SDO HMI 2014-09-24 16:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.80 | 0.00 | 14.92 | -15.32 | 246.57 | -21.76 | 136.07 | 0.5173 | -806.1 | -684.1 | |
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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 | 1.24 | 0.00 | 0.71 | -15.31 | 247.76 | -20.56 | 137.67 | 0.5050 | -720.0 | -634.0 | |
| 0.00 | 3.01 | 0.00 | 1.73 | -15.70 | 247.15 | -21.17 | 137.36 | 0.5153 | -878.0 | -667.6 | |
| 0.00 | 1.59 | 0.00 | 0.91 | -15.12 | 247.11 | -21.21 | 136.51 | 0.5095 | -825.0 | -572.5 | |
| 0.00 | 1.41 | 0.00 | 0.81 | -14.56 | 247.14 | -21.18 | 135.76 | 0.5034 | -862.0 | -704.9 | |
| 0.00 | 1.50 | 0.00 | 0.87 | -15.74 | 246.95 | -21.38 | 137.14 | 0.5179 | -821.0 | -694.6 | |
| 0.00 | 1.59 | 0.00 | 0.91 | -14.21 | 247.07 | -21.25 | 135.17 | 0.5004 | -756.0 | -642.6 | |
| 0.00 | 2.47 | 0.00 | 1.43 | -15.29 | 246.86 | -21.46 | 136.41 | 0.5139 | -965.0 | -795.6 | |
| 0.00 | 1.41 | 0.00 | 0.82 | -15.18 | 246.50 | -21.82 | 135.78 | 0.5164 | -578.0 | -522.6 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -15.61 | 246.15 | -22.17 | 135.93 | 0.5247 | -694.0 | -585.2 | |
| 0.00 | 1.15 | 0.00 | 0.67 | -15.07 | 246.05 | -22.28 | 135.04 | 0.5201 | -972.0 | -785.4 | |
| 0.00 | 6.54 | 0.00 | 3.80 | -15.30 | 245.99 | -22.34 | 135.28 | 0.5231 | -813.0 | -764.7 | |
| 0.00 | 3.01 | 0.00 | 1.75 | -15.95 | 245.88 | -22.45 | 136.04 | 0.5310 | -789.0 | -585.9 | |
| 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. | |