SDO HMI 2014-02-25 05:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.52 | 230.75 | 84.40 | 422.22 | -13.13 | 107.33 | -75.18 | 101.66 | 0.9620 | -61.1 | -347.5 | |
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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 | 1.81 | 0.00 | 1.63 | -15.27 | 125.08 | -57.43 | 103.60 | 0.8386 | 476.0 | 396.4 | |
| 0.00 | 1.03 | 0.00 | 0.90 | -11.49 | 126.35 | -56.15 | 99.05 | 0.8263 | 659.0 | 478.8 | |
| 0.00 | 0.52 | 0.00 | 0.46 | -11.16 | 126.07 | -56.44 | 98.66 | 0.8291 | 478.0 | 375.8 | |
| 0.00 | 0.95 | 0.00 | 0.82 | -4.58 | 127.32 | -55.18 | 90.58 | 0.8206 | 324.0 | 379.2 | |
| 0.00 | 0.69 | 0.00 | 0.63 | -3.24 | 125.14 | -57.37 | 89.25 | 0.8430 | 343.0 | 271.1 | |
| 0.69 | 1.72 | 1.05 | 2.62 | -17.72 | 110.22 | -72.29 | 106.33 | 0.9470 | -18.5 | -6.0 | |
| 0.00 | 0.60 | 0.00 | 0.83 | -15.16 | 112.47 | -70.04 | 103.54 | 0.9347 | -348.0 | -383.4 | |
| 1.64 | 3.96 | 2.40 | 5.81 | -12.42 | 111.23 | -71.28 | 100.67 | 0.9427 | -577.4 | -505.7 | |
| 0.00 | 1.55 | 0.00 | 2.30 | -12.03 | 111.00 | -71.50 | 100.27 | 0.9441 | -28.0 | 57.0 | |
| 0.00 | 0.60 | 0.00 | 1.00 | -13.45 | 108.82 | -73.69 | 101.90 | 0.9553 | -333.0 | -338.3 | |
| 11.37 | 211.98 | 20.44 | 394.45 | -14.12 | 107.29 | -75.22 | 102.70 | 0.9624 | -665.8 | -360.0 | |
| 0.00 | 2.15 | 0.00 | 4.25 | -15.03 | 105.66 | -76.85 | 103.74 | 0.9693 | -396.0 | -323.2 | |
| 0.00 | 3.19 | 0.00 | 6.52 | -14.85 | 105.17 | -77.33 | 103.59 | 0.9713 | -436.0 | -404.0 | |
| 32.82 | -11.00 | 60.51 | -11.00 | -12.74 | 106.98 | -75.53 | 101.28 | 0.9643 | 140.6 | 999999 | |
| 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. | |