SDO HMI 2014-11-10 04:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.53 | 0.00 | 9.96 | -9.46 | 337.59 | -37.35 | 109.50 | 0.6364 | 84.2 | -8.6 | |
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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 | 1.21 | 0.00 | 0.73 | -10.03 | 342.33 | -32.61 | 112.84 | 0.5780 | 661.0 | 563.6 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -9.92 | 342.20 | -32.74 | 112.57 | 0.5791 | 719.0 | 600.6 | |
| 0.00 | 1.64 | 0.00 | 1.01 | -10.26 | 341.04 | -33.90 | 112.43 | 0.5960 | 540.0 | 432.1 | |
| 0.00 | 1.29 | 0.00 | 0.81 | -11.34 | 339.76 | -35.18 | 113.38 | 0.6178 | 663.0 | 510.8 | |
| 0.00 | 1.12 | 0.00 | 0.69 | -6.99 | 339.89 | -35.05 | 106.61 | 0.5971 | 720.0 | 593.8 | |
| 0.00 | 1.90 | 0.00 | 1.17 | -6.97 | 339.71 | -35.23 | 106.49 | 0.5994 | 712.0 | 527.7 | |
| 0.00 | 1.21 | 0.00 | 0.80 | -12.07 | 335.86 | -39.08 | 112.40 | 0.6691 | -642.0 | -541.9 | |
| 0.00 | 1.64 | 0.00 | 1.10 | -10.16 | 334.48 | -40.46 | 109.07 | 0.6782 | -395.0 | -387.9 | |
| 0.00 | 1.21 | 0.00 | 0.81 | -9.31 | 334.33 | -40.61 | 107.81 | 0.6770 | -780.0 | -693.1 | |
| 0.00 | 2.59 | 0.00 | 1.74 | -9.13 | 334.28 | -40.66 | 107.53 | 0.6770 | -618.0 | -528.9 | |
| 0.00 | 0.86 | 0.00 | 0.58 | -8.50 | 334.24 | -40.70 | 106.60 | 0.6753 | -654.0 | -605.7 | |
| 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. | |