LIDAR MEASUREMENTS DURING THE AUGUST 1999 SOLAR ECLIPSE

2001 ◽  
Vol 32 ◽  
pp. 431-432
Author(s):  
P.F. AMBRICO ◽  
P. DI GIROLAMO
2020 ◽  
Vol 12 (4) ◽  
pp. 591 ◽  
Author(s):  
Phillip M. Stepanian ◽  
Charlotte E. Wainwright

The daytime atmospheric boundary layer is characterized by vertical convective motions that are driven by solar radiation. Lift provided by thermal updrafts is sufficiently ubiquitous that some diurnal birds and arthropods have evolved specialized flight behaviors to soar or embed in these atmospheric currents. While the diel periodicity of boundary-layer dynamics and animal flight has been characterized, rare disruptions to this cycle provide a chance to investigate animal behavioral responses to boundary layer motion and photoperiod that are disjointed from their expected circadian rhythm. To analyze these interactions, we couple radar-derived animal observations with co-located lidar measurements of the convective boundary layer over north-central Oklahoma, USA during the solar eclipse of 21 August 2017. Analysis of animal flight behavior confirmed that ascending and descending flight effort did change in the time period encompassing the solar eclipse, however, the response in behavior was coincident with proximate changes in boundary-layer turbulence. Both the animal behavioral response and decrease in atmospheric turbulence lagged changes in solar irradiance by approximately 30 min, suggesting that changes in flight activity were not cued by the eclipse directly, but rather by the modification of vertical air motions caused by the 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

2009 ◽  
Vol 15 (4) ◽  
pp. 12-21 ◽  
Author(s):  
L.Ya. Emelyanov ◽  
◽  
I.B. Sklyarov ◽  
L.F. Chernogor ◽  
◽  
...  
Keyword(s):  

2009 ◽  
Vol 15 (3) ◽  
pp. 70-81 ◽  
Author(s):  
L.Ya. Emelyanov ◽  
◽  
M.V. Lyashenko ◽  
L.F. Chernogor ◽  
◽  
...  

2012 ◽  
Vol 3 (4) ◽  
pp. 311-324 ◽  
Author(s):  
I. F. Domnin ◽  
Leonid Ya. Emelyanov ◽  
L. F. Chernogor

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