SDO HMI 2014-09-26 01:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.89 | 23.24 | 2.62 | 15.73 | 6.67 | 206.88 | -43.27 | 87.67 | 0.6834 | 33.6 | 207.4 | |
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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 | 0.35 | 0.00 | 0.23 | 5.90 | 210.01 | -40.15 | 89.09 | 0.6437 | -480.0 | -526.0 | |
| 0.00 | 0.80 | 0.00 | 0.52 | 6.24 | 209.66 | -40.50 | 88.54 | 0.6481 | -697.0 | -494.8 | |
| 0.00 | 1.41 | 0.00 | 0.92 | 7.04 | 209.42 | -40.73 | 87.29 | 0.6507 | -643.0 | -556.3 | |
| 1.50 | 3.18 | 0.98 | 2.07 | 6.46 | 209.36 | -40.80 | 88.18 | 0.6519 | -600.8 | -423.0 | |
| 0.53 | 1.77 | 0.35 | 1.16 | 5.79 | 208.94 | -41.22 | 89.16 | 0.6579 | -640.0 | -463.9 | |
| 0.00 | 0.44 | 0.00 | 0.29 | 6.59 | 208.70 | -41.45 | 87.92 | 0.6604 | -417.0 | -488.6 | |
| 0.00 | 0.97 | 0.00 | 0.65 | 7.07 | 207.96 | -42.20 | 87.14 | 0.6697 | -556.0 | -381.9 | |
| 0.00 | 1.59 | 0.00 | 1.08 | 5.69 | 206.90 | -43.26 | 89.10 | 0.6843 | 695.0 | 553.9 | |
| 0.00 | 0.97 | 0.00 | 0.66 | 6.50 | 206.49 | -43.67 | 87.88 | 0.6889 | 715.0 | 589.5 | |
| 0.00 | 2.03 | 0.00 | 1.40 | 6.69 | 205.83 | -44.33 | 87.55 | 0.6969 | 782.0 | 607.2 | |
| 0.00 | 0.80 | 0.00 | 0.55 | 7.26 | 205.42 | -44.73 | 86.71 | 0.7017 | 535.0 | 469.2 | |
| 1.86 | 6.36 | 1.29 | 4.40 | 6.98 | 205.41 | -44.74 | 87.10 | 0.7019 | 631.5 | 616.2 | |
| 0.00 | 1.24 | 0.00 | 0.86 | 8.69 | 204.88 | -45.28 | 84.64 | 0.7078 | 644.0 | 453.9 | |
| 0.00 | 1.33 | 0.00 | 0.94 | 5.55 | 204.23 | -45.93 | 89.01 | 0.7175 | 551.0 | 453.7 | |
| 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. | |