The flux-gap between bright and dark solar magnetic structures

@inproceedings{Puschmann2005TheFB,
  title={The flux-gap between bright and dark solar magnetic structures},
  author={Katharina Puschmann and E. Wiehr},
  year={2005}
}
The upper size limit of solar small-scale magnetic flux concentrations (“G-band bright points”, BP) is reconsidered from speckle-reconstructed images taken at the 1-m SST on La Palma. The size-histogram shows a sharp drop towards 250 km diameter, variation of the noise filter threshold diminishes that value due to segmentation of the elongated structures. A… CONTINUE READING