Anti-interference methods in solar radio high time-resolution observation

1995 ◽  
Vol 19 (3) ◽  
pp. 399
Keyword(s):  
Time Resolution ◽  
Solar Radio ◽  
High Time ◽  
High Time Resolution ◽  
Resolution Observation

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

A solar radio spectrograph with high time resolution

Solar Physics ◽  
1972 ◽  
Vol 26 (2) ◽  
pp. 386-392 ◽  
Author(s):  
B. L. Gotwols ◽  
J. Phipps
Keyword(s):  
Time Resolution ◽  
Solar Radio ◽  
High Time ◽  
High Time Resolution

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

Fast Drift Bursts, Spikes, and Continua Observations in the 100-4200 MHz Band

1994 ◽  
Vol 144 ◽  
pp. 285-287
Author(s):  
K. Jiřička ◽  
M. Karlický ◽  
O. Kepka ◽  
A. Tlamicha
Keyword(s):  
Time Resolution ◽  
Solar Radio ◽  
High Time ◽  
High Time Resolution ◽  
Observational System ◽  
Fast Drift

AbstractNew Ondřejov solar radio observational system consisting of a high-time resolution 3000 MHz receiver and of a 100-4200 MHz radiospectrograph is described and some results of observation of fast drift bursts, spikes, and continua are presented.

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.

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