Trimpi perturbations from large ionisation enhancement patches
نویسندگان
چکیده
A number of increasingly sophisticated and realistic models have been developed in order to investigate the interaction between sub-ionospherically propagating VLF waves and regions of ionisation enhancement (LIE) in the D-region caused by lightning-induced electron precipitation enhancements (LEP). This LEP-produced LIE can result in phase and amplitude perturbations on received VLF radio signals that are referred to as Trimpis or more precisely, classic Trimpis, to distinguish them from ``early/fast Trimpis'' or ``VLF sprites'' which are not caused by LEP and are not considered here. It is important, for comparison with experimentally observed Trimpi eects, that the spatial extent of the D-region electron density (Ne) perturbation is modeled accurately. Here, it is argued that most previous modeling has used patch (LIE) sizes that are typically up to 100 km in both latitudinal and longitudinal extent, which are generally smaller than those that actually occur for real lightning induced electron precipitation events. It would also appear that maximum DNe values assumed have often been too large, and the patches (LIEs) have been incorrectly modelled as circular rather than elliptical in horizontal extent. Consequently, in the present work, Trimpi perturbations are determined for LIEs with smaller maximum DNe, larger spatial extent and elliptical shape. Calculations of VLF Trimpis have been made as a function of the horizontal coordinates of the LIE centre, over the whole rectangular corridor linking transmitter and receiver. The Trimpi modelling program is fully 3D, and takes account of modal mixing at the LIE. The underlying theory assumes weak Born scattering, but the code calculates a non-Born skin depth attenuation function for the LIE in question. The LIE is modelled as an electron density enhancement with a Gaussian pro®le in all coordinates. Results for a large elliptical LIE0200 600 km show that signi®cant Trimpis, 0ÿ0.4 dB in amplitude and 0+48 in phase are predicted, using modest maximum DNe values 0 1.5 el/cc. Such an electron density enhancement is well within the range that would be expected to result from experimentally observed ̄uxes of electron precipitation following wave particle interactions with whistler-mode waves. 7 2000 Elsevier Science Ltd. All rights reserved.
منابع مشابه
Gravitational waves from an early matter era
We investigate the generation of gravitational waves due to the gravitational instability of primordial density perturbations in an early matter-dominated era which could be detectable by experiments such as LIGO and LISA. We use relativistic perturbation theory to give analytic estimates of the tensor perturbations generated at second order by linear density perturbations. We find that large e...
متن کاملTesting B-ball Cosmology with the Cmb
In D-term inflation models, the fluctuations of squark fields in the flat directions give rise to isocurvature density fluctuations stored in the Affleck-Dine condensate. After the condensate breaks up in B-balls, these can be perturbations in the baryon number, or, in the case where the present neutralino density comes directly from B-ball decay, perturbations in the number of dark matter neut...
متن کاملAn ensemble of rapidly interconverting orientations in electrostatic protein-peptide complexes characterized by NMR spectroscopy.
Protein complex formation involves an encounter state in which the proteins are associated in a nonspecific manner and often stabilized by interactions between charged surface patches. Such patches are thought to bind in many different orientations with similar affinity. To obtain experimental evidence for the dynamics in encounter complexes, a model was created using the electron transfer prot...
متن کاملEnhancement of Non-Gaussianity after Inflation
We study the evolution of cosmological perturbations on large scales, up to second order, for a perfect fluid with generic equation of state. Taking advantage of super-horizon conservation laws, it is possible to follow the evolution of the non-Gaussianity of perturbations through the different stages after inflation. We find that a large non-linearity is generated by the gravitational dynamics...
متن کاملHF radar polar patch formation revisited: summer and winter variations in dayside plasma structuring
Three intervals of polar patch formation, as observed by the CUTLASS Finland HF coherent radar, are presented. Simultaneous observations from a vertical ionosonde located at Longyearbyen on Svalbard, situated in the dayside convection throat region, allow for F-region plasma structuring, leading to polar cap patch formation to be determined. Solar wind and interplanetary magnetic field (IMF) pr...
متن کامل