SDO HMI 2014-12-04 04:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.67 | 46.53 | 26.94 | 66.49 | -15.72 | 127.23 | 68.64 | 252.95 | 0.9375 | 143.4 | 18.1 | |
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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 |
| 5.98 | 9.14 | 10.84 | 16.58 | -15.18 | 132.02 | 73.43 | 254.06 | 0.9632 | 302.1 | 66.1 | |
| 3.16 | 22.71 | 4.52 | 32.24 | -15.65 | 127.40 | 68.81 | 253.09 | 0.9399 | -190.8 | 75.4 | |
| 4.61 | -2.00 | 6.50 | -2.00 | -15.16 | 127.05 | 68.46 | 253.58 | 0.9375 | 375.4 | 999999 | |
| 2.13 | -2.00 | 3.00 | -2.00 | -15.34 | 127.01 | 68.42 | 253.38 | 0.9374 | 378.2 | 999999 | |
| 0.00 | 1.62 | 0.00 | 2.21 | -15.24 | 126.36 | 67.77 | 253.41 | 0.9335 | 465.0 | 343.9 | |
| 0.00 | 1.54 | 0.00 | 1.94 | -15.35 | 124.46 | 65.86 | 253.05 | 0.9217 | 139.0 | 213.5 | |
| 0.00 | 1.96 | 0.00 | 2.54 | -17.30 | 124.75 | 66.16 | 251.00 | 0.9253 | 443.0 | 295.5 | |
| 0.00 | 1.11 | 0.00 | 1.34 | -15.55 | 123.17 | 64.58 | 252.66 | 0.9133 | -89.0 | -100.9 | |
| 0.00 | 0.94 | 0.00 | 1.13 | -15.70 | 123.05 | 64.46 | 252.47 | 0.9126 | -260.0 | -236.7 | |
| 0.00 | 0.85 | 0.00 | 1.02 | -16.38 | 122.74 | 64.14 | 251.69 | 0.9112 | -333.0 | -288.4 | |
| 0.85 | 5.29 | 1.00 | 6.14 | -17.68 | 121.92 | 63.33 | 250.15 | 0.9070 | -368.4 | -397.7 | |
| 0.94 | -11.00 | 1.08 | -11.00 | -17.55 | 121.63 | 63.04 | 250.24 | 0.9048 | -514.8 | 999999 | |
| 0.00 | 1.37 | 0.00 | 1.35 | -20.44 | 115.95 | 57.36 | 245.86 | 0.8667 | -559.0 | -483.3 | |
| 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. | |