IVM Magnetograms
Each magnetogram is a 168 kbyte GIF image. Celestial north is at the top;
east is at the left. The magnetogram is displayed as four panels:
- Continuum brightness
- This is in arbitrary units, but on a linear scale.
- Line-of-sight component of magnetic field
- Projection of magnetic field vector onto the line between the solar feature
and the observer. The units are Gauss. The color changes linearly with the cube
root of the field strength, to better show both strong and weak features. Thus if
the top of the scale is 1000 = 10^3, the midpoint is 5^3 or 125.
- Transverse component of magnetic field
- Magnitude of the projection of the field vector onto the plane perpendicular to
the line of sight. The units are Gauss; cube-root scaling is used here too.
- Direction of transverse component
- The orientation of the transverse component is indicated by the pixel color,
as in the key wheel at the lower left. Note that there is a 180-degree ambiguity in
the direction: the polarization data does not tell us whether the field vector points
to the right or to the left.
AR9620_20010928.1722_ivm
AR9620_20010928.1722_ivm
AR9624_20010928.1718_ivm
AR9624_20010928.1718_ivm
AR9628_20010928.1751_ivm
AR9628_20010928.1751_ivm
AR9632_20010928.1738_ivm
AR9632_20010928.1738_ivm
AR9633_20010928.1706_ivm
AR9633_20010928.1706_ivm
AR9634_20010928.1701_ivm
AR9634_20010928.1701_ivm
AR9635_20010928.1711_ivm
AR9635_20010928.1711_ivm
AR9636_20010928.1650_ivm
AR9636_20010928.1650_ivm
AR9637_20010928.1733_ivm
AR9637_20010928.1733_ivm
AR9638_20010928.1644_ivm
AR9638_20010928.1644_ivm
AR9639_20010928.1656_ivm
AR9639_20010928.1656_ivm
AR9640_20010928.1636_ivm
AR9640_20010928.1636_ivm
AR9641_20010928.1727_ivm
AR9641_20010928.1727_ivm
webmaster@kukui.ifa.hawaii.edu