SDO HMI 2014-04-08 22:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.32 | 0.00 | 9.78 | -19.86 | 323.37 | -16.11 | 135.02 | 0.3570 | 245.3 | 147.1 | |
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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 | 1.32 | 0.00 | 0.67 | -14.16 | 332.76 | -6.72 | 141.19 | 0.1820 | 1036.0 | 876.1 | |
| 0.00 | 1.59 | 0.00 | 0.81 | -17.82 | 331.29 | -8.19 | 146.45 | 0.2465 | 979.0 | 829.3 | |
| 0.00 | 2.29 | 0.00 | 1.18 | -17.85 | 329.21 | -10.27 | 140.46 | 0.2677 | 940.0 | 721.6 | |
| 0.00 | 1.41 | 0.00 | 0.72 | -17.57 | 329.07 | -10.41 | 139.37 | 0.2657 | 945.0 | 735.8 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -17.72 | 328.68 | -10.80 | 138.72 | 0.2719 | 737.0 | 715.8 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -23.06 | 327.75 | -11.73 | 147.53 | 0.3500 | 22.0 | 17.7 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -18.25 | 327.71 | -11.77 | 137.68 | 0.2891 | 836.0 | 646.5 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -18.82 | 326.07 | -13.41 | 135.49 | 0.3144 | 800.0 | 653.2 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -21.60 | 317.02 | -22.46 | 127.75 | 0.4511 | -710.0 | -525.4 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -23.09 | 316.48 | -23.00 | 129.86 | 0.4703 | -176.0 | -241.5 | |
| 0.00 | 2.82 | 0.00 | 1.58 | -22.52 | 316.54 | -22.94 | 128.93 | 0.4646 | -791.0 | -651.1 | |
| 0.00 | 1.94 | 0.00 | 1.08 | -22.22 | 316.07 | -23.41 | 127.87 | 0.4679 | -792.0 | -505.9 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -23.16 | 315.86 | -23.62 | 129.32 | 0.4781 | -637.0 | -559.2 | |
| 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. | |