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takes place when velocity vectors and the vectors of induction of magneticfield are parallel before interaction with the magnetosphere, can be preservedin stagnation zone of magnetosphere even if plasma has finite magnetic andregular viscosity.4. In stagnation zone of magnetosphere, as in the ideal conductive as well in theapproximation of mechanical and magnetic viscous compressible plasma, thegeneration of magnetohydrodynamic waves with the frequency spectrumequal to the cyclotron frequency spectrum of protons in magnetopause ispossible. It turned out, that besides the equatorial magnetopause, generation ofvery low frequency Rossby like magnetogradient waves is possible also in thefocal area of magnetosheath (stagnation zone); in the approximation ofstagnation zone model for the different models of linear and nonlineardistribution of magnetic field, the frequency spectrum of Rossby like waves,which completly covers the frequency range of regular geomagnetic (Pc1-Pc6)pulsations is derived.8
შინაარსიSesavali --------------------------------------------------------------------------------------------11Tavi I. magnituri hidrodinamikis gantolebebi-------------------------141.1. mhd msgavsebis ganuzomeli parametrebi--------------------------------------141.2. dedamiwis magnituri sasazRvro fena (magnitopauza)---------------231.3. Svecis mimdevrobiTi miaxloebis meTodi-----------------------------------37Tavi II. dedamiwis magnituri sasazrvro fenis modelirebaplazmis eleqtruli gamtareblobis impulsuri cvlilebisgaTvaliswinebiT-------------------------------------------------------------------------------462.1. mzis qaris Mplazmis eleqtruli gamtareblobis buneba---------462.2. dedamiwis meridionaluri magnituri sasazRvro fenismodelireba mzis qaris eleqtruli gamtareblobis impulsuricvlilebisas---------------------------------------------------------------------------------------61Tavi III. magnitosferos mdgari zonis magnituri struqturatopologiuri formalizmis CarCoebSi damagnitogradientuli talRebibi------------------------------------------------------793.1. saplanetaTaSoriso magnituri velisa da geomagnituri velisZalwirebis gadaerTebis movlena algebruli mrudebistopologiuri formalizmis CarCoebSi ------------------------------------------793.2. mdgari zonis magnituri zedapiris topologia-----------------------903.3. plazmis siCqareTa velisa da magnituri velis topologiurimsgavsebis modeli magnitosferos winamdebare mdgar zonaSi-----1013.4. mdgari zona magnitosferos gardamaval areSi, helmholcisgantolebebis Tvisobrivi analizi da magnitogradientulitalRebis parametrebis Sefaseba-----------------------------------------------------110daskvna---------------------------------------------------------------------------------------------125gamoyenebuli literature ----------------------------------------------------------1279
Page 1 and 2: marine CxituniZemagnituri velis top
Page 3 and 4: საქართველოს
Page 5 and 6: miRebuli mzis qaris plazmis anomalu
Page 7: the identification of the top of st
Page 11 and 12: შესავალიkosmosuri e
Page 13 and 14: talRebis maxasiaTeblebi, rogorc ide
Page 15 and 16: lebis denis gaTvaliswinebis gareSe,
Page 17 and 18: om uwyveti eleqtrogamtari garemo, m
Page 19 and 20: orive mxare unda gavyoTρCV-ze da S
Page 21 and 22: σBρE0 02V0l020B µ 0σlE0σlV0B0B
Page 23 and 24: prandlis ricxvi damokidebulia garem
Page 25 and 26: magnituri velisa da dinebis fizikur
Page 27 and 28: magnitosferos zedapirs saSualod ece
Page 29 and 30: velis urTierTqmedeba mzis qarSi Cay
Page 31 and 32: agreTve magnituri velis Zalwirebis
Page 33 and 34: iseTi modeli, romelic Sesaferisi iq
Page 35 and 36: magnitosferosTan SedarebiT, xolo ne
Page 37 and 38: 1.3 Svecis mimdevrobiTi miaxloebis
Page 39 and 40: saWiroa aRiniSnos, rom nebismieri r
Page 41 and 42: mniSvnelovania mxolod fundamentalur
Page 43 and 44: mudmivia. meore SemTxvevaSi sasazRv
Page 45 and 46: ⎛ξ ξdξ⎞δ oH ϕ hozexp a h x
Page 47 and 48: RrubelSi induqciis efeqti SeiZleba
Page 49 and 50: Ed−19nlnΛ= 3,02 ⋅10CGSE, (2.1.
Page 51 and 52: ionur-ciklotronuli aramdgradobis ga
Page 53 and 54: temperaturebis fardobaze. cnobilia,
Page 55 and 56: Seicvalos, rac, cxadia, imoqmedebs
Page 57 and 58: msjelobis safuZvelze mivida daskvna
Page 59 and 60:
wverodan fuZisaken. Aamrigad, magni
Page 61 and 62:
2.2. dedamiwis meridionaluri magnit
Page 63 and 64:
kosmosuri plazmuri garemosaTvis, ma
Page 65 and 66:
komponenta, romelic plazmis dinebis
Page 67 and 68:
1) modelisaTvis (2.2.6) gantoleba m
Page 69 and 70:
⎛ ∂H⎜⎝ ∂xy⎞⎟⎠x=δ1
Page 71 and 72:
( δ )2⎡⎛ 22cE⎞z δ ′ x 1
Page 73 and 74:
turad aramdgradia mcire SeSfoTebebi
Page 75 and 76:
t → ∞ , 2) modeli iZleva δ →
Page 77 and 78:
modelisa da magnituri siblantis dro
Page 79 and 80:
Tavi III. magnitosferos mdgari zoni
Page 81 and 82:
anu, Tu mzis qaris winaRoba yovelTv
Page 83 and 84:
oqsimirebeli elifsoidis mcire naxev
Page 85 and 86:
velis sasazRvro centralur Zalwirs g
Page 87 and 88:
gaxsna magnitosferos energomomarage
Page 89 and 90:
adganac aq gadaerTebis movlenas mxo
Page 91 and 92:
3.2 mdgari zonis magnituri zedapiri
Page 93 and 94:
ganawileba myardeba mas Semdeg, roc
Page 95 and 96:
CarCoebSi, maTematikurad koreqtulia
Page 97 and 98:
azimutalur simetrias, SeiZleba brty
Page 99 and 100:
CavTvaloT mdgari zonis maaproqsimir
Page 101 and 102:
3.3. plazmis siCqaris velisa da mag
Page 103 and 104:
SeSfoTebas mdgari zonis RerZis mima
Page 105 and 106:
2∂ h= V2∂t2ar2∂ h,∂2zr2∂
Page 107 and 108:
SeiZleba gamowveuli iyos agreTve md
Page 109 and 110:
∂2by2∂t= V2a∂2by2∂z(3.3.28)
Page 111 and 112:
moZraoba erTmaneTisagan damoukidebe
Page 113 and 114:
mzis qaris Termodinamikuri parametr
Page 115 and 116:
zustad, misi cvlilebis diapasons, i
Page 117 and 118:
sferosTan urTierTqmedebamde mzis qa
Page 119 and 120:
cvlilebis Semdeg intervals:45V ≈
Page 121 and 122:
SevafasoT magnitogradientuli talReb
Page 123 and 124:
y / δ =0.916C ( )+ ≈ 1,2 ⋅10sm
Page 125 and 126:
daskvna1. mzis qaris eleqtruli gamt
Page 127 and 128:
gamoyenebuli literatura1. Тамм
Page 129 and 130:
магнитогидродинам
Page 131 and 132:
48. Ванишвили Г., Габ
Page 133 and 134:
72. Теория турбулент
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