SDO HMI 2014-07-04 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.27 | 29.43 | 9.64 | 22.43 | -16.33 | 232.36 | -45.91 | 114.80 | 0.7605 | -199.8 | 17.9 | |
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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 | 0.82 | 0.00 | 0.55 | -16.69 | 239.86 | -38.41 | 118.91 | 0.6822 | 578.0 | 454.1 | |
| 0.00 | 0.27 | 0.00 | 0.19 | -17.64 | 239.58 | -38.69 | 120.01 | 0.6903 | 487.0 | 463.3 | |
| 0.73 | 1.54 | 0.51 | 1.09 | -14.13 | 236.05 | -42.22 | 113.54 | 0.7131 | 806.9 | 726.6 | |
| 0.00 | 1.36 | 0.00 | 0.96 | -14.36 | 235.87 | -42.40 | 113.76 | 0.7161 | 744.0 | 570.7 | |
| 0.82 | 2.09 | 0.58 | 1.48 | -14.40 | 235.60 | -42.67 | 113.70 | 0.7192 | 744.3 | 552.3 | |
| 0.00 | 2.09 | 0.00 | 1.50 | -14.96 | 235.12 | -43.15 | 114.22 | 0.7268 | 567.0 | 390.7 | |
| 0.00 | 0.91 | 0.00 | 0.67 | -15.96 | 234.28 | -43.99 | 115.13 | 0.7399 | 535.0 | 442.3 | |
| 0.00 | 1.18 | 0.00 | 0.86 | -14.52 | 234.18 | -44.09 | 113.24 | 0.7353 | 514.0 | 380.5 | |
| 0.00 | 2.63 | 0.00 | 1.97 | -16.03 | 233.19 | -45.08 | 114.75 | 0.7517 | -819.0 | -651.7 | |
| 0.00 | 0.73 | 0.00 | 0.55 | -16.17 | 233.01 | -45.26 | 114.85 | 0.7541 | -486.0 | -436.9 | |
| 10.72 | 15.81 | 8.55 | 12.61 | -17.22 | 230.25 | -48.02 | 115.02 | 0.7858 | -758.9 | -310.3 | |
| 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. | |