SDO HMI 2014-03-15 09:01:14 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.39 | 190.55 | 43.35 | 267.48 | 11.27 | 10.41 | 67.24 | 284.93 | 0.9371 | -6.1 | -88.8 | |
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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 |
| 5.22 | 91.37 | 8.03 | 138.06 | 11.80 | 12.21 | 69.05 | 285.09 | 0.9482 | -148.1 | -183.2 | |
| 5.30 | -1.00 | 7.92 | -1.00 | 11.67 | 11.63 | 68.46 | 285.08 | 0.9449 | -676.4 | 999999 | |
| 1.48 | -1.00 | 2.20 | -1.00 | 11.99 | 11.47 | 68.30 | 285.45 | 0.9444 | -420.8 | 999999 | |
| 0.00 | 2.87 | 0.00 | 4.07 | 10.63 | 10.70 | 67.54 | 284.20 | 0.9384 | -128.0 | -130.9 | |
| 0.61 | 5.56 | 0.86 | 7.86 | 11.62 | 10.46 | 67.29 | 285.29 | 0.9383 | -558.9 | -435.1 | |
| 0.00 | 2.17 | 0.00 | 3.03 | 11.31 | 10.14 | 66.98 | 285.03 | 0.9360 | -670.0 | -623.3 | |
| 0.52 | 1.83 | 0.72 | 2.52 | 11.59 | 9.89 | 66.72 | 285.38 | 0.9349 | -541.0 | -490.4 | |
| 0.00 | 1.39 | 0.00 | 1.91 | 11.36 | 9.78 | 66.61 | 285.16 | 0.9339 | -492.0 | -498.8 | |
| 0.00 | 1.56 | 0.00 | 2.12 | 11.17 | 9.54 | 66.37 | 285.02 | 0.9322 | -479.0 | -470.6 | |
| 0.00 | 1.91 | 0.00 | 2.62 | 11.78 | 9.67 | 66.51 | 285.63 | 0.9338 | -380.0 | -375.8 | |
| 4.09 | 79.02 | 5.45 | 101.72 | 10.95 | 9.21 | 66.04 | 284.86 | 0.9299 | -121.5 | 143.8 | |
| 14.17 | -11.00 | 18.17 | -11.00 | 10.45 | 8.40 | 65.24 | 284.52 | 0.9241 | 588.6 | 999999 | |
| 0.00 | 0.87 | 0.00 | 1.14 | 11.53 | 8.65 | 65.48 | 285.61 | 0.9272 | -596.0 | -516.3 | |
| 0.00 | 0.61 | 0.00 | 0.74 | 11.08 | 6.88 | 63.71 | 285.55 | 0.9150 | 425.0 | 353.3 | |
| 0.00 | 1.39 | 0.00 | 1.69 | 11.43 | 6.67 | 63.51 | 285.97 | 0.9142 | 314.0 | 264.2 | |
| 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. | |