SDO HMI 2014-11-02 23:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.83 | 0.00 | 10.17 | -19.72 | 77.87 | -32.11 | 128.44 | 0.6397 | 612.1 | 510.4 | |
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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 | 1.04 | 0.00 | 0.59 | -14.05 | 85.86 | -24.13 | 127.77 | 0.5037 | 513.0 | 409.2 | |
| 0.00 | 1.56 | 0.00 | 0.94 | -20.90 | 84.82 | -25.17 | 136.45 | 0.5789 | 760.0 | 616.9 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -20.85 | 81.47 | -28.52 | 132.95 | 0.6118 | 605.0 | 473.6 | |
| 0.00 | 0.86 | 0.00 | 0.56 | -20.02 | 76.84 | -33.15 | 127.85 | 0.6529 | 690.0 | 524.7 | |
| 0.00 | 2.16 | 0.00 | 1.42 | -20.35 | 76.65 | -33.34 | 128.12 | 0.6574 | 661.0 | 524.8 | |
| 0.00 | 0.95 | 0.00 | 0.62 | -20.13 | 76.55 | -33.44 | 127.76 | 0.6568 | 550.0 | 472.2 | |
| 0.00 | 1.30 | 0.00 | 0.85 | -20.17 | 76.35 | -33.64 | 127.66 | 0.6592 | 425.0 | 414.9 | |
| 0.00 | 0.95 | 0.00 | 0.62 | -19.75 | 76.22 | -33.77 | 127.02 | 0.6575 | 748.0 | 614.2 | |
| 0.00 | 1.73 | 0.00 | 1.13 | -19.56 | 76.19 | -33.79 | 126.75 | 0.6565 | 644.0 | 557.8 | |
| 0.00 | 1.56 | 0.00 | 1.02 | -19.76 | 75.99 | -34.00 | 126.86 | 0.6600 | 689.0 | 583.1 | |
| 0.00 | 1.21 | 0.00 | 0.80 | -19.74 | 75.77 | -34.22 | 126.66 | 0.6622 | 609.0 | 478.4 | |
| 0.00 | 1.56 | 0.00 | 1.03 | -19.68 | 75.55 | -34.44 | 126.43 | 0.6641 | 451.0 | 404.2 | |
| 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. | |