SDO HMI 2014-12-05 01:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.66 | 0.00 | 10.51 | 14.15 | 16.38 | -30.68 | 64.07 | 0.5505 | -549.9 | -415.3 | |
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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 | 1.88 | 0.00 | 1.04 | 15.23 | 24.25 | -22.81 | 55.56 | 0.4554 | -916.0 | -686.9 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 16.33 | 20.15 | -26.91 | 57.65 | 0.5163 | -660.0 | -478.0 | |
| 0.00 | 0.68 | 0.00 | 0.39 | 14.12 | 19.31 | -27.74 | 62.20 | 0.5124 | -727.0 | -645.5 | |
| 0.00 | 1.37 | 0.00 | 0.79 | 14.03 | 18.70 | -28.35 | 62.83 | 0.5200 | -688.0 | -600.6 | |
| 0.00 | 1.37 | 0.00 | 0.79 | 13.73 | 18.26 | -28.80 | 63.69 | 0.5242 | -672.0 | -525.7 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 13.42 | 17.95 | -29.11 | 64.45 | 0.5266 | -705.0 | -612.6 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 13.24 | 17.66 | -29.40 | 64.97 | 0.5294 | -745.0 | -606.2 | |
| 0.00 | 1.02 | 0.00 | 0.60 | 13.12 | 17.29 | -29.76 | 65.43 | 0.5338 | -758.0 | -627.0 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 13.66 | 17.15 | -29.91 | 64.57 | 0.5386 | -685.0 | -515.8 | |
| 0.00 | 2.22 | 0.00 | 1.28 | 9.60 | 17.42 | -29.64 | 71.76 | 0.5155 | -667.0 | -540.5 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 11.06 | 16.74 | -30.32 | 69.42 | 0.5313 | -780.0 | -652.1 | |
| 0.00 | 1.19 | 0.00 | 0.72 | 15.37 | 15.50 | -31.56 | 62.81 | 0.5696 | -630.0 | -482.9 | |
| 0.00 | 1.02 | 0.00 | 0.62 | 13.72 | 13.71 | -33.35 | 66.57 | 0.5843 | -549.0 | -456.3 | |
| 0.00 | 1.28 | 0.00 | 0.86 | 20.69 | 8.70 | -38.36 | 59.04 | 0.6794 | 322.0 | 309.5 | |
| 0.00 | 1.19 | 0.00 | 0.83 | 15.77 | 5.00 | -42.06 | 67.52 | 0.7001 | 611.0 | 505.1 | |
| 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. | |