SDO HMI 2014-05-16 15:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.25 | 25.36 | 1.14 | 12.86 | 8.41 | 195.90 | -5.35 | 25.16 | 0.2140 | 143.1 | -119.1 | |
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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 |
| 0.81 | 2.78 | 0.41 | 1.41 | 8.20 | 198.62 | -2.63 | 13.73 | 0.1921 | -1261.0 | -966.4 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 6.97 | 198.44 | -2.80 | 16.44 | 0.1724 | -942.0 | -738.9 | |
| 1.44 | 5.75 | 0.73 | 2.91 | 8.54 | 197.73 | -3.52 | 17.58 | 0.2019 | -1106.6 | -822.0 | |
| 0.00 | 1.98 | 0.00 | 1.00 | 8.39 | 197.42 | -3.82 | 19.25 | 0.2010 | -983.0 | -776.4 | |
| 0.00 | 2.07 | 0.00 | 1.05 | 8.42 | 196.81 | -4.44 | 22.00 | 0.2053 | -1077.0 | -856.8 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 8.92 | 195.79 | -5.46 | 25.40 | 0.2201 | -729.0 | -566.0 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 6.96 | 194.92 | -6.33 | 33.68 | 0.1981 | 774.0 | 630.1 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 9.73 | 194.82 | -6.43 | 27.53 | 0.2399 | 801.0 | 599.6 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 7.54 | 194.45 | -6.80 | 33.95 | 0.2110 | 995.0 | 752.6 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 9.30 | 194.36 | -6.89 | 30.07 | 0.2372 | 855.0 | 687.6 | |
| 0.00 | 0.63 | 0.00 | 0.32 | 9.40 | 194.05 | -7.20 | 30.97 | 0.2413 | 904.0 | 744.9 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 8.60 | 193.32 | -7.92 | 35.34 | 0.2367 | 808.0 | 637.6 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 7.71 | 193.28 | -7.97 | 37.84 | 0.2250 | 986.0 | 773.6 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 8.79 | 193.13 | -8.11 | 35.52 | 0.2411 | 762.0 | 692.1 | |
| 0.00 | 1.62 | 0.00 | 0.82 | 8.45 | 193.14 | -8.11 | 36.35 | 0.2364 | 832.0 | 721.7 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 9.74 | 190.37 | -10.88 | 41.36 | 0.2828 | 909.0 | 693.7 | |
| 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. | |