scholarly journals ATMOSPHERIC PRESSURE PERTURBATION DURING TOTAL SOLAR ECLIPSE

MAUSAM ◽  
2021 ◽  
Vol 60 (1) ◽  
pp. 103-106
Author(s):  
SUKUMAR LALA ◽  
SEEMA SHARMA ◽  
SWATI CHAKRABARTI ◽  
NABAJIT CHAKRAVARTY
1992 ◽  
Vol 54 (2) ◽  
pp. 113-115 ◽  
Author(s):  
Barrie W. Jones ◽  
Gerald J. Miseldine ◽  
Robert J.A. Lambourne

2016 ◽  
Vol 771 ◽  
pp. 012009 ◽  
Author(s):  
Lala Septem Riza ◽  
Yaya Wihardi ◽  
Enjang Ali Nurdin ◽  
Nanang Dwi Ardi ◽  
Cahyo Puji Asmoro ◽  
...  

Author(s):  
J. M. Pasachoff ◽  
M. A. Peñaloza-Murillo ◽  
A. L. Carter ◽  
M. T. Roman

This article reports on the near-surface atmospheric response at the High Arctic site of Svalbard, latitude 78° N, as a result of abrupt changes in solar insolation during the 20 March 2015 equinox total solar eclipse and notifies the atmospheric science community of the availability of a rare dataset. Svalbard was central in the path of totality, and had completely clear skies. Measurements of shaded air temperature and atmospheric pressure show only weak, if any, responses to the reduced insolation. A minimum in the air temperature at 1.5 m above the ground occurred starting 2 min following the end of totality, though this drop was only slightly beyond the observed variability for the midday period. Eclipse-produced variations in surface pressure, if present, were less than 0.3 hPa. This article is part of the themed issue ‘Atmospheric effects of solar eclipses stimulated by the 2015 UK eclipse’.


1994 ◽  
Vol 144 ◽  
pp. 593-596
Author(s):  
O. Bouchard ◽  
S. Koutchmy ◽  
L. November ◽  
J.-C. Vial ◽  
J. B. Zirker

AbstractWe present the results of the analysis of a movie taken over a small field of view in the intermediate corona at a spatial resolution of 0.5“, a temporal resolution of 1 s and a spectral passband of 7 nm. These CCD observations were made at the prime focus of the 3.6 m aperture CFHT telescope during the 1991 total solar eclipse.


1994 ◽  
Vol 144 ◽  
pp. 541-547
Author(s):  
J. Sýkora ◽  
J. Rybák ◽  
P. Ambrož

AbstractHigh resolution images, obtained during July 11, 1991 total solar eclipse, allowed us to estimate the degree of solar corona polarization in the light of FeXIV 530.3 nm emission line and in the white light, as well. Very preliminary analysis reveals remarkable differences in the degree of polarization for both sets of data, particularly as for level of polarization and its distribution around the Sun’s limb.


1917 ◽  
Vol 83 (2145supp) ◽  
pp. 93-93
Author(s):  
Edison Pettit

2017 ◽  
Vol 1 (1) ◽  
pp. 68-71 ◽  
Author(s):  
Hui Tian ◽  
◽  
ZhongQuan Qu ◽  
YaJie Chen ◽  
LinHua Deng ◽  
...  

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