SDO HMI 2014-07-09 21:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.67 | 0.00 | 13.42 | -19.92 | 221.99 | 18.72 | 215.85 | 0.5419 | -483.5 | -404.9 | |
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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 | 1.54 | 0.00 | 1.03 | -15.28 | 240.90 | 37.63 | 241.97 | 0.6695 | 700.0 | 638.7 | |
| 0.00 | 1.45 | 0.00 | 0.96 | -16.00 | 240.41 | 37.14 | 240.70 | 0.6679 | 635.0 | 519.2 | |
| 0.00 | 1.91 | 0.00 | 1.17 | -16.78 | 233.01 | 29.74 | 234.16 | 0.5880 | -701.0 | -555.2 | |
| 0.00 | 2.27 | 0.00 | 1.36 | -17.08 | 230.37 | 27.10 | 231.26 | 0.5604 | -455.0 | -372.8 | |
| 0.00 | 1.72 | 0.00 | 0.97 | -12.24 | 227.21 | 23.95 | 235.71 | 0.4820 | -641.0 | -542.7 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -13.20 | 226.59 | 23.32 | 233.33 | 0.4825 | -852.0 | -727.6 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -13.33 | 226.43 | 23.17 | 232.94 | 0.4816 | -729.0 | -523.7 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -15.36 | 225.76 | 22.49 | 228.79 | 0.4924 | -668.0 | -559.0 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -21.90 | 216.20 | 12.93 | 205.67 | 0.4812 | -555.0 | -538.0 | |
| 0.00 | 1.72 | 0.00 | 0.98 | -22.61 | 215.56 | 12.29 | 203.91 | 0.4867 | -808.0 | -660.6 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -25.61 | 210.84 | 7.57 | 193.61 | 0.5066 | -745.0 | -574.6 | |
| 0.00 | 3.99 | 0.00 | 2.35 | -28.63 | 205.18 | 1.91 | 183.13 | 0.5390 | -780.0 | -665.8 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -27.73 | 203.03 | -0.24 | 179.60 | 0.5248 | -687.0 | -568.7 | |
| 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. | |