SDO HMI 2014-04-12 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.91 | 0.00 | 10.71 | -19.95 | 324.28 | 30.44 | 239.56 | 0.5518 | 39.4 | 58.1 | |
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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 |
| 0.00 | 0.71 | 0.00 | 0.46 | -15.47 | 333.78 | 39.95 | 252.89 | 0.6498 | 509.0 | 394.8 | |
| 0.00 | 0.88 | 0.00 | 0.57 | -15.93 | 332.88 | 39.04 | 251.95 | 0.6393 | 647.0 | 464.7 | |
| 0.00 | 1.41 | 0.00 | 0.91 | -16.84 | 332.61 | 38.77 | 250.47 | 0.6382 | 717.0 | 572.9 | |
| 0.00 | 1.85 | 0.00 | 1.18 | -16.55 | 331.70 | 37.86 | 250.64 | 0.6258 | 598.0 | 437.0 | |
| 0.00 | 1.32 | 0.00 | 0.84 | -16.78 | 331.51 | 37.67 | 250.22 | 0.6241 | 612.0 | 490.2 | |
| 0.00 | 0.53 | 0.00 | 0.34 | -20.96 | 332.35 | 38.51 | 244.14 | 0.6484 | 546.0 | 516.0 | |
| 0.00 | 2.21 | 0.00 | 1.34 | -18.34 | 327.93 | 34.09 | 246.31 | 0.5832 | 718.0 | 657.2 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -19.70 | 325.16 | 31.32 | 242.59 | 0.5535 | 801.0 | 679.7 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -22.77 | 320.28 | 26.45 | 233.72 | 0.5114 | -722.0 | -527.5 | |
| 0.00 | 1.41 | 0.00 | 0.81 | -22.31 | 319.97 | 26.13 | 234.23 | 0.5042 | -675.0 | -462.8 | |
| 0.00 | 2.03 | 0.00 | 1.15 | -23.91 | 317.15 | 23.31 | 228.68 | 0.4837 | -801.0 | -620.7 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -22.21 | 316.17 | 22.34 | 230.58 | 0.4574 | -802.0 | -689.9 | |
| 0.00 | 1.68 | 0.00 | 0.91 | -23.78 | 311.20 | 17.36 | 221.13 | 0.4169 | -812.0 | -648.4 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -25.54 | 307.10 | 13.26 | 211.34 | 0.3997 | -785.0 | -695.3 | |
| 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. | |