TY - JOUR
T1 - Small scale ionospheric irregularities near regions of soft particle precipitation
T2 - scintillation and EISCAT observations
AU - Kersley, L.
AU - Pryse, S. E.
AU - Wheadon, N. S.
N1 - Funding Information:
Acknowledgements-This work has been supported by the U.K. Radio Propagation Programme. The assistanceo f staff from the Rutherford Appleton Laboratory in severala spects, and in particular the contribution of Mr A. STEVENSt o software development, is gratefully acknowledged. Financial support has alsb been reieived from U.S. Ai; Force under Grant No. AFOSR 85-0190.T he coooeration of the Director and Staff of the Kiruna Geophysical Institute is also gratefully acknowledged.
Copyright:
Copyright 2014 Elsevier B.V., All rights reserved.
PY - 1988/12
Y1 - 1988/12
N2 - Results are presented from a coordinated experiment involving scintillation observations using transmissions from NNSS satellites and simultaneous measurements with the EISCAT ionospheric radar facility. The scintillation was used to indicate the presence of sub-kilometre scale irregularities while the radar yielded information on the larger structures in the background ionosphere. Two examples are discussed in which localised patches of scintillation were observed at L-shells near 'blob' like enhancements in F-region ionisation density. Elevated electron temperatures indicated that the enhancements may have had their origins in soft particle precipitation. While structuring of the precipitation on the 100 m scale cannot be completely ruled out as a source of the irregularities, in one case the blob gradient can be shown to be stable to the E λ B mechanism. The most likely cause of the irregularities appears to be shearing of the high velocity plasma flow in a region adjacent to the density enhancement. This region is characterised by a high ion temperature while the resulting scintillation has a shallow spectral slope.
AB - Results are presented from a coordinated experiment involving scintillation observations using transmissions from NNSS satellites and simultaneous measurements with the EISCAT ionospheric radar facility. The scintillation was used to indicate the presence of sub-kilometre scale irregularities while the radar yielded information on the larger structures in the background ionosphere. Two examples are discussed in which localised patches of scintillation were observed at L-shells near 'blob' like enhancements in F-region ionisation density. Elevated electron temperatures indicated that the enhancements may have had their origins in soft particle precipitation. While structuring of the precipitation on the 100 m scale cannot be completely ruled out as a source of the irregularities, in one case the blob gradient can be shown to be stable to the E λ B mechanism. The most likely cause of the irregularities appears to be shearing of the high velocity plasma flow in a region adjacent to the density enhancement. This region is characterised by a high ion temperature while the resulting scintillation has a shallow spectral slope.
UR - http://www.scopus.com/inward/record.url?scp=38249029362&partnerID=8YFLogxK
U2 - 10.1016/0021-9169(88)90094-3
DO - 10.1016/0021-9169(88)90094-3
M3 - Article
AN - SCOPUS:38249029362
SN - 0021-9169
VL - 50
SP - 1047
EP - 1055
JO - Journal of Atmospheric and Terrestrial Physics
JF - Journal of Atmospheric and Terrestrial Physics
IS - 12
ER -