The Size Distribution of Magnetic Bright Points derived from Hinode/SOT Observations

Details The Size Distribution of Magnetic Bright Points derived from Hinode/SOT Observations The Size Distribution of Magnetic Bright Points derived from Hinode/SOT Observations

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.2.50u&link_type=abstract

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,

Physics

Scientific paper

In our poster we will present our results regarding the size distribution of Magnetic Bright Points (MBPs) in the solar photosphere.
The data sets were obtained through the Solar Optical Telescope (SOT) of the recent Hinode satellite. Hinode was launched in autumn 2006 and delivers (among other data) high resolution seeing free filtergrams in the magnetic sensitive G-Band. We analyzed two different data sets (with different pixel resolutions) near disk center in a network region of the quiet sun. The interesting outcome is that the derived size distribution depends on the used pixel resolution. Discretisation effects and physical implications on the derived size distributions will be discussed.

Affiliated with

Also associated with

No associations

Rating

The Size Distribution of Magnetic Bright Points derived from Hinode/SOT Observations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Size Distribution of Magnetic Bright Points derived from Hinode/SOT Observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Size Distribution of Magnetic Bright Points derived from Hinode/SOT Observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1795808