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Lili Sapar

https://etis.ee/CV/Lili_Sapar/est
12.10.1947
7410465
lilli@aai.ee

Teenistuskäik

Töökohad ja ametid
Töötanud astrofüüsika erialal Füüsika ja Astronoomia Insti-tuudis (1971-1973), AAI-s (1973-1995) ning Tartu Obser-vatooriumis (alates 1995.a.) laborandina (1971-1974), noorem teadurina (1974-1986) ning teadurina alates 1986.a.
1995–31.12.2013   
Tartu Observatoorium, Teadur (1,00)
 
 
Haridustee
Kõrgem, Kaasani Riiklik Ülikool (1971), astronoom
 
 
Teadusorganisatsiooniline ja -administratiivne tegevus
Euroopa Astronoomiaühingu liige, Eesti Astronoomia Seltsi liige, Rahvusvahelise Astronoomialiidu liige.

Kvalifikatsioon

Teaduskraadid
Lili Sapar, doktorikraad, 1990, (juh) Arved-Ervin Sapar, Kuumade tähtede atmosfääriväliste ultraviolettspektrite uurimine, Tartu Observatoorium.
 
 
Lisainfo
kandidaat
Astronoomia ja Atmosfäärifüüsika Instituut (AAI), 1990.a.

Publikatsioonid

Klass
Aasta
Publikatsioon
 
1.1.
2008
Sapar, A.; Aret, A.; Sapar, L.; Poolamäe, R. (2008). Formulae for study of LID induced diffusion in CP star model atmospheres. Contributions of the Astronomical Observatory Skalnaté Pleso, 38 (2), 445−446.
1.1.
2008
Sapar, A.; Aret, A.; Poolamäe, R.; Sapar, L. (2008). Segregation of isotopes of heavy metals due to light-induced drift: results and problems. Contributions of the Astronomical Observatory Skalnaté Pleso, 38 (2), 273−278.
3.1.
2008
Sapar, Arved-Ervin; Aret, Anna; Sapar, Lili; Poolamäe, Raivo (2008). A Pan-Spectral Method of Abundance Determination. Precision Spectroscopy in Astrophysics: Precision Spectroscopy in Astrophysics, Lisborn/Aveiro, Portugal, 11-15 September 2006. Ed. N.G. Santos, L. Pasquini, A.C.M. Correia, M. Romaniello. Springer Verlag, 145−148. (ESO Astrophysics Symposia; XXII).
3.4.
2007
Sapar, A.; Aret, A.; Sapar, L.; Poolamäe, R. (2007). The separation of isotopes of chemical elements in the atmospheres of CP stars due to light-induced drift. Spectroscopic Methods in Modern Astrophysics: INASAN, Moscow, Russia, 13.09-15.09.2006. Toim. L. Mashonkina, M. Sachkov. Moscow, 220−235.
3.4.
2007
Sapar, A.; Poolamäe, R.; Sapar, L.; Aret, A. (2007). Computation of Model Atmospheres and Spectra of Hot Stars by Program SMART: Results and Problems. Spectroscopic Methods in Modern Astrophysics: INASAN, Moscow, Russia, 13.09-15.09.2006. Toim. L. Mashonkina, M. Sachkov. Moscow, 236−254.
1.1.
2006
Sapar, Arved; Poolamäe, Raivo; Sapar, Lili (2006). High-Precision Approximation Expressions for Line Profiles of Hydrogenic Particles. Baltic Astronomy, 15, 435−447.
1.1.
2005
Sapar, A.; Sapar, L.; Poolamäe, R. (2005). Scattered Light Redistribution Functions for Spectral Lines in Media with Anisotropic Macroturbulence. Baltic Astronomy, 14, 122−143.
1.1.
2003
Sapar, A.; Sapar, L.; Poolamäe, R. (2003). Analytical Solutions forthe Saturated P Cygni Type Profiles II: General Case. Astrophysics and Space Science, 286, 333−345.
1.1.
2002
Sapar, A.; Sapar, L.; Poolamäe, R. (2002). Analytical Solutions for Saturated P Cygni Type Profiles. Astrophysics and Space Science, 279, 229−244.
3.1.
2000
Sapar, A.; Sapar, L.; Poolamäe, R. (2000). Standard Saturated P Cyg Profiles. Thermal and Ionization Aspects of Flows from Hot Stars: Observations and Theory, 204. Ed. H.J.G.L.M. Lamers and A. Sapar., 237−238. (ASP Conf. Series).
1.1.
1999
Sapar, A.; Sapar, L. (1999). Formation of Resonance Spectral Line Profiles in Stellar Wind: Theory and Observations. Astronomical and Astrophysical Transactions, 18, 475−486.
21.04.2019

Lili Sapar

https://etis.ee/CV/Lili_Sapar/eng
12.10.1947
7410465
lilli@aai.ee

Career

Institutions and positions
worked at Institute of Physics and Astronomy (1971-1973)Institute of Astrophysics and Atmospheric Physics(1973-1995), Tartu Observatory (since 1995) as laborant (1971-1974), junior research associate (1974-1986), research associate (since 1986).
1995–31.12.2013   
Tartu Observatory, Researcher (1,00)
 
 
Education
Kazan State University (1971), astronomy
 
 
R&D related managerial and administrative work
Member of European Astronomical Society, member of Estonian Astronomical Society, member of International Astronomical Union.

Qualifications

Academic degrees
Lili Sapar, Doctor's Degree, 1990, (sup) Arved-Ervin Sapar, Kuumade tähtede atmosfääriväliste ultraviolettspektrite uurimine (Investigation of Extraterrestrial Ultraviolet Spectra of hot stars), Tartu Observatory.
 
 
Additional information
Ph. D. Institute of Astrophysics and Atmospheric Physics, 1990.

Publications

Category
Year
Publication
 
1.1.
2013
Sapar Arved-Ervin, Poolamäe Raivo, Sapar Lili (2013). New Methods in Modeling of Hot Stellar Atmospheres. Baltic Astronomy, 22, 161−179. DOI: 10.1515/astro-2017-0155.
1.1.
2013
Sapar Arved-Ervin, Poolamäe Raivo, Sapar Lili (2013). New High-precision Method of Temperature Distribution in Model Stellar Atmospheres. Baltic Astronomy, 22, 145−159. DOI: 10.1515/astro-2017-0154.
1.1.
2009
Sapar, A.; Aret, A.; Sapar, L.; Poolamäe, R. (2009). Modelling of mercury isotope separation in CP stellar atmospheres: results and problems. New Astronomy Reviews, 53, 240−245. DOI: 10.1016/j.newar.2009.08.010.
1.1.
2008
Sapar, A.; Aret, A.; Sapar, L.; Poolamäe, R. (2008). Formulae for study of LID induced diffusion in CP star model atmospheres. Contributions of the Astronomical Observatory Skalnaté Pleso, 38 (2), 445−446.
1.1.
2008
Sapar, A.; Aret, A.; Poolamäe, R.; Sapar, L. (2008). Segregation of isotopes of heavy metals due to light-induced drift: results and problems. Contributions of the Astronomical Observatory Skalnaté Pleso, 38 (2), 273−278.
3.1.
2008
Sapar, Arved-Ervin; Aret, Anna; Sapar, Lili; Poolamäe, Raivo (2008). A Pan-Spectral Method of Abundance Determination. Precision Spectroscopy in Astrophysics: Precision Spectroscopy in Astrophysics, Lisborn/Aveiro, Portugal, 11-15 September 2006. Ed. N.G. Santos, L. Pasquini, A.C.M. Correia, M. Romaniello. Springer Verlag, 145−148. (ESO Astrophysics Symposia; XXII).
3.1.
2008
Aret, A.; Sapar, A.; Poolamäe, R.; Sapar, L. (2008). SMART – a computer program for modelling stellar atmospheres. The Art of Modeling Stars in the 21st Century: IAU Symposium S252, Sanya, China, April 6-11, 2008. Ed. Deng, L,; Chan, K.L. Cambridge University Press, 41−42. (Proceedings of the International Astronomical Union; 4, S252). DOI: 10.1017/S1743921308022394.
3.4.
2007
Sapar, A.; Aret, A.; Sapar, L.; Poolamäe, R. (2007). The separation of isotopes of chemical elements in the atmospheres of CP stars due to light-induced drift. Spectroscopic Methods in Modern Astrophysics: INASAN, Moscow, Russia, 13.09-15.09.2006. Toim. L. Mashonkina, M. Sachkov. Moscow, 220−235.
3.4.
2007
Sapar, A.; Poolamäe, R.; Sapar, L.; Aret, A. (2007). Computation of Model Atmospheres and Spectra of Hot Stars by Program SMART: Results and Problems. Spectroscopic Methods in Modern Astrophysics: INASAN, Moscow, Russia, 13.09-15.09.2006. Toim. L. Mashonkina, M. Sachkov. Moscow, 236−254.
1.1.
2006
Sapar, Arved; Poolamäe, Raivo; Sapar, Lili (2006). High-Precision Approximation Expressions for Line Profiles of Hydrogenic Particles. Baltic Astronomy, 15, 435−447.
1.1.
2005
Sapar, A.; Sapar, L.; Poolamäe, R. (2005). Scattered Light Redistribution Functions for Spectral Lines in Media with Anisotropic Macroturbulence. Baltic Astronomy, 14, 122−143.
1.1.
2003
Sapar, A.; Sapar, L.; Poolamäe, R. (2003). Analytical Solutions forthe Saturated P Cygni Type Profiles II: General Case. Astrophysics and Space Science, 286, 333−345.
1.1.
2002
Sapar, A.; Sapar, L.; Poolamäe, R. (2002). Analytical Solutions for Saturated P Cygni Type Profiles. Astrophysics and Space Science, 279, 229−244.
3.1.
2000
Sapar, A.; Sapar, L.; Poolamäe, R. (2000). Standard Saturated P Cyg Profiles. Thermal and Ionization Aspects of Flows from Hot Stars: Observations and Theory, 204. Ed. H.J.G.L.M. Lamers and A. Sapar., 237−238. (ASP Conf. Series).
1.1.
1999
Sapar, A.; Sapar, L. (1999). Formation of Resonance Spectral Line Profiles in Stellar Wind: Theory and Observations. Astronomical and Astrophysical Transactions, 18, 475−486.
21.04.2019

Otsi projekti

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Asutus on projekti finantseerija   Asutus on projekti teostaja  
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Kõik   Tavaprojektid   Ülemprojektid   Alamprojektid  
Uus Frascati (2015)
Uus ja vana Frascati (otsing uue järgi väljastab ka seotud vanad)
Kõik
Käimasolevad
Lõppenud
Algus
Hajus
Täpne
Lihtotsing Tühjenda
  • Leitud 3 kirjet
ProgrammLiikNumberNimiProjekti algusProjekti lõppVastutav täitjaAsutusFinantseerijapoolne rahastamine
SFSF0060030s08Evolutsiooni hilisfaasides tähtede ja nende ümbriste vaatluslik ja teoreetiline uurimine.01.01.200831.12.2013Tõnu KipperTartu Observatoorium1 741 486,12 EUR
ETFETF6105Täheatmosfääride ja tähetuulte ehitus ja spektrid; füüsikalised protsessid neis01.01.200531.12.2008Arved-Ervin SaparTartu Observatoorium42 738,10 EUR
SFSF0062464s03Tähtede ehitus, keemiline koostis ja evolutsioon.01.01.200331.12.2007Tõnu KipperTartu Observatoorium894 251,78 EUR