SDO HMI 2014-04-06 15:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.82 | 0.00 | 11.58 | -16.44 | 353.54 | -16.20 | 128.56 | 0.3557 | -517.6 | -470.8 | |
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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 | 1.14 | 0.00 | 0.60 | -23.00 | 16.60 | 6.86 | 200.79 | 0.3110 | 760.0 | 526.0 | |
| 0.00 | 0.62 | 0.00 | 0.31 | -19.23 | 14.80 | 5.06 | 200.26 | 0.2416 | 552.0 | 368.3 | |
| 0.00 | 1.14 | 0.00 | 0.59 | -21.09 | 14.38 | 4.64 | 196.35 | 0.2690 | 760.0 | 517.7 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -17.42 | 356.49 | -13.25 | 132.01 | 0.2956 | -867.0 | -669.8 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -22.05 | 354.01 | -15.73 | 137.74 | 0.3752 | -754.0 | -586.8 | |
| 0.00 | 1.41 | 0.00 | 0.72 | -11.45 | 354.62 | -15.12 | 110.36 | 0.2739 | -807.0 | -623.1 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -15.84 | 353.48 | -16.26 | 122.45 | 0.3207 | -909.0 | -684.3 | |
| 0.00 | 1.50 | 0.00 | 0.78 | -15.77 | 353.29 | -16.45 | 121.99 | 0.3228 | -807.0 | -679.9 | |
| 0.00 | 2.02 | 0.00 | 1.06 | -15.72 | 352.80 | -16.94 | 121.18 | 0.3292 | -938.0 | -773.7 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -9.99 | 350.61 | -19.13 | 102.54 | 0.3320 | -779.0 | -595.2 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -15.96 | 349.12 | -20.62 | 117.46 | 0.3832 | -969.0 | -765.6 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -12.62 | 349.08 | -20.65 | 108.97 | 0.3656 | -799.0 | -609.6 | |
| 0.00 | 1.67 | 0.00 | 0.92 | -20.28 | 348.06 | -21.68 | 125.84 | 0.4292 | -735.0 | -562.4 | |
| 0.00 | 2.11 | 0.00 | 1.14 | -15.55 | 348.06 | -21.67 | 115.49 | 0.3959 | -861.0 | -708.9 | |
| 0.00 | 3.26 | 0.00 | 1.76 | -15.46 | 347.30 | -22.44 | 114.62 | 0.4064 | -484.0 | -429.8 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -15.90 | 346.17 | -23.57 | 114.70 | 0.4252 | -645.0 | -480.8 | |
| 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. | |