The height dependence of temperature - velocity correlation in the solar photosphere

Details The height dependence of temperature - velocity correlation in the solar photosphere The height dependence of temperature - velocity correlation in the solar photosphere

2007-04-04

arxiv.org/abs/0704.0603v1

Astronomy and Astrophysics

Astrophysics

In press,"Modern Solar Facilities - Advanced Solar Science", (Gottingen), Universitatsverlag Gottingen, 139-142, 2007

Scientific paper

We derive correlation coefficients between temperature and line-of-sight velocity as a function of optical depth throughout the solar photosphere for the non-magnetic photosphere and a small area of enhanced magnetic activity. The maximum anticorrelation of about -0.6 between temperature and line-of-sight velocity in the non-magnetic photosphere occurs at log tau5 = -0.4. The magnetic field is another decorrelating factor along with 5-min oscillations and seeing.

Affiliated with

Also associated with

No associations

Rating

The height dependence of temperature - velocity correlation in the solar photosphere 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 height dependence of temperature - velocity correlation in the solar photosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The height dependence of temperature - velocity correlation in the solar photosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-213881