What can p-mode absorption and phase shift data currently tell us about the subsurface structure of sunspots? Preliminary results

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 559, 2004, Pages 392-395

  Crouch, A D ^a   Cally, P S ^b  

^a UNIVERSITÉ DE MONTRÉAL   (Canada)

^b MONASH UNIVERSITY   (Australia)

Author keywords

[No Author keywords available]

Indexed keywords

ACOUSTIC EMISSIONS; ASTRONOMY; BOUNDARY CONDITIONS; GRAVITATION; GRAVITY WAVES; HEAT CONVECTION; MAGNETIC FIELDS; MATHEMATICAL MODELS;

ADIABATIC INDEX; SOLAR CONVECTION ZONE; SUNSPOTS; VERTICAL MAGNETIC FIELDS;

SUN;

EID: 22144457652     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

References (8)

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2. Bogdan, T. J., and Cally, P. S. 1995, Astrophys. J., 453, 919.
3. Braun, D. C.: 1995, Astrophys. J. 451, 859.
4. Cally, P. S., Bogdan, T. J., and Zweibel, E. G.: 1994, Astrophys. J. 437, 505.
5. Cally, P. S., Crouch, A. D., and Braun, D. C.: 2003, Monthly Notices Royal Astron. Soc. 346, 381.
6. Christensen-Dalsgaard J., 1997, Aarhus adiabatic pulsation package, http://www.obs.aau.dk/~jcd/adipack.n/.
7. Crouch, A. D. and Cally, P. S.: 2003, Solar Phys. 214, 201.
8. Donea, A.-C., Lindsey, C., and Braun, D. C.: 2000, Solar Phys. 192, 321.