMI 2014-04-24 02:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.17 | 0.00 | 6.90 | -20.38 | 164.02 | 24.83 | 235.51 | 0.4832 | -663.0 | -563.7 | |
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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 | 0.80 | 0.00 | 0.48 | -16.64 | 171.97 | 32.77 | 247.30 | 0.5643 | -739.0 | -633.1 | |
| 0.00 | 1.60 | 0.00 | 0.99 | -27.49 | 170.19 | 31.00 | 229.13 | 0.6064 | -667.0 | -519.8 | |
| 0.00 | 1.42 | 0.00 | 0.85 | -26.50 | 166.77 | 27.57 | 227.66 | 0.5625 | -452.0 | -327.1 | |
| 0.00 | 0.62 | 0.00 | 0.33 | -9.87 | 161.60 | 22.40 | 256.00 | 0.3886 | -243.0 | -458.1 | |
| 0.00 | 1.51 | 0.00 | 0.83 | -17.25 | 162.27 | 23.07 | 239.45 | 0.4364 | -708.0 | -602.9 | |
| 0.00 | 1.69 | 0.00 | 0.93 | -17.44 | 161.88 | 22.68 | 238.66 | 0.4326 | -839.0 | -690.8 | |
| 0.00 | 1.24 | 0.00 | 0.68 | -17.01 | 161.83 | 22.63 | 239.50 | 0.4288 | -801.0 | -715.3 | |
| 0.00 | 0.62 | 0.00 | 0.34 | -18.10 | 160.67 | 21.47 | 236.01 | 0.4214 | -760.0 | -662.0 | |
| 0.00 | 0.71 | 0.00 | 0.39 | -19.75 | 160.65 | 21.45 | 232.67 | 0.4347 | -646.0 | -434.8 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -18.08 | 160.39 | 21.19 | 235.75 | 0.4176 | -758.0 | -607.1 | |
| 0.00 | 1.07 | 0.00 | 0.60 | -24.96 | 160.18 | 20.98 | 222.95 | 0.4784 | -680.0 | -545.6 | |
| 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. | |