SDO HMI 2014-06-05 20:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.63 | 21.79 | 0.34 | 12.12 | 4.41 | 268.27 | -25.59 | 79.66 | 0.4356 | -638.5 | -489.4 | |
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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 | 2.17 | 0.00 | 1.15 | 4.29 | 273.36 | -20.49 | 77.60 | 0.3590 | -868.0 | -714.1 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 4.14 | 273.34 | -20.52 | 78.03 | 0.3589 | -901.0 | -677.5 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 4.14 | 273.14 | -20.71 | 78.13 | 0.3620 | -838.0 | -679.8 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 3.92 | 273.05 | -20.81 | 78.76 | 0.3629 | -946.0 | -753.8 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 5.91 | 272.95 | -20.90 | 73.53 | 0.3717 | -972.0 | -770.7 | |
| 0.00 | 3.98 | 0.00 | 2.12 | 3.50 | 272.86 | -20.99 | 80.01 | 0.3646 | -1057.0 | -764.3 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 2.92 | 272.09 | -21.77 | 81.87 | 0.3757 | -767.0 | -648.4 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 4.11 | 270.57 | -23.28 | 79.42 | 0.4027 | -767.0 | -577.7 | |
| 0.63 | 2.89 | 0.34 | 1.57 | 3.14 | 270.30 | -23.55 | 81.92 | 0.4047 | -1031.6 | -802.5 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 2.59 | 269.81 | -24.04 | 83.39 | 0.4114 | -661.0 | -522.5 | |
| 0.00 | 1.81 | 0.00 | 1.02 | 1.90 | 265.55 | -28.31 | 85.78 | 0.4772 | -517.0 | -492.2 | |
| 0.00 | 0.99 | 0.00 | 0.62 | 4.05 | 256.57 | -37.28 | 83.17 | 0.6108 | 616.0 | 496.5 | |
| 0.00 | 2.17 | 0.00 | 1.48 | 9.99 | 251.48 | -42.38 | 75.23 | 0.6887 | 543.0 | 413.6 | |
| 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. | |