SDO HMI 2014-11-14 12:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.98 | 33.21 | 7.30 | 23.88 | 8.69 | 4.22 | 46.38 | 279.25 | 0.7271 | -161.0 | 32.5 | |
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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 |
| 7.66 | 10.92 | 5.69 | 8.12 | 8.13 | 6.07 | 48.23 | 278.29 | 0.7485 | -763.6 | -498.6 | |
| 0.00 | 1.12 | 0.00 | 0.83 | 8.58 | 6.14 | 48.31 | 278.88 | 0.7497 | -350.0 | -292.5 | |
| 0.00 | 3.35 | 0.00 | 2.46 | 8.19 | 5.40 | 47.57 | 278.42 | 0.7408 | -772.0 | -669.1 | |
| 0.00 | 1.29 | 0.00 | 0.94 | 8.37 | 5.21 | 47.37 | 278.69 | 0.7387 | -687.0 | -583.6 | |
| 0.00 | 0.95 | 0.00 | 0.69 | 8.15 | 4.82 | 46.98 | 278.42 | 0.7340 | -639.0 | -594.1 | |
| 0.00 | 0.86 | 0.00 | 0.62 | 5.88 | 4.08 | 46.25 | 275.34 | 0.7240 | -334.0 | -352.8 | |
| 0.00 | 0.86 | 0.00 | 0.61 | 9.75 | 3.52 | 45.68 | 280.76 | 0.7201 | 518.0 | 457.6 | |
| 0.00 | 2.24 | 0.00 | 1.57 | 10.78 | 2.63 | 44.79 | 282.32 | 0.7108 | 457.0 | 423.9 | |
| 0.00 | 0.95 | 0.00 | 0.66 | 10.45 | 2.40 | 44.56 | 281.90 | 0.7076 | 571.0 | 475.3 | |
| 0.00 | 0.95 | 0.00 | 0.66 | 10.28 | 2.24 | 44.40 | 281.68 | 0.7054 | 762.0 | 654.6 | |
| 1.98 | 6.80 | 1.37 | 4.69 | 8.67 | 1.93 | 44.10 | 279.44 | 0.6997 | 809.7 | 613.4 | |
| 0.34 | 2.92 | 0.24 | 2.03 | 9.78 | 1.90 | 44.06 | 281.03 | 0.7006 | 744.8 | 610.5 | |
| 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. | |