SDO HMI 2014-02-26 03:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.57 | 25.06 | 3.35 | 18.42 | 5.99 | 124.64 | -45.79 | 75.00 | 0.7403 | -445.5 | -170.2 | |
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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 | 1.29 | 9.85 | 127.63 | -42.80 | 68.76 | 0.7205 | -605.0 | -428.1 | |
| 0.00 | 0.69 | 0.00 | 0.49 | 8.81 | 127.54 | -42.89 | 70.17 | 0.7173 | -653.0 | -534.5 | |
| 0.00 | 1.12 | 0.00 | 0.80 | 8.08 | 127.15 | -43.28 | 71.31 | 0.7189 | -644.0 | -545.8 | |
| 0.00 | 1.12 | 0.00 | 0.79 | 7.53 | 127.14 | -43.29 | 72.05 | 0.7170 | -461.0 | -463.9 | |
| 0.00 | 1.03 | 0.00 | 0.73 | 6.90 | 127.01 | -43.42 | 72.94 | 0.7162 | -711.0 | -536.9 | |
| 0.00 | 1.12 | 0.00 | 0.79 | 7.22 | 126.89 | -43.54 | 72.57 | 0.7187 | -755.0 | -594.4 | |
| 0.00 | 0.86 | 0.00 | 0.62 | 6.99 | 126.41 | -44.02 | 73.07 | 0.7233 | -277.0 | -273.7 | |
| 0.00 | 1.21 | 0.00 | 0.87 | 8.22 | 125.96 | -44.47 | 71.64 | 0.7329 | -591.0 | -496.7 | |
| 0.00 | 1.03 | 0.00 | 0.75 | 8.08 | 125.85 | -44.58 | 71.87 | 0.7336 | -529.0 | -421.1 | |
| 0.00 | 0.86 | 0.00 | 0.63 | 7.81 | 125.42 | -45.01 | 72.39 | 0.7374 | -281.0 | -199.7 | |
| 0.00 | 1.55 | 0.00 | 1.12 | 4.54 | 125.27 | -45.16 | 76.75 | 0.7285 | -446.0 | -405.2 | |
| 4.57 | 7.06 | 3.35 | 5.18 | 3.98 | 124.15 | -46.28 | 77.87 | 0.7398 | -773.2 | -520.8 | |
| 0.00 | 1.72 | 0.00 | 1.31 | 4.97 | 122.58 | -47.85 | 77.07 | 0.7602 | 684.0 | 605.7 | |
| 0.00 | 3.88 | 0.00 | 3.05 | 5.06 | 120.75 | -49.68 | 77.52 | 0.7801 | 576.0 | 515.4 | |
| 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. | |