SDO HMI 2014-06-01 04:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.69 | 153.27 | 33.56 | 139.58 | -4.37 | 298.61 | -56.99 | 94.77 | 0.8410 | 554.7 | 312.5 | |
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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 |
| 21.42 | 105.10 | 19.18 | 94.14 | -4.22 | 299.25 | -56.35 | 94.62 | 0.8350 | 856.2 | 359.1 | |
| 1.63 | -1.00 | 1.47 | -1.00 | -3.88 | 298.90 | -56.70 | 94.20 | 0.8383 | 495.1 | 999999 | |
| 1.08 | 2.17 | 0.99 | 1.98 | -5.34 | 298.49 | -57.11 | 95.93 | 0.8427 | 579.4 | 492.6 | |
| 0.00 | 2.89 | 0.00 | 2.65 | -4.85 | 298.44 | -57.16 | 95.34 | 0.8429 | 578.0 | 503.8 | |
| 1.90 | 19.97 | 1.75 | 18.53 | -4.70 | 298.07 | -57.54 | 95.14 | 0.8464 | 624.3 | 341.8 | |
| 2.08 | -5.00 | 1.92 | -5.00 | -4.48 | 298.09 | -57.51 | 94.89 | 0.8460 | 601.3 | 999999 | |
| 1.54 | -5.00 | 1.43 | -5.00 | -4.75 | 297.71 | -57.89 | 95.19 | 0.8497 | 478.7 | 999999 | |
| 0.90 | 1.81 | 0.85 | 1.69 | -3.71 | 297.61 | -58.00 | 93.96 | 0.8503 | 187.3 | 90.3 | |
| 0.00 | 1.27 | 0.00 | 1.19 | -4.54 | 297.51 | -58.09 | 94.93 | 0.8514 | 314.0 | 223.7 | |
| 1.17 | 3.98 | 1.12 | 3.78 | -6.22 | 297.13 | -58.47 | 96.88 | 0.8556 | 720.4 | 587.1 | |
| 0.00 | 2.53 | 0.00 | 2.41 | -4.81 | 297.00 | -58.60 | 95.22 | 0.8561 | 325.0 | 211.7 | |
| 1.08 | 2.80 | 1.05 | 2.71 | -5.93 | 296.59 | -59.02 | 96.52 | 0.8603 | 489.5 | 376.4 | |
| 1.99 | 9.67 | 1.94 | 9.43 | -4.10 | 296.08 | -59.52 | 94.36 | 0.8641 | -607.0 | -395.0 | |
| 1.90 | -13.00 | 1.86 | -13.00 | -3.91 | 296.04 | -59.56 | 94.15 | 0.8644 | -444.1 | 999999 | |
| 0.00 | 1.08 | 0.00 | 1.07 | -4.34 | 295.93 | -59.67 | 94.64 | 0.8655 | -514.0 | -449.6 | |
| 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. | |