USING THE METHODS OF PHYSICAL THERAPY IN CHILDREN WITH THE VEGETOVASCULAR DYSTONIAS

The aim of rehabilitation may be: the restoration of the anatomical structure of the damaged tissues and organs, restoration of the dysfunctions, development of the compensatory possibilities, normalization of psycho-emotional disorders. Principles of medical rehabilitation in pediatrics: the use of modern achievements of the medical science and technology, systematic character, sequence and staging character of rehabilitation (hospital, sanatorium and dispensary- polyclinic stages), accountability of the influence of growth and development of organism on the dynamics of the pathologic processes, complexity of the methods (physio-, kinesi-, psycho-, diet, manual and pharmacotherapy, massage and others), combination of rehabilitation with teaching, the active participation of parents in rehabilitation, its completeness (reaching of the maximum result), use of the supporting therapy. Modern methods of rehabilitation of children with the vegetovascular dystonias: a)by the hypertensive type: - endonasal electrophoresis with a mixture of Ca -Mg (2% solution, 10 min, daily or in a day, Nq8-10); - electrophoresis with Mg (2% solution MgSO4, the currents of apparatuses Amplipulse on the collar zone, 10-15 min, in a day, N8-10); - general franklinization (10-15 min, in a day, N7-8); - electric sleep at the low frequencies (5-10-15 Hz, 30-40 min, in a day, N8-10); - oxygen baths (36-37°C, 10-15 min daily or in a day N8-10); - iodine-bromine baths (36-37°C, 10-15 min, daily or in a day, N8-10); - sea bathings in the not cold water (t° is above 21 -22°C); - baths with the sea water (36-37°C, 10-15 min, daily or in a day, N8-10); b)by the hypotensive type: - electric sleep (20-40 Hz, 30-40 min, daily or in a day, N8-10); - electrophoresis with Ca on the collar zone (8-15 min, daily or in a day, N8-10); - massage of the spine and collar zone (energetic); - carbonate or pearl baths (35-36°C, 5-10 min, daily or in a day, N8-10); - circular douche with water of indifferent or cool temperature (35-36°C, 5-6 min, daily or in a day); - sea bathings in the cool water (t° is higher than 18-20°C); - cool douches and rubdown (28-32°C, 5-10 min, daily or in a day, N8-10); - electrophoresis with 0.5% solution of Mezaton to the children of school age, employing the collar procedure (5-10 min, N 6-8 in the presence of the physiotherapist). Indications to the application of INFEMF (impulse low frequency electromagnetic field) 1. Vegetative dysfunctions of permanent course in initial vagotonia, sympathicotonia or eutonia, beginning from the age of 3. 2. Vegetative dysfunctions in combination with neurosis-like syndromes. 3. Vegetative dysfunctions against the background of somatic pathology, which is accompanied by the weakly expressed pain syndrome (diseases of loco-motor apparatus, gastrointestinal tract and others). 4. The most effective INFEMF is in the children of the younger age (7-11 years old) in reduction of protective- adaptive compensating mechanisms. The advantages of INFEMF in children and adolescents with VD (vegetative dysfunction) are: good tolerance of the procedures by all patients; simplicity and convenience in carrying out the procedure (distance influence); universality and possible range width of the influence; the possibility of integration and association with other methods of rehabilitation treatment and application for prevention. Contraindications to the application of INFEMF 1. Age up to 3 years. 2. Paroxysmal course of the vegetative dysfunctions with frequent vegetative crises, expressed orthostatic hypotension, syncope in anamnesis. 3. Vegetative dysfunctions in the period of exacerbation. 4. Vegetative dysfunctions against the background of the severe disturbance of the central nervous system of traumatic, infectious-allergic nature with presence of the convulsive of syndrome in anamnesis. 5. Exacerbation and acute course of the chronic disease, which requires adequate drug (or surgical) treatment. 6. Diseases of the eyes

Long term variability of the Broad Emission Line profiles in AGN

Results of a long-term monitoring ($\gtrsim 10$ years) of the broad line and continuum fluxes of three Active Galactic Nuclei (AGN), 3C 390.3, NGC 4151, and NGC 5548, are presented. We analyze the H$\alpha$ and H$\beta$ profile variations during the monitoring period and study different details (as bumps, absorption bands) which can indicate structural changes in the Broad Line Region (BLR). The BLR dimensions are estimated using the time lags between the continuum and the broad lines flux variations. We find that in the case of 3C 390.3 and NGC 5548 a disk geometry can explain both the broad line profiles and their flux variations, while the BLR of NGC 4151 seems more complex and is probably composed of two or three kinematically different regions.Comment: 10 pages, 9 figures, New Astronomy Reviews (Proceeding of 7th SCSLSA), in pres

The SCR flare of 16 February 1984 as recorded by the Sayan spectrograph

The Sayan cosmic ray (CR) spectrograph recorded an SCR flare that occurred on 16 February 1984. Data from both 1-hour and 110-minute duration measurements in 10 channels with different energy sensitivity (of neutron monitors HM-64 located at different depths in the atmosphere, and of a neutron, multiple neutron and rigid mumeson component lead-less detector) is presented. The parameters of the SCR variation spectrum are evaluated and it is shown that the recording of multiple neutrons at the same geographic point and at the same level in the atmosphere provides information similar to that from a spectrographic complex of instruments

On the methanol emission detection in the TW Hya disc: the role of grain surface chemistry and non-LTE excitation

The recent detection of gas-phase methanol (CH$_3$OH) lines in the disc of TW Hya by Walsh et al. provided the first observational constraints on the complex O-bearing organic content in protoplanetary discs. The emission has a ring-like morphology, with a peak at $\sim 30-50$ au and an inferred column density of $\sim 3-6\times10^{12}$ cm$^{-2}$. A low CH$_3$OH fractional abundance of $\sim 0.3-4\times 10^{-11}$ (with respect to H$_2$) is derived, depending on the assumed vertical location of the CH$_3$OH molecular layer. In this study, we use a thermo-chemical model of the TW Hya disc, coupled with the ALCHEMIC gas-grain chemical model, assuming laboratory-motivated, fast diffusivities of the surface molecules to interpret the CH$_3$OH detection. Based on this disc model, we performed radiative transfer calculations with the LIME code and simulations of the observations with the CASA simulator. We found that our model allows to reproduce the observations well. The CH$_3$OH emission in our model appears as a ring with radius of $\sim60$ au. Synthetic and observed line flux densities are equal within the rms noise level of observations. The synthetic CH$_3$OH spectra calculated assuming local thermodynamic equilibrium (LTE) can differ by up to a factor of 3.5 from the non-LTE spectra. For the strongest lines, the differences between LTE and non-LTE flux densities are very small and practically negligible. Variations in the diffusivity of the surface molecules can lead to variations of the CH$_3$OH abundance and, therefore, line flux densities by an order of magnitude.Comment: Accepted for publication in MNRAS, 8 pages, 8 figure

Получение пористых полимерных композитов

В данной работе мы экспериментально убедились в целесообразности использования метода прессования форм из композита с примесью NaCl с последующим удалением соли для получения пористой структуры композитов