SDO HMI 2014-01-06 07:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.03 | 0.00 | 10.78 | -17.30 | 79.06 | -40.74 | 112.01 | 0.6737 | 285.1 | 317.7 | |
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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 | 2.89 | 0.00 | 1.84 | -19.16 | 83.29 | -36.51 | 116.45 | 0.6300 | 870.0 | 652.4 | |
| 0.00 | 1.87 | 0.00 | 1.19 | -18.72 | 83.09 | -36.71 | 115.70 | 0.6306 | 795.0 | 643.7 | |
| 0.00 | 0.68 | 0.00 | 0.44 | -19.28 | 82.43 | -37.37 | 116.23 | 0.6409 | 511.0 | 401.0 | |
| 0.00 | 1.10 | 0.00 | 0.72 | -13.49 | 80.34 | -39.46 | 106.69 | 0.6476 | -689.0 | -560.8 | |
| 0.00 | 1.10 | 0.00 | 0.72 | -14.77 | 79.99 | -39.81 | 108.53 | 0.6553 | 350.0 | 372.8 | |
| 0.00 | 1.44 | 0.00 | 0.95 | -13.24 | 79.51 | -40.29 | 106.11 | 0.6575 | -609.0 | -450.6 | |
| 0.00 | 0.59 | 0.00 | 0.39 | -12.88 | 79.47 | -40.33 | 105.55 | 0.6573 | -600.0 | -499.4 | |
| 0.00 | 1.19 | 0.00 | 0.81 | -16.28 | 77.79 | -42.01 | 110.08 | 0.6863 | 685.0 | 543.7 | |
| 0.00 | 1.19 | 0.00 | 0.83 | -17.12 | 76.63 | -43.17 | 110.90 | 0.7023 | 566.0 | 393.9 | |
| 0.00 | 0.93 | 0.00 | 0.64 | -15.94 | 76.84 | -42.96 | 109.31 | 0.6968 | 516.0 | 502.5 | |
| 0.00 | 0.85 | 0.00 | 0.59 | -16.95 | 76.21 | -43.59 | 110.54 | 0.7066 | 328.0 | 288.3 | |
| 0.00 | 1.27 | 0.00 | 0.96 | -20.97 | 73.08 | -46.72 | 114.98 | 0.7523 | 503.0 | 516.3 | |
| 0.00 | 0.93 | 0.00 | 0.70 | -21.18 | 72.90 | -46.90 | 115.20 | 0.7548 | 480.0 | 401.9 | |
| 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. | |