SDO HMI 2014-03-29 22:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.49 | 0.00 | 7.98 | -27.25 | 85.27 | -26.15 | 134.47 | 0.5329 | -30.2 | -31.2 | |
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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 | 1.23 | 0.00 | 0.64 | -21.67 | 102.25 | -9.17 | 150.35 | 0.3007 | 625.0 | 445.4 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -20.64 | 97.95 | -13.48 | 138.26 | 0.3290 | 751.0 | 582.1 | |
| 0.00 | 1.84 | 0.00 | 1.03 | -26.95 | 90.95 | -20.47 | 138.55 | 0.4729 | 913.0 | 691.0 | |
| 0.00 | 0.96 | 0.00 | 0.54 | -26.88 | 90.78 | -20.64 | 138.23 | 0.4739 | 642.0 | 553.5 | |
| 0.00 | 0.61 | 0.00 | 0.35 | -27.18 | 89.60 | -21.82 | 137.26 | 0.4891 | 592.0 | 460.3 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -25.98 | 87.02 | -24.40 | 132.47 | 0.5055 | 505.0 | 509.5 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -27.69 | 82.21 | -29.21 | 130.71 | 0.5722 | -594.0 | -433.0 | |
| 0.00 | 0.96 | 0.00 | 0.60 | -30.20 | 79.80 | -31.62 | 132.43 | 0.6161 | -648.0 | -417.6 | |
| 0.00 | 0.96 | 0.00 | 0.61 | -29.97 | 78.62 | -32.80 | 131.25 | 0.6265 | -645.0 | -500.5 | |
| 0.00 | 1.84 | 0.00 | 1.17 | -30.03 | 78.06 | -33.37 | 130.95 | 0.6326 | -738.0 | -605.2 | |
| 0.00 | 0.53 | 0.00 | 0.34 | -29.81 | 77.68 | -33.74 | 130.39 | 0.6350 | -511.0 | -499.8 | |
| 0.00 | 1.14 | 0.00 | 0.73 | -28.19 | 76.85 | -34.57 | 127.58 | 0.6334 | -640.0 | -526.5 | |
| 0.00 | 0.44 | 0.00 | 0.28 | -27.36 | 75.04 | -36.38 | 125.33 | 0.6480 | -645.0 | -499.4 | |
| 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. | |