SDO HMI 2014-04-05 23:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.85 | 20.96 | 0.93 | 10.60 | -8.50 | 7.03 | -11.49 | 102.59 | 0.2062 | -23.6 | 83.0 | |
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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 | 0.97 | 0.00 | 0.48 | -8.08 | 11.52 | -7.00 | 104.99 | 0.1254 | 940.0 | 785.4 | |
| 1.85 | 6.24 | 0.93 | 3.13 | -9.83 | 9.77 | -8.75 | 112.83 | 0.1634 | 1008.8 | 788.4 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -9.76 | 9.37 | -9.15 | 111.61 | 0.1693 | 956.0 | 815.4 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -2.03 | 8.32 | -10.20 | 67.74 | 0.1921 | 819.0 | 635.3 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -11.52 | 6.04 | -12.48 | 113.92 | 0.2327 | 753.0 | 503.0 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -12.20 | 5.54 | -12.98 | 115.76 | 0.2449 | 710.0 | 574.3 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -6.56 | 5.69 | -12.82 | 91.97 | 0.2216 | -863.0 | -741.3 | |
| 0.00 | 1.41 | 0.00 | 0.72 | -7.26 | 5.08 | -13.43 | 94.99 | 0.2324 | -918.0 | -667.2 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -6.90 | 5.03 | -13.49 | 93.42 | 0.2330 | -900.0 | -738.1 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -7.43 | 4.74 | -13.78 | 95.62 | 0.2384 | -848.0 | -652.5 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -7.04 | 4.66 | -13.86 | 93.96 | 0.2394 | -990.0 | -836.2 | |
| 0.00 | 1.76 | 0.00 | 0.90 | -6.63 | 4.01 | -14.50 | 92.22 | 0.2501 | -889.0 | -791.0 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -12.00 | 3.59 | -14.93 | 112.29 | 0.2736 | 742.0 | 587.0 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -7.34 | 3.49 | -15.03 | 94.93 | 0.2593 | -779.0 | -567.1 | |
| 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. | |