head echo
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2020 ◽  
Vol 125 (1) ◽  
Author(s):  
Yanlin Li ◽  
Qihou Zhou ◽  
Mark Scott ◽  
Marco Milla

Icarus ◽  
2018 ◽  
Vol 309 ◽  
pp. 177-186 ◽  
Author(s):  
Carsten Schult ◽  
Peter Brown ◽  
Petr Pokorný ◽  
Gunter Stober ◽  
Jorge L. Chau

Icarus ◽  
2017 ◽  
Vol 297 ◽  
pp. 1-13 ◽  
Author(s):  
Carsten Schult ◽  
Gunter Stober ◽  
Diego Janches ◽  
Jorge L. Chau
Keyword(s):  

2017 ◽  
Vol 843 (1) ◽  
pp. 1 ◽  
Author(s):  
D. Janches ◽  
N. Swarnalingam ◽  
J. D. Carrillo-Sanchez ◽  
J. C. Gomez-Martin ◽  
R. Marshall ◽  
...  

2017 ◽  
Vol 122 (4) ◽  
pp. 4697-4711 ◽  
Author(s):  
Y. S. Dimant ◽  
M. M. Oppenheim
Keyword(s):  

2017 ◽  
Vol 10 (2) ◽  
pp. 527-535 ◽  
Author(s):  
Toralf Renkwitz ◽  
Carsten Schult ◽  
Ralph Latteck

Abstract. The Middle Atmosphere Alomar Radar System (MAARSY) with its active phased array antenna is designed and used for studies of phenomena in the mesosphere and lower atmosphere. The flexible beam forming and steering combined with a large aperture array allows for observations with a high temporal and angular resolution. For both the analysis of the radar data and the configuration of experiments, the actual radiation pattern needs to be known. For that purpose, various simulations as well as passive and active experiments have been conducted. Here, results of meteor head echo observations are presented, which allow us to derive detailed information of the actual radiation pattern for different beam-pointing positions and the current health status of the entire radar. For MAARSY, the described method offers robust beam pointing and width estimations for a minimum of a few days of observations.


2016 ◽  
Author(s):  
Toralf Renkwitz ◽  
Carsten Schult ◽  
Ralph Latteck

Abstract. The Middle Atmosphere Alomar Radar SYstem (MAARSY) with its active phased array antenna is designed and used for studies of phenomena in the mesosphere and lower atmosphere. The flexible beam forming and steering combined with a large aperture array allows observations with high temporal and angular resolution. For both, the analysis of the radar data and the configuration of experiments, the actual radiation pattern needs to be known. For that purpose various simulations as well as passive and active experiments have been conducted. Here, results of meteor head echo observations are presented, which allow derivation of detailed information of the actual radiation pattern for different beam pointing positions and the current health status of the entire radar. For MAARSY, the described method offers robust beam pointing and width estimations for a minimum of a few days of observations.


2015 ◽  
Vol 455 (3) ◽  
pp. 3273-3280 ◽  
Author(s):  
Yasunori Fujiwara ◽  
Johan Kero ◽  
Makoto Abo ◽  
Csilla Szasz ◽  
Takuji Nakamura
Keyword(s):  
Mu Radar ◽  

2014 ◽  
Vol 796 (1) ◽  
pp. 41 ◽  
Author(s):  
D. Janches ◽  
J. M. C. Plane ◽  
D. Nesvorný ◽  
W. Feng ◽  
D. Vokrouhlický ◽  
...  

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