SDO HMI 2014-07-02 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.44 | 0.00 | 16.69 | 5.93 | 270.65 | -34.09 | 83.82 | 0.5521 | -192.5 | -319.7 | |
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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 | 1.45 | 0.00 | 0.80 | 4.41 | 279.04 | -25.71 | 86.03 | 0.4353 | -864.0 | -768.8 | |
| 0.00 | 8.81 | 0.00 | 4.85 | 4.69 | 278.99 | -25.75 | 85.41 | 0.4362 | -935.0 | -761.9 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 6.41 | 278.40 | -26.34 | 81.60 | 0.4476 | -758.0 | -637.6 | |
| 0.00 | 1.09 | 0.00 | 0.60 | 4.77 | 278.48 | -26.26 | 85.28 | 0.4443 | -640.0 | -501.7 | |
| 0.00 | 2.27 | 0.00 | 1.26 | 6.68 | 278.18 | -26.56 | 81.06 | 0.4515 | -711.0 | -460.8 | |
| 0.00 | 3.91 | 0.00 | 2.21 | 5.44 | 275.78 | -28.96 | 84.17 | 0.4864 | -356.0 | -604.6 | |
| 0.00 | 0.91 | 0.00 | 0.52 | 4.33 | 274.18 | -30.56 | 86.55 | 0.5100 | -816.0 | -497.2 | |
| 0.00 | 1.91 | 0.00 | 1.28 | 8.18 | 262.63 | -42.11 | 81.12 | 0.6741 | 501.0 | 456.0 | |
| 0.00 | 0.82 | 0.00 | 0.56 | 8.33 | 260.79 | -43.95 | 81.10 | 0.6974 | 506.0 | 393.0 | |
| 0.00 | 0.73 | 0.00 | 0.50 | 8.26 | 260.54 | -44.20 | 81.23 | 0.7004 | 439.0 | 462.4 | |
| 0.00 | 1.09 | 0.00 | 0.76 | 8.00 | 260.01 | -44.73 | 81.66 | 0.7066 | 137.0 | 237.3 | |
| 0.00 | 1.00 | 0.00 | 0.83 | 7.92 | 251.49 | -53.26 | 82.35 | 0.8030 | 215.0 | 323.0 | |
| 0.00 | 0.91 | 0.00 | 0.78 | 6.08 | 249.95 | -54.79 | 84.67 | 0.8181 | 244.0 | 300.4 | |
| 0.00 | 1.09 | 0.00 | 0.94 | 5.70 | 249.69 | -55.06 | 85.14 | 0.8208 | 343.0 | 260.4 | |
| 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. | |