naveden je 5 puta dok je nedavno objav eni rad

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2 doktorsku tezu u kojoj je unapredio teorij spektroskopije kvazi-termalnih xumova koja se odnosi na tzv. udarne signale, odnosno signale koji dolaze od elektrona koji, osim xto stvaraju fluktuirajue mer ivo elektriqno po e u kosmiqkim uslovima ostvaruju i fiziqki kontakt sa antenom na svemirskim modulima, stvarajui dodatnu komponentu signala. Tokom obrade podataka na dosadax im svemirskim misijama doprinos ove komponente je bio zanemar iv jer su antene koje su korixene, imale veliku duinu i mali preqnik u odnosu na karakteristiqne duine koje opisuju svemirsku plazmu i plazmu sunqevog vetra. U tom kontekstu, kako satelit STEREO, sa kojeg su podaci obraivani u ovoj disertaciji, ima kratke antene relativno velikog preqnika, teorija udarnih signala je morala biti unapreena kako bi interpretacija satelickih mere a bila zadovo avajua. Obradom podataka sa ove misije dobijene su vrednosti elektronske temperature, koje nisu dobijene eksperimentalno jer na ovom satelitu elektronski analizatori koji su naprav eni da mere ovu veliqinu nisu radili i ne rade ispravno. Tako je ustanov en je metod za masovnu obradu podataka, koji je pokazao dobro slaga e i koji je uporeen sa sliqnim metodama na drugim misijama. Metod je stvorio osnovu za prav e e baze podataka temperature elektrona. U periodu od do godine objavio je i vixe radova u kojima su dati rezultati proraquna parametara Xtarkovog pomeraja profila spektralnih linija bazirani na semiklasiqnoj teoriji (Foster 1927), kao i teorijska razmatra a elektronskog fluksa plazme sunqevog vetra na telima razliqitih geometrijskih oblika koja su unapredila standardno korixenu teoriju ograniqenog orbitalnog kreta a (Laframoaz i Parker, 1973). Takoe je aktivan na razvoju metoda primene spektroskopije kvazi-termalnih xumova u jonosferskim i laboratorijskim plazmama. Dosadax i rad dr Mihaila Martinovia predstav en je u ukupno 12 nauqnih referenci (2 rada u vrhunskim meunarodnim qasopisima, 1 rad u meunarodnom qasopisu, 7 saopxte a sa meunarodnih skupova xtampana u celini ili izvodu i dve teze). Indikator nauqne kompetentnosti (M) za dr Mihaila Martinovia je: M = 30, ili po pojedinim stavkama: M21=16; M23=3; M33=3;M34=2; M71=6; O znaqaju publikovanih rezultata kandidata govori navoe e egovih radova u domaim i inostranim nauqnim qasopisima. Rad N. Cvetanović, M. M. Martinović, B. M. Obradović, M. M. Kuraica (2015) Electric field measurement in gas discharges using stark shifts of He I lines and their forbidden counterparts, Journal of Physics D: Applied Physics, 48, naveden je 5 puta dok je nedavno objav eni rad M. M. Martinović, A. Zaslavsky, M. Maksimović, N. Meyer-Vernet, S. Šegan, I. Zouganelis, C. Salem, M. Pulupa, S. D. Bale (2016) Quasi-thermal noise measurements on STEREO: Kinetic temperature deduction using electron shot noise model, Journal of Geophysical Research: Space Physics, 121, 129 raen u sarad i sa dva principijalna istraivaqa radio instrumenata koji e biti instalirani na buduim na meunarodnim svemirskim misijama i oqekuje se da se nastavi u stvara e baze podataka elektronske temperature na misiji STEREO gde nedostatak adekvatnog mere a datog parametra trenutno spreqava adekvatnu 2

3 analizu mnogih posmatranih pojava u sunqevom vetru. 3. Ostali podaci Pored navedenog nauqnog rada dr Mihailo Martinovi je obav ao sledee delatnosti znaqajne za nauqnoistraivaqki rad: Drao je vixe predava a u Laboratoriji za svemirske nauke Univerziteta Kalifornije u Berkliju (decembar 2014, decembar 2015), Pariskoj opservatoriji (maj 2014, mart 2016, maj 2016), Matematiqkom (decembar 2014) i Fiziqkom (jul 2013) fakultetu Univerziteta u Beogradu kao i dva kratka predava a u sklopu pripreme mladih astronoma za Meunarodnu Olimpijadu iz astronomije (novembar 2016). Qlan je Druxtva astronoma Srbije i Ameriqke geofiziqke unije 4. Spisak radova dr Mihaila Martinovia Rad u vrhunskom meunarodnom qasopisu (M21) [1] N. Cvetanović, M. M. Martinović, B. M. Obradović, M. M. Kuraica (2015) Electric field measurement in gas discharges using stark shifts of He I lines and their forbidden counterparts, Journal of Physics D: Applied Physics, 48, [2] M. M. Martinović, A. Zaslavsky, M. Maksimović, N. Meyer-Vernet, S. Šegan, I. Zouganelis, C. Salem, M. Pulupa, S. D. Bale (2016) Quasi-thermal noise measurements on STEREO: Kinetic temperature deduction using electron shot noise model, Journal of Geophysical Research: Space Physics, 121, 129 Rad u meunarodnom qasopisu (M23) [3] M. M. Martinović (2016) Orbit limited theory in the solar wind kappa distributions, Serbian Astronomical Journal, 192, 27 Saopxte e sa meunarodnog skupa xtampano u celini (M33) [4] I. P. Dojčinović, K. Vuković, M. M. Martinović, J. Purić (2011) Plasma flow interaction with materials of interest for fusion devices, Advances in Applied Plasma Science, 8, 63 [5] M. M. Martinović, A. Zaslavsky, M. Maksimović, K. Issautier (2014) Quasi-thermal noise spectroscopy in Earths magnetosheath: Theory and application to plasma diagnostic on WIND spacecraft, Publications of Astronomical Observatory of Belgrade, 94, 112 3

4 [6] M. M. Martinović, I. P. Dojčinović, J. Purić (2012) Perpendicular magnetic field influence on silicon surface modification by quasistationary plasma flow, Contributed papers of SPIG, 26, 216 Saopxte e sa meunarodnog skupa xtampano u izvodu (M34) [7] M. M. Martinović, A. Zaslavsky, M. Maksimović, I. Zouganelis, (2014) Measurements of plasma quasi-thermal noise on STEREO spacecraft and plasma temperature deduction using antenna electron shot noise model, AGU Fall Meeting, SH21B, 4125 [8] I. Zouganelis, M. Moncuquet, N. Meyer-Vernet, K. Issautier, A. Zaslavsky, M. Maksimović, G. Le Chat, M. M. Martinović, (2014) Probing the inner heliosphere and corona with electric antennas: quasi-thermal noise spectroscopy on Solar Orbiter and Solar Probe Plus, AGU Fall Meeting, SH21B, 4106 [9] M. M. Martinović, A. Zaslavsky, M. Maksimović, I. Zouganelis, (2015) Shot noise measured by an antenna in a plasma with suprathermal electron tails: Application to Solar Orbiter, First joint Solar Probe Plus - Solar Orbiter Workshop, Artimino, Italija [10] M. M. Martinović, A. Zaslavsky, M. Maksimović, S. Šegan, M. Svetlik (2015) (2015) Quasi-thermal noise observed by CASSINI during the first flyby of Venus, AGU Fall Meeting, SH31C, 2433 Odbra ena doktorska disertacija (M71) [11] M. M. Martinovi, (2016) Spektroskopija kvazi termalnih xumova i udarnih elektronskih signala u svemirskoj plazmi LESIA, Pariska opservatprija, Medon i Katedra za astronomiju Matematiqkog fakulteta, Beograd Tabela: Vrsta i kvantifikacija nauqnoistraivaqkih rezultata po grupama za dr Mihaila Martinovia: Oznaka grupe Vrsta rezultata Oznaka vrste Vrednost Broj rezultata rezultata rezultata radova, sopxte a... M20 Rad u vrhunskom maunarodnom qasopisu M Rad u maunarodnom qasopisu M M30 Saopxte a sa meunarodnog skupa xtampano u celini M Saopxte a sa meunarodnog skupa xtampano u izvodu M M70 Odbra ena doktorska disertacija M

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