Items where Author is "Pinter, B."
Jump to: None
Number of items: 9.
None
CHAPLIN, W. J., ELSWORTH, Y., ISAAK, G. R., MILLER, B. A., NEW, R. and PINTER, B.
(2005).
Noise characteristics of full-disc helioseismic observations made by resonant scattering spectrometers.
Monthly notices of the Royal Astronomical Society, 359 (2), 607-614.
[Article]
CHAPLIN, W. J., DUMBILL, A. M., ELSWORTH, Y. P., ISAAK, G. R., MCLEOD, C. P., MILLER, B. A., NEW, R. and PINTER, B.
(2005).
The search for correlation between BiSONSMMF data and CME events.
In: ENGVOLD, O., (ed.)
Highlights of Astronomy, Vol 13.
Iau Symposia, 13
.
Astronomical Society of the Pacific, p. 141.
[Book Section]
CHAPLIN, W. J., DUMBILL, A. M., ELSWORTH, Y. P., ISAAK, G. R., MCLEOD, C. P., MILLER, B. A., NEW, R. and PINTER, B.
(2004).
Extended search for correlation between solar mean magnetic field bison data and coronal mass ejections.
Solar Physics, 220 (2), 307-316.
[Article]
CHAPLIN, W. J., ELSWORTH, Y., ISAAK, G. R., MILLER, B. A., NEW, R., PINTER, B. and THIERY, S.
(2003).
On the measurement bias of low-l solar p-mode excitation parameters: The impact of a ground-based window function.
Astronomy and Astrophysics, 398 (1), 305-314.
[Article]
CHAPLIN, W. J., DUMBILL, A. M., ELSWORTH, Y., ISAAK, G. R., MCLEOD, C. P., MILLER, B. A., NEW, R. and PINTER, B.
(2003).
Studies of the solar mean magnetic field with the Birmingham Solar-Oscillations Network (BiSON).
Monthly notices of the Royal Astronomical Society, 343 (3), 813-818.
[Article]
CHAPLIN, W. J., ELSWORTH, Y., ISAAK, G. R., MARCHENKOV, K. I., MILLER, B. A., NEW, R., PINTER, B. and APPOURCHAUX, T.
(2002).
Peak finding at low signal-to-noise ratio: low-l solar acoustic eigenmodes at n <= 9 from the analysis of BiSON data.
Monthly notices of the Royal Astronomical Society, 336 (3), 979-991.
[Article]
PINTER, B., ERDELYI, R. and NEW, R.
(2001).
Damping of helioseismic modes in steady state.
Astronomy and Astrophysics, 372 (1), L17-L20.
[Article]
PINTER, B., ERDELYI, R., NEW, R. and GOOSSENS, M.
(2001).
Influence of equilibrium flows and the atmospheric magnetic field on solar oscillation modes.
In: WILSON, A., (ed.)
Proceedings of the Soho 10/Gong 2000 Workshop on Helio- and Asteroseismology at the Dawn of the Millennium.
Esa Special Publications, 464
.
ESA, 227-230.
[Book Section]
PINTER, B., NEW, R. and ERDELYI, R.
(2001).
Rotational splitting of helioseismic modes influenced by a magnetic atmosphere.
Astronomy and Astrophysics Supplement Series, 378 (1), L1-L4.
[Article]