SDO HMI 2014-07-03 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.08 | 39.95 | 12.10 | 33.84 | -16.04 | 233.10 | -51.24 | 112.40 | 0.8118 | -55.8 | 29.6 | |
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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 | 1.00 | 0.00 | 0.74 | -15.87 | 239.78 | -44.57 | 114.70 | 0.7453 | 419.0 | 358.3 | |
| 0.00 | 1.91 | 0.00 | 1.41 | -15.52 | 239.79 | -44.56 | 114.26 | 0.7438 | 696.0 | 536.2 | |
| 4.09 | 9.53 | 3.24 | 7.57 | -14.31 | 235.61 | -48.74 | 111.15 | 0.7832 | 774.9 | 555.8 | |
| 1.09 | -3.00 | 0.87 | -3.00 | -14.60 | 235.48 | -48.87 | 111.46 | 0.7854 | 641.5 | 999999 | |
| 0.00 | 2.00 | 0.00 | 1.60 | -14.49 | 235.17 | -49.17 | 111.22 | 0.7881 | 444.0 | 376.8 | |
| 0.00 | 0.82 | 0.00 | 0.66 | -14.69 | 234.92 | -49.43 | 111.38 | 0.7913 | 205.0 | 234.9 | |
| 0.00 | 1.18 | 0.00 | 0.96 | -14.76 | 234.70 | -49.65 | 111.39 | 0.7937 | 491.0 | 369.8 | |
| 0.00 | 1.18 | 0.00 | 0.98 | -16.23 | 234.11 | -50.24 | 112.96 | 0.8038 | 524.0 | 419.5 | |
| 0.00 | 1.63 | 0.00 | 1.37 | -15.94 | 233.36 | -50.99 | 112.36 | 0.8101 | -468.0 | -482.5 | |
| 0.00 | 0.73 | 0.00 | 0.63 | -16.39 | 232.01 | -52.34 | 112.45 | 0.8239 | -638.0 | -567.8 | |
| 0.00 | 1.27 | 0.00 | 1.11 | -16.72 | 231.83 | -52.52 | 112.77 | 0.8264 | -508.0 | -379.1 | |
| 0.00 | 1.45 | 0.00 | 1.30 | -17.40 | 231.07 | -53.28 | 113.32 | 0.8350 | -223.0 | -244.2 | |
| 8.90 | 17.25 | 7.99 | 15.51 | -17.02 | 230.80 | -53.55 | 112.80 | 0.8365 | -656.3 | -274.3 | |
| 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. | |