SDO HMI 2014-04-09 08:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.27 | 0.00 | 7.89 | -19.03 | 324.56 | -9.43 | 150.13 | 0.2809 | 27.3 | 145.8 | |
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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 |
| 0.00 | 1.76 | 0.00 | 0.88 | -14.55 | 332.20 | -1.79 | 168.48 | 0.1518 | 983.0 | 811.0 | |
| 0.00 | 1.94 | 0.00 | 0.98 | -17.86 | 331.69 | -2.30 | 169.45 | 0.2095 | 994.0 | 797.0 | |
| 0.00 | 1.50 | 0.00 | 0.76 | -17.92 | 329.41 | -4.57 | 159.81 | 0.2207 | 932.0 | 642.9 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -16.26 | 327.91 | -6.07 | 150.30 | 0.2059 | 710.0 | 641.6 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -17.79 | 328.87 | -5.11 | 157.42 | 0.2220 | 972.0 | 816.4 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -17.29 | 327.12 | -6.87 | 149.76 | 0.2278 | 870.0 | 661.3 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -18.93 | 319.52 | -14.47 | 133.76 | 0.3286 | -769.0 | -625.8 | |
| 0.00 | 1.59 | 0.00 | 0.84 | -21.99 | 320.40 | -13.59 | 141.88 | 0.3544 | -683.0 | -570.3 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -21.33 | 319.69 | -14.30 | 139.23 | 0.3539 | -748.0 | -592.8 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -21.10 | 317.46 | -16.53 | 134.84 | 0.3759 | -753.0 | -591.8 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -22.50 | 316.29 | -17.70 | 135.73 | 0.4040 | -713.0 | -600.8 | |
| 0.00 | 0.71 | 0.00 | 0.38 | -22.64 | 316.04 | -17.94 | 135.61 | 0.4081 | -725.0 | -568.0 | |
| 0.00 | 0.71 | 0.00 | 0.39 | -23.74 | 313.14 | -20.85 | 133.62 | 0.4519 | -715.0 | -538.9 | |
| 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. | |