SDO HMI 2014-09-22 03:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 10.80 | 0.00 | 6.21 | -17.20 | 285.63 | -16.22 | 147.17 | 0.4850 | 670.1 | 541.0 | |
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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 | 1.06 | 0.00 | 0.55 | -8.20 | 297.48 | -4.37 | 163.99 | 0.2749 | 720.0 | 513.7 | |
| 0.00 | 1.33 | 0.00 | 0.71 | -11.03 | 291.13 | -10.73 | 149.38 | 0.3602 | 742.0 | 570.3 | |
| 0.00 | 1.24 | 0.00 | 0.66 | -11.20 | 290.78 | -11.08 | 148.80 | 0.3654 | 843.0 | 598.6 | |
| 0.00 | 0.80 | 0.00 | 0.41 | -1.86 | 288.87 | -12.98 | 124.11 | 0.2723 | 767.0 | 603.4 | |
| 0.00 | 0.71 | 0.00 | 0.43 | -23.84 | 285.18 | -16.67 | 152.73 | 0.5747 | 442.0 | 456.1 | |
| 0.00 | 1.15 | 0.00 | 0.69 | -22.04 | 282.41 | -19.45 | 147.26 | 0.5728 | 652.0 | 568.9 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -21.53 | 282.20 | -19.65 | 146.47 | 0.5684 | 754.0 | 535.4 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -17.39 | 282.29 | -19.56 | 141.89 | 0.5197 | 502.0 | 493.8 | |
| 0.00 | 1.24 | 0.00 | 0.78 | -23.95 | 280.14 | -21.71 | 146.32 | 0.6119 | 693.0 | 548.7 | |
| 0.00 | 0.80 | 0.00 | 0.50 | -23.77 | 280.10 | -21.75 | 146.10 | 0.6103 | 650.0 | 487.8 | |
| 0.00 | 0.44 | 0.00 | 0.28 | -24.10 | 279.83 | -22.02 | 146.10 | 0.6160 | 606.0 | 535.2 | |
| 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. | |