Measurements and variations of the solar diameter

Solar Physics ◽  
1996 ◽  
Vol 166 (2) ◽  
pp. 211-229 ◽  
Author(s):  
F. Laclare ◽  
C. Delmas ◽  
J. P. Coin ◽  
A. Irbah
Keyword(s):  
1988 ◽  
Vol 8 (7) ◽  
pp. 119-128 ◽  
Author(s):  
Philippe Delache
Keyword(s):  

Solar Physics ◽  
1983 ◽  
Vol 82 (1-2) ◽  
pp. 139-150 ◽  
Author(s):  
J. R�sch ◽  
R. Yerle
Keyword(s):  

Solar Physics ◽  
2008 ◽  
Vol 247 (2) ◽  
pp. 225-248 ◽  
Author(s):  
D. Djafer ◽  
G. Thuillier ◽  
S. Sofia ◽  
A. Egidi

2013 ◽  
Vol 23 ◽  
pp. 451-453 ◽  
Author(s):  
COSTANTINO SIGISMONDI

The role of Venus and Mercury transits is crucial to know the past history of the solar diameter. Through the W parameter, the logarithmic derivative of the radius with respect to the luminosity, the past values of the solar luminosity can be recovered. The black drop phenomenon affects the evaluation of the instants of internal and external contacts between the planetary disk and the solar limb. With these observed instants compared with the ephemerides the value of the solar diameter is recovered. The black drop and seeing effects are overcome with two fitting circles, to Venus and to the Sun, drawn in the undistorted part of the image. The corrections of ephemerides due to the atmospheric refraction will also be taken into account. The forthcoming transit of Venus will allow an accuracy on the diameter of the Sun better than 0.01 arcsec, with good images of the ingress and of the egress taken each second. Chinese solar observatories are in the optimal conditions to obtain valuable data for the measurement of the solar diameter with the Venus transit of 5/6 June 2012 with an unprecedented accuracy, and with absolute calibration given by the ephemerides.


2021 ◽  
Vol 912 (2) ◽  
pp. 122
Author(s):  
I. Tovar ◽  
A. J. P. Aparicio ◽  
V. M. S. Carrasco ◽  
M. C. Gallego ◽  
J. M. Vaquero

Author(s):  
John H. Parkinson ◽  
F. R. Stephenson ◽  
L. V. Morrison
Keyword(s):  

2001 ◽  
Vol 24 (3) ◽  
pp. 230-230
Author(s):  
Lyes Lakhal

Diameter measurements performed with the solar astrolabe are affected by atmospheric effects. In order to deduce significant astrophysical results, it is necessary to know how these effects contribute to the error of diameter measurement. For this purpose, a numerical simulation was developed leading to a law of error behaviour with observing conditions. In order to validate these results, recorded data obtained at the Calern observatory astrolabe (France) during the period 1996 – 1997 are used. A good agreement is observed with the simulation, which permit salso to give access to daily atmospheric time constants. (Co-author is A. Irbah, Algeria.)


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