Diurnal variations in the D-region during a storm after-effect

Measurements of electron concentration in the D- and lower E-regions of the ionosphere are reported for seven rocket flights from South Uist, Scotland, in April 1973. They took place during a 12-hour period starting 30 hours after the main phase of a severe geomagnetic storm. The principal feature of the results is that the electron concentrations below 85 km varied between 4 and 10 times the concentrations found on normal days. The variability was correlated with changes in radio wave absorption.The observed electron concentrations are compared with results of other workers for storm conditions and in particular with the model of Spjeldvik and Thorne (1975), and are found to be in reasonable agreement.The possibility of changes in positive ion composition occurring during the post-storm period is inferred.     

The impact of gravity waves on nitric oxide in the lower thermosphere

Observations of nitric oxide (NO) by the Solar Mesosphere Explorer (SME) during equinox indicate a lower-thermosphere equatorial minimum which is at variance with theoretical predictions. To address this discrepancy a zonally averaged model of the thermosphere and upper mesosphere is used to evaluate the influence of a latitude variation in turbulence. Five numerical simulations were performed with different latitude structures of eddy diffusion (K_T), ranging from uniform in latitude, peaks at low, mid-, or high-latitude, to a hemispherically asymmetric distribution. A local increase in eddy diffusion causes the lower thermosphere to cool and induces a latitude pressure gradient that drives horizontal and vertical winds. The circulation, turbulent transport and temperature dependent chemistry act to change the distribution of species. Comparison of the model predictions of NO with SME data, and simulated wind and temperature structure with empirical climatology, indicates a preference for a midlatitude peak in K_T.     

Vertical penetration of planetary waves into the lower ionosphere

Earlier work which provided evidence for coupling between pressure variations in the stratosphere and lower ionosphere in winter has been extended. Day-to-day changes in the height of fixed electron density isopleths in the E-region at a middle latitude often exhibit quasi-oscillations with amplitudes between 2 and 10km and periods between 5 and 30 days. It is found that the correlation between these oscillations and corresponding variations in the height of winter isobaric surfaces in the stratosphere, resulting from the presence of planetary-scale waves, is sometimes good and sometimes poor. Examination of the type of wave disturbance in the stratosphere and of the stratospheric zonal wind profiles suggests that the conditions for stratosphere-ionosphere coupling are met only when well-defined planetary waves of increasing amplitude with height are seen in the lower stratosphere and when the stratospheric zonal wind pattern is favourable to the vertical propagation of such waves.     

Large-amplitude standing planetary waves induced in the troposphere by the Sun

Investigations have been made of the global morphologies of two different Sun-weather relationships: the effect of the 27.5-day solar rotations and the effect of the 11-year sunspot cycles on tropospheric pressure. In both cases solar-induced perturbations occur in the form of large-amplitude standing planetary waves (or some combination of waves) of the (0, n), (1, n) and (2, n) types. Certain spatial features of Sun-weather relationships which have hitherto appeared puzzling are merely manifestations of these planetary waves.The range of the solar-induced 27.5-day oscillations of the height of the 500-mbar level reaches 14 Dm (decametres) in certain parts of the World. Such oscillations are of considerable practical importance; for example, the average pressure gradient responsible for driving the westerlies at upper-middle latitudes in winter varies by as much as a factor of two during the solar rotations. It appears that other short-term changes of solar radiation may also evoke a response in the lower atmosphere; the implications for theoretical studies of tropospheric dynamics are considerable.     

Winter-time disturbances in the mid-latitude D-region

Radio-wave absorption data from sixteen mid-latitude stations distributed in longitude, together with magnetic-field disturbance parameters and satellite measurements of thermal radiances, have been examined for the winter of 1976–1977. It has been demonstrated that D-region disturbances at mid-latitudes in winter can be associated with both the delayed effects of geomagnetic storms and with changes in mesospheric temperature.     

Lunar and planetary influences upon the peak electron density of the ionosphere

Observable effects of semidiurnal tidal character caused by the Sun (radiation and gravity) and Moon (gravity only) seem to be influenced by the planet Jupiter and, during approach, by Venus. These effects can be identified during summer for suitably selected planetary configurations. The importance of the lunar effect is found to depend on the solar hour, season and planetary constellation.     

Modelling of the electron density profile in the lowest part of ionosphere D-region on the basis of radiowave absorption data: 2. Seasonal variations

A new model of the lowest part of the D-region is obtained by a trial-and-error inversion method. Its basic feature is a step-like transition between 55 and 70 km which is not depicted in most ionospheric models. The seasonal differences of this are considered to be quite important: the bottom of the ionsphere is found to be lower in summer and spring, the gradient of the profile below the CR-layer is stronger in winter, and a well defined ‘valley’ exists around 70 km in spring. By simulating the ionospheric response to a, solar flare (SID-effect) in summer and in winter, an attempt was made to verify the obtained seasonal peculiarities of the quiet ionosphere.     

Temporal variations of ionospheric waves in the D- and F-regions

It is shown that mesoscale ionospheric wave disturbances in the D- and F-regions regularly occur at all times of day, night and season (characteristic periods ~100, 24, 12.6 min) and are a characteristic property of dynamic processes in the ionosphere.     

Simulation of the global structure of stationary planetary waves in the mesosphere and lower thermosphere

When simulating the global structure of stationary planetary waves (SPW) the problem of obtaining the numerical solution in the equatorial region appears. It results from the presence of apparent singularities in the operator of the SPW latitudinal structure when the Coriolis parameter is small. The new method based on SPW latitudinal operator inversion is proposed. This method permits the difficulties arising from the simulation of stationary large scale disturbances at low latitudes to be avoided. The global structure of SPW with zonal wave number m = 1 at the mesosphere and lower thermosphere heights has been calculated for the background zonal wind distribution representing a climatic picture of the solstice conditions. In the region of the mean zonal westerlies the SPW penetration across the equator is obtained. The SPW at low latitudes are shown to appear most significantly in the zonal component of the wind velocity. The influence of planetary wave motions on the distribution of longlived species in the ionospheric D-region and at the heights of lower thermosphere are discussed.     

On the linear electron loss process in the D-region

Chakrabarty's mechanism for the linear electron loss process in the middle D-region is shown to be incorrect. Possibilities of explaining the linear electron loss process are briefly discussed.     

Rocket measurements of nitric oxide in the equatorial region

Measurements of nitric oxide (NO) concentrations were carried out from Thumba, India, using rocket-borne radiometers. The technique of measurement is based on the detection of day-glow emissions of the NO gamma (1,0) band. The results obtained are presented in this paper. The peak NO concentration shows a very good correlation with integrated value of the solar X-ray flux in the 0.1–0.8 nm band, thereby indicating the influence of the X-ray flux on the NO concentration. The observed variability of NO is thought to be mainly due to solar activity and partly due to different X-ray flux values on the days of the flights. Theoretical model calculations for rocket flight conditions were found to be in fairly good agreement with the observed profiles. The differences below 90 km altitude in the NO profiles are thought to be due to eddy turbulence. This model is also used to study changes in the NO concentration with solar activity and latitude.     

EISCAT incoherent scatter radar observations and model studies of day to twilight variations in the D-region during the PCA event of August 1989

An intense solar proton event causing enhanced ionization in the ionospheric D-region occurred on 12 August 1989. The event was partially observed during three successive nights by the EISCAT UHF incoherent scatter radar at Ramfjordmoen near Tromsa, Norway. Ion production rates calculated from GOES-7 satellite measurements of proton flux and a detailed ion chemistry model of the D-region are used together with the radar data to deduce electron concentration, negative ion to electron concentration ratio, mean ion mass and neutral temperature in the height region from 70 to 90 km, at selected times which correspond to the maximum and minimum solar elevations occurring during the radar observations. The quantitative interpretation of EISCAT data as physical parameters is discussed. The obtained temperature values are compared with nearly simultaneous temperature measurements at Andøya based on lidar technique.     

Recent advances in the study of the D-region winter anomaly

D-region work as concerns the winter anomaly of electron density is screened for the period 1974–78. The following topics are dealt with: electron density distribution; ion production processes; neutral atmosphere effects by trace constituents, temperature and transports; ion composition and chemistry; coupling between atmospheric/ionospheric layers. A summary is given which might be read first, and which leads to some aspects of future work.     

Eiscat observations of the ionospheric D-region during auroral radio absorption events

Electron densities in the D-region have been observed with EISCAT during energetic electron precipitation events. Sample results are presented which demonstrate the value of the technique in studying variations of electron density with fine temporal and spatial resolution. Different types of absorption event can be characterized in terms of the changes in the incoming electron spectrum inferred from profiles of electron density. We contrast the D-region behaviour of night- and day-time events in terms of precipitating spectrum and absorption profile. A softening of the electron spectrum during the course of a morning event is clearly seen.     

Model studies of the D-region negative-ion composition during day-time and night-time

A model for the negative-ion composition of the D-region is constructed, based on gas-phase reactions and photodissociation and photodetachment processes. The height distributions of negative-ion species, electrons and total positive ions for day-time and night-time are examined using time-dependent solutions of their continuity equations which incorporate simultaneous solutions for the minor neutral constituents involved. A distinction is drawn between the two isomers of NO₃⁻ and particular attention is paid to the influence of possible chemical and photodestruction of the more stable form of this ion.     

An observational study of the D-region winter anomaly and sudden stratospheric warmings

An observational study of the link between the winter anomaly in ionospheric absorption and sudden stratospheric warmings for the 1967/1968 winter has been made. On the basis of the daily large-scale distributions of the absorption index, f_min, it is found that the winter anomaly during sudden warming could result from a NO increase induced by southward transport from the polar region, where NO is most abundant associated with a well-developed vortex in the D-region (large amplitude planetary wave).     

Incoherent scatter spectral measurements of the summertime high-latitude D-region with the EISCAT UHF radar

Measurements of incoherent scatter spectra from the auroral D-region were obtained during the summer of 1985 using a sophisticated pulse-to-pulse correlation technique with the EISCAT UHF radar. The spectral width variations with altitude are interpreted in terms of ion-neutral collision frequency, neutral temperature, mean positive ion mass and negative ion number density. Close agreement with predictions of currently available atmospheric models is obtained, except for a narrow layer around 86 km altitude. This layer showed evidence of increased positive ion mass for most of the experiment, and for short intervals indicated a mean ion mass close to 200 a.m.u. It is suggested that the layer is composed of proton hydrates in the vicinity of a structured noctilucent cloud, and that the index of hydration is occasionally large.     

An attempt to identify the obscured paths of water cluster ions build-up in the D-region

Existing ion-chemical scheme has been applied to reproduce the positive ion composition measured on 30 June 1973 by a rocket-borne mass spectrometer flown from Wallops Island. It is found that reactions analogous to the conversion of NO⁺ to NO⁺·H₂O are able to reproduce the observed densities of NO⁺·(H₂O)₂ and NO⁺·(H₂O)₃. The theoretical values of O₂⁺ and O₂⁺·H₂O are found to be about an order of magnitude higher and lower respectively than those measured. The direct hydration rates of H⁺·(H₂O)_n ions given by Good et al (1970) yield much less hydrates for n > 2. To properly reproduce the observed positive ions we need the following:

• 1.(a) a reaction which will convert O₂⁺ to O₂⁺·H₂O in the form
  O with U1 = 10⁻³¹[M]²(300/T)^4.4s⁻¹ and U2 = 10⁻⁹[H₂O]s⁻¹; and
• 2.(b) formation of hydrated protons via intermediate ions in the form
  with S=10⁻⁹[H₂0]s⁻¹, F = 8 × 10⁻³²[M]²(300/T)^4.4s⁻¹ and B increasing from 10⁻³ to 10²S⁻¹ as n increases from 2 to 6.