SDO HMI 2014-10-04 22:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.05 | 0.00 | 10.55 | -18.98 | 106.86 | -26.19 | 135.41 | 0.5978 | 243.2 | 241.1 | |
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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 | 2.20 | 0.00 | 1.34 | -22.65 | 112.55 | -20.49 | 146.11 | 0.5817 | 802.0 | 649.5 | |
| 0.00 | 1.23 | 0.00 | 0.75 | -22.67 | 112.06 | -20.98 | 145.51 | 0.5858 | 438.0 | 399.9 | |
| 0.00 | 1.05 | 0.00 | 0.65 | -22.35 | 110.79 | -22.26 | 143.61 | 0.5927 | 554.0 | 482.0 | |
| 0.00 | 1.41 | 0.00 | 0.81 | -14.60 | 111.04 | -22.01 | 134.20 | 0.5079 | 774.0 | 562.1 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -15.22 | 110.87 | -22.18 | 134.87 | 0.5161 | 742.0 | 616.3 | |
| 0.00 | 0.79 | 0.00 | 0.49 | -22.26 | 109.71 | -23.33 | 142.24 | 0.6008 | 195.0 | 288.8 | |
| 0.00 | 1.49 | 0.00 | 0.97 | -24.85 | 107.58 | -25.47 | 142.63 | 0.6452 | 427.0 | 411.3 | |
| 0.00 | 1.67 | 0.00 | 0.98 | -15.12 | 108.20 | -24.84 | 131.51 | 0.5438 | 659.0 | 488.9 | |
| 0.00 | 1.41 | 0.00 | 0.86 | -17.29 | 105.80 | -27.25 | 131.88 | 0.5893 | 641.0 | 535.4 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -15.08 | 105.82 | -27.23 | 128.89 | 0.5697 | 742.0 | 607.5 | |
| 0.00 | 0.79 | 0.00 | 0.52 | -17.37 | 99.47 | -33.58 | 126.27 | 0.6569 | -598.0 | -597.2 | |
| 0.00 | 1.23 | 0.00 | 0.81 | -17.30 | 99.07 | -33.98 | 125.86 | 0.6607 | -651.0 | -549.6 | |
| 0.00 | 1.23 | 0.00 | 0.81 | -17.52 | 98.76 | -34.29 | 125.89 | 0.6655 | -643.0 | -554.0 | |
| 0.00 | 0.79 | 0.00 | 0.52 | -17.00 | 98.18 | -34.87 | 124.80 | 0.6680 | -677.0 | -571.2 | |
| 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. | |