Mid‐latitude E region field‐aligned irregularities observed with the MU radar

dc.contributor.authorYamamoto, Mamoru
dc.contributor.authorFukao, Shoichiro
dc.contributor.authorWoodman Pollitt, Ronald Francisco
dc.contributor.authorOgawa, Tadahiko
dc.contributor.authorTsuda, Toshitaka
dc.contributor.authorKato, Susumu
dc.date.accessioned2018-07-06T19:32:54Z
dc.date.available2018-07-06T19:32:54Z
dc.date.issued1991-09
dc.description.abstractFine structures E region field-aligned irregularities were observed on June 24–25, 1989, with the MU radar at Shigaraki, Japan (34.9N, 136.1E; geomagnetic latitude 25.0N). The 3.2-m scale irregularities were observed with the MU radar in five main beam directions, each of which was nearly perpendicular to the geomagnetic field at 100 km altitude. Doppler spectra were obtained every 20 s with a range resolution of 600 m. Field-perpendicular echoes appeared from 2130 to 2330 LT and from 0400 to 1100 LT, times that correspond to postsunset and postsunrise period in the E region. A preliminary examination of the Doppler spectra indicates spectral widths of 50–120 m s−1 and the mean Doppler velocities are well below the ion acoustic speed. These spectral characteristics are consistent with those obtained in the equatorial and auroral electrojets, and have been attributed to the gradient drift instability. The echoes observed during the postsunset and postsunrise periods showed quite different morphologies in the time-height distribution. For this reason, they are classified into two types, ‘continuous’ and ‘quasi-periodic.’ The appearance of the ‘continuous’ echoes was mainly continuous in time and situated between 90 and 100 km altitude during the postsunrise period. The appearance of the ‘quasi-periodic’ echoes was intermittent with periods of 5–10 min and situated above 100 km altitude during the postsunset period. The quasi-periodic echoes showed phase propagation toward the radar, while the averaged mean Doppler velocity was away from the radar. By measuring the time delays in echo regions from five directions, an apparent westward motion (approximately 120 m s−1) of the irregularity regions was estimated.es_ES
dc.description.peer-reviewPor pareses_ES
dc.formatapplication/pdfes_ES
dc.identifier.citationYamamoto, M., Fukao, S., Woodman, R. F., Ogawa, T., Tsuda, T., & Kato, S. (1991). Mid‐latitude E region field‐aligned irregularities observed with the MU radar.==$Journal of Geophysical Research: Space Physics, 96$==(A9), 15943-15949. https://doi.org/10.1029/91JA01321es_ES
dc.identifier.doihttps://doi.org/10.1029/91JA01321es_ES
dc.identifier.journalJournal of Geophysical Research: Space Physicses_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/1753
dc.language.isoenges_ES
dc.publisherAmerican Geophysical Uniones_ES
dc.relation.ispartofurn:issn:2169-9380
dc.rightsinfo:eu-repo/semantics/restrictedAccesses_ES
dc.subjectE Regiones_ES
dc.subjectMagnetic fieldses_ES
dc.subjectRadares_ES
dc.subjectGeomagnetismes_ES
dc.subjectEchoeses_ES
dc.subjectDoppler effectes_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.01es_ES
dc.titleMid‐latitude E region field‐aligned irregularities observed with the MU radares_ES
dc.typeinfo:eu-repo/semantics/articlees_ES

Files

Original bundle
Now showing 1 - 1 of 1
No Thumbnail Available
Name:
AAI00139.pdf
Size:
714.36 KB
Format:
Adobe Portable Document Format
Description:
License bundle
Now showing 1 - 1 of 1
No Thumbnail Available
Name:
license.txt
Size:
1.71 KB
Format:
Item-specific license agreed upon to submission
Description: