SDO HMI 2014-03-22 01:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.00 | 339.52 | 45.43 | 264.18 | 11.94 | 262.32 | 47.06 | 291.86 | 0.7734 | -583.6 | -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 |
| 58.00 | 329.60 | 45.43 | 257.80 | 11.91 | 262.64 | 47.38 | 291.63 | 0.7768 | -794.9 | -298.1 | |
| 0.00 | 0.87 | 0.00 | 0.67 | 12.82 | 261.60 | 46.33 | 293.20 | 0.7697 | -476.0 | -441.1 | |
| 0.00 | 1.13 | 0.00 | 0.80 | 10.86 | 257.19 | 41.92 | 292.83 | 0.7142 | -620.0 | -478.5 | |
| 0.00 | 1.31 | 0.00 | 0.83 | 11.39 | 249.43 | 34.16 | 298.18 | 0.6268 | 557.0 | 498.5 | |
| 0.00 | 0.78 | 0.00 | 0.49 | 12.24 | 248.41 | 33.14 | 300.13 | 0.6201 | 580.0 | 515.7 | |
| 0.00 | 1.05 | 0.00 | 0.66 | 12.55 | 248.39 | 33.12 | 300.59 | 0.6218 | 571.0 | 468.9 | |
| 0.00 | 0.87 | 0.00 | 0.54 | 11.30 | 247.09 | 31.82 | 299.79 | 0.5980 | 790.0 | 631.2 | |
| 0.00 | 0.78 | 0.00 | 0.48 | 13.28 | 246.00 | 30.73 | 303.56 | 0.5990 | 616.0 | 560.9 | |
| 0.00 | 1.57 | 0.00 | 0.97 | 16.53 | 244.07 | 28.80 | 309.79 | 0.6034 | 602.0 | 446.0 | |
| 0.00 | 0.78 | 0.00 | 0.47 | 13.30 | 242.69 | 27.42 | 306.66 | 0.5609 | 505.0 | 500.4 | |
| 0.00 | 0.78 | 0.00 | 0.47 | 15.24 | 242.50 | 27.23 | 309.61 | 0.5753 | 637.0 | 562.2 | |
| 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. | |