SDO HMI 2014-03-29 00:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.56 | 0.00 | 11.93 | -26.09 | 88.12 | -35.39 | 124.95 | 0.6241 | 29.7 | 86.8 | |
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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 | 4.29 | 0.00 | 2.38 | -23.04 | 101.56 | -21.95 | 130.01 | 0.4510 | 967.0 | 766.1 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -22.10 | 97.00 | -26.51 | 123.79 | 0.4995 | 670.0 | 562.6 | |
| 0.00 | 0.96 | 0.00 | 0.56 | -21.27 | 94.30 | -29.21 | 120.24 | 0.5285 | 570.0 | 429.4 | |
| 0.00 | 1.31 | 0.00 | 0.81 | -26.89 | 90.90 | -32.61 | 126.94 | 0.6035 | 718.0 | 616.5 | |
| 0.00 | 1.66 | 0.00 | 1.03 | -26.84 | 90.56 | -32.95 | 126.63 | 0.6070 | 787.0 | 499.1 | |
| 0.00 | 1.23 | 0.00 | 0.78 | -26.64 | 88.93 | -34.58 | 125.30 | 0.6239 | 478.0 | 408.9 | |
| 0.00 | 1.66 | 0.00 | 1.15 | -28.64 | 82.94 | -40.57 | 124.88 | 0.6981 | -601.0 | -443.4 | |
| 0.00 | 1.23 | 0.00 | 0.85 | -28.12 | 82.64 | -40.87 | 124.06 | 0.6989 | -546.0 | -455.4 | |
| 0.00 | 0.79 | 0.00 | 0.54 | -27.57 | 82.59 | -40.92 | 123.28 | 0.6970 | -502.0 | -430.7 | |
| 0.00 | 1.40 | 0.00 | 0.98 | -28.32 | 81.82 | -41.69 | 123.96 | 0.7082 | -555.0 | -424.1 | |
| 0.00 | 0.79 | 0.00 | 0.55 | -27.94 | 81.87 | -41.64 | 123.47 | 0.7060 | -522.0 | -403.6 | |
| 0.00 | 1.49 | 0.00 | 1.14 | -26.92 | 75.58 | -47.93 | 119.84 | 0.7654 | -714.0 | -631.9 | |
| 0.00 | 0.79 | 0.00 | 0.61 | -27.20 | 74.70 | -48.81 | 119.94 | 0.7746 | -364.0 | -303.4 | |
| 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. | |