SDO HMI 2014-05-17 05:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.21 | 151.28 | 31.70 | 77.14 | -16.05 | 194.50 | 0.99 | 183.84 | 0.2376 | 292.5 | 281.0 | |
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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 | 1.44 | 0.00 | 0.74 | -17.02 | 196.18 | 2.67 | 190.04 | 0.2569 | 699.0 | 579.3 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -17.27 | 195.93 | 2.42 | 188.95 | 0.2603 | 699.0 | 488.9 | |
| 3.33 | 66.69 | 1.70 | 34.08 | -16.05 | 195.60 | 2.09 | 188.47 | 0.2391 | 1182.6 | 671.1 | |
| 0.00 | 2.34 | 0.00 | 1.19 | -15.42 | 195.50 | 1.99 | 188.47 | 0.2283 | 891.0 | 628.5 | |
| 23.73 | -3.00 | 12.14 | -3.00 | -16.73 | 195.38 | 1.88 | 187.23 | 0.2501 | 1133.4 | 999999 | |
| 1.89 | -3.00 | 0.96 | -3.00 | -16.30 | 195.35 | 1.84 | 187.33 | 0.2427 | 934.3 | 999999 | |
| 0.00 | 1.89 | 0.00 | 0.97 | -17.11 | 195.16 | 1.66 | 186.22 | 0.2560 | 634.0 | 446.8 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -16.23 | 195.03 | 1.52 | 186.11 | 0.2410 | 433.0 | 317.6 | |
| 0.00 | 5.21 | 0.00 | 2.67 | -16.80 | 194.47 | 0.96 | 183.69 | 0.2497 | 642.0 | 601.4 | |
| 0.54 | 64.09 | 0.27 | 32.58 | -15.48 | 193.93 | 0.42 | 181.78 | 0.2270 | -980.7 | -231.2 | |
| 27.50 | -10.00 | 13.98 | -10.00 | -15.36 | 193.58 | 0.07 | 180.31 | 0.2247 | -429.1 | 999999 | |
| 1.89 | -10.00 | 0.96 | -10.00 | -15.89 | 193.39 | -0.12 | 179.52 | 0.2337 | -963.2 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -14.96 | 193.02 | -0.49 | 177.81 | 0.2180 | 853.0 | 683.1 | |
| 3.33 | 4.85 | 1.69 | 2.47 | -15.33 | 192.48 | -1.03 | 175.57 | 0.2248 | -1026.9 | -735.2 | |
| 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. | |