SDO HMI 2014-07-02 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.07 | 150.02 | 37.87 | 173.29 | -8.00 | 239.49 | -63.61 | 100.36 | 0.9031 | 233.2 | -20.7 | |
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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 |
| 3.27 | 4.82 | 3.50 | 5.15 | -8.17 | 241.55 | -61.55 | 100.84 | 0.8880 | 505.7 | 449.9 | |
| 1.27 | 2.27 | 1.39 | 2.47 | -8.63 | 241.03 | -62.07 | 101.27 | 0.8926 | 444.3 | 342.3 | |
| 0.00 | 1.36 | 0.00 | 1.49 | -8.20 | 240.95 | -62.15 | 100.78 | 0.8927 | 406.0 | 348.1 | |
| 13.72 | 84.32 | 14.91 | 93.93 | -7.42 | 240.96 | -62.14 | 99.92 | 0.8919 | 788.2 | 130.3 | |
| 0.27 | -4.00 | 0.30 | -4.00 | -7.69 | 240.55 | -62.55 | 100.16 | 0.8952 | 267.0 | 999999 | |
| 4.45 | 21.26 | 5.07 | 24.39 | -8.84 | 239.81 | -63.29 | 101.33 | 0.9020 | 355.0 | -27.0 | |
| 0.00 | 1.64 | 0.00 | 1.93 | -9.17 | 238.78 | -64.32 | 101.54 | 0.9098 | -320.0 | -275.2 | |
| 2.73 | -4.00 | 3.15 | -4.00 | -7.23 | 239.16 | -63.94 | 99.46 | 0.9053 | 342.7 | 999999 | |
| 0.00 | 9.09 | 0.00 | 10.95 | -8.64 | 238.24 | -64.86 | 100.88 | 0.9131 | -745.0 | -564.4 | |
| 0.91 | -4.00 | 1.07 | -4.00 | -7.04 | 238.57 | -64.53 | 99.18 | 0.9094 | -304.9 | 999999 | |
| 0.00 | 3.91 | 0.00 | 4.90 | -9.49 | 237.26 | -65.84 | 101.67 | 0.9206 | -594.0 | -452.7 | |
| 0.00 | 1.00 | 0.00 | 1.28 | -8.74 | 236.77 | -66.33 | 100.79 | 0.9232 | -438.0 | -314.7 | |
| 0.00 | 5.27 | 0.00 | 6.68 | -8.18 | 236.88 | -66.22 | 100.20 | 0.9219 | -330.0 | -377.6 | |
| 0.00 | 4.45 | 0.00 | 5.83 | -9.05 | 236.18 | -66.92 | 101.04 | 0.9272 | -159.0 | -114.5 | |
| 6.45 | 9.09 | 8.48 | 11.95 | -8.59 | 236.03 | -67.07 | 100.53 | 0.9278 | -428.4 | -123.7 | |
| 0.00 | 1.54 | 0.00 | 2.34 | -9.33 | 232.99 | -70.11 | 100.95 | 0.9465 | -299.0 | -282.9 | |
| 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. | |