SCIENTIFIC ABSTRACT LIKHACHEV, A. I. - LIKHACHEV, I.

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CIA-RDP86-00513R000929910013-7
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December 31, 1967
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SCIENTIFIC ABSTRACT
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LIKHAGHEV, A.I. Ionization of the P2 layer as dependent on the penetration of solar energy into the atmosphere. Goomag. i aer. 2 no.3:1+81-488 My-Je 162, (MIRA 15:1-1) 1. Sibirakiy fiziko-tekhnicheekiy institut pri Tcmskom gosudarstvennom universitete. (Ionosphere) ACCESSION Nit: AT013055 AUTHOR: Likhachev, A. Card 1/3 S/3658/62/000/041/0044/0048 TITLE: The phenomenon of the limited Increise In Ionization In the F2 layer SOURCE: Tomsk. Universitet. -Sibirs'kly flzl'kotakhnlcheskly .Insti'tut. Trudy*, no. 41, 1962., Rezulltaty* obrabotki,materialov po Issledo.vanlyu lonosfery* I m;gnitnogo polya Zemli za period MGG.I MGS, 41-48 TOPIC TAGS: Ionosphere, F2 layer, atmospheHc ioni'zation, loniz@tlon growth limi- tation, atmospheric ionization solar activity dependence, recombination coefficient 1, - . i# ABSTRACT: On the basis of data obtained at.,the Tomsk Ionospheric station, the author considers the limitation of the growth In electron density In the F2 layer during years of h;gh solar activity' For th'is purpose, a study was made of the material obtained at 40 of the worl@ls ionospheric stations during 1958 in order to consider the phenomenon of the latitudinal Nmitation of the Ionization increment In the F-region. An attempt Is made to explain this phenomenon on the basis of a temperature hypothesis Involving a large-scale intrusion of solar radiation into the Earth's atmosphere and a resultSnt change In the physical state of the at- mosphere in the F2 layer. The equation for the Ionization of a simple layer: ACCESSION NR: AT4013055 dNe., - . i - dt presupposes that the Ionization balance Is the result of the equi libration of only two processes: Ionization and recombination. However, In real ionospheric condi- tions (and particularly at the level of the F2 layer), the severe temperature change that may. take place wil I Inevitably lead to a change In the value of the effective coefficient of recombination and also to a change In the value of Ne- On the other hand, the value of the temperature Is, In all likelihood, related to the influx of solar radiation into the terrestrial atmosphere and an increase in temperature. should be accompanied by an increase in Ion-formation, and vice versa. Under conditions of equilibrium In the processes of increasing electron density due to rising solar radiation and falling electron density due to rising tempera- ture, with an Increased influx Into the Earth's atmosphere of solar radiation, the result can be a condition of "heat balance", or the phenomenon of ionization growth limitation, despite an Increase In the Intensity of Ionizing radiation. This "temperature balance" can apparently provide an explanation for the disrup- tion In the linearity of the behavior of experimentally obtained critical fre- quency values for the F2 layer and their constancy (invariability) during years of heightened solar activity. In conclusion, the author advances the following hypothetical mechanism to explain this phenomenon: the process of Ionization is Card 2/3 ACCESSION NR: AT4oI3055 related to the phenomenon of recombination. With Increasing solar activity the electron density rises, but thereAs a concomitant Increase In the t'emperature and decrease in the value of the effective recombination factor; as a result, re- combination will occur more slowly and the vAlue of the critical frequencies dur- ing the morning hours will be considerably higher; that Is, the minimum critical frequencies will rise. Orig. art. has: 3 figures and I formula. ASSOCIATION: SIBIRSKIY FIZIKO-TEKHNICHESKIY INSTITUT, T014SKIYGOSUDARSTVENNY*Y UNIVERSITET IM. V. V. KUYBY*SHEVA (Siberian physico-technical institute, Tomsk State University) SUBMITTED: 00 DATE ACQ: 27Feb64 ENCL: 00 SUB CODE: AS NO REF SOV: 005 OTHER: 001 Card 3/3 ACCESSION NR: AT4o]3053 S/3058/62/000/041/0062/0067 AUTHOR: TITLE: Anomalous yearly behavior of the F2 layer as a function of the Influx of solar radiation into the Earth's atmosphere SOURCE: Tomsk. Universitet. Sibirskiy fizikotekhnicheskiy institut. Trudy*, no. 41, 1962. Rezulltaty* obrabotki materialov po issledovaniyu ionosfery* I magnitnogo polya Zemll za period MGG I MGS, 62-67 TOPIC TAGS: ionosphere, F2 layer, atmospheric ionization, solar radiation, at- mospheric ionization solar activity dependence, F2 layer anomalous behavior, critical frequency variation ABSTRACT: The magnitude of the yearly anomaly of F2 layer Ionization is defined by the author as the difference between the variation in the ionization of the layer according to the law of a-simple layer and the actually measured values of the critical frequencies. The author demonstratesthat thils',yearly anomaly shows a high degree of correlation with the magnitude of the solar radiation Influx in- to the Earth's atmosphere. He also shows that the yearly anomaly depends on the cyclic a.ctivity of the Sun. A method is proposed for forecasting the median rSon d critical freqtfency values. The so-called yearly anomaly consists of the Cjn _71 ACCESSION NR: AT4013053 fact that the noon-time values of the critical frequencies are lower in the summer than in.the winter. According to the theory of the formation of a simple ionized layer, the Ionization change during the year should obey the formula: 4, Q.) f us B -os Z cr V noon where zn?gn is the zenith angle of the Sun at noon. While this equation accurate- ly descr es the annual variation of the critical frequencies of the E and FI layers, it Is wholly Inadequate to explain the changes that occur in the F2 layer. in order to determine the effect of the influx of solar radiation Into the at- mosphere on the value of F2 layer Ionization, the author postulates that during the winter months at mean latitudes the temperature effect of the solar radiation is small. He further assumes that the observed values of the critical frequencies In December at noon differ only slightly from those of a simple layer. Knowing the December noon-time critical frequency value, a calculation is made, for the latitude of Tomsk, for the noon-time critical frequencies for the other months, according to the formula for the variation of a simple layer. On the basis of this methodological approach, the author concludes that, In the first place,'the yearly FZ layer anomaly in noon-time values of critical frequencies Is caused by Cord 2/3 ACCESSION' NR: AT4ci53r@-- the photon radiation of the Sun; in the second place, this anomaly is a tempera- ture-connected anomaly, since the photon radiation energy must, In the final analysis, become heat energy; In the third place, the temperature in the F2 layer has, at the end of summer, a higher value, which may be caused either by the duration of the formative processes or by other factors. Orig. art. has; 3 figures and 2 formulas. ASSOCIATION; Slbirrakiy fiziko-tekhnicheskiy institut., Tawkiy d6suAwstvenny*y tmiversitet im. V. V. M.&yx9heva ($iberian Pbysiaotecb-' cal Z=titute,, Tcmsk' State University) SUBMITTED: '00 DATE ACQ: 27Feb64 ENCL: 00 SUB CODE: AS NO REF SOV: 001 OTHER: 000 Card 3/3 ACCESSION NR: AT4013059 S/3058/62/000/041/0068/0071 AUTHOR: L TITLE: The relationship between the daytime Ionization increment of the F2 layer and the influx of solar radiation Into the atmosphere SOURCE: Tomsk. Universitet. Sibirskly fizikotekhnicheskly institut. Trudy*, no. 41, 1962. Rezulltaty*obrabotki materialov po issledovaniyu lonosfery*i magnitnogo polya Zemli za period MGG I MGS, 68-71 .1 TOPIC TAGS: ionosphere, atmospheric ionization, F2 layer, solar radiation, atmospheric ionization solar activity dependence, daytime ionization increment, ionization increment latitude dependence ABSTRACT: The author discusses the latitude-yearly distribution of the diurnal increment of ionization in the F2 layer. A comparison is made between the influx of diurnal-solar radiation into the atmosphere of the Earth and the distribution of the diurnal radiation increment in the F2 layer. it is indicated that the lati- tudinal anomaly in increment distribution during the summer solstice is the re- sult of the high influx Of solar radiation into the atmosphere. The author also concludes that, during solstice- days, the increment distribution Is not proportion- al to the longitudinal distribution of the Influx of solar radiation; the smaller Card 1/2 ACCESSION NR: AT4013059 the influx of radiation, the larger the increment. On equinoctial days, the varla- tion of the increment with latitude agrees with the path of the longitudinal dis- tribution of the influx of radiation. It was also found that, in solstice periods, the latitudinal distribution of the Increment is sharply influenced by a limitation phenomenon which occurs in the event of large-scale intrusion of solar radiation into the atmosphere; since this is the case, eqqations describing the ionization state of the F2 layer should take into consideration, in addition to ionization attenuation due to temperature change, this limitation phenomenon as well. In the solution of the problem of the relationship between atmospheric ionization and the sun, a direct link between the Ionization state of the F2 layer and the zenith angle is not possible unless temperature change and related phenomena are consid- ered. Orig. art. has: 3 figures. ASSOCIATION: Sibirskiy fiziko-tekhnJ alciy iustitut, Tonskiy gosudarstvenny*y tmiverzitet im. V. V. Kuyby*shava (Sibc:@ian Physicoteabidcal Institute, Tcask @_itate University) SUBMITTED: 00 DATE ACQ: 27Feb64 ENCL: 00 ,SUB CODE: AS NO REF SOV: 001 OTHERt 000 Card 2/2 74 _LlJZM(; GW -66 _gLiff @ SOURCE CODE: UR/626-976@/-doo/oon,, 5 5 44C NR: AR5023007 AUTHOR: Likhachev A. :1 TITLE: of the gain in daily Ionization On thYgx-f rj Sal-Oar energy into the atmosphere of the earth SOURCE: Ref. zh. Astronomiya., Abu, 8,51-473 REP SOURCE: Tr. Sibirsk. fiz,-tekhn. in-ta pri Tomskom un-te@ vyp .. `, 45, 1964,-108-112- $ -TOPIC- TAGSt astronomic data, solar radiation 'effect Sckc@.r crle- ABSILRACT: Data obtained from studies of the dependence.off A ff2pp on the entry 'of solar wave radiat'ion into the atmosvherel7of thd ear- is given. The character of the mechanism of*this dependence is clar fied, as well as the types of deviations, according to data obtained fr m observations of the Tomsk station during the solar cycles and from a 3eries of other stations in the northern hemisphere during the IGY. General observations are expressed on possible causes of discrepancies in the regular relationship, Author's resume SUB CODE: 03/ SUBM DATEt none Card 1/1 ____EWT(I)ZfVCAWA:(h) ACC NRB An5ol6451 SOURCE CODE: UR/ol69/65/OOO/OO6/AO34/A034 AUTHOR: Likhachev, Ael.; Gordeyev, O.K. ORG: none v/ TIM Interrelation between the @onospherl parameters of the F2 stratum and the quite-sun variations in Tomsk the magnetic field SOURCE: Ref. zh. Geofizika, Abs. 6A192 SOURICE: Tr. Sibirsk. fiz,telchn. in-ta pri Tomskom un-te, vyp- 45, 19-44, 3-3-92 TOMC TAGS: ionosphere, Geomagnetic field, solar energy TRABSIATION: On the basis -of an established relationship between ionosj@heric param- eters and variations in elements of a geomagnetic field under the effect of solar energy entering the atmosyhere, regression equations are given for the interrelation- ship between ionospheric parameters and Sq variations in a magnetic field. It is shown that the regression equations define the relationship between the observed values of ionospheric parameters and the Sq variations. SUB. CODE: 03 04-1 O'S. UDC: 550-388.2 Card iLl 1 17794-66 Ew(l p cj.E w h GT ACCESSION NR: AIR5023008 SOUEM CO-Dg-t--'UR/(2(0/65/(=/CW/0055/0056 AUTHOR: Likhachey, ORG: none TITLE i Functional dependence of the yearLy course of midday critical frequencies of the F2 ]aYer on the zenith angle of the nun, SOURCE: Ref zh.Astronomiya, Abs. 8.51-474 REP SOURCE:' Tr. Sibirsk. fiz.-tekhn. ia-ta Pri Toms k et vyp 64 ool un-t 45, 19 138-143, TOPIC TAGS: astronomic date, solar activity, solar energy, F layer, sun TRANSIATION: Based on the dependence of the entry of solar energy into the atmosphere of the earth on the zenith angle of the sun, an empirical formula was deduced for determining the midday critical frequencies of the F2 layer.as a func-! tiot of the zenith angle of the sun. SUB CODE: 03 -C 3L L 43719-6 V1 6, E T(l)IFCC GW ACC NR, AT6023733 SOURCE CODE: AUTHOR: LlUkdhachev A. 1.1, "Ke@arl@yev, Yu. N.; Yegorova, G. V.; Tiznchenko, N. 1. ........... ........... ORG: none TITLE: Dependence of sphert@@ n of solar radiation into the _jqk p rameters on the admissio earth'B atmosphere SOURCE: AN SSSR. Mezhduvedomstvennyy geofizichesldy komitet. V razdel programmy A,IGG: Ionosfera. Sbornik statey, no. 14, 1965. lonosfernyye Issledovanlya, 129-140 TOPIC TAGS: F layer, solar radiation effect, atmospheric Ionization ABSTRACT: This article presentd data from a study of the relations between Ionization para- meters of the F2 layer and the zenith angle of the Bun and the influx of solar energy into the earth's atmosphere. An Investigation of the time variations of the diurnal increment of toniza.-i tion, which represents the difference between critical frequencies at the maximum (midday hours) and minimum of the dimmal variation, showed that the maximal value of the increment of Ionization fig reached during the winter and the minimal value during the summer, and that 1 during the year the change In the increment correlates well with the change of the sine of the zenith angle of the Bun; the maximal values of the diurnal increment observed during the wintei L