SDO HMI 2014-01-14 03:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 88.16 | 482.56 | 44.72 | 244.96 | -16.51 | 12.96 | -3.67 | 163.78 | 0.2198 | 1039.4 | 388.1 | |
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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 | 0.77 | 0.00 | 0.39 | -19.07 | 18.22 | 1.59 | 185.95 | 0.2549 | 739.0 | 584.0 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -18.46 | 17.72 | 1.09 | 184.27 | 0.2438 | 936.0 | 689.3 | |
| 46.33 | 303.07 | 23.50 | 153.72 | -16.61 | 13.74 | -2.89 | 167.09 | 0.2170 | 1425.8 | 449.9 | |
| 4.93 | -3.00 | 2.50 | -3.00 | -16.67 | 13.07 | -3.57 | 164.28 | 0.2208 | 1109.2 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -16.78 | 12.72 | -3.91 | 163.02 | 0.2244 | 792.0 | 673.5 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -15.34 | 12.42 | -4.21 | 159.44 | 0.2027 | 806.0 | 640.7 | |
| 6.21 | 163.65 | 3.15 | 83.12 | -16.60 | 12.23 | -4.40 | 160.77 | 0.2240 | 1123.8 | 344.5 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -14.86 | 12.18 | -4.45 | 157.47 | 0.1966 | 977.0 | 822.9 | |
| 30.69 | -7.00 | 15.57 | -7.00 | -16.24 | 12.06 | -4.57 | 159.47 | 0.2192 | 1310.9 | 999999 | |
| 0.00 | 2.04 | 0.00 | 1.05 | -16.91 | 7.38 | -9.25 | 144.64 | 0.2669 | -790.0 | -721.9 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -15.46 | 7.11 | -9.52 | 140.30 | 0.2506 | -855.0 | -699.6 | |
| 0.00 | 1.96 | 0.00 | 1.00 | -15.39 | 6.16 | -10.48 | 137.44 | 0.2604 | -897.0 | -707.7 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -18.29 | 4.47 | -12.16 | 140.28 | 0.3145 | -829.0 | -622.4 | |
| 0.00 | 2.30 | 0.00 | 1.19 | -17.68 | 4.35 | -12.28 | 138.68 | 0.3083 | -669.0 | -690.5 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -18.40 | 3.50 | -13.13 | 138.41 | 0.3261 | -700.0 | -591.8 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -11.22 | 3.30 | -13.33 | 117.92 | 0.2571 | -783.0 | -589.1 | |
| 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. | |