SDO HMI 2014-10-06 11:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 29.01 | 0.00 | 15.70 | 13.62 | 90.10 | -22.62 | 70.44 | 0.3981 | -140.0 | 229.4 | |
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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 | 1.76 | 0.00 | 0.90 | 12.92 | 99.20 | -13.52 | 63.03 | 0.2569 | -934.0 | -645.1 | |
| 0.00 | 1.67 | 0.00 | 0.86 | 10.36 | 96.87 | -15.86 | 74.88 | 0.2797 | -788.0 | -671.8 | |
| 0.00 | 1.41 | 0.00 | 0.73 | 10.33 | 96.01 | -16.71 | 75.60 | 0.2934 | -756.0 | -656.4 | |
| 0.00 | 1.41 | 0.00 | 0.73 | 11.18 | 95.26 | -17.46 | 73.39 | 0.3086 | -735.0 | -546.1 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 14.51 | 94.63 | -18.09 | 64.11 | 0.3356 | -796.0 | -616.6 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 8.91 | 94.65 | -18.07 | 80.99 | 0.3117 | -781.0 | -591.0 | |
| 0.00 | 1.41 | 0.00 | 0.74 | 10.86 | 93.74 | -18.99 | 75.42 | 0.3316 | -855.0 | -551.8 | |
| 0.00 | 1.41 | 0.00 | 0.75 | 15.46 | 91.44 | -21.28 | 64.85 | 0.3881 | 840.0 | 729.0 | |
| 0.00 | 8.87 | 0.00 | 4.81 | 13.41 | 89.38 | -23.34 | 71.32 | 0.4086 | 1233.0 | 941.7 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 16.17 | 88.69 | -24.03 | 65.48 | 0.4317 | 655.0 | 563.9 | |
| 0.00 | 2.72 | 0.00 | 1.50 | 13.48 | 87.00 | -25.72 | 72.45 | 0.4445 | 725.0 | 684.6 | |
| 0.00 | 2.11 | 0.00 | 1.22 | 20.28 | 83.93 | -28.79 | 60.82 | 0.5196 | 632.0 | 337.1 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 18.48 | 81.50 | -31.22 | 65.49 | 0.5425 | 617.0 | 545.2 | |
| 0.00 | 1.32 | 0.00 | 0.76 | 11.83 | 82.49 | -30.23 | 77.53 | 0.5067 | -758.0 | -609.4 | |
| 0.00 | 0.53 | 0.00 | 0.30 | 11.83 | 81.96 | -30.76 | 77.66 | 0.5145 | -399.0 | -393.0 | |
| 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. | |