High time resolution observation and statistical analysis of atmospheric light extinction properties and the chemical speciation of fine particulates

2010 ◽  
Vol 53 (8) ◽  
pp. 1801-1808 ◽  
Author(s):  
TingTing Yao ◽  
XiaoFeng Huang ◽  
LingYan He ◽  
Min Hu ◽  
TianLe Sun ◽  
...  
Keyword(s):  
Statistical Analysis ◽  
Time Resolution ◽  
Chemical Speciation ◽  
High Time ◽  
Light Extinction ◽  
High Time Resolution ◽  
Fine Particulates ◽  
Resolution Observation ◽  
Atmospheric Light

Insights into the characteristics and sources of primary and secondary organic carbon: High time resolution observation in urban Shanghai

2018 ◽  
Vol 233 ◽  
pp. 1177-1187 ◽  
Author(s):  
Jian Xu ◽  
Qiongzhen Wang ◽  
Congrui Deng ◽  
V. Faye McNeill ◽  
Alison Fankhauser ◽  
...  
Keyword(s):  
Organic Carbon ◽  
Time Resolution ◽  
High Time ◽  
High Time Resolution ◽  
Resolution Observation ◽  
Secondary Organic Carbon

scholarly journals Characteristics of Aerosol WSI With High‐Time‐Resolution Observation Over Arctic Ocean

2020 ◽  
Vol 7 (9) ◽  
Author(s):  
Congcong Yu ◽  
Jinpei Yan ◽  
Honghai Zhang ◽  
Qi Lin ◽  
Hongguo Zheng ◽  
...  
Keyword(s):  
Arctic Ocean ◽  
Time Resolution ◽  
High Time ◽  
High Time Resolution ◽  
Resolution Observation

scholarly journals Investigations of the Magnetic Star 53 Cam Variations Using the Spectra of High Time Resolution

1986 ◽  
Vol 90 ◽  
pp. 243-252
Author(s):  
N.S. Polosukhina ◽  
V.P. Malanushenko ◽  
I. Tuominen ◽  
H. Karttunen ◽  
H. Virtanen
Keyword(s):  
Statistical Analysis ◽  
Time Resolution ◽  
High Time ◽  
Magnetic Star ◽  
High Time Resolution

AbstractThe results of automatic reduction of spectral observations of 53 Cam with high time resolution are presented. The statistical analysis of deviations of individual spectrograms of a star from the averaged one for one night permits one to allocate variable details of spectra and estimate the amplitudes of their variability.

Solar Corona Investigation by the Coronal Line Photometer at Lomnický Peak

1994 ◽  
Vol 144 ◽  
pp. 431-434
Author(s):  
M. Minarovjech ◽  
M. Rybanský
Keyword(s):  
Solar Corona ◽  
Time Resolution ◽  
Active Regions ◽  
High Time ◽  
High Time Resolution ◽  
List Type ◽  
Type Number ◽  
Coronal Line ◽  
Global Cycle

AbstractThis paper deals with a possibility to use the ground-based method of observation in order to solve basic problems connected with the solar corona research. Namely:1.heating of the solar corona2.course of the global cycle in the corona3.rotation of the solar corona and development of active regions.There is stressed a possibility of high-time resolution of the coronal line photometer at Lomnický Peak coronal station, and use of the latter to obtain crucial observations.

Discovery of the fast optical variability of GRB 080319B and the prospects for wide-field optical monitoring with high time resolution

2010 ◽  
Vol 180 (4) ◽  
pp. 424 ◽  
Author(s):  
G.M. Beskin ◽  
S.V. Karpov ◽  
S.F. Bondar ◽  
V.L. Plokhotnichenko ◽  
A. Guarnieri ◽  
...  
Keyword(s):  
Time Resolution ◽  
High Time ◽  
High Time Resolution ◽  
Optical Variability ◽  
Wide Field ◽  
Optical Monitoring
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