SDO HMI 2014-06-07 21:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.65 | 0.00 | 10.01 | 4.95 | 260.08 | -6.75 | 154.99 | 0.2183 | 360.0 | 158.4 | |
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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 | 3.80 | 0.00 | 1.90 | 4.25 | 273.59 | 6.76 | 301.50 | 0.1384 | -961.0 | -731.7 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 5.11 | 272.90 | 6.07 | 309.52 | 0.1371 | -900.0 | -757.4 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 3.34 | 271.93 | 5.10 | 302.28 | 0.1055 | -683.0 | -534.7 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 5.23 | 271.73 | 4.90 | 316.28 | 0.1237 | -847.0 | -663.5 | |
| 0.00 | 0.63 | 0.00 | 0.32 | 4.21 | 260.45 | -6.38 | 57.27 | 0.1323 | 761.0 | 548.6 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 6.32 | 257.90 | -8.93 | 55.04 | 0.1891 | 576.0 | 473.1 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 11.24 | 256.81 | -10.02 | 41.50 | 0.2586 | 859.0 | 663.2 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 3.72 | 256.20 | -10.63 | 71.16 | 0.1953 | 895.0 | 799.3 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 9.58 | 252.44 | -14.38 | 56.16 | 0.2962 | 862.0 | 665.1 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 1.63 | 252.38 | -14.45 | 83.99 | 0.2519 | 782.0 | 636.6 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 5.41 | 250.46 | -16.37 | 71.83 | 0.2966 | 816.0 | 630.1 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 5.19 | 250.43 | -16.40 | 72.55 | 0.2960 | 837.0 | 686.7 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 4.92 | 250.21 | -16.61 | 73.64 | 0.2982 | 783.0 | 590.4 | |
| 0.00 | 0.45 | 0.00 | 0.24 | 1.57 | 247.93 | -18.90 | 85.54 | 0.3261 | 779.0 | 648.2 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -0.32 | 246.78 | -20.05 | 91.27 | 0.3444 | 841.0 | 658.6 | |
| 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. | |