Browse by Journals
![[up]](/style/images/multi_up.png)
Up a levelJump to: None
Number of items: 6.
None
CHAPLIN, W. J., APPOURCHAUX, T., ELSWORTH, Y., ISAAK, G. R., MILLER, B. A. and NEW, R.
(2004).
On comparing estimates of low-l solar p-mode frequencies from Sun-as-a-star and resolved observations.
Astronomy and Astrophysics, 424 (2), 713-717.
[Article]
CHAPLIN, W. J., APPOURCHAUX, T., ELSWORTH, Y., ISAAK, G. R., MILLER, B. A., NEW, R. and TOUTAIN, T.
(2004).
Solar p-mode frequencies at l=2: What do analyses of unresolved observations actually measure?
Astronomy and Astrophysics, 416 (1), 341-351.
[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., ELSWORTH, Y., ISAAK, G. R., MILLER, B. A., NEW, R. and SALABERT, D.
(2004).
Impact of observational duty cycle on the measurement of low-l solar p-mode frequencies.
Astronomy and Astrophysics, 424 (1), 301-309.
[Article]
CHAPLIN, W. J., HOUDEK, G., APPOURCHAUX, T., ELSWORTH, Y., NEW, R. and TOUTAIN, T.
(2008).
Challenges for asteroseismic analysis of Sun-like stars.
Astronomy and Astrophysics, 485 (3), 813-822.
[Article]
PINTER, B., ERDELYI, R. and NEW, R.
(2001).
Damping of helioseismic modes in steady state.
Astronomy and Astrophysics, 372 (1), L17-L20.
[Article]