SDO HMI 2014-08-03 05:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.83 | 0.00 | 11.69 | 16.35 | 259.11 | 17.77 | 289.39 | 0.3602 | 73.1 | 81.3 | |
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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 | 0.45 | 0.00 | 0.25 | 13.28 | 268.65 | 27.31 | 287.31 | 0.4696 | -679.0 | -577.8 | |
| 0.00 | 1.27 | 0.00 | 0.72 | 17.06 | 268.55 | 27.21 | 295.02 | 0.4842 | -617.0 | -551.9 | |
| 0.00 | 0.91 | 0.00 | 0.51 | 16.00 | 268.00 | 26.65 | 293.26 | 0.4712 | -693.0 | -490.2 | |
| 0.00 | 1.63 | 0.00 | 0.91 | 15.89 | 267.70 | 26.35 | 293.23 | 0.4665 | -875.0 | -723.2 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 14.79 | 266.64 | 25.29 | 291.61 | 0.4461 | -759.0 | -636.9 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 15.93 | 266.09 | 24.74 | 294.42 | 0.4438 | -625.0 | -538.5 | |
| 0.00 | 1.90 | 0.00 | 1.04 | 19.57 | 262.31 | 20.97 | 305.70 | 0.4169 | -824.0 | -643.0 | |
| 0.00 | 1.99 | 0.00 | 1.05 | 11.76 | 260.22 | 18.88 | 288.64 | 0.3358 | 645.0 | 574.7 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 10.99 | 258.35 | 17.00 | 287.87 | 0.3029 | 852.0 | 600.1 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 17.63 | 257.65 | 16.30 | 307.69 | 0.3396 | 806.0 | 643.0 | |
| 0.00 | 2.62 | 0.00 | 1.38 | 17.59 | 257.01 | 15.67 | 308.62 | 0.3310 | 702.0 | 662.3 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 31.48 | 258.64 | 17.30 | 329.77 | 0.5057 | 731.0 | 494.1 | |
| 0.00 | 2.17 | 0.00 | 1.09 | 10.30 | 248.30 | 6.96 | 302.79 | 0.1425 | 830.0 | 492.0 | |
| 0.00 | 1.72 | 0.00 | 0.87 | 15.39 | 247.95 | 6.60 | 326.10 | 0.1996 | 806.0 | 510.1 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 18.81 | 238.55 | -2.80 | 11.71 | 0.2288 | 797.0 | 654.1 | |
| 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. | |