SDO HMI 2014-12-02 03:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.55 | 25.63 | 3.92 | 19.22 | -15.48 | 39.13 | -46.37 | 111.68 | 0.7521 | 104.0 | -38.5 | |
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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 |
| 5.55 | 10.08 | 3.92 | 7.12 | -16.46 | 42.80 | -42.69 | 114.23 | 0.7155 | 822.0 | 586.0 | |
| 0.00 | 0.51 | 0.00 | 0.37 | -18.40 | 41.58 | -43.92 | 116.26 | 0.7363 | 638.0 | 518.0 | |
| 0.00 | 0.94 | 0.00 | 0.69 | -16.39 | 40.29 | -45.21 | 113.15 | 0.7429 | 512.0 | 469.3 | |
| 0.00 | 1.79 | 0.00 | 1.36 | -15.23 | 38.54 | -46.96 | 111.06 | 0.7580 | 668.0 | 551.0 | |
| 0.00 | 0.77 | 0.00 | 0.59 | -15.82 | 38.04 | -47.45 | 111.65 | 0.7650 | 439.0 | 370.2 | |
| 0.00 | 0.85 | 0.00 | 0.65 | -15.42 | 38.08 | -47.42 | 111.15 | 0.7635 | 525.0 | 369.3 | |
| 0.00 | 0.85 | 0.00 | 0.66 | -13.81 | 37.27 | -48.23 | 108.85 | 0.7677 | -524.0 | -406.0 | |
| 0.00 | 0.60 | 0.00 | 0.47 | -15.53 | 36.23 | -49.27 | 110.72 | 0.7829 | -654.0 | -567.3 | |
| 0.00 | 1.20 | 0.00 | 0.94 | -14.67 | 36.27 | -49.23 | 109.66 | 0.7803 | -439.0 | -433.1 | |
| 0.00 | 4.02 | 0.00 | 3.17 | -14.40 | 36.12 | -49.38 | 109.27 | 0.7812 | -797.0 | -597.1 | |
| 0.00 | 0.94 | 0.00 | 0.73 | -12.63 | 36.48 | -49.02 | 107.13 | 0.7732 | -615.0 | -514.9 | |
| 0.00 | 1.45 | 0.00 | 1.15 | -14.46 | 35.91 | -49.59 | 109.29 | 0.7835 | -452.0 | -432.6 | |
| 0.00 | 1.03 | 0.00 | 0.83 | -15.08 | 35.33 | -50.17 | 109.90 | 0.7908 | -482.0 | -423.1 | |
| 0.00 | 0.60 | 0.00 | 0.49 | -16.11 | 34.79 | -50.71 | 111.01 | 0.7988 | -282.0 | -257.9 | |
| 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. | |