SDO HMI 2014-07-07 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 |
| 35.52 | 157.64 | 20.93 | 93.50 | 6.63 | 203.62 | -33.31 | 83.31 | 0.5512 | -745.1 | -369.0 | |
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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 |
| 0.00 | 1.09 | 0.00 | 0.63 | 8.28 | 206.17 | -30.75 | 79.77 | 0.5161 | -769.0 | -562.2 | |
| 5.09 | 12.08 | 2.97 | 7.07 | 7.08 | 204.94 | -31.99 | 82.30 | 0.5325 | -1056.3 | -568.7 | |
| 2.36 | -2.00 | 1.38 | -2.00 | 7.20 | 204.82 | -32.11 | 82.09 | 0.5344 | -881.1 | 999999 | |
| 27.62 | 127.11 | 16.31 | 75.05 | 6.53 | 203.96 | -32.97 | 83.45 | 0.5463 | -1221.3 | -421.1 | |
| 0.00 | 2.00 | 0.00 | 1.19 | 8.53 | 203.38 | -33.54 | 79.91 | 0.5571 | -682.0 | -501.2 | |
| 0.00 | 1.45 | 0.00 | 0.87 | 7.58 | 203.13 | -33.79 | 81.67 | 0.5593 | -774.0 | -584.8 | |
| 0.45 | 1.91 | 0.27 | 1.14 | 7.57 | 202.91 | -34.01 | 81.72 | 0.5624 | -691.8 | -566.3 | |
| 0.00 | 0.73 | 0.00 | 0.44 | 8.15 | 202.78 | -34.14 | 80.71 | 0.5650 | -563.0 | -456.4 | |
| 0.00 | 4.09 | 0.00 | 2.49 | 3.79 | 201.41 | -35.51 | 88.44 | 0.5820 | -144.0 | -265.9 | |
| 0.00 | 1.18 | 0.00 | 0.74 | 6.78 | 199.49 | -37.43 | 83.47 | 0.6097 | 594.0 | 501.8 | |
| 0.00 | 0.36 | 0.00 | 0.23 | 6.12 | 198.18 | -38.74 | 84.63 | 0.6272 | 568.0 | 540.8 | |
| 0.00 | 1.27 | 0.00 | 0.82 | 7.96 | 197.44 | -39.48 | 81.78 | 0.6384 | 737.0 | 626.4 | |
| 0.00 | 1.64 | 0.00 | 1.06 | 9.38 | 196.86 | -40.06 | 79.65 | 0.6477 | 513.0 | 463.0 | |
| 0.00 | 1.73 | 0.00 | 1.12 | 6.92 | 196.71 | -40.21 | 83.47 | 0.6473 | 635.0 | 493.8 | |
| 0.00 | 1.00 | 0.00 | 0.65 | 7.46 | 196.49 | -40.43 | 82.65 | 0.6506 | 502.0 | 415.0 | |
| 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. | |