SDO HMI 2014-11-09 14:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 9.31 | 0.00 | 6.79 | -10.29 | 337.24 | -45.42 | 107.47 | 0.7363 | -56.3 | -113.0 | |
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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 | 0.95 | 0.00 | 0.63 | -8.26 | 342.12 | -40.54 | 106.39 | 0.6728 | 651.0 | 502.8 | |
| 0.00 | 0.43 | 0.00 | 0.29 | -9.61 | 341.85 | -40.80 | 108.22 | 0.6806 | 623.0 | 587.2 | |
| 0.00 | 0.69 | 0.00 | 0.48 | -10.42 | 339.98 | -42.68 | 108.61 | 0.7058 | 339.0 | 368.2 | |
| 0.00 | 1.21 | 0.00 | 0.85 | -11.72 | 339.66 | -43.00 | 110.24 | 0.7141 | 583.0 | 474.9 | |
| 0.00 | 0.60 | 0.00 | 0.42 | -6.41 | 338.77 | -43.89 | 102.68 | 0.7085 | 467.0 | 449.6 | |
| 0.00 | 0.86 | 0.00 | 0.65 | -12.05 | 335.58 | -47.08 | 109.16 | 0.7605 | -609.0 | -523.3 | |
| 0.00 | 0.43 | 0.00 | 0.33 | -11.84 | 335.36 | -47.30 | 108.82 | 0.7623 | -416.0 | -455.0 | |
| 0.00 | 0.60 | 0.00 | 0.46 | -11.57 | 335.33 | -47.33 | 108.47 | 0.7618 | -541.0 | -487.6 | |
| 0.00 | 2.07 | 0.00 | 1.56 | -10.04 | 335.29 | -47.37 | 106.50 | 0.7579 | -658.0 | -503.4 | |
| 0.00 | 0.69 | 0.00 | 0.53 | -10.58 | 334.78 | -47.88 | 107.04 | 0.7649 | -539.0 | -520.6 | |
| 0.00 | 0.78 | 0.00 | 0.59 | -10.04 | 334.66 | -48.00 | 106.31 | 0.7647 | -519.0 | -421.8 | |
| 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. | |