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Страница 1, Результатов: 4

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22.3
S22

Sarsembayeva, A. T.
    Solar activity monitoring for the period march 20-25, 2019 [Текст] / A. T. Sarsembayeva, M. Odsuren [et al.] // News of the National Academy Ofsciences of the Republic of Kazakhstan. - 2020. - №4. - P. 35-41
ББК 22.3

Рубрики: Physics

Кл.слова (ненормированные):
solar flares -- x-rays -- reconnection rate
Аннотация: During a large solar flare, the flux of hard electromagnetic radiation from the sun increases many times.
Держатели документа:
WKU
Доп.точки доступа:
Odsuren, M.
Belisarova, F.B.
Sarsembay, A.T.
Abyshev, M.E.

Sarsembayeva, A.T. Solar activity monitoring for the period march 20-25, 2019 [Текст] / A. T. Sarsembayeva, M. Odsuren [et al.] // News of the National Academy Ofsciences of the Republic of Kazakhstan. - 2020. - №4.- P.35-41

1.

Sarsembayeva, A.T. Solar activity monitoring for the period march 20-25, 2019 [Текст] / A. T. Sarsembayeva, M. Odsuren [et al.] // News of the National Academy Ofsciences of the Republic of Kazakhstan. - 2020. - №4.- P.35-41


22.3
S22

Sarsembayeva, A. T.
    Solar activity monitoring for the period march 20-25, 2019 [Текст] / A. T. Sarsembayeva, M. Odsuren [et al.] // News of the National Academy Ofsciences of the Republic of Kazakhstan. - 2020. - №4. - P. 35-41
ББК 22.3

Рубрики: Physics

Кл.слова (ненормированные):
solar flares -- x-rays -- reconnection rate
Аннотация: During a large solar flare, the flux of hard electromagnetic radiation from the sun increases many times.
Держатели документа:
WKU
Доп.точки доступа:
Odsuren, M.
Belisarova, F.B.
Sarsembay, A.T.
Abyshev, M.E.

22.3
M73

Minasyants, G. S.
    Comparison of characteristics of photos fluxes various energies in the development of solar gamma flares [Текст] / G. S. Minasyants, T. M. Minasyants, V. M. Tomozov // News of the National Academy of sciences of the Republic of Kazakhstan. - 2020. - №3. - Р. 59-65
ББК 22.3

Рубрики: Physics

Кл.слова (ненормированные):
solar flares -- flare plasma emission -- coronal mas ejection -- x-ray and gamma ray
Аннотация: The characteristics of photons fluxes of various energies during the development of flares with hight-energy gamma rays are considered.
Держатели документа:
WKU
Доп.точки доступа:
Minasyants, T.M.
Tomozov, V.M.

Minasyants, G.S. Comparison of characteristics of photos fluxes various energies in the development of solar gamma flares [Текст] / G. S. Minasyants, T. M. Minasyants, V. M. Tomozov // News of the National Academy of sciences of the Republic of Kazakhstan. - 2020. - №3.- Р.59-65

2.

Minasyants, G.S. Comparison of characteristics of photos fluxes various energies in the development of solar gamma flares [Текст] / G. S. Minasyants, T. M. Minasyants, V. M. Tomozov // News of the National Academy of sciences of the Republic of Kazakhstan. - 2020. - №3.- Р.59-65


22.3
M73

Minasyants, G. S.
    Comparison of characteristics of photos fluxes various energies in the development of solar gamma flares [Текст] / G. S. Minasyants, T. M. Minasyants, V. M. Tomozov // News of the National Academy of sciences of the Republic of Kazakhstan. - 2020. - №3. - Р. 59-65
ББК 22.3

Рубрики: Physics

Кл.слова (ненормированные):
solar flares -- flare plasma emission -- coronal mas ejection -- x-ray and gamma ray
Аннотация: The characteristics of photons fluxes of various energies during the development of flares with hight-energy gamma rays are considered.
Держатели документа:
WKU
Доп.точки доступа:
Minasyants, T.M.
Tomozov, V.M.

22.3
S17

Salikhov, N. M.
    Ionospheric effects of solar flares and earthquake according to doppler frequency shift on an inclined radio path [Текст] / N. M. Salikhov, G. D. Pak // News of the National Academy of sciences of the Republic of Kazakhstan. - 2020. - №3. - Р. 108-117
ББК 22.3

Рубрики: Physics

Кл.слова (ненормированные):
doppler frequency shift -- ionosphere -- solar flares -- earthquake
Аннотация: The effects in ionosphere and the fine structure of ionospheric response to the action of X-ray and ultraviolet radiation of C1.7-M5.2 classes flares occurred during solar cycle 24 have been studied.
Держатели документа:
WKU
Доп.точки доступа:
Pak, G.D.

Salikhov, N.M. Ionospheric effects of solar flares and earthquake according to doppler frequency shift on an inclined radio path [Текст] / N. M. Salikhov, G. D. Pak // News of the National Academy of sciences of the Republic of Kazakhstan. - 2020. - №3.- Р.108-117

3.

Salikhov, N.M. Ionospheric effects of solar flares and earthquake according to doppler frequency shift on an inclined radio path [Текст] / N. M. Salikhov, G. D. Pak // News of the National Academy of sciences of the Republic of Kazakhstan. - 2020. - №3.- Р.108-117


22.3
S17

Salikhov, N. M.
    Ionospheric effects of solar flares and earthquake according to doppler frequency shift on an inclined radio path [Текст] / N. M. Salikhov, G. D. Pak // News of the National Academy of sciences of the Republic of Kazakhstan. - 2020. - №3. - Р. 108-117
ББК 22.3

Рубрики: Physics

Кл.слова (ненормированные):
doppler frequency shift -- ionosphere -- solar flares -- earthquake
Аннотация: The effects in ionosphere and the fine structure of ionospheric response to the action of X-ray and ultraviolet radiation of C1.7-M5.2 classes flares occurred during solar cycle 24 have been studied.
Держатели документа:
WKU
Доп.точки доступа:
Pak, G.D.

22.3
S22

Sarsembayeva, A.
    Definition of the reconnection Rate of most powerful solar flares. [Текст] / A. Sarsembayeva, F. Belisanova, M. Odsuren, A. Sarsembay [и др.] // News of national academy of sciences of the republic of Kazakhstan. 2020. - №6. - P. 61-67
ББК 22.3

Рубрики: physics

Кл.слова (ненормированные):
solar flares -- X-rays -- reconnection rate
Аннотация: We made a brieft analysis of solar flares registered in there days, also has shown the duration of time and peak of solar flares in Universal time.
Держатели документа:
WKU
Доп.точки доступа:
Belisanova, F.
Odsuren, M.
Sarsembay, A.
Tutebayeva, A.
Orazymbet, A.
Abyshev, M.

Sarsembayeva, A. Definition of the reconnection Rate of most powerful solar flares. [Текст] / A. Sarsembayeva, F. Belisanova, M. Odsuren, A. Sarsembay [и др.] // News of national academy of sciences of the republic of Kazakhstan. 2020. - №6.- P.61-67

4.

Sarsembayeva, A. Definition of the reconnection Rate of most powerful solar flares. [Текст] / A. Sarsembayeva, F. Belisanova, M. Odsuren, A. Sarsembay [и др.] // News of national academy of sciences of the republic of Kazakhstan. 2020. - №6.- P.61-67


22.3
S22

Sarsembayeva, A.
    Definition of the reconnection Rate of most powerful solar flares. [Текст] / A. Sarsembayeva, F. Belisanova, M. Odsuren, A. Sarsembay [и др.] // News of national academy of sciences of the republic of Kazakhstan. 2020. - №6. - P. 61-67
ББК 22.3

Рубрики: physics

Кл.слова (ненормированные):
solar flares -- X-rays -- reconnection rate
Аннотация: We made a brieft analysis of solar flares registered in there days, also has shown the duration of time and peak of solar flares in Universal time.
Держатели документа:
WKU
Доп.точки доступа:
Belisanova, F.
Odsuren, M.
Sarsembay, A.
Tutebayeva, A.
Orazymbet, A.
Abyshev, M.

Страница 1, Результатов: 4

 

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