SDO HMI 2014-07-04 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.81 | 0.00 | 10.19 | 7.29 | 263.65 | -11.33 | 105.74 | 0.2262 | 419.0 | 401.7 | |
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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 | 1.00 | 0.00 | 0.50 | 3.74 | 279.42 | 4.43 | 276.74 | 0.0780 | -833.0 | -698.5 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 4.03 | 276.51 | 1.53 | 297.68 | 0.0302 | -813.0 | -716.7 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 4.00 | 276.14 | 1.16 | 303.60 | 0.0244 | -800.0 | -663.6 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 9.27 | 269.95 | -5.03 | 39.35 | 0.1371 | 1023.0 | 804.2 | |
| 0.00 | 4.91 | 0.00 | 2.45 | 8.69 | 269.68 | -5.30 | 43.74 | 0.1327 | 876.0 | 689.7 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 8.66 | 268.72 | -6.26 | 48.63 | 0.1443 | 905.0 | 719.2 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 9.61 | 261.55 | -13.44 | 63.81 | 0.2564 | 619.0 | 565.1 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 7.28 | 259.21 | -15.77 | 74.88 | 0.2805 | 441.0 | 338.8 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 7.37 | 259.05 | -15.93 | 74.71 | 0.2835 | 964.0 | 825.5 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 8.61 | 251.32 | -23.66 | 76.05 | 0.4105 | 728.0 | 575.0 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 8.77 | 251.28 | -23.70 | 75.71 | 0.4117 | 812.0 | 587.2 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 6.15 | 250.42 | -24.56 | 82.28 | 0.4188 | 858.0 | 691.7 | |
| 0.00 | 1.82 | 0.00 | 0.99 | 5.90 | 250.36 | -24.62 | 82.88 | 0.4193 | 667.0 | 556.8 | |
| 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. | |