SDO HMI 2014-07-01 23:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.51 | 95.09 | 53.94 | 137.59 | -7.98 | 238.97 | -69.07 | 99.63 | 0.9391 | 111.3 | -97.8 | |
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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 | 0.82 | 0.00 | 1.06 | -8.41 | 241.33 | -66.71 | 100.36 | 0.9253 | 307.0 | 306.6 | |
| 2.18 | 4.09 | 2.81 | 5.27 | -8.13 | 241.35 | -66.70 | 100.06 | 0.9250 | 542.2 | 437.9 | |
| 1.45 | 3.00 | 1.91 | 3.94 | -8.58 | 240.95 | -67.09 | 100.50 | 0.9279 | 377.9 | 306.9 | |
| 0.00 | 1.27 | 0.00 | 1.68 | -8.07 | 240.73 | -67.31 | 99.92 | 0.9289 | 416.0 | 361.2 | |
| 9.81 | 51.85 | 13.02 | 71.88 | -7.39 | 240.63 | -67.41 | 99.18 | 0.9291 | 578.9 | -108.6 | |
| 2.72 | -5.00 | 3.71 | -5.00 | -7.36 | 239.99 | -68.06 | 99.08 | 0.9331 | 285.4 | 999999 | |
| 4.00 | 7.45 | 5.62 | 10.51 | -8.94 | 239.40 | -68.64 | 100.69 | 0.9377 | 246.9 | -43.5 | |
| 1.73 | -5.00 | 2.37 | -5.00 | -7.61 | 239.90 | -68.14 | 99.34 | 0.9338 | 125.3 | 999999 | |
| 4.45 | -5.00 | 6.33 | -5.00 | -7.25 | 239.09 | -68.96 | 98.86 | 0.9385 | 295.4 | 999999 | |
| 0.00 | 1.36 | 0.00 | 1.99 | -8.39 | 238.58 | -69.47 | 100.01 | 0.9422 | -353.0 | -376.3 | |
| 0.00 | 0.73 | 0.00 | 1.14 | -9.51 | 237.25 | -70.79 | 101.04 | 0.9503 | -470.0 | -433.9 | |
| 11.17 | 19.34 | 18.17 | 31.31 | -8.55 | 236.44 | -71.60 | 99.95 | 0.9540 | -394.1 | -329.1 | |
| 0.00 | 3.27 | 0.00 | 5.42 | -9.06 | 236.20 | -71.85 | 100.45 | 0.9555 | 161.0 | 164.6 | |
| 0.00 | 1.27 | 0.00 | 2.07 | -8.00 | 236.39 | -71.65 | 99.36 | 0.9539 | -168.0 | -199.4 | |
| 0.00 | 0.64 | 0.00 | 1.32 | -10.83 | 232.66 | -75.38 | 101.91 | 0.9723 | -345.0 | -352.9 | |
| 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. | |