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Nina Dresing Profile
Nina Dresing

@NinaDresing

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133
Following
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Statuses
31

Space physicist | Academy Research Fellow at @UniTurku, Finland

Turku, Finland
Joined March 2020
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@NinaDresing
Nina Dresing
2 months
RT @NonlinearChris: Recently, I sat down with @AASNova to discuss our recent work on detecting synchrotron radiation from interplanetary sh…
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@NinaDresing
Nina Dresing
3 months
RT @NonlinearChris: Proud to finally present this banger! We found synchrotron radiation from two extreme, near-Sun shocks! With @NASA's PS…
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@NinaDresing
Nina Dresing
11 months
RT @diana_morosan: Interested in solar activity or radio astronomy? Join our team at the Space Research Laboratory. Looking for a PhD stude…
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@NinaDresing
Nina Dresing
11 months
RT @H2020Serpentine: SERPENTINE’s @NinaDresing led a very comprehensive study of a widespread solar energetic particle event, which occurre…
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@NinaDresing
Nina Dresing
1 year
RT @diana_morosan: Looking for a postdoctoral researcher to join our team at the Space Research Laboratory @PhysUtu @UniTurku to work on so…
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@NinaDresing
Nina Dresing
1 year
RT @Rami_Vainio: Do you have new results on solar energetic particles and/or shock waves that you want to report in the #EGU24? Consider su…
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@NinaDresing
Nina Dresing
1 year
RT @dr_radiochris: We found isolated beams of electrons extending from sub-relativistic to relativistic energies roughly 13 minutes upstrea…
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@NinaDresing
Nina Dresing
1 year
RT @JanGieseler: can now obtain solar wind speeds automatically for you! 🥳 Check the newly updated documentation at…
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@NinaDresing
Nina Dresing
2 years
RT @dtrottao: Looking for a #holiday #read ? Our new paper where we look at the complex face of a #shock while it interacts with pre-exist…
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@NinaDresing
Nina Dresing
2 years
RT @H2020Serpentine: The SERPENTINE Scientific Symposium on Particle Acceleration and Transport was held in the beautiful Toulouse. ☀️☀️ We…
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@NinaDresing
Nina Dresing
2 years
Our multi-spacecraft analysis of the 17 April 2021 SEP event revealed a possible new scenario for the generation of widespread events. @SolarOrbiter @ParkerSolar @BepiColombo Check out our new paper:
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@NinaDresing
Nina Dresing
2 years
RT @H2020Serpentine: SERPENTINE has made new releases of its #DataAnalysis tools for solar eruptions missions, based on Python and Jupyter…
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@NinaDresing
Nina Dresing
2 years
We are hiring! We have a 2.5 year postdoc position in Space Physics to work with me and @Rami_Vainio @PhysUtu, @UniTurku. Come to Turku, Finland, to help us study Solar Energetic Particle events observed with the new spacecraft fleet.
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@NinaDresing
Nina Dresing
3 years
RT @H2020Serpentine: The SERPENTINE team organized a graduate level course on solar energetic particles @PhysUtu. The hybrid mode course ha…
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@NinaDresing
Nina Dresing
3 years
Thanks so much everybody! 🥳 I still can't believe it. Thanks @SuomenAkatemia for this opportunity and @TCSMT_UTU for a great platform to develop! 🚀 Looking forward to shed more light on shocks and electrons @PhysUtu @UniTurku
@Rami_Vainio
Rami Vainio
3 years
Congratulations to ⁦@NinaDresing⁩ of ⁦@PhysUtu⁩ for the Academy Research Fellow position! 🥳 Well deserved! I am so happy for you, and also thankful for the ⁦@SuomenAkatemia⁩ for supporting solar energetic particle research with the new missions!
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@NinaDresing
Nina Dresing
3 years
@halocme That's one of the questions we will tackle next within @H2020Serpentine! Where does the flare contribution stop and where starts the shock? When do they mix, how to disentangle them? Observations close to the Sun by @SolarOrbiter, @ParkerSunProbe, and @BepiColombo will be key! 🛰️
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@NinaDresing
Nina Dresing
3 years
@halocme Yes, I mean the first explanation. We also compared the electron and proton peak intensities with the shock normal angels at the magnetic footpoints of the spacecraft but did not find any differences between proton and electron correlations with the shock geometry.
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@NinaDresing
Nina Dresing
3 years
RT @H2020Serpentine: A study led by @NinaDresing of @PhysUtu finds strong evidence for acceleration of MeV-electrons in coronal shocks. The…
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