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C. Consolandi

20 papers hereh-index 295.9k citations96 works total

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

author position
  • sole author1
  • middle author15

Across the 16 of 20 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE6
  • astro-ph.SR4
  • astro-ph.EP3
  • astro-ph.IM3
  • physics.space-ph2
  • physics.atom-ph1
same name
  • C. Consolandi — 1 paper

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
20102019
most citedSolar Modulation of the Proton Local Interstellar Spectrum with AMS-02, Voyager 1 and PAMELA

88 citations · 267 across the 20 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

3 papers · 1 filter

astro-ph.IM2013★ 3 cited

GeoMag and HelMod webmodels version for magnetosphere and heliosphere transport of cosmic rays

P. Bobik, M. J. Boschini, C. Consolandi +10

We implemented a website to deal with main effects on Cosmic Ray access to the Earth, i.e. the Solar Modulation and the Geomagnetic Field effect. In helmod.org the end user can eas…

astro-ph.IM2013

Suprathermal particle addition to solar wind pressure: possible influence on magnetospheric transmissivity of low energy cosmic rays?

P. Bobik, M. J. Boschini, C. Consolandi +10

Energetic (suprathermal) solar particles, accelerated in the interplanetary medium, contribute to the solar wind pressure, in particular during high solar activity periods. We esti…

astro-ph.IM2013

Geomagnetic Backtracing: A comparison of Tsyganenko 1996 and 2005 External Field models with AMS-02 data

M. J. Boschini, C. Consolandi, S. Della Torre +8

We used a backtracing code to reconstruct particle trajectory inside the Earth Magnetosphere during the last solar active period (2011 and 2012) when very high Solar Wind pressure…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.