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41by Heon-Young Chang“...In helioseismology it is normally assumed that p-mode oscillations are excited in a statistically...”
Published 2009-09-01
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42“...-indices, the indication of a changed pattern of internal torsional waves (helioseismology...”
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43by Cobden, Laura Jacqueline“.... On the Sun, this is a relatively new field (helioseismology), in which cross-correlation is used to extract...”
Published 2008
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44Seismology of Giant Planets: General Overview and Results from the Kepler K2 Observations of Neptuneby Gaulme Patrick“... to that of solar-like stars than that of terrestrial planets. Hence, helioseismology techniques naturally transfer...”
Published 2017-01-01
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45by Burrows, Keiran Robert“...Ring Diagram Analysis (RDA) is one of the cornerstones of local helioseismology. The technique...”
Published 2014
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46by Chunkao Ruan, Yongyi Chen, Li Qin, Peng Jia, Yugang Zeng, Yue Song, Yuxin Lei, Zhijun Zhang, Nan Zhang, Zaijin Li“... region is important for helioseismology, solar atmospheric studies, the pumping of atomic clocks...”
Published 2021-02-01
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47by A. Barreto, E. Cuevas, P. Pallé, P. M. Romero, C. Guirado, C. J. Wehrli, F. Almansa“... as a reference instrument for helioseismology, and its ability to determine AOD from transmitted...”
Published 2014-12-01
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48by Luiz Themystokliz Sanctos Mendes“... the flat solar rotation rate obtained from helioseismology, indicating that, in the Sun, angular momentum...”
Published 1999
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49by Hazra, Gopal“... development in helioseismology, plenty of results have come out about various spatial structure of meridional...”
Published 2018
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50by Barbouteau, Sandra“... Lobkis (2001)), seismic exploration and even helioseismology (Duvall et al. (1993)). In all these cases...”
Published 2014
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51by Raimondi, Francesca“... to the estimation of the impulse response of the Sun for helioseismology....”
Published 2017
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52by V. N. Krivodubskij“... the non-linear effects of turbulent plasma and recent data of helioseismological experiments one can...”
Published 2014-10-01
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53by Sule, Aniket“.... Helioseismological estimates put this layer at roughly $0.7R_{sun}$. The tachocline mostly resides in the sub...”
Published 2007
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Doctoral Thesis