SDO HMI 2014-04-10 05:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.73 | 0.00 | 9.99 | -15.10 | 303.96 | -18.47 | 122.60 | 0.3527 | -127.7 | -54.3 | |
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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 | 1.24 | 0.00 | 0.61 | -11.08 | 320.40 | -2.03 | 158.68 | 0.0959 | 824.0 | 577.2 | |
| 0.00 | 1.24 | 0.00 | 0.62 | -11.44 | 320.31 | -2.12 | 159.14 | 0.1024 | 974.0 | 730.3 | |
| 0.00 | 1.76 | 0.00 | 0.92 | -18.07 | 309.61 | -12.82 | 135.13 | 0.3003 | 814.0 | 570.2 | |
| 0.00 | 2.03 | 0.00 | 1.04 | -11.07 | 309.21 | -13.22 | 112.14 | 0.2434 | 865.0 | 610.8 | |
| 0.00 | 2.56 | 0.00 | 1.39 | -20.52 | 302.44 | -19.99 | 128.75 | 0.4122 | 793.0 | 633.6 | |
| 0.00 | 1.24 | 0.00 | 0.66 | -11.28 | 301.60 | -20.83 | 105.86 | 0.3641 | -876.0 | -733.7 | |
| 0.00 | 1.24 | 0.00 | 0.67 | -16.53 | 300.45 | -21.98 | 117.93 | 0.4079 | -732.0 | -620.2 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -15.97 | 300.38 | -22.05 | 116.61 | 0.4054 | -598.0 | -492.2 | |
| 0.00 | 1.59 | 0.00 | 0.86 | -15.55 | 300.36 | -22.07 | 115.61 | 0.4031 | -620.0 | -592.3 | |
| 0.00 | 1.15 | 0.00 | 0.63 | -14.50 | 297.98 | -24.45 | 111.42 | 0.4323 | -778.0 | -602.5 | |
| 0.00 | 1.68 | 0.00 | 0.94 | -16.60 | 296.35 | -26.08 | 114.77 | 0.4659 | -808.0 | -669.8 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -16.29 | 296.22 | -26.21 | 114.05 | 0.4661 | -773.0 | -582.3 | |
| 0.00 | 1.24 | 0.00 | 0.68 | -11.87 | 296.19 | -26.24 | 104.65 | 0.4491 | -745.0 | -652.4 | |
| 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. | |