SDO HMI 2014-04-08 08:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.01 | 0.00 | 15.64 | -19.72 | 323.27 | -23.91 | 123.08 | 0.4522 | 38.4 | -39.1 | |
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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 | 2.20 | 0.00 | 1.15 | -16.93 | 332.24 | -14.94 | 127.79 | 0.3135 | 897.0 | 741.4 | |
| 0.00 | 1.94 | 0.00 | 1.01 | -17.07 | 331.80 | -15.38 | 127.41 | 0.3206 | 948.0 | 706.6 | |
| 0.00 | 2.73 | 0.00 | 1.44 | -17.38 | 330.76 | -16.42 | 126.50 | 0.3371 | 719.0 | 719.3 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -15.14 | 328.55 | -18.64 | 117.76 | 0.3502 | 574.0 | 441.7 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -17.26 | 328.07 | -19.12 | 122.48 | 0.3723 | 872.0 | 834.6 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -17.46 | 327.74 | -19.44 | 122.56 | 0.3783 | 722.0 | 655.5 | |
| 0.00 | 1.67 | 0.00 | 0.89 | -17.00 | 327.63 | -19.55 | 121.33 | 0.3764 | 733.0 | 639.9 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -19.11 | 326.57 | -20.62 | 124.83 | 0.4071 | 702.0 | 716.3 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -20.31 | 321.06 | -26.13 | 121.75 | 0.4877 | -722.0 | -574.7 | |
| 0.00 | 4.67 | 0.00 | 2.64 | -18.95 | 320.52 | -26.67 | 118.77 | 0.4862 | -755.0 | -677.5 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -20.95 | 318.76 | -28.42 | 121.10 | 0.5212 | -667.0 | -573.4 | |
| 0.00 | 1.67 | 0.00 | 1.01 | -25.91 | 317.33 | -29.86 | 128.13 | 0.5715 | -581.0 | -370.2 | |
| 0.00 | 1.94 | 0.00 | 1.13 | -20.90 | 318.41 | -28.78 | 120.76 | 0.5254 | -762.0 | -572.8 | |
| 0.00 | 0.71 | 0.00 | 0.42 | -23.35 | 317.09 | -30.09 | 123.92 | 0.5569 | -636.0 | -490.1 | |
| 0.00 | 2.91 | 0.00 | 1.73 | -22.95 | 316.81 | -30.37 | 123.08 | 0.5578 | -777.0 | -610.9 | |
| 0.00 | 1.59 | 0.00 | 0.95 | -23.58 | 316.19 | -30.99 | 123.67 | 0.5691 | -652.0 | -496.0 | |
| 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. | |