SDO HMI 2014-04-08 06:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.06 | 0.00 | 8.29 | -19.72 | 351.07 | 2.79 | 190.72 | 0.2670 | -384.3 | -294.6 | |
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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 | 1.06 | 0.00 | 0.59 | -23.39 | 9.63 | 21.36 | 227.74 | 0.4535 | 785.0 | 624.5 | |
| 0.00 | 1.59 | 0.00 | 0.82 | -18.14 | 359.21 | 10.93 | 220.62 | 0.2781 | 680.0 | 602.6 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -18.40 | 356.05 | 7.78 | 210.99 | 0.2505 | -650.0 | -524.6 | |
| 0.00 | 2.03 | 0.00 | 1.04 | -18.68 | 355.81 | 7.53 | 209.61 | 0.2524 | -803.0 | -697.6 | |
| 0.00 | 1.41 | 0.00 | 0.71 | -17.49 | 351.56 | 3.28 | 195.44 | 0.2057 | -562.0 | -544.1 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -16.18 | 349.66 | 1.38 | 187.54 | 0.1772 | -849.0 | -577.3 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -15.91 | 349.59 | 1.32 | 187.40 | 0.1723 | -1033.0 | -800.5 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -13.96 | 348.81 | 0.53 | 183.78 | 0.1375 | -965.0 | -829.4 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -22.57 | 347.53 | -0.75 | 177.55 | 0.2848 | -742.0 | -546.9 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -26.42 | 346.16 | -2.12 | 174.55 | 0.3503 | 4.0 | -2.1 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -18.28 | 345.31 | -2.97 | 166.87 | 0.2175 | -849.0 | -648.7 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -25.49 | 341.60 | -6.67 | 162.49 | 0.3501 | 1.0 | 0.3 | |
| 0.00 | 2.03 | 0.00 | 1.07 | -24.14 | 338.36 | -9.92 | 153.17 | 0.3499 | -13.0 | -1.4 | |
| 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. | |