SDO HMI 2014-09-29 06:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.06 | 12.08 | 0.78 | 8.80 | -15.01 | 165.97 | -41.86 | 117.96 | 0.7343 | 400.4 | 358.7 | |
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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 |
| 0.00 | 0.79 | 0.00 | 0.56 | -23.76 | 173.57 | -34.25 | 133.55 | 0.7131 | 525.0 | 473.6 | |
| 0.00 | 0.88 | 0.00 | 0.60 | -17.17 | 171.35 | -36.47 | 124.07 | 0.6880 | 637.0 | 512.1 | |
| 0.00 | 0.97 | 0.00 | 0.75 | -22.58 | 166.19 | -41.63 | 127.04 | 0.7708 | 477.0 | 385.2 | |
| 0.53 | 2.56 | 0.37 | 1.79 | -13.27 | 167.17 | -40.65 | 116.44 | 0.7105 | 661.2 | 560.9 | |
| 0.00 | 0.62 | 0.00 | 0.48 | -21.50 | 164.83 | -42.99 | 125.02 | 0.7770 | 367.0 | 345.3 | |
| 0.00 | 1.32 | 0.00 | 0.95 | -14.59 | 166.64 | -41.19 | 117.83 | 0.7229 | 252.0 | 326.1 | |
| 0.00 | 0.97 | 0.00 | 0.65 | -6.21 | 167.46 | -40.36 | 107.03 | 0.6756 | 601.0 | 425.3 | |
| 0.00 | 0.44 | 0.00 | 0.30 | -7.42 | 166.25 | -41.57 | 108.18 | 0.6949 | 567.0 | 480.0 | |
| 0.00 | 0.79 | 0.00 | 0.60 | -16.20 | 163.84 | -43.98 | 118.29 | 0.7596 | 677.0 | 519.8 | |
| 0.00 | 1.15 | 0.00 | 0.88 | -17.06 | 163.33 | -44.50 | 119.05 | 0.7687 | 494.0 | 417.2 | |
| 0.53 | 1.59 | 0.41 | 1.24 | -10.15 | 160.02 | -47.80 | 109.16 | 0.7743 | -557.3 | -435.8 | |
| 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. | |