SDO HMI 2014-12-08 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 |
| 62.17 | 366.97 | 30.99 | 182.92 | -3.74 | 1.19 | -5.24 | 125.82 | 0.1129 | 1187.7 | 399.7 | |
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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 | 1.11 | 0.00 | 0.55 | -4.33 | 5.99 | -0.44 | 174.19 | 0.0762 | 901.0 | 691.6 | |
| 0.00 | 1.45 | 0.00 | 0.72 | -4.95 | 4.33 | -2.10 | 157.04 | 0.0941 | 1007.0 | 789.4 | |
| 32.66 | 356.92 | 16.28 | 177.90 | -3.88 | 1.49 | -4.94 | 128.19 | 0.1099 | 1500.5 | 408.9 | |
| 0.51 | -3.00 | 0.26 | -3.00 | -4.32 | 1.33 | -5.10 | 130.40 | 0.1168 | 895.0 | 999999 | |
| 1.54 | -3.00 | 0.76 | -3.00 | -3.41 | 1.28 | -5.15 | 123.55 | 0.1080 | 987.2 | 999999 | |
| 2.47 | -3.00 | 1.23 | -3.00 | -3.38 | 1.07 | -5.36 | 122.29 | 0.1107 | 1138.3 | 999999 | |
| 24.99 | -3.00 | 12.46 | -3.00 | -3.55 | 0.86 | -5.57 | 122.63 | 0.1155 | 1455.1 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.51 | -4.74 | 0.47 | -5.96 | 128.58 | 0.1330 | 776.0 | 567.3 | |
| 0.00 | 1.11 | 0.00 | 0.55 | -1.81 | 359.21 | -7.22 | 104.09 | 0.1301 | 827.0 | 605.5 | |
| 0.00 | 1.02 | 0.00 | 0.51 | -2.02 | 358.76 | -7.67 | 104.76 | 0.1385 | -862.0 | -658.3 | |
| 0.00 | 1.79 | 0.00 | 0.90 | -5.09 | 358.31 | -8.12 | 122.24 | 0.1670 | -819.0 | -636.2 | |
| 0.00 | 1.36 | 0.00 | 0.68 | -4.35 | 358.26 | -8.17 | 118.16 | 0.1614 | 619.0 | 446.4 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -4.41 | 357.93 | -8.50 | 117.55 | 0.1669 | -790.0 | -514.2 | |
| 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. | |