Thermal-magnetic relation of a sunspot as inferred from the inversion of 1.5 μm spectral data

Details Thermal-magnetic relation of a sunspot as inferred from the inversion of 1.5 μm spectral data Thermal-magnetic relation of a sunspot as inferred from the inversion of 1.5 μm spectral data

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.505..501m&link_type=abstract

In: SOLMAG 2002. Proceedings of the Magnetic Coupling of the Solar Atmosphere Euroconference and IAU Colloquium 188, 11 - 15 Jun

Computer Science

1

Sunspots, Magnetic Field, Spectropolarimetry, Infrared

Scientific paper

We present the thermal-magnetic relation in a simple, isolated sunspot deduced from the inversion of 1.56 μm spectropolarimetric data. Due to the high Zeeman sensitivity of the g = 3, Fe I 1.5648 μm line, we can study this relationship in the entire sunspot. An inversion technique based on response functions is used to derive various parameters, both as a function of location within the sunspot and of height in the atmosphere. In this paper we attempt to relate field strength, vertical and radial field components and the field inclination with temperature.

Affiliated with

Also associated with

No associations

Rating

Thermal-magnetic relation of a sunspot as inferred from the inversion of 1.5 μm spectral data 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 Thermal-magnetic relation of a sunspot as inferred from the inversion of 1.5 μm spectral data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Thermal-magnetic relation of a sunspot as inferred from the inversion of 1.5 μm spectral data will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1422744