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researcher

V. Mikhailov

6 papers hereh-index 9701 citations86 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author5

Across the 5 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • physics.space-ph2
  • astro-ph1
same name
  • V. Mikhailov — 48 papers, h 55
  • V. Mikhailov — 24 papers, h 15
  • V. Mikhailov — 3 papers, h 16
  • V. Mikhailov — 3 papers, h 5
  • V. Mikhailov — 2 papers, h 1
  • V. Mikhailov — 2 papers, h 6

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20062016
most citedPAMELA - A Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics

440 citations · 826 across the 6 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2016★ 65 cited

Time dependence of the electron and positron components of the cosmic radiation measured by the PAMELA experiment between July 2006 and December 2015

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +52

Cosmic-ray electrons and positrons are a unique probe of the propagation of cosmic rays as well as of the nature and distribution of particle sources in our Galaxy. Recent measurem…

astro-ph.HE2015

Re-Entrant Albedo Proton Fluxes Measured by the PAMELA Experiment

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +56

We present a precise measurement of downward-going albedo proton fluxes for kinetic energy above ∼ 70 MeV performed by the PAMELA experiment at an altitude between 350 and 610…

astro-ph.HE2013★ 285 cited

Time dependence of the proton flux measured by PAMELA during the July 2006 - December 2009 solar minimum

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +61

The energy spectra of galactic cosmic rays carry fundamental information regarding their origin and propagation. These spectra, when measured near Earth, are significantly affected…

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