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Mualliflar

Š. Piskoř

Soʻnggi maʼlum muassasa:
Czech Academy of Sciences, Nuclear Physics Institute
2
h-indeks
0
i10-indeksi
9
Iqtiboslar
8
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
01013451978198319881990199820062010201120151978: Nashrlar 1, Iqtiboslar 01983: Nashrlar 1, Iqtiboslar 11988: Nashrlar 1, Iqtiboslar 21990: Nashrlar 1, Iqtiboslar 31998: Nashrlar 1, Iqtiboslar 02006: Nashrlar 1, Iqtiboslar 12010: Nashrlar 1, Iqtiboslar 02011: Nashrlar 0, Iqtiboslar 22015: Nashrlar 1, Iqtiboslar 0

Iqtibos tarixi

013451978198319881990199820062010201120151978: Iqtiboslar 01983: Iqtiboslar 11988: Iqtiboslar 21990: Iqtiboslar 31998: Iqtiboslar 02006: Iqtiboslar 12010: Iqtiboslar 02011: Iqtiboslar 22015: Iqtiboslar 0

Nashr tarixi

011978198319881990199820062010201120151978: Nashrlar 11983: Nashrlar 11988: Nashrlar 11990: Nashrlar 11998: Nashrlar 12006: Nashrlar 12010: Nashrlar 12011: Nashrlar 02015: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0121978198319881990199820062010201120151978: h-indeks 01983: h-indeks 11988: h-indeks 11990: h-indeks 21998: h-indeks 22006: h-indeks 22010: h-indeks 22011: h-indeks 22015: h-indeks 2

Eng koʻp iqtibos qilingan asarlar

  1. An automatic nuclear emulsion scanner with moving microscope19783 iqtibos
  2. Asymptotic normalization coefficients from the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>,<i>d</i>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Na</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>21</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reaction and astrophysical factor for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Na</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>21</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>20063 iqtibos
  3. Least-squares analysis of nuclear reaction spectra19832 iqtibos
  4. Spectroscopic information on 36Cl from the (d,p) reaction19881 iqtibos
  5. Spectroscopic information on 13,14C, 15N, 17O, 29–31Si, 33S, 28Cl and 111,113,115,117Cd from the (d,p) reaction19900 iqtibos
  6. Asymptotic normalization coefficients and astrophysical radiative capture reactions19980 iqtibos
  7. Pole approximation validation in the study of the [sup 6]Li(d,α)[sup 4]He reaction20100 iqtibos
  8. Some Insights into Cluster Structure of &amp;lt;sup&amp;gt;9&amp;lt;/sup&amp;gt;Be from &amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;He + &amp;lt;sup&amp;gt;9&amp;lt;/sup&amp;gt;Be Reaction20150 iqtibos

Hammualliflar

  1. V. Burjan4 ta umumiy asar1998–2015
  2. V. Kroha4 ta umumiy asar1998–2015
  3. W. Schäferlingová3 ta umumiy asar1983–1990
  4. J. Mrázek2 ta umumiy asar2010–2015
  5. L. Trache2 ta umumiy asar1998–2010
  6. A. M. Mukhamedzhanov2 ta umumiy asar1998–2006
  7. J. Vincour2 ta umumiy asar1998–2006
  8. C. A. Gagliardi2 ta umumiy asar1998–2006
  9. R. E. Tribble2 ta umumiy asar1998–2006
  10. P. Franc2 ta umumiy asar1983–1988

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