How to build a scientific career: Marie Sklodowska Curie Actions (MSCA) experience. Mateja Dumbovic Institute of Physics University of Graz
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1 How to build a scientific career: Marie Sklodowska Curie Actions (MSCA) experience Mateja Dumbovic Institute of Physics University of Graz
2 About
3 About EXCELLENT SCIENCE INDUSTRIAL LEADERSHIP SOCIETAL CHALLENGES
4 About EXCELLENT SCIENCE INDUSTRIAL LEADERSHIP SOCIETAL CHALLENGES
5 About EXCELLENT SCIENCE INDUSTRIAL LEADERSHIP SOCIETAL CHALLENGES MARIE SKLODOWSKA CURIE ACTIONS (MSCA) FUTURE AND EMERGING TECHNOLOGIES EUROPEAN RESEARCH COUNCIL RESEARCH INFRASTRUCTURE
6 About EXCELLENT SCIENCE INDUSTRIAL LEADERSHIP SOCIETAL CHALLENGES MARIE SKLODOWSKA CURIE ACTIONS (MSCA) FUTURE AND EMERGING TECHNOLOGIES EUROPEAN RESEARCH COUNCIL RESEARCH INFRASTRUCTURE
7 About EXCELLENT SCIENCE INDUSTRIAL LEADERSHIP SOCIETAL CHALLENGES MARIE SKLODOWSKA CURIE ACTIONS (MSCA) FUTURE AND EMERGING TECHNOLOGIES EUROPEAN RESEARCH COUNCIL RESEARCH INFRASTRUCTURE Individual Fellowship Co-Funding Staff Exchange Research networks
8 About EXCELLENT SCIENCE INDUSTRIAL LEADERSHIP SOCIETAL CHALLENGES MARIE SKLODOWSKA CURIE ACTIONS (MSCA) FUTURE AND EMERGING TECHNOLOGIES EUROPEAN RESEARCH COUNCIL RESEARCH INFRASTRUCTURE Individual Fellowship Co-Funding Staff Exchange Research networks
9 About R S + Group Researcher: PhD or >4 year research experience Supervisor: Expert in the field OR a well known group
10 About Secondments: expert-based or group-based R S + Group Researcher: PhD or >4 year research experience Supervisor: Expert in the field OR a well known group
11 About Secondments: expert-based or group-based R + Dr. Manuela Temmer + Solar & Heliophysics group Institute of Physics, Uni. Graz
12 About Secondments 2: Uni. Kiel Dr. Bernd Heber & Dr. Jingnan Guo R + Dr. Manuela Temmer + Solar & Heliophysics group Institute of Physics, Uni. Graz Secondments 1: Dr. Christian Möstl Space Research Institute, Graz
13 How to R PROJECT PROPOSAL Scientific excellence: Research Researcher Supervisor Impact: Researcher Society Implementation: How will you do it? Can you do it?
14 How to
15 Tips and Tricks Constantly work to improve your CV and track record!
16 Tips and Tricks Have a good idea! Study the material well!
17 Tips and Tricks Find a good supervisor!
18 Tips and Tricks Work on your project writing skills! (Workshops, etc..) Look at winning proposals!
19 WHY? Why do it in the first place? Why Marie Curie? What is the benefit? Is it worth it?
20 My experience.. PROJECT ForbMod Forbush decrease model for expanding CMEs affecting Earth and Mars Run-Time: UNIGRAZ
21 Project ForbMod What are Forbush decreases? CR count(%) -1 TIXIE BAY APATITY INUVIK AVERAGE DAY Dumbovic PhD thesis,215 First observed by Forbush, 1937 and Hess & Demmelmair, 1937 Short term decreases in galactic cosmic ray count Typical duration several days Typical amplitudes several % (depends on the detector)
22 Project ForbMod What are Coronal Mass Ejections (CMES)? CORONAGRAPHIC OBSERVATION (direct observations): bright, white-light feature in the coronagraph field of view visible-light observations show the electron-scattered emission of photospheric light the intensity depends on the line-of-sight column density of the corona Bright feature - mass moving trough corona e.g. Hudson et al. (26)
23 Forbush decreases caused by Interplanetary Coronal Mass Ejections (ICMEs) REMOTE OBSERVATION VISUALISATION IN SITU MEASUREMENTS Adapted from Richardson & Cane, 211, SolPhys N 6 w B (nt) Bi (nt) db (nt) Bx By Bz 2 N (cm -3 ) T ( 1 5 K) v (kms -1 ) beta CR count (%) DOY 2 CME in SOHO/LASCO C3 2 September 16 6:18 UT First C2 detection at 5:18 ICME detected in situ by Wind 2 September 17 Shock arrival at 17: + 2step Forbush decrease detected by NMs at Earth adapted from Dumbovic+, 211, A&A
24 Forbush decreases caused by Interplanetary Coronal Mass Ejections (ICMEs) REMOTE OBSERVATION VISUALISATION IN SITU MEASUREMENTS w N Adapted from Richardson & Cane (211) SHOCK-effect B (nt) Bi (nt) db (nt) Bx By Bz 2 N (cm -3 ) T ( 1 5 K) CME in SOHO/LASCO C3 2 September 16 6:18 UT First C2 detection at 5:18 à magnetic connectivity à Turbulence à Compression à Prolonged effect v (kms -1 ) CR count (%) DOY 2 ICME detected in situ by Wind 2 September 17 Shock arrival at 17: + 2step Forbush decrease detected by NMs at Earth adapted from Dumbovic+(211) beta
25 Forbush decreases caused by Interplanetary Coronal Mass Ejections (ICMEs) REMOTE OBSERVATION VISUALISATION IN SITU MEASUREMENTS w N EJECTA-effect Adapted from Richardson & Cane (211) SHOCK-effect B (nt) Bi (nt) db (nt) Bx By Bz 2 à no magnetic connectivity N (cm -3 ) v (kms -1 ) T ( 1 5 K) beta CME in SOHO/LASCO C3 2 September 16 6:18 UT First C2 detection at 5:18 à Smooth & strong field à Timespan limited to ICME à magnetic connectivity à Turbulence à Compression à Prolonged effect CR count (%) DOY 2 ICME detected in situ by Wind 2 September 17 Shock arrival at 17: + 2step Forbush decrease detected by NMs at Earth adapted from Dumbovic+(211)
26 Forbush decreases caused by Interplanetary Coronal Mass Ejections (ICMEs) REMOTE OBSERVATION VISUALISATION IN SITU MEASUREMENTS ForbMod Adapted from Richardson & Cane (211) N 6 w EJECTA-effect SHOCK-effect B (nt) Bi (nt) db (nt) Bx By Bz 2 à no magnetic connectivity N (cm -3 ) v (kms -1 ) T ( 1 5 K) beta CME in SOHO/LASCO C3 2 September 16 6:18 UT First C2 detection at 5:18 à Smooth & strong field à Timespan limited to ICME à magnetic connectivity à Turbulence à Compression à Prolonged effect CR count (%) DOY 2 ICME detected in situ by Wind 2 September 17 Shock arrival at 17: + 2step Forbush decrease detected by NMs at Earth adapted from Dumbovic+(211)
27 To summarize.. Opportunity to do excellent science wherever you choose
28 Thank you for your attention! Acknowledgements: This research has received funding from the European Union s Horizon 22 research and innovation programme under the Marie Sklodowska-Curie grant agreement No
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