Acoustic noise interferometry in the Straits of Florida at 600 m depth: Preliminary results

2014 ◽  
Vol 135 (4) ◽  
pp. 2167-2167
Author(s):  
Michael G. Brown ◽  
Neil J. Williams ◽  
Xiaoqin Zang ◽  
Oleg A. Godin ◽  
Nikolay A. Zabotin ◽  
...  
2014 ◽  
Vol 135 (4) ◽  
pp. 2167-2167
Author(s):  
Michael G. Brown ◽  
Neil J. Williams ◽  
Geoffrey Banker ◽  
Oleg A. Godin ◽  
Nikolay A. Zabotin ◽  
...  

2014 ◽  
Vol 135 (4) ◽  
pp. 2167-2167
Author(s):  
Oleg A. Godin ◽  
Nikolay A. Zabotin ◽  
Liudmila Zabotina ◽  
Justin S. Ball ◽  
Michael G. Brown ◽  
...  

2019 ◽  
Vol 146 (4) ◽  
pp. 2321-2334 ◽  
Author(s):  
Tsu Wei Tan ◽  
Oleg A. Godin ◽  
Michael G. Brown ◽  
Nikolay A. Zabotin

2015 ◽  
Vol 137 (4) ◽  
pp. 2242-2242
Author(s):  
Sergei Sergeev ◽  
Andrey Shurup ◽  
Alisa Scherbina ◽  
Pavel Mukhanov

2014 ◽  
Vol 136 (4) ◽  
pp. 2156-2156
Author(s):  
Boris Katsnelson ◽  
Oleg Godin ◽  
Jixing Qin ◽  
Nikolai Zabotin ◽  
Liudmila Zabotina ◽  
...  

1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss

AbstractA widely used tool in studying quasi-monoperiodic processes is the O–C diagram. This paper deals with the application of this diagram in minor planet studies. The main difference between our approach and the classical O–C diagram is that we transform the epoch (=time) dependence into the geocentric longitude domain. We outline a rotation modelling using this modified O–C and illustrate the abilities with detailed error analysis. The primary assumption, that the monotonity and the shape of this diagram is (almost) independent of the geometry of the asteroids is discussed and tested. The monotonity enables an unambiguous distinction between the prograde and retrograde rotation, thus the four-fold (or in some cases the two-fold) ambiguities can be avoided. This turned out to be the main advantage of the O–C examination. As an extension to the theoretical work, we present some preliminary results on 1727 Mette based on new CCD observations.


2000 ◽  
Vol 179 ◽  
pp. 163-165
Author(s):  
S. K. Solanki ◽  
M. Fligge ◽  
P. Pulkkinen ◽  
P. Hoyng

AbstractThe records of sunspot number, sunspot areas and sunspot locations gathered over the centuries by various observatories are reanalysed with the aim of finding as yet undiscovered connections between the different parameters of the sunspot cycle and the butterfly diagram. Preliminary results of such interrelationships are presented.


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