Abstract
I point out that the flare energetics has a central role in our understanding of the nature of the flare phenomena /see also Grandpierre, 1986/. Combining the recent observational data with the values expected by the magnetic flare theories/MFT/ I show here that they are inconsistent with a lot of basic observational fact. I calculate the energies and the respective time scales of flares by the convective flare theory/CFT/ and I find that the results seem to be consistent with the observations. I present some prophecies of the CFT for the future observations as the relation between the energy liberation in central stellar regions and the flare activity, dependence of flare activity on stellar ages and spot dynamics.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
X.-Z. Chen et al.,1984, Chin. Astron. Astrophys. 8,pp.299–305
H.W. Dodson, E.R. Hedeman,1970, Solar Phys., 13,pp.401–419
O.Engvold,1987, personal communication
W.M. Glencross, 1979, Monthly Notices of R.A.S., 186 pp. 305–316
A. Grandpierre, 1981, Astrophys. Space Sci.,75, pp.307–314
A. Grandpierre,1984, in “Theoretical Problems in Stellar Stability and Oscillations”, Proc.25th Liege Intern. Astrophys. Coll., July 10–13,ed. by A. Noels and M. Gabriel
A. Grandpierre, 1986, in“Flare Stars and Related Objects”,Proc. Symp. Byur. Astrophys. Obs., Oct.16–19, 1984, Ed. by L.V. Mirzoyan, pp. 176–182
A.Grandpierre, (1987) in preparation
A.Grandpierre, (1988) in preparation
A. Grandpierre, N.D. Melikyan, 1985, Astrophys.Space Sci., 116, pp.189–195
T. Hirayama, 1961, Publ. Astron. Soc. Japan 13, pp.152–165
M.E. Machado, J.L. Linsky,1975, Solar Phys. 42,pp.395–420
Z. Mouradian et al.,1983, Solar Phys. 87, pp.309–328
D.F. Neidig, E.W. Cliver,1983, Air Force Geophysics Laboratory, AFGL-TR-83–0257
V.S. Oskanyan,1986, in“Flare Stars and Related Objects”, pp.11–18
E.N. Parker,1963, Ap. J. Suppl. Vol 8, pp. 177–211
J.H. Piddington,1973, Solar Phys. 31, p. 229–241
E.R. Priest, 1981, in “Solar Flare Magnetohydrodynamics”,ed. by E.R. Priest, Gordon and Breach Sci. Publ., p.16.
D.M. Rust,1984, Solar Phys. 93, pp.73–83
H.C. Spruit, 1970, Solar Phys. 34, pp.277–290
Z.E. Hiei, 1959, Publ. Astron. Soc. Japan 11, pp.185–194
Z. Svestka, 1976, “Solar Flares”,Dordrecht-Reidel
M.K. Tsvetkov et al.,1986, Intern. Bull. Var. Stars, No.2972
D.G. Wentzel, 1963, in “AAS - NASA Symp. on the Physics of Solar Flares”, pp.397–407
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1988 Kluwer Academic Publishers
About this paper
Cite this paper
Grandpierre, A. (1988). Flares: Magnetic or Convective Origin?. In: Havnes, O., Pettersen, B.R., Schmitt, J.H.M.M., Solheim, J.E. (eds) Activity in Cool Star Envelopes. Astrophysics and Space Science Library, vol 143. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2951-7_25
Download citation
DOI: https://doi.org/10.1007/978-94-009-2951-7_25
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7827-6
Online ISBN: 978-94-009-2951-7
eBook Packages: Springer Book Archive