SDO HMI 2014-04-21 09:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.09 | 80.43 | 20.49 | 74.81 | -23.25 | 117.80 | -57.19 | 114.33 | 0.8494 | 526.5 | 353.7 | |
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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 | 0.62 | 0.00 | 0.57 | -25.38 | 118.58 | -56.41 | 116.95 | 0.8464 | 395.0 | 380.0 | |
| 0.00 | 0.53 | 0.00 | 0.50 | -25.30 | 118.02 | -56.97 | 116.75 | 0.8509 | 453.0 | 414.2 | |
| 15.18 | 64.00 | 13.93 | 58.72 | -23.19 | 118.46 | -56.53 | 114.36 | 0.8439 | 821.4 | 398.9 | |
| 1.95 | -3.00 | 1.82 | -3.00 | -23.46 | 117.79 | -57.20 | 114.57 | 0.8499 | 395.7 | 999999 | |
| 2.57 | -3.00 | 2.40 | -3.00 | -23.30 | 117.78 | -57.21 | 114.38 | 0.8498 | 357.9 | 999999 | |
| 0.00 | 1.51 | 0.00 | 1.41 | -22.55 | 117.61 | -57.38 | 113.47 | 0.8501 | 480.0 | 377.9 | |
| 0.44 | 1.60 | 0.42 | 1.51 | -22.96 | 117.15 | -57.84 | 113.88 | 0.8546 | 309.4 | 225.2 | |
| 0.44 | 1.51 | 0.41 | 1.41 | -22.13 | 117.64 | -57.35 | 112.99 | 0.8494 | 412.0 | 330.9 | |
| 0.00 | 1.60 | 0.00 | 1.50 | -22.31 | 117.52 | -57.47 | 113.19 | 0.8506 | 217.0 | 251.5 | |
| 0.00 | 3.91 | 0.00 | 3.90 | -23.90 | 115.32 | -59.67 | 114.68 | 0.8704 | 606.0 | 432.2 | |
| 0.00 | 1.33 | 0.00 | 1.31 | -22.70 | 115.81 | -59.18 | 113.38 | 0.8651 | 131.0 | 72.9 | |
| 1.51 | 2.75 | 1.51 | 2.76 | -22.74 | 115.00 | -59.98 | 113.31 | 0.8716 | -460.0 | -371.1 | |
| 0.00 | 1.07 | 0.00 | 1.22 | -25.84 | 111.14 | -63.84 | 116.29 | 0.9028 | -104.0 | -169.5 | |
| 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. | |