LIEN
发表于 2025-3-28 18:18:20
M. J. Thompson,S. Zharkovn. Den eindimensionalen Fall haben wir in Kapitel 10 eingehend behandelt. Aufgrund der Sätze . und . kann man z.B. folgendes sagen: Ist die Funktion .:].[→ ℝ stetig differenzierbar und ist .(t.)≠0, so ist . in einer ganzen Umgebung . von . streng monoton, besitzt somit in . eine Umkehrfunktion . un
idiopathic
发表于 2025-3-28 21:51:28
D. C. Braun,A. C. Birchtics skillfully with didactical and historical consideration.Volume III sets out classical Cauchy theory. It is much more geared towards its innumerable applications than towards a more or less complete theory of analytic functions. Cauchy-type curvilinear integrals are then shown to generalize to a
书法
发表于 2025-3-29 00:25:38
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exophthalmos
发表于 2025-3-29 06:49:56
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发电机
发表于 2025-3-29 08:50:03
,Global Effects of Local Sound-Speed Perturbations in the Sun: A Theoretical Study,ugh comparisons with error estimates obtained from Michelson Doppler Imager (MDI; Scherrer ., .., 129, .) observations, we find that the frequency differences are detectable with a sufficiently long time series (70 – 642 days).
摄取
发表于 2025-3-29 11:26:02
Influence of Low-Degree High-Order ,-Mode Splittings on the Solar Rotation Profile, velocities measured with the GOLF instrument. We carried out a theoretical study of the influence of the low-degree modes in the region from 2 to 3.5 mHz on the inferred rotation profile as a function of their error bars.
Hemodialysis
发表于 2025-3-29 19:31:11
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CRUMB
发表于 2025-3-29 23:13:36
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membrane
发表于 2025-3-30 02:01:14
Uncovering the Bias in Low-Degree ,-Mode Linewidth Fitting,scatter to increase the sample standard deviation per 40-second measurement. In all cases, the observational duration required to accurately obtain width estimates increases beyond that required for sufficient spectral resolution below a certain threshold frequency. For modes at ≈ 1500 μHz, with an
sphincter
发表于 2025-3-30 04:15:03
,Analysis of MDI High-Degree Mode Frequencies and their Rotational Splittings,a correction to the Carrington elements. We also present variations of the mode frequencies caused by the solar activity cycle. We have analyzed seven observational periods from 1999 to 2005 and correlated their frequency shift with four different solar indices. The frequency shift scaled by the rel