SDO HMI 2011-06-04 05:59:10 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 |
| 47.31 | 266.49 | 24.57 | 138.75 | 17.38 | 19.95 | -0.76 | 2.09 | 0.3084 | -442.0 | -268.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-06-04 05:59:10 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 | 1.45 | 0.00 | 0.78 | 22.05 | 29.63 | 8.92 | 339.31 | 0.4084 | 707.0 | 617.8 | |
| 0.00 | 1.72 | 0.00 | 0.93 | 22.44 | 26.27 | 5.56 | 346.97 | 0.3988 | -608.0 | -369.1 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 20.70 | 25.29 | 4.58 | 348.24 | 0.3680 | -796.0 | -618.5 | |
| 0.00 | 2.80 | 0.00 | 1.49 | 20.25 | 24.01 | 3.30 | 351.26 | 0.3569 | -813.0 | -605.5 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 19.44 | 21.57 | 0.86 | 357.60 | 0.3398 | -627.0 | -489.5 | |
| 29.31 | 197.91 | 15.19 | 102.58 | 16.71 | 21.11 | 0.40 | 358.68 | 0.2942 | -1316.8 | -487.6 | |
| 7.51 | -6.00 | 3.90 | -6.00 | 17.25 | 21.05 | 0.34 | 358.92 | 0.3033 | -995.9 | 999999 | |
| 0.00 | 2.35 | 0.00 | 1.23 | 18.79 | 21.05 | 0.34 | 359.01 | 0.3288 | -896.0 | -768.6 | |
| 3.89 | -6.00 | 2.02 | -6.00 | 17.09 | 20.60 | -0.11 | 0.34 | 0.3005 | -1075.5 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 18.05 | 19.58 | -1.13 | 3.40 | 0.3171 | -746.0 | -528.3 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 17.86 | 19.32 | -1.38 | 4.21 | 0.3142 | -959.0 | -773.2 | |
| 0.00 | 2.08 | 0.00 | 1.09 | 17.89 | 19.10 | -1.61 | 4.88 | 0.3150 | -856.0 | -695.3 | |
| 0.00 | 1.99 | 0.00 | 1.04 | 17.67 | 17.31 | -3.39 | 10.36 | 0.3153 | -900.0 | -690.2 | |
| 0.00 | 2.62 | 0.00 | 1.37 | 17.48 | 17.12 | -3.58 | 11.04 | 0.3127 | -945.0 | -783.8 | |
| 2.35 | 3.08 | 1.23 | 1.61 | 17.73 | 16.96 | -3.75 | 11.36 | 0.3174 | -835.3 | -800.0 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 17.38 | 16.84 | -3.87 | 11.96 | 0.3121 | -788.0 | -601.4 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 19.60 | 15.40 | -5.31 | 14.36 | 0.3532 | 858.0 | 601.9 | |
| 0.00 | 1.99 | 0.00 | 1.06 | 20.15 | 15.15 | -5.56 | 14.58 | 0.3629 | 895.0 | 673.1 | |
| 1.54 | 18.45 | 0.81 | 9.73 | 18.73 | 14.65 | -6.06 | 17.03 | 0.3428 | 1046.0 | 848.6 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 20.28 | 14.59 | -6.12 | 15.86 | 0.3673 | 672.0 | 470.9 | |
| 0.00 | 4.25 | 0.00 | 2.23 | 18.28 | 14.60 | -6.11 | 17.58 | 0.3360 | 1119.0 | 865.1 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 19.70 | 14.52 | -6.19 | 16.53 | 0.3585 | 742.0 | 612.3 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 20.74 | 14.41 | -6.30 | 15.94 | 0.3752 | 771.0 | 597.7 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 17.86 | 14.45 | -6.25 | 18.38 | 0.3302 | 929.0 | 730.2 | |
| 2.71 | 4.34 | 1.42 | 2.27 | 17.29 | 14.41 | -6.30 | 19.10 | 0.3214 | 1081.8 | 854.4 | |
| 0.00 | 2.17 | 0.00 | 1.14 | 17.64 | 14.40 | -6.31 | 18.76 | 0.3270 | 778.0 | 800.3 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 18.22 | 14.25 | -6.46 | 18.58 | 0.3368 | 762.0 | 558.3 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 17.45 | 14.24 | -6.46 | 19.39 | 0.3248 | 982.0 | 831.0 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 18.47 | 14.14 | -6.57 | 18.61 | 0.3413 | 966.0 | 864.1 | |
| 0.00 | 1.72 | 0.00 | 0.94 | 23.64 | 13.91 | -6.80 | 14.96 | 0.4220 | 848.0 | 587.6 | |
| 0.00 | 0.72 | 0.00 | 0.39 | 20.25 | 13.74 | -6.96 | 17.94 | 0.3708 | 695.0 | 587.1 | |
| 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. | |