SDO HMI 2014-04-24 15:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.10 | 351.08 | 36.05 | 229.23 | 17.94 | 166.27 | 34.20 | 304.89 | 0.6541 | -777.7 | -288.0 | |
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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 |
| 0.27 | 331.28 | 0.17 | 216.68 | 17.45 | 166.92 | 34.86 | 303.75 | 0.6580 | -515.3 | -338.5 | |
| 54.83 | -1.00 | 35.88 | -1.00 | 17.94 | 166.42 | 34.35 | 304.77 | 0.6558 | -1223.3 | 999999 | |
| 0.00 | 1.42 | 0.00 | 0.93 | 19.02 | 165.66 | 33.60 | 306.75 | 0.6552 | -105.0 | -82.1 | |
| 0.00 | 2.75 | 0.00 | 1.75 | 17.14 | 164.58 | 32.51 | 305.11 | 0.6301 | 353.0 | 237.8 | |
| 0.00 | 3.55 | 0.00 | 2.24 | 17.73 | 163.32 | 31.25 | 306.95 | 0.6205 | 608.0 | 534.2 | |
| 0.00 | 1.42 | 0.00 | 0.90 | 18.22 | 163.30 | 31.23 | 307.62 | 0.6241 | 512.0 | 446.0 | |
| 0.00 | 2.22 | 0.00 | 1.40 | 17.95 | 163.17 | 31.11 | 307.37 | 0.6207 | 767.0 | 653.8 | |
| 0.00 | 1.60 | 0.00 | 1.01 | 18.34 | 162.99 | 30.92 | 308.04 | 0.6216 | 601.0 | 461.2 | |
| 0.00 | 1.07 | 0.00 | 0.67 | 18.11 | 162.91 | 30.84 | 307.80 | 0.6189 | 722.0 | 622.9 | |
| 0.00 | 1.60 | 0.00 | 1.01 | 18.26 | 162.72 | 30.65 | 308.18 | 0.6181 | 499.0 | 450.4 | |
| 0.00 | 1.87 | 0.00 | 1.18 | 18.52 | 162.73 | 30.66 | 308.51 | 0.6203 | 601.0 | 483.6 | |
| 0.00 | 1.24 | 0.00 | 0.78 | 17.96 | 162.55 | 30.48 | 307.92 | 0.6139 | 778.0 | 604.6 | |
| 0.00 | 0.53 | 0.00 | 0.34 | 18.88 | 162.54 | 30.48 | 309.14 | 0.6211 | 500.0 | 384.2 | |
| 0.00 | 0.53 | 0.00 | 0.34 | 20.36 | 162.49 | 30.42 | 311.12 | 0.6324 | 514.0 | 442.5 | |
| 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. | |