SDO HMI 2014-09-18 06:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.53 | 24.79 | 0.28 | 13.08 | 7.49 | 333.52 | -19.49 | 86.05 | 0.3329 | -195.6 | -2.7 | |
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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 | 2.22 | 0.00 | 1.11 | 8.74 | 343.60 | -9.41 | 79.74 | 0.1650 | -880.0 | -774.5 | |
| 0.00 | 1.07 | 0.00 | 0.54 | 8.72 | 342.67 | -10.34 | 80.63 | 0.1806 | -964.0 | -809.8 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 9.22 | 342.35 | -10.66 | 78.18 | 0.1874 | -838.0 | -648.9 | |
| 0.00 | 1.60 | 0.00 | 0.81 | 9.84 | 341.77 | -11.24 | 75.61 | 0.1992 | -887.0 | -631.9 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 10.17 | 341.66 | -11.35 | 74.13 | 0.2022 | -891.0 | -719.9 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 10.03 | 338.56 | -14.45 | 77.59 | 0.2527 | -751.0 | -578.6 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 9.07 | 337.81 | -15.20 | 81.70 | 0.2628 | -863.0 | -640.7 | |
| 0.00 | 1.07 | 0.00 | 0.55 | 4.20 | 335.44 | -17.57 | 98.64 | 0.3059 | -833.0 | -669.8 | |
| 0.53 | 1.86 | 0.28 | 0.97 | 5.03 | 334.97 | -18.03 | 95.75 | 0.3113 | 1080.3 | 807.8 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 11.08 | 334.70 | -18.31 | 76.39 | 0.3186 | -844.0 | -694.2 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 7.67 | 329.71 | -23.30 | 87.22 | 0.3941 | 771.0 | 580.4 | |
| 0.00 | 2.04 | 0.00 | 1.10 | 7.66 | 329.44 | -23.56 | 87.25 | 0.3984 | 785.0 | 663.3 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 7.60 | 327.17 | -25.84 | 87.33 | 0.4343 | 815.0 | 610.9 | |
| 0.00 | 3.91 | 0.00 | 2.15 | 8.01 | 326.94 | -26.07 | 86.38 | 0.4378 | 605.0 | 515.5 | |
| 0.00 | 3.82 | 0.00 | 2.11 | 3.92 | 326.64 | -26.37 | 95.61 | 0.4471 | 404.0 | 355.6 | |
| 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. | |