يعرض 1 - 10 نتائج من 250 نتيجة بحث عن '"Gieseler, J"', وقت الاستعلام: 1.01s تنقيح النتائج
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    دورية أكاديمية

    المساهمون: Space Physics Research Group, Department of Physics, Particle Physics and Astrophysics

    وصف الملف: application/pdf

    العلاقة: Solar Orbiter is a space mission of international collaboration between ESA and NASA, operated by ESA. The STIX instrument is an international collaboration between Switzerland, Poland, France, Czech Republic, Germany, Austria, Ireland, and Italy. We acknowledge funding by the European Union's Horizon 2020 research and innovation program under grant agreements No. 101004159 (SERPENTINE), and No. 870405 (EUHFORIA 2.0). BepiColombo is a joint ESA-JAXA science mission with instruments and contributions directly funded by ESA Member States and JAXA. Parker Solar Probe was designed, built, and is now operated by the Johns Hopkins Applied Physics Laboratory as part of NASA's Living with a Star (LWS) program (contract NNN06AA01C). Support from the LWS management and technical team has played a critical role in the success of the Parker Solar Probe mission. Work in the University of Turku was performed under the umbrella of Finnish Centre of Excellence in Research of Sustainable Space (Academy of Finland Grant No. 336809). N.D. is grateful for support by the Turku Collegium for Science, Medicine and Technology of the University of Turku, Finland. N.D. and I.C.J. are grateful for support by the Academy of Finland (SHOCKSEE, grant No. 346902). L.R.G. thanks Toni Galvin for her assistance in the use of STEREO/PLASTIC data and Leila Mays, Dusan Odstrcil, Nick Arge, and Shaela Jones-Mecholsky regarding the use of WSA-ENLIL model. The UAH team acknowledges the financial support by the Spanish Ministerio de Ciencia, Innovacion y Universidades FEDER/MCIU/AEI Projects ESP2017-88436-R and PID2019-104863RB-I00/AEI/10.13039/501100011033. I.C.J. acknowledges funding by the BRAIN-be project SWiM (Solar Wind Modelling with EUHFORIA for the new heliospheric missions). A.K. acknowledges support from NASA's NNN06AA01C (SO-SIS Phase-E) contract. V.K. acknowledges the support by NASA under grants No. 18-2HSWO218_2-0010 and 19-HSR-19_2-0143. E.P. acknowledges support from NASA's PSP-GI (grant No. 80NSSC22K0349), O2R (grant No. 80NSSC20K0285), and LWS-SC (grant No. 80NSSC22K0893) programmes. E.A. acknowledges support from the Academy of Finland (Postdoctoral Researcher Grant 322455). W.D. and Y.K. acknowledge ISSI for the possibility to discuss the questions related to particle propagation in interplanetary space during the meeting of the team No. 459 (led by G. Li and L. Wang). B.S.-C. acknowledges support through UK-STFC Ernest Rutherford Fellowship ST/V004115/1 and STFC grant ST/V000209/1. The work of F.S. was supported by DLR grant No. 50 OT 1904. N.W. acknowledges support from NASA program NNH17ZDA001N-LWS and from the Research Foundation - Flanders (FWO-Vlaanderen, fellowship No. 1184319N). C.O.L. acknowledges support from NASA's LWS Program (Grant No. 80NSSC21K1325) and the MAVEN project funded through the NASA Mars Exploration Program. C.O.L. and C.M.S.C. acknowledge support from the IMPACT Investigation by the NASA Heliophysics Division through the STEREO Project Office at NASA GSFC (Grant No. 80NSSC18K1446). M.L. acknowledges support from the Italian Space Agency and the National Institute of Astrophysics through the ASI-INAF n. 2020-35-HH.0 agreement for the development of the ASPIS prototype of scientific data centre for Space Weather. ENLIL simulation results have been provided by the CCMC at NASA Goddard Space Flight Center (GSFC) through their public Runs on Request system (http://ccmc.gsfc.nasa.govTest; run ID Laura_Rodriguez-Garcia_041322_SH_1). The WSA model was developed by N. Arge, currently at GSFC, and the ENLIL Model was developed by D. Odstrcil, currently at George Mason University.; Dresing , N , Rodríguez-García , L , Jebaraj , I C , Warmuth , A , Wallace , S , Balmaceda , L , Podladchikova , T , Strauss , R D , Kouloumvakos , A , Palmroos , C , Krupar , V , Gieseler , J , Xu , Z , Mitchell , J G , Cohen , C M S , de Nolfo , G A , Palmerio , E , Carcaboso , F , Kilpua , E K J , Trotta , D , Auster , U , Asvestari , E , Da Silva , D , Dröge , W , Getachew , T , Gómez-Herrero , R , Grande , M , Heyner , D , Holmström , M , Huovelin , J , Kartavykh , Y , Laurenza , M , Lee , C O , Mason , G , Maksimovic , M , Mieth , J , Murakami , G , Oleynik , P , Pinto , M , Pulupa , M , Richter , I , Rodriguez-Pacheco , J , Sánchez-Cano , B , Schuller , F , Ueno , H , Vainio , R , Vecchio , A , Veronig , A M & Wijsen , N 2023 , ' The 17 April 2021 widespread solar energetic particle event ' , Astronomy & Astrophysics , vol. 674 , A105 . https://doi.org/10.1051/0004-6361/202345938Test; ORCID: /0000-0002-4489-8073/work/153472475; ORCID: /0000-0002-6276-5776/work/153475398; ORCID: /0000-0002-6998-7224/work/153480415; 85163207520; 679cf48d-52bd-4000-94b3-a7484bdb5cb8; http://hdl.handle.net/10138/571303Test; 001005589600008

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    دورية أكاديمية

    المساهمون: STEMM - Stem Cells and Metabolism Research Program

    وصف الملف: application/pdf

    العلاقة: This work received funding from the European Union's Horizon 2020 research and innovation program under grant agreement No. 870405 (EUHFORIA 2.0), and No. 101004159 (SERPENTINE). I.C.J. and J.M. acknowledge funding by the BRAIN-be project SWiM (Solar Wind Modelling with EUHFORIA for the new heliospheric missions) J.M. acknowledges the funding from the FED-tWIN project PERIHELION. N.D. and I.C.J. are grateful for support by the Academy of Finland (SHOCKSEE, grant no. 346902). A.K. acknowledges financial support from NASA's NNN06AA01C (SO-SIS Phase-E) contract. Work in the University of Turku was performed under the umbrella of Finnish Centre of Excellence in Research of Sustainable Space (FORESAIL, Academy of Finland grant no. 336809). N.D. is grateful for support by the Turku Collegium for Science, Medicine and Technology of the University of Turku, Finland and support of Academy of Finland (SHOCKSEE, grant no. 346902). N.W. acknowledges support from the NASA program NNH17ZDA001N-LWS and from the Research Foundation - Flanders (FWO - Vlaanderen, fellowship no. 1184319N) T.W. acknowledges DLR grant 50 OC 2101 and DLR grant 50 OC 2301. The work of F.S. was supported by DLR grant No. 50 OT 1904. I.C.J. thanks Dr. Vladimir Krasnoselskikh for the productive discussions regarding the various aspects of collisionless shocks. Solar Orbiter is a space mission of international collaboration between ESA and NASA, operated by ESA. The STIX instrument is an international collaboration between Switzerland, Poland, France, Czech Republic, Germany, Austria, Ireland, and Italy. The authors also thank Dr. Milan Maksimovic for providing data products from the Radio Plasma Waves (RPW) instrument on board Solar Orbiter. EIT and LASCO data have been used courtesy of the SOHO/EIT and SOHO/LASCO consortiums, respectively. The STEREO SECCHI data are produced by a consortium of RAL(UK), NRL(USA), LMSAL(USA), GSFC(USA), MPS(Germany), CSL(Belgium), IOTA(France), and IAS(France). The Wind/WAVES instrument was designed and built as a joint effort of the Paris-Meudon Observatory, the University of Minnesota, and the Goddard Space Flight Center, and the data are available at the instrument Web site. The authors are grateful to Dr. Xavier Bonnin for providing direction finding data from the WAVES experiment on board Wind. We thank the radio monitoring service at LESIA (Observatoire de Paris) for providing value-added data that have been used for this study. HMI data are provided courtesy of NASA/SDO science teams.; Jebaraj , I C , Kouloumvakos , A , Dresing , N , Warmuth , A , Wijsen , N , Palmroos , C , Gieseler , J , Marmyleva , A , Vainio , R , Krupar , V , Wiegelmann , T , Magdalenic , J , Schuller , F , Battaglia , A F & Fedeli , A 2023 , ' Multiple injections of energetic electrons associated with the flare and CME event on 9 October 2021 ' , Astronomy & Astrophysics , vol. 675 , A27 . https://doi.org/10.1051/0004-6361/202245716Test; 85164538242; 74f134af-45ec-450c-b2c0-395abb47a60c; http://hdl.handle.net/10138/571166Test; 001023752300010

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