IBI: AJ178; Ivan Milić***, viši naučni saradnik, Astronomska opservatorija u Beogradu; Polje: prirodno-matematičke i medicinske nauke; Period: 2018-2024;
eNauka profil: rp06684; ORCID: 0000-0002-0189-5550;
WOS indikatori: NR = 38; TC = 284; HIndex = 8;
eNauka WOS indikatori: NR = 39; TC = 294; HIndex = 9 ;
Lista A broj bodova: 197.0032 (569) 5.6%; Lista B broj bodova: 190.00241 (569) 42.4%; Lista C broj bodova: 0.000 (0) nan%; Lista A broj bodova kolaboracije: 0.000 (0) nan%; Lista B broj bodova kolaboracije: 0.000 (0) nan%;
Statistika svih rezultata
| Statistika | Ukupno | 2013-2024 | 2015-2024 | 2018-2024 | 2020-2024 |
|---|---|---|---|---|---|
| Broj rezultata | 38 | 27 | 22 | 18 | 17 |
| Broj citata | 284 | 190 | |||
| Broj M bodova | 202.00 | 202 | 199.00 | 190 | |
| Normirani broj citata | 284.00 | 190.00 | |||
| Normirani broj M bodova rezultata kategorije M21a++M21a+M21+M22+M23+M24 | 200.00 | 200.00 | 197.00 | 188.00 | |
| Normirani broj M bodova rezultata kategorije M11+M12+M13+M14+M41 | 0.00 | 0.00 | 0.00 | 0.00 | |
| Normirani broj M bodova rezultata kategorije M11+M12+M13+M14+M41+M42 | 0.00 | 0.00 | 0.00 | 0.00 | |
| Normirani broj M bodova rezultata kategorije M51 | 0.00 | 0.00 | 0.00 | 0.00 | |
| Normirani broj M bodova rezultata kategorije M43+M44 | 0.00 | 0.00 | 0.00 | 0.00 |
Statistika rezultata nastalih u medunarodnim kolaboracijama
| Statistika | Ukupno | 2013-2024 | 2015-2024 | 2018-2024 | 2020-2024 |
|---|---|---|---|---|---|
| Broj rezultata sa 20 i više autora | 0 | 0 | 0 | 0 | 0 |
| Broj citata rezultata sa 20 i više autora | 0 | 0 | |||
| Broj M bodova rezultata M21a++M21a+M21+M22+M23 sa 20 i više autora | 0.00 | 0 | 0.00 | 0 | |
| Normirani broj citata rezultata sa 20 i više autora | 0.00 | 0.00 | |||
| Normirani broj M bodova rezultata M21a++M21a+M21+M22+M23 sa 20 i više autora | 0.00 | 0.00 |
Rezultati
| RB | IBI | Godina | Kat | Tip | Vrsta | Referenca | TC | TCP | BA | NBB | NTC | Naslov | Autori | 1. | AJ178 | 2009 | E | PROCEEDINGS OF THE XV NATIONAL CONFERENCE OF ASTRONOMERS OF SERBIA Vol. 86 (): # 283 - + (2), (DOI: ) 2009WOS | 1 | 1 | 3 | 0 | 1.0000 | ON ESTIMATION OF THE OPTICAL THICKNESS OF SOLAR PROMINENCES | Milic I, Dejanic S, Kotrc P | 2. | AJ178 | 2011 | E | SERBIAN ASTRONOMICAL JOURNAL Vol. 182 (): # 35 - 41 (7), (DOI: 10.2298/SAJ1182035D) 2011WOS | 2 | 1 | 2 | 0 | 1.0000 | CORRECTED μδ FOR STARS OF HIPPARCOS CATALOGUE FROM INDEPENDENT LATITUDE OBSERVATIONS OVER MANY DECADES | Damljianovic G, Milic I | 3. | AJ178 | 2012 | E | ASTRONOMY & ASTROPHYSICS Vol. 539 (): #A10 - (8), (DOI: 10.1051/0004-6361/201117727) MAR 2012WOS | 7 | 3 | 2 | 0 | 3.0000 | Modeling scattering polarization in molecular solar lines in spherical geometry | Milic I, Faurobert M | 4. | AJ178 | 2012 | E | ASTRONOMY & ASTROPHYSICS Vol. 547 (): #A38 - (7), (DOI: 10.1051/0004-6361/201219737) NOV 2012WOS | 11 | 4 | 2 | 0 | 4.0000 | Hanle diagnostics of weak solar magnetic fields: Inversion of scattering polarization in C2 and MgH molecular lines | Milic I, Faurobert M | 5. | AJ178 | 2012 | E | UNDERSTANDING SOLAR ACTIVITY: ADVANCES AND CHALLENGES Vol. 55 (): # 65 - + (2), (DOI: 10.1051/eas/1255008) 2012WOS | 0 | 0 | 2 | 0 | 0.0000 | NUMERICAL MODELING OF THE LINEAR POLARIZATION IN MOLECULAR LINES OF THE SOLAR FLASH SPECTRUM | Milic I, Faurobert M | 6. | AJ178 | 2012 | E | SERBIAN ASTRONOMICAL JOURNAL Vol. 184 (): # 97 - 104 (8), (DOI: 10.2298/SAJ1284097C) 2012WOS | 7 | 4 | 6 | 0 | 4.0000 | FOCAL LENGTH DETERMINATION FOR THE 60 cm TELESCOPE AT ASTRONOMICAL STATION VIDOJEVICA | Cvetkovic Z, Damljanovic G, Pavlovic R, Vince O, Milic I, Stojanovic M | 7. | AJ178 | 2013 | E | ASTRONOMY & ASTROPHYSICS Vol. 555 (): #A130 - (11), (DOI: 10.1051/0004-6361/201321212) JUL 2013WOS | 5 | 1 | 1 | 0 | 1.0000 | Transfer of polarized line radiation in 2D cylindrical geometry | Milic I | 8. | AJ178 | 2013 | E | ASTRONOMY & ASTROPHYSICS Vol. 559 (): #A68 - (5), (DOI: 10.1051/0004-6361/201322307) NOV 2013WOS | 1 | 1 | 3 | 0 | 1.0000 | Boundary conditions for polarized radiative transfer with incident radiation | Faurobert M, Milic I, Atanackovic O | 9. | AJ178 | 2014 | E | ADVANCES IN SPACE RESEARCH Vol. 54 (7): # 1297 - 1307 (11), (DOI: 10.1016/j.asr.2014.05.025) OCT 1 2014WOS | 4 | 3 | 2 | 0 | 3.0000 | Accelerating NLTE radiative transfer by means of the Forth-and-Back Implicit Lambda Iteration: A two-level atom line formation in 2D Cartesian coordinates | Milic I, Atanackovic O | 10. | AJ178 | 2014 | E | ASTRONOMY & ASTROPHYSICS Vol. 571 (): #A79 - (14), (DOI: 10.1051/0004-6361/201424641) NOV 2014WOS | 4 | 4 | 2 | 0 | 4.0000 | Scattering line polarization in rotating, optically thick disks | Milic I, Faurobert M | 11. | AJ178 | 2014 | E | SOLAR POLARIZATION 7 Vol. 489 (): # 157 - 166 (10), (DOI: ) 2014WOS | 0 | 0 | 2 | 0 | 0.0000 | Inferring Depth-Dependent Quiet Sun Magnetic Fields | Milic I, Faurobert M | 12. | AJ178 | 2015 | E | PHILOSOPHICAL QUARTERLY Vol. 65 (261): # 813 - 821 (9), (DOI: 10.1093/pq/pqv024) OCT 2015WOS | 2 | 2 | 1 | 0 | 2.0000 | A NOTE ON EXISTENTIALLY KNOWN ASSERTIONS | Milic I | 13. | AJ178 | 2016 | E | ASTRONOMY & ASTROPHYSICS Vol. 586 (): #A87 - (13), (DOI: 10.1051/0004-6361/201527598) FEB 2016WOS | 10 | 7 | 4 | 0 | 7.0000 | Center-to-limb variation of intensity and polarization in continuum spectra of FGK stars for spherical atmospheres | Kostogryz N, Milic I, Berdyugina S, Hauschildt P | 14. | AJ178 | 2017 | E | ASTRONOMY & ASTROPHYSICS Vol. 601 (): #A6 - (8), (DOI: 10.1051/0004-6361/201628762) MAY 2017WOS | 8 | 8 | 4 | 0 | 8.0000 | Polarimetry of transiting planets: Differences between plane-parallel and spherical host star atmosphere models | Kostogryz N, Yakobchuk T, Berdyugina S, Milic I | 15. | AJ178 | 2017 | E | ASTRONOMY & ASTROPHYSICS Vol. 597 (): #A31 - (10), (DOI: 10.1051/0004-6361/201628961) JAN 2017WOS | 4 | 4 | 3 | 0 | 4.0000 | Inference of magnetic fields in inhomogeneous prominences | Milic I, Faurobert M, Atanackovic O | 16. | AJ178 | 2018 | M21a | E | Article | ASTRONOMY & ASTROPHYSICS Vol. 617 (): #A24 - (11), (DOI: 10.1051/0004-6361/201833382) SEP 18 2018WOS | 62 | 48 | 2 | 9.0000 | 48.0000 | Spectropolarimetric NLTE inversion code SNAPI | Milic I, van N | 17. | AJ178 | 2020 | M21a | E | Article | ASTRONOMY & ASTROPHYSICS Vol. 644 (): #A129 - (13), (DOI: 10.1051/0004-6361/201936537) DEC 9 2020WOS | 21 | 14 | 2 | 12.0000 | 14.0000 | Mimicking spectropolarimetric inversions using convolutional neural networks | Milic I, Gafeira R | 18. | AJ178 | 2020 | M21a | E | Article | ASTROPHYSICAL JOURNAL LETTERS Vol. 900 (2): #L29 - (7), (DOI: 10.3847/2041-8213/abb1a5) SEP 2020WOS | 15 | 12 | 5 | 12.0000 | 12.0000 | Chromospheric Resonances above Sunspots and Potential Seismological Applications | Felipe T, Kuckein C, Manrique S, Milic I, Sangeetha C | 19. | AJ178 | 2020 | M22 | E | Article | FRONTIERS IN ASTRONOMY AND SPACE SCIENCES Vol. 7 (): #29 - (7), (DOI: 10.3389/fspas.2020.00029) JUN 23 2020WOS | 5 | 5 | 4 | 5.0000 | 5.0000 | Spectral Deconvolution With Deep Learning: Removing the Effects of Spectral PSF Broadening | Molnar M, Reardon K, Osborne C, Milic I | 20. | AJ178 | 2021 | M21a | E | Article | ASTRONOMY & ASTROPHYSICS Vol. 651 (): #A31 - (12), (DOI: 10.1051/0004-6361/201936910) JUL 6 2021WOS | 29 | 22 | 6 | 12.0000 | 22.0000 | Machine learning initialization to accelerate Stokes profile inversions | Gafeira R, Suárez D, Milic, Noda C, Cobo B, Uitenbroek H | 21. | AJ178 | 2021 | M21a | E | Article | ASTROPHYSICAL JOURNAL Vol. 917 (1): #14 - (17), (DOI: 10.3847/1538-4357/ac02be) AUG 2021WOS | 28 | 18 | 2 | 12.0000 | 18.0000 | The Lightweaver Framework for Nonlocal Thermal Equilibrium Radiative Transfer in Python | Osborne C, Milic I | 22. | AJ178 | 2021 | M21a | E | Article | ASTROPHYSICAL JOURNAL Vol. 918 (2): #47 - (14), (DOI: 10.3847/1538-4357/ac111c) SEP 2021WOS | 7 | 5 | 4 | 12.0000 | 5.0000 | Limitations of the Ca ii 8542 Å Line for the Determination of Magnetic Field Oscillations | Felipe T, Navarro H, Sangeetha C, Milic I | 23. | AJ178 | 2022 | M21a | E | Article | ASTRONOMY & ASTROPHYSICS Vol. 664 (): #A182 - (10), (DOI: 10.1051/0004-6361/202142015) AUG 29 2022WOS | 5 | 1 | 3 | 12.0000 | 1.0000 | Investigating magnetic field inference from the spectral region around the Mg I b2 line using the weak-field approximation | Vukadinovic D, Milic, Atanackovic O | 24. | AJ178 | 2022 | M21a | E | Article | ASTROPHYSICAL JOURNAL Vol. 933 (2): #244 - (19), (DOI: 10.3847/1538-4357/ac6f00) JUL 1 2022WOS | 7 | 6 | 6 | 12.0000 | 6.0000 | Evaluating Non-LTE Spectral Inversions with ALMA and IBIS | Hofmann R, Reardon K, Milic I, Molnar M, Chai Y, Uitenbroek H | 25. | AJ178 | 2023 | M21a | E | Article | ASTROPHYSICAL JOURNAL Vol. 945 (2): #154 - (15), (DOI: 10.3847/1538-4357/acbc75) MAR 1 2023WOS | 8 | 6 | 5 | 12.0000 | 6.0000 | Constraining the Systematics of (Acoustic) Wave Heating Estimates in the Solar Chromosphere | Molnar M, Reardon K, Cranmer S, Kowalski A, Milic I | 26. | AJ178 | 2023 | M21a | E | Article | ASTROPHYSICAL JOURNAL Vol. 951 (1): #23 - (14), (DOI: 10.3847/1538-4357/acd178) JUL 1 2023WOS | 8 | 3 | 5 | 12.0000 | 3.0000 | Limitations and Biases in the Retrieval of the Polar Magnetic Field. I. The Role of the Magnetic Filling Factor in Milne-Eddington Inversions of Simulated Hinode/SP Data | Centeno R, Milic I, Rempel M, Nitta N, Sun X | 27. | AJ178 | 2023 | M21a | E | Article | ASTROPHYSICAL JOURNAL Vol. 956 (2): #83 - (13), (DOI: 10.3847/1538-4357/ace621) OCT 1 2023WOS | 8 | 3 | 6 | 12.0000 | 3.0000 | Quantifying Poynting Flux in the Quiet Sun Photosphere | Tilipman D, Kazachenko M, Tremblay B, Milic I, Pillet V, Rempel M | 28. | AJ178 | 2024 | M21a | E | Article | ASTRONOMY & ASTROPHYSICS Vol. 683 (): #A134 - (7), (DOI: 10.1051/0004-6361/202347272) MAR 15 2024WOS | 7 | 3 | 5 | 12.0000 | 3.0000 | Spatial resolution effects on the solar open flux estimates | Milic I, Centeno R, Sun X, Rempel M, Rodríguez J | 29. | AJ178 | 2024 | M21a | E | Article | ASTRONOMY & ASTROPHYSICS Vol. 688 (): #A56 - (16), (DOI: 10.1051/0004-6361/202349020) AUG 1 2024WOS | 2 | 0 | 5 | 12.0000 | 0.0000 | One-dimensional, geometrically stratified semi-empirical models of the quiet-Sun photosphere and lower chromosphere | Borrero J, Milic I, Yabar A, Kaithakkal A, Rodríguez D | 30. | AJ178 | 2024 | M21a | E | Article | ASTRONOMY & ASTROPHYSICS Vol. 691 (): #A176 - (12), (DOI: 10.1051/0004-6361/202451079) NOV 13 2024WOS | 1 | 0 | 3 | 12.0000 | 0.0000 | Solar internetwork magnetic fields: Statistical comparison between observations and MHD simulations | Ebert E, Milic I, Borrero J | 31. | AJ178 | 2024 | M21a | E | Article | ASTROPHYSICAL JOURNAL Vol. 976 (1): #21 - (16), (DOI: 10.3847/1538-4357/ad81d4) NOV 1 2024WOS | 2 | 0 | 6 | 12.0000 | 0.0000 | Constraints on Acoustic Wave Energy Fluxes and Radiative Losses in the Solar Chromosphere from Non-LTE Inversions | Santos J, Molnar M, Milic I, Rempel M, Reardon K, Rodríguez J | 32. | AJ178 | 2024 | M21a | E | Article | ASTROPHYSICAL JOURNAL LETTERS Vol. 971 (1): #L1 - (9), (DOI: 10.3847/2041-8213/ad62f8) AUG 1 2024WOS | 0 | 0 | 8 | 10.0000 | 0.0000 | Observations of Locally Excited Waves in the Low Solar Atmosphere Using the Daniel K. Inouye Solar Telescope | Bahauddin S, Fischer C, Rast M, Milic I, Woeger F, Rempel M, Keys P, Rimmele T | 33. | AJ178 | 2024 | M22 | E | Article | SOLAR PHYSICS Vol. 299 (9): #123 - (19), (DOI: 10.1007/s11207-024-02358-z) SEP 2024WOS | 1 | 1 | 6 | 5.0000 | 1.0000 | High-Resolution Sun-as-a-Star Spectroscopy of the Partial Solar Eclipse of 2017 August 21 | Dineva E, Denker C, Verma M, Strassmeier K, Ilyin I, Milic I | 34. | AJ178 | 2025 | E | ASTRONOMY & ASTROPHYSICS Vol. 693 (): #A272 - (15), (DOI: 10.1051/0004-6361/202452331) JAN 24 2025WOS | 1 | 0 | 4 | 0 | 0.0000 | Spectral resolution effects on the information content in solar spectra | Baso C, Milic I, van d, Schlichenmaier R | 35. | AJ178 | 2025 | E | ASTRONOMY & ASTROPHYSICS Vol. 697 (): #L7 - (7), (DOI: 10.1051/0004-6361/202554498) MAY 14 2025WOS | 1 | 0 | 6 | 0 | 0.0000 | Fine-scale opposite-polarity magnetic fields in a solar plage revealed by integral field spectropolarimetry | Liu G, Milic I, Durán J, Borrero J, van N, Kuckein C | 36. | AJ178 | 2025 | E | ASTRONOMY & ASTROPHYSICS Vol. 701 (): #A80 - (11), (DOI: 10.1051/0004-6361/202555911) SEP 5 2025WOS | 0 | 0 | 4 | 0 | 0.0000 | An inversion approach to retrieve the vector magnetic field from scattering polarization in strong solar resonance lines | Janett G, Milic I, Riva F, Belluzzi L | 37. | AJ178 | 2025 | E | ASTRONOMY & ASTROPHYSICS Vol. 702 (): #A253 - (14), (DOI: 10.1051/0004-6361/202556482) OCT 24 2025WOS | 0 | 0 | 7 | 0 | 0.0000 | Modeling Helioseismic and Magnetic Imager observables for the study of solar oscillations | Fournier D, Kostogryz N, Gizon L, Schou J, Witzke V, Shapiro A, Milic I | 38. | AJ178 | 2025 | E | ASTROPHYSICAL JOURNAL Vol. 986 (2): #124 - (16), (DOI: 10.3847/1538-4357/add0ad) JUN 20 2025WOS | 0 | 0 | 4 | 0 | 0.0000 | A High-resolution, Inversion-based Synoptic Study of Solar Granulation | Crowley J, Milic I, Cauzzi G, Reardon K |
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27. 04. 2026.; 00:09:42; Trajanje procesiranja: 0.020 s
Legenda:
RB - redni broj rezultata
IBI - identifikacioni broj istraživača
Godina - godina u kojoj je rezultat publikovan (isključivo sa kompletnom paginacijom)
Kat - kategorija rezulata
Tip - tip rezultata (teorijski, simulacioni ili eksperimentalni)
Vrsta - vrsta rezultata
Referenca - referenca rezultata (bez autora i naslova rezultata) sa direktnim linkom na rezultat (ako ima DOI broj), sa linkom na zapis u eNauci ili WOS
TC - ukupan broj citata rezulata na dan 31. 1. 2026. godine
TCP - ukupan broj citata rezultata u periodu 2015-2024
BA - broj autora na rezultatu
NBB - normirani broj bodova rezultata
NTC - normirani broj citata rezultata u periodu 2015-2024
Naslov - naslov rezultata
Autori - spisak svih autora ili najviše prvih 30 autora
Primer:
Primer normiranja broja M poena i broja citata ostvarenih na jednom rezultatu: eksperimentalni rad sa 11 autora u časopisu kategorije M21a+ koji je publikovan 2020. godine, citiran je 65 puta, od čega 55 puta u periodu 2015-2024. godine.
Normirani broj M poena koje istraživač ostvaruje na rezultatu je 20/(1+0.2*(11-10))=16.6667 a normirani broj citata je 55/(1+0.2*(11-10))=45.8333.
Ukupan broj ostaverinih bodova utvrđuje se na naznačenom periodu za sabiranje normiranih M poena svakog istraživača i u periodu za određivanje ukupnog broja normiranih citata (2015-2024).