The sunspot cycle and “auroral”Flayer irregularities

Aarons, J.; Kersley, L.; Rodger, A.S.. 1995 The sunspot cycle and “auroral”Flayer irregularities. Radio Science, 30 (3). 631-638. 10.1029/94RS03191

Full text not available from this repository. (Request a copy)

Official URL: http://dx.doi.org/10.1029/94RS03191

Abstract/Summary

The use of the word “aurora” for many different observations at high latitudes has limited the concepts involved; this is particularly true for F region irregularities. Observations setting the position of the auroral oval (Starkov and Fel'dshtein, 1970) were made using primarily the 555.7-nm green line, which is emitted predominantly at E layer heights. These observations have shown that the change in position of the auroral oval for low values of Kp as a function of sunspot cycle is of the order of 1° to 2° between sunspot maximum and sunspot minimum. However, irregularities in the F region show much larger solar cycle variations in the locations of the equatorward boundary, typically 10°. A review of scintillation data indicates that at a given auroral latitude, the scintillation activity increases with sunspot number. In addition, for a constant scintillation intensity, the equatorward boundary moves to lower latitudes as sunspot maximum is approached. We review existing spread F studies and show that for quiet geomagnetic conditions, there is lower occurrence during years of low sunspot numbers than during years of high sunspot numbers. However, the spread F index, related to Δ ƒ/ƒ0F2, is higher during years of low sunspot number than during years of high sunspot number. We demonstrate that this apparent dichotomy can be reconciled by using a new method of normalizing the spread F index by the maximum electron concentration of the F layer. We briefly discuss the possible explanations for the observed solar cycle variations of irregularity occurrence in terms of the absolute values and gradients of electron concentration and the E region conductivity.

Item Type:	Publication - Article
Digital Object Identifier (DOI):	10.1029/94RS03191
Programmes:	BAS Programmes > Pre 2000 programme
ISSN:	00486604
Date made live:	06 Dec 2016 11:33 +0 (UTC)
URI:	https://nora.nerc.ac.uk/id/eprint/515391

Item Type:

Publication - Article

Digital Object Identifier (DOI):

10.1029/94RS03191

Programmes:

BAS Programmes > Pre 2000 programme

ISSN:

00486604

Date made live:

06 Dec 2016 11:33 +0 (UTC)

URI:

https://nora.nerc.ac.uk/id/eprint/515391