SDO HMI 2014-07-07 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.78 | 155.15 | 18.80 | 86.84 | 6.67 | 203.75 | -27.65 | 82.44 | 0.4667 | -646.1 | -371.0 | |
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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 | 1.09 | 0.00 | 0.60 | 5.93 | 205.64 | -25.76 | 83.73 | 0.4367 | 301.0 | 196.0 | |
| 7.81 | 10.53 | 4.32 | 5.83 | 7.17 | 205.06 | -26.34 | 81.06 | 0.4475 | -1049.2 | -680.5 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 4.45 | 204.82 | -26.59 | 87.18 | 0.4486 | -720.0 | -557.7 | |
| 25.97 | 125.92 | 14.48 | 70.21 | 6.47 | 204.10 | -27.30 | 82.79 | 0.4612 | -1281.3 | -436.4 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 7.01 | 203.69 | -27.71 | 81.72 | 0.4683 | -496.0 | -333.1 | |
| 0.00 | 4.54 | 0.00 | 2.55 | 8.69 | 203.50 | -27.90 | 78.22 | 0.4745 | -755.0 | -709.1 | |
| 0.00 | 1.63 | 0.00 | 0.92 | 8.30 | 202.97 | -28.43 | 79.18 | 0.4816 | -721.0 | -572.0 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 7.92 | 200.45 | -30.96 | 80.55 | 0.5185 | 636.0 | 476.9 | |
| 0.00 | 1.18 | 0.00 | 0.69 | 6.19 | 199.57 | -31.84 | 84.01 | 0.5294 | 685.0 | 546.5 | |
| 0.00 | 1.36 | 0.00 | 0.81 | 8.40 | 198.11 | -33.30 | 80.13 | 0.5533 | 612.0 | 564.0 | |
| 0.00 | 1.09 | 0.00 | 0.65 | 7.68 | 197.58 | -33.82 | 81.52 | 0.5598 | 641.0 | 563.4 | |
| 0.00 | 1.54 | 0.00 | 0.93 | 9.03 | 196.78 | -34.63 | 79.29 | 0.5733 | 732.0 | 579.9 | |
| 0.00 | 1.00 | 0.00 | 0.60 | 7.41 | 196.75 | -34.65 | 82.13 | 0.5714 | 581.0 | 445.7 | |
| 0.00 | 0.91 | 0.00 | 0.55 | 9.06 | 196.59 | -34.82 | 79.28 | 0.5760 | 373.0 | 402.3 | |
| 0.00 | 1.09 | 0.00 | 0.66 | 5.94 | 196.76 | -34.65 | 84.70 | 0.5701 | 671.0 | 586.8 | |
| 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. | |