A search for atmospheric pressure waves from the total solar eclipse of 9 March 1997

1999 ◽  
Vol 61 (14) ◽  
pp. 1017-1024 ◽  
Author(s):  
Barrie W Jones
Keyword(s):  
Solar Eclipse ◽  
Atmospheric Pressure ◽  
Total Solar Eclipse ◽  
Pressure Waves

A possible atmospheric pressure wave from the total solar eclipse of 22 July 1990

1992 ◽  
Vol 54 (2) ◽  
pp. 113-115 ◽  
Author(s):  
Barrie W. Jones ◽  
Gerald J. Miseldine ◽  
Robert J.A. Lambourne
Keyword(s):  
Solar Eclipse ◽  
Atmospheric Pressure ◽  
Pressure Wave ◽  
Total Solar Eclipse

scholarly journals Analysis on atmospheric pressure, temperature, and wind speed profiles during total solar eclipse 9 March 2016 using time series clustering

2016 ◽  
Vol 771 ◽  
pp. 012009 ◽  
Author(s):  
Lala Septem Riza ◽  
Yaya Wihardi ◽  
Enjang Ali Nurdin ◽  
Nanang Dwi Ardi ◽  
Cahyo Puji Asmoro ◽  
...  
Keyword(s):  
Time Series ◽  
Wind Speed ◽  
Solar Eclipse ◽  
Atmospheric Pressure ◽  
Total Solar Eclipse ◽  
Time Series Clustering

scholarly journals Terrestrial atmospheric responses on Svalbard to the 20 March 2015 Arctic total solar eclipse under extreme conditions

2016 ◽  
Vol 374 (2077) ◽  
pp. 20160188 ◽  
Author(s):  
J. M. Pasachoff ◽  
M. A. Peñaloza-Murillo ◽  
A. L. Carter ◽  
M. T. Roman
Keyword(s):  
Air Temperature ◽  
Solar Eclipse ◽  
Atmospheric Pressure ◽  
High Arctic ◽  
Total Solar Eclipse ◽  
Atmospheric Effects ◽  
Solar Insolation ◽  
Near Surface ◽  
Abrupt Changes ◽  
Science Community

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’.

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
Keyword(s):  
Solar Eclipse ◽  
Atmospheric Pressure ◽  
Total Solar Eclipse ◽  
Pressure Perturbation

Very High Resolution Analysis of the Dynamics of a Coronal Plasmoid

1994 ◽  
Vol 144 ◽  
pp. 593-596
Author(s):  
O. Bouchard ◽  
S. Koutchmy ◽  
L. November ◽  
J.-C. Vial ◽  
J. B. Zirker
Keyword(s):  
High Resolution ◽  
Solar Eclipse ◽  
Total Solar Eclipse ◽  
Field Of View ◽  
Small Field ◽  
High Resolution Analysis ◽  
Ccd Observations ◽  
Resolution Analysis ◽  
Very High ◽  
Small Field Of View

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.

FeXIV Line Emission Polarization of the July 11, 1991 Solar Corona

1994 ◽  
Vol 144 ◽  
pp. 541-547
Author(s):  
J. Sýkora ◽  
J. Rybák ◽  
P. Ambrož
Keyword(s):  
High Resolution ◽  
Solar Corona ◽  
Emission Line ◽  
Solar Eclipse ◽  
White Light ◽  
Preliminary Analysis ◽  
Line Emission ◽  
Total Solar Eclipse ◽  
Degree Of Polarization ◽  
High Resolution Images

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.

The Total Solar Eclipse of June 8, 1918

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

scholarly journals Observations of the solar corona during the total solar eclipse on 21 August 2017

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