SDO HMI 2011-10-11 12:59:02 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 |
| 93.67 | 444.93 | 50.08 | 237.94 | -14.69 | 118.87 | 7.33 | 199.10 | 0.3784 | 303.5 | 271.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-10-11 12:59:02 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 |
| 7.18 | 73.01 | 3.85 | 39.15 | -14.13 | 121.05 | 9.50 | 204.90 | 0.3819 | 1079.9 | 434.4 | |
| 0.00 | 1.66 | 0.00 | 0.89 | -14.82 | 120.42 | 8.87 | 202.71 | 0.3880 | 566.0 | 354.1 | |
| 0.00 | 2.80 | 0.00 | 1.49 | -13.70 | 120.31 | 8.77 | 203.65 | 0.3707 | 881.0 | 797.6 | |
| 0.00 | 1.49 | 0.00 | 0.80 | -15.01 | 120.36 | 8.82 | 202.39 | 0.3905 | 573.0 | 424.2 | |
| 0.00 | 1.31 | 0.00 | 0.70 | -14.34 | 120.18 | 8.64 | 202.65 | 0.3793 | 967.0 | 866.3 | |
| 1.05 | 4.55 | 0.56 | 2.43 | -13.89 | 120.10 | 8.56 | 202.94 | 0.3722 | 842.0 | 849.2 | |
| 0.00 | 2.63 | 0.00 | 1.42 | -15.94 | 120.09 | 8.55 | 200.87 | 0.4027 | -245.0 | -342.9 | |
| 0.35 | 253.00 | 0.19 | 135.51 | -14.91 | 120.01 | 8.47 | 201.69 | 0.3869 | 765.0 | 455.0 | |
| 0.00 | 1.31 | 0.00 | 0.70 | -13.79 | 119.94 | 8.40 | 202.66 | 0.3697 | 506.0 | 402.0 | |
| 3.33 | -8.00 | 1.78 | -8.00 | -14.11 | 119.80 | 8.25 | 201.98 | 0.3736 | 1067.2 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -14.36 | 119.77 | 8.23 | 201.67 | 0.3773 | 916.0 | 742.9 | |
| 0.00 | 2.80 | 0.00 | 1.49 | -13.63 | 119.65 | 8.11 | 202.14 | 0.3655 | 906.0 | 719.9 | |
| 53.40 | -8.00 | 28.62 | -8.00 | -14.90 | 119.39 | 7.85 | 200.23 | 0.3831 | 1181.7 | 999999 | |
| 0.00 | 1.58 | 0.00 | 0.85 | -16.61 | 119.39 | 7.85 | 198.74 | 0.4090 | 823.0 | 589.6 | |
| 0.44 | -8.00 | 0.24 | -8.00 | -15.35 | 119.22 | 7.67 | 199.42 | 0.3890 | 689.8 | 999999 | |
| 0.00 | 2.01 | 0.00 | 1.07 | -13.27 | 119.08 | 7.54 | 201.08 | 0.3566 | 996.0 | 848.0 | |
| 0.00 | 1.84 | 0.00 | 0.97 | -13.45 | 118.59 | 7.05 | 199.64 | 0.3567 | 769.0 | 745.8 | |
| 2.71 | -8.00 | 1.45 | -8.00 | -14.76 | 118.57 | 7.03 | 198.39 | 0.3767 | 1103.5 | 999999 | |
| 0.00 | 1.31 | 0.00 | 0.70 | -13.95 | 117.74 | 6.20 | 196.99 | 0.3600 | 770.0 | 632.3 | |
| 0.00 | 0.96 | 0.00 | 0.52 | -16.23 | 117.81 | 6.26 | 195.42 | 0.3958 | 755.0 | 606.9 | |
| 0.00 | 1.40 | 0.00 | 0.75 | -14.33 | 117.72 | 6.18 | 196.62 | 0.3659 | -453.0 | -374.4 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -13.79 | 117.61 | 6.07 | 196.79 | 0.3569 | 882.0 | 738.7 | |
| 0.00 | 2.28 | 0.00 | 1.20 | -13.63 | 117.48 | 5.94 | 196.59 | 0.3538 | 643.0 | 497.7 | |
| 0.00 | 3.76 | 0.00 | 1.99 | -13.88 | 117.18 | 5.64 | 195.59 | 0.3564 | 187.0 | 88.1 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -14.71 | 117.17 | 5.63 | 194.94 | 0.3694 | -786.0 | -542.9 | |
| 0.00 | 3.24 | 0.00 | 1.72 | -14.61 | 116.79 | 5.25 | 194.05 | 0.3663 | -910.0 | -722.8 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -14.35 | 116.73 | 5.18 | 194.05 | 0.3620 | -636.0 | -597.7 | |
| 2.19 | 15.15 | 1.17 | 8.09 | -15.06 | 116.46 | 4.92 | 192.92 | 0.3721 | -830.6 | -522.8 | |
| 1.75 | 2.10 | 0.93 | 1.12 | -14.38 | 116.38 | 4.84 | 193.15 | 0.3611 | -857.4 | -617.5 | |
| 1.23 | 1.93 | 0.65 | 1.02 | -14.41 | 116.11 | 4.56 | 192.40 | 0.3606 | -854.1 | -720.4 | |
| 0.00 | 2.36 | 0.00 | 1.25 | -14.09 | 116.07 | 4.53 | 192.50 | 0.3553 | -799.0 | -756.7 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -15.47 | 116.10 | 4.56 | 191.76 | 0.3774 | -757.0 | -717.7 | |
| 2.10 | 5.52 | 1.12 | 2.93 | -14.51 | 115.95 | 4.41 | 191.94 | 0.3616 | -887.5 | -818.5 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -14.76 | 115.96 | 4.42 | 191.80 | 0.3657 | -629.0 | -461.4 | |
| 2.45 | 4.73 | 1.30 | 2.50 | -13.96 | 115.79 | 4.25 | 191.82 | 0.3523 | -1066.6 | -862.7 | |
| 4.64 | 7.09 | 2.45 | 3.75 | -13.93 | 115.51 | 3.97 | 191.08 | 0.3509 | -1093.7 | -932.0 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -14.02 | 115.29 | 3.75 | 190.45 | 0.3517 | -772.0 | -697.8 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -17.12 | 115.16 | 3.62 | 188.70 | 0.4008 | -615.0 | -352.3 | |
| 0.00 | 2.89 | 0.00 | 1.52 | -13.77 | 115.04 | 3.50 | 189.89 | 0.3468 | -1092.0 | -913.5 | |
| 0.00 | 2.01 | 0.00 | 1.06 | -13.83 | 114.83 | 3.29 | 189.27 | 0.3473 | -778.0 | -659.8 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -16.53 | 114.71 | 3.17 | 187.84 | 0.3904 | -750.0 | -638.4 | |
| 2.10 | 5.25 | 1.13 | 2.81 | -15.98 | 114.58 | 3.04 | 187.72 | 0.3813 | -992.1 | -853.9 | |
| 1.40 | 3.68 | 0.75 | 1.97 | -16.40 | 114.53 | 2.98 | 187.43 | 0.3879 | -744.0 | -683.5 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -16.10 | 114.33 | 2.79 | 187.05 | 0.3829 | -764.0 | -685.7 | |
| 0.00 | 1.66 | 0.00 | 0.89 | -15.23 | 114.23 | 2.69 | 187.08 | 0.3686 | -938.0 | -839.0 | |
| 0.00 | 1.58 | 0.00 | 0.85 | -16.29 | 113.71 | 2.17 | 185.44 | 0.3849 | -579.0 | -439.8 | |
| 0.00 | 1.40 | 0.00 | 0.74 | -14.01 | 113.63 | 2.09 | 185.85 | 0.3477 | -743.0 | -530.5 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -14.30 | 113.57 | 2.03 | 185.61 | 0.3523 | -634.0 | -559.4 | |
| 7.35 | 8.23 | 3.89 | 4.35 | -14.30 | 113.26 | 1.72 | 184.76 | 0.3518 | -971.8 | -709.5 | |
| 0.00 | 2.10 | 0.00 | 1.13 | -16.33 | 113.21 | 1.67 | 184.19 | 0.3847 | -724.0 | -519.5 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -14.55 | 113.04 | 1.50 | 184.11 | 0.3557 | -753.0 | -538.9 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -16.07 | 112.84 | 1.30 | 183.29 | 0.3801 | -927.0 | -708.7 | |
| 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. | |