SDO HMI 2014-04-21 13:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.77 | 78.19 | 14.88 | 69.35 | -23.32 | 117.57 | -55.23 | 114.77 | 0.8327 | 431.5 | 389.1 | |
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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 |
| 8.96 | 59.81 | 7.81 | 52.20 | -23.17 | 118.40 | -54.40 | 114.75 | 0.8252 | 938.2 | 470.3 | |
| 5.15 | -1.00 | 4.56 | -1.00 | -23.45 | 117.83 | -54.97 | 114.97 | 0.8308 | 431.7 | 999999 | |
| 0.00 | 2.22 | 0.00 | 1.97 | -22.53 | 117.59 | -55.21 | 113.83 | 0.8314 | 521.0 | 405.1 | |
| 0.00 | 0.27 | 0.00 | 0.24 | -22.92 | 117.12 | -55.68 | 114.20 | 0.8361 | 283.0 | 275.0 | |
| 0.00 | 1.69 | 0.00 | 1.55 | -23.99 | 116.36 | -56.44 | 115.33 | 0.8444 | 567.0 | 542.9 | |
| 0.00 | 1.06 | 0.00 | 0.98 | -23.74 | 116.41 | -56.39 | 115.04 | 0.8435 | 500.0 | 343.7 | |
| 0.00 | 1.24 | 0.00 | 1.15 | -24.00 | 116.05 | -56.75 | 115.29 | 0.8470 | 570.0 | 501.3 | |
| 0.00 | 1.33 | 0.00 | 1.21 | -22.68 | 116.56 | -56.24 | 113.83 | 0.8406 | 255.0 | 249.5 | |
| 1.33 | 4.44 | 1.25 | 4.20 | -23.98 | 115.33 | -57.47 | 115.14 | 0.8530 | 427.5 | 252.0 | |
| 0.00 | 0.62 | 0.00 | 0.56 | -21.82 | 116.62 | -56.18 | 112.82 | 0.8389 | -506.0 | -478.0 | |
| 0.00 | 1.51 | 0.00 | 1.46 | -24.01 | 114.31 | -58.49 | 114.99 | 0.8613 | -232.0 | -179.6 | |
| 0.00 | 0.27 | 0.00 | 0.25 | -23.11 | 114.88 | -57.91 | 114.05 | 0.8554 | -190.0 | -198.7 | |
| 1.33 | 2.22 | 1.26 | 2.10 | -22.75 | 114.88 | -57.92 | 113.64 | 0.8550 | -522.5 | -427.4 | |
| 0.00 | 1.51 | 0.00 | 1.48 | -24.00 | 113.80 | -59.00 | 114.91 | 0.8653 | -204.0 | -174.1 | |
| 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. | |