SDO HMI 2014-07-06 06:00:40 UT
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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.09 | 81.42 | 10.82 | 45.97 | 11.84 | 278.76 | 27.50 | 288.93 | 0.4802 | -537.3 | -269.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-06 06:00:40 UT
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 | 1.27 | 0.00 | 0.74 | 11.45 | 282.40 | 31.14 | 286.28 | 0.5301 | -548.0 | -477.8 | |
| 0.00 | 1.18 | 0.00 | 0.69 | 11.86 | 282.08 | 30.83 | 287.17 | 0.5270 | -705.0 | -553.0 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 12.21 | 281.95 | 30.70 | 287.87 | 0.5263 | -654.0 | -553.5 | |
| 0.00 | 0.64 | 0.00 | 0.37 | 10.09 | 281.66 | 30.41 | 283.99 | 0.5156 | -440.0 | -513.0 | |
| 0.00 | 1.36 | 0.00 | 0.79 | 10.52 | 281.64 | 30.38 | 284.82 | 0.5164 | -866.0 | -581.5 | |
| 0.00 | 0.91 | 0.00 | 0.52 | 7.34 | 281.34 | 30.09 | 278.72 | 0.5050 | -663.0 | -526.5 | |
| 0.00 | 0.55 | 0.00 | 0.31 | 7.77 | 281.37 | 30.12 | 279.55 | 0.5062 | -456.0 | -388.3 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 9.97 | 281.47 | 30.22 | 283.83 | 0.5125 | -762.0 | -648.6 | |
| 0.00 | 0.73 | 0.00 | 0.42 | 7.44 | 281.17 | 29.92 | 278.94 | 0.5026 | -758.0 | -654.6 | |
| 0.00 | 0.36 | 0.00 | 0.21 | 11.08 | 281.41 | 30.16 | 285.98 | 0.5149 | -447.0 | -480.2 | |
| 0.00 | 1.27 | 0.00 | 0.74 | 14.65 | 281.17 | 29.91 | 292.76 | 0.5252 | -627.0 | -533.4 | |
| 0.00 | 0.73 | 0.00 | 0.42 | 14.47 | 281.10 | 29.85 | 292.45 | 0.5235 | -660.0 | -465.1 | |
| 0.00 | 3.45 | 0.00 | 2.00 | 14.60 | 280.98 | 29.72 | 292.76 | 0.5224 | -842.0 | -577.8 | |
| 0.00 | 1.82 | 0.00 | 1.03 | 10.54 | 280.07 | 28.81 | 285.46 | 0.4936 | -513.0 | -502.5 | |
| 17.54 | 34.98 | 9.95 | 19.85 | 10.83 | 279.71 | 28.45 | 286.19 | 0.4893 | -1002.0 | -509.6 | |
| 0.73 | 3.27 | 0.41 | 1.86 | 11.41 | 279.63 | 28.38 | 287.40 | 0.4902 | -910.8 | -745.2 | |
| 0.00 | 0.73 | 0.00 | 0.42 | 14.54 | 279.81 | 28.56 | 293.34 | 0.5060 | -648.0 | -537.0 | |
| 0.00 | 2.36 | 0.00 | 1.33 | 11.28 | 279.05 | 27.80 | 287.40 | 0.4812 | -1087.0 | -837.9 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 11.26 | 278.42 | 27.16 | 287.69 | 0.4719 | -817.0 | -643.6 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 11.30 | 278.25 | 26.99 | 287.85 | 0.4695 | -926.0 | -782.9 | |
| 0.82 | 2.00 | 0.46 | 1.12 | 11.83 | 278.02 | 26.77 | 289.07 | 0.4683 | -878.3 | -767.5 | |
| 0.00 | 1.64 | 0.00 | 0.91 | 12.05 | 277.73 | 26.48 | 289.70 | 0.4650 | -843.0 | -693.5 | |
| 0.00 | 1.73 | 0.00 | 0.96 | 12.41 | 276.94 | 25.68 | 290.94 | 0.4551 | -614.0 | -551.2 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 13.89 | 275.10 | 23.84 | 295.42 | 0.4363 | 729.0 | 594.3 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 14.27 | 274.59 | 23.34 | 296.67 | 0.4314 | 775.0 | 689.5 | |
| 0.00 | 1.91 | 0.00 | 1.04 | 11.43 | 274.17 | 22.92 | 290.66 | 0.4097 | 887.0 | 736.3 | |
| 0.00 | 4.27 | 0.00 | 2.34 | 14.49 | 274.41 | 23.16 | 297.31 | 0.4303 | 601.0 | 677.6 | |
| 0.00 | 2.18 | 0.00 | 1.19 | 13.63 | 274.11 | 22.86 | 295.70 | 0.4207 | 666.0 | 589.1 | |
| 0.00 | 2.54 | 0.00 | 1.39 | 15.57 | 273.57 | 22.32 | 300.41 | 0.4260 | 692.0 | 590.0 | |
| 0.00 | 2.73 | 0.00 | 1.49 | 15.29 | 273.54 | 22.29 | 299.85 | 0.4235 | 667.0 | 513.1 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |