The influence of changing stratification conditions on barotropic tidal transport and its implications for seasonal and secular changes of tides

2012 ◽  
Vol 47 ◽  
pp. 107-118 ◽  
Author(s):  
M. Müller
1998 ◽  
Vol 11 (1) ◽  
pp. 346-346
Author(s):  
E. Zsldos

The light curves of luminous stars often show spectacular secular changes which can be connected to stellar evolution. Such events are, e.g. the outbursts of P Cygni in the 17th century and 77 Carinae in the last century. Both stars belong to the Luminous Blue Variables, but these changes are not restricted to blue stars. The light curve of HR 8752 (V509 Cassiopeiae) shows a certain similarity to that of the former two stars. When it was first catalogued in the middle of the 19th century, it had been a 6m star. During 100 years the star showed a secular brightening of lm. A similar yellow hypergiant, p Cassiopeiae produced at least two outbursts this century, though both have smaller amplitudes than it is in the case of the LBVs. Moreover, these yellow variables also have an apparently secular colour change: the B − V colour of HR 8752 is decreasing while that of ρ Cassiopeiae is increasing. In both cases evolutionary changes are possible but one cannot exclude other causes. Besides these well studied stars there are several other yellow hypergiants with promising light curves. One of the most interesting cases seems to be R Puppis, which was discovered to be variable in the last century, but then did not show any appreciable change in the following 70-80 years. In the late 1970s, however, it began to vary once more.


Author(s):  
Vasubandhu Misra ◽  
Akhilesh Mishra ◽  
Amit Bhardwaj ◽  
Krishnan Viswanathan ◽  
Dan Schmutz

2018 ◽  
Vol 3 (2) ◽  
pp. 276-280 ◽  
Author(s):  
Charlotte Tye ◽  
Laura E. Thomas ◽  
Julian R. Sampson ◽  
Julia Lewis ◽  
Finbar O'Callaghan ◽  
...  

2010 ◽  
Vol 69 (4) ◽  
pp. 381-389 ◽  
Author(s):  
Non E Thomas ◽  
DRR Williams ◽  
David A Rowe ◽  
Bruce Davies ◽  
Julien S Baker

2013 ◽  
Vol 24 (2) ◽  
pp. 451-452 ◽  
Author(s):  
T.M. Kusky ◽  
R.J. Stern ◽  
J.F. Dewey

Author(s):  
Roger Edwards ◽  
Harold E. Brooks ◽  
Hannah Cohn

AbstractUnited States tornado records form the basis for a variety of meteorological, climatological and disaster-risk analyses, but how reliable are they in light of changing standards for rating, as with the 2007 transition of Fujita (F) to Enhanced Fujita (EF) damage scales? To what extent are recorded tornado metrics subject to such influences that may be nonmeteorological in nature? While addressing these questions with utmost thoroughness is too large of a task for any one study, and may not be possible given the many variables and uncertainties involved, some variables that are recorded in large samples are ripe for new examination. We assess basic tornado-path characteristics—damage rating, length, width, and occurrence time, as well as some combined and derived measures—for a 24-yr period of constant path-width recording standard that also coincides with National Weather Service modernization and the WSR-88D deployment era. The middle of that period (in both time and approximate tornado counts) crosses the official switch from F to EF. At least minor shifts in all assessed path variables are associated directly with that change, contrary to the intent of EF implementation. Major and essentially stepwise expansion of tornadic path widths occurred immediately upon EF usage, and widths have expanded still further within the EF era. We also document lesser increases in path lengths, and in tornadoes rated at least EF1 compared to EF0. These apparently secular changes in the tornado data can impact research dependent on bulk tornado-path characteristics and damage-assessment results.


1998 ◽  
Vol 25 (3-4) ◽  
pp. 241-262 ◽  
Author(s):  
S. Zerbini ◽  
T. Baker ◽  
M. Negusini ◽  
H.-P. Plag ◽  
C. Romagnoli
Keyword(s):  

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