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T. Hackman

36 papers hereh-index 18944 citations91 works total

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

author position
  • first author5
  • middle author23
  • last author5

Across the 33 of 36 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR32
  • astro-ph2
  • astro-ph.CO1
  • astro-ph.EP1
same name
  • T. Hackman — 5 papers, h 2
  • T. Hackman — 2 papers

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
20002023
most citedHidden magnetic fields of young suns

87 citations · 897 across the 36 of their papers we have counts for

collaborators
Showing 2015 · astro-ph.SRShow all

4 papers · 2 filters

astro-ph.SR2015★ 84 cited

Activity trends in young solar-type stars

Jyri Lehtinen, Lauri Jetsu, Thomas Hackman +2

We study a sample of 21 young and active solar-type stars with spectral types ranging from late F to mid K and characterize the behaviour of their activity. We apply the continuous…

astro-ph.SR2015★ 25 cited

Zeeman-Doppler imaging of active young solar type stars

Thomas Hackman, Jyri Lehtinen, Lisa Rosén +2

By studying young magnetically active late-type stars, i.e. analogues to the young Sun, one can draw conclusions on the evolution of the solar dynamo. We determine the topology of…

astro-ph.SR2015★ 11 cited

Study of FK Comae Berenices: VII. Correlating photospheric and chromospheric activity

K. Vida, H. Korhonen, I. V. Ilyin +3

We study the connection between the chromospheric and photospheric behaviour of the active late-type star FK Comae. We use spot temperature modelling, light curve inversion based o…

astro-ph.SR2015★ 12 cited

Doppler Imaging of LQ Hya for 1998-2002

E. M. Cole, T. Hackman, M. J. Käpylä +3

We study the spot distribution on the surface of LQ~Hya during the observing seasons October 1998 -- November 2002. We look for persistent active longitudes, trends in the level of…

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