Mostrar el registro sencillo del ítem Malhotra, Akshay Mathews, John D. Ray, Kimberly 2018-11-05T17:47:48Z 2018-11-05T17:47:48Z 2009-11-24
dc.identifier.citation Malhotra, A., Mathews, J. D., & Ray, K. (2009). Aspect sensitivity considerations in determining day‐to‐night variations in meteor trail durations.==$Geophysical Research Letters, 36$==(22), L22105. es_ES
dc.description.abstract Recently there has been an interest in the day‐to‐night variations in the duration of non‐specular meteor trails or Range Spread Trail Echoes (RSTE). The reported differences between the day and night durations of meteor trails have been used to arrive at conclusions on the role played by background plasma concentration and background electric field and/or winds in the formation and evolution of RSTEs in general. However, the work done to‐date does not account for the aspect sensitivity of meteor trails. We present the duration distribution of meteor trails — the most comprehensive study yet on RSTE durations — considering the aspect sensitivity of these trails. In contrast to the previous reports, the day‐night trail durations are statistically similar in our observations. These results stress the importance of considering aspect sensitivity while performing any such study and how a failure to do so might result in misleading results and conclusions. es_ES
dc.format application/pdf es_ES
dc.language.iso eng es_ES
dc.publisher American Geophysical Union es_ES
dc.relation.ispartof urn:issn:0094-8276
dc.rights info:eu-repo/semantics/restrictedAccess es_ES
dc.subject Radars es_ES
dc.subject Meteors es_ES
dc.subject Aspect sensitivity es_ES
dc.title Aspect sensitivity considerations in determining day‐to‐night variations in meteor trail durations es_ES
dc.type info:eu-repo/semantics/article es_ES
dc.subject.ocde es_ES
dc.identifier.journal Geophysical Research Letters es_ES
dc.description.peer-review Por pares es_ES
dc.identifier.doi es_ES




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