The Sun's Hydrostatic Structure from LOWL Data | Zendy

Sarbani Basu | Zendy; J. ChristensenDalsgaard | Zendy; J. Schou | Zendy; M. J. Thompson | Zendy; S. Tomczyk | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

The Sun's Hydrostatic Structure from LOWL Data

Author(s) -

Sarbani Basu,

J. ChristensenDalsgaard,

J. Schou,

M. J. Thompson,

S. Tomczyk

Publication year - 1996

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/177032

Subject(s) - physics , hydrostatic equilibrium , helioseismology , astrophysics , theoretical physics , statistical physics , computational physics , astronomy , quantum mechanics , magnetic field

Recent observations with the LOWL instrument have for the first time provideda uniform set of frequencies that allow detailed inversion for the structure of muchof the Sun's deep interior. We present the results of inverting the LOWL data andcompare them with the corresponding results obtained using inhomogeneous data setsfrom more than one instrument. Furthermore, improvements in the description of therequired physics motivates the calculation of new solar models. Thus we present...

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research