Traveling Waves In Network Bright Points

Details Traveling Waves In Network Bright Points Traveling Waves In Network Bright Points

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..848..229k&link_type=abstract

RECENT ADVANCES IN ASTRONOMY AND ASTROPHYSICS: 7th International Conference of the Hellenic Astronomical Society. AIP Conferenc

Astronomy and Astrophysics

Astrophysics

1

Chromosphere, Magnetohydrodynamics And Plasmas

Scientific paper

One of the main features of the quiet solar chromosphere is the Network Bright Points (NBP), formed by the emerging magnetic flux, at the boundaries of supergranular cells. Triggered by the motions of magnetic loop foot-points, at the top of the convection zone, MHD waves propagate inside the NBP's. Using SSW IDL routines and wavelet analysis of series of images in four bandpasses (CaII K3, Mgb1-0.4, Mgb2 and Ha core) we detected these MHD wave modes. The observations have been analyzed using cross-correlation techniques and we have drawn conclusions on wave propagation and mode coupling.

Affiliated with

Also associated with

No associations

Rating

Traveling Waves In Network Bright Points 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 Traveling Waves In Network Bright Points, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Traveling Waves In Network Bright Points will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1130757