SDO HMI 2014-04-09 02:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.99 | 0.00 | 10.26 | -17.84 | 329.19 | -8.08 | 148.29 | 0.2464 | 642.5 | 516.9 | |
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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 | 1.67 | 0.00 | 0.84 | -14.27 | 332.82 | -4.46 | 152.20 | 0.1622 | 1065.0 | 898.8 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -14.42 | 332.72 | -4.55 | 152.14 | 0.1653 | 901.0 | 779.9 | |
| 0.00 | 1.67 | 0.00 | 0.85 | -16.36 | 332.30 | -4.98 | 155.06 | 0.1983 | 901.0 | 648.9 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -15.38 | 332.14 | -5.14 | 151.97 | 0.1846 | 872.0 | 666.8 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -14.41 | 332.16 | -5.11 | 149.31 | 0.1699 | 888.0 | 619.8 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -14.32 | 331.82 | -5.45 | 147.38 | 0.1716 | 828.0 | 644.1 | |
| 0.00 | 1.67 | 0.00 | 0.85 | -17.85 | 331.43 | -5.84 | 154.67 | 0.2274 | 990.0 | 788.1 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -17.94 | 329.27 | -8.01 | 147.34 | 0.2466 | 937.0 | 730.4 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -17.60 | 328.96 | -8.31 | 145.57 | 0.2447 | 881.0 | 750.0 | |
| 0.00 | 3.61 | 0.00 | 1.85 | -17.81 | 328.73 | -8.54 | 145.35 | 0.2498 | 855.0 | 658.9 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -24.59 | 328.32 | -8.96 | 156.06 | 0.3504 | -1.0 | 4.7 | |
| 0.00 | 3.17 | 0.00 | 1.68 | -22.86 | 325.32 | -11.95 | 146.75 | 0.3495 | -10.0 | 4.1 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -22.43 | 316.20 | -21.07 | 130.94 | 0.4418 | -755.0 | -629.8 | |
| 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. | |