يعرض 1 - 10 نتائج من 236 نتيجة بحث عن '"SHOCK ACCELERATION"', وقت الاستعلام: 1.49s تنقيح النتائج
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    المساهمون: Department of Physics, Space Physics Research Group, Doctoral Programme in Particle Physics and Universe Sciences, Particle Physics and Astrophysics

    وصف الملف: application/pdf

    العلاقة: The results presented here have been achieved under the framework of the Finnish Centre of Excellence in Research of Sustainable Space (FORESAIL; Academy of Finland grant numbers 312390 and 336809), which we gratefully acknowledge. EK acknowledges the ERC under the European Union's Horizon 2020 Research and Innovation Programme Project 724391 (SolMAG), and EK and SG acknowledge Academy of Finland Project 310445 (SMASH). This study has also been partially funded through the European Union's Horizon 2020 research and innovation programme under grant agreement No 101004159 (SERPENTINE). We thank the Solar Orbiter EPD team at the University of Kiel, Germany for the development of the EPD data processing and analysis pipeline. RGH and JRP acknowledge financial support from the Spanish MICIU under project PID2019-104863RB-I00/AEI/10.13039/501100011033. EA would like to acknowledge the financial support by the Academy of Finland (Postdoctoral Grant No 322455). EED was supported by funding from the Science and Technology Facilities Council (STFC) studentship ST/N504336/1. DH was supported by the German Ministerium fur Wirtschaft und Energie and the German Zentrum fur Luft- und Raumfahrt under contract 50 QW1501.; Kilpua , E K J , Good , S W , Dresing , N , Vainio , R , Davies , E E , Forsyth , R J , Gieseler , J , Lavraud , B , Asvestari , E , Morosan , D E , Pomoell , J , Price , D J , Heyner , D , Horbury , T S , Angelini , C , O'Brien , H , Evans , B , Rodriguez-Pacheco , J , Herrero , R G , Ho , G C & Kiel , U 2021 , ' Multi-spacecraft observations of the structure of the sheath of an interplanetary coronal mass ejection and related energetic ion enhancement ' , Astronomy & Astrophysics , vol. 656 , 8 . https://doi.org/10.1051/0004-6361/202140838Test; ORCID: /0000-0003-1175-7124/work/106338085; ORCID: /0000-0002-4489-8073/work/106341641; ORCID: /0000-0002-8065-2847/work/106341721; ORCID: /0000-0002-6998-7224/work/106341741; ORCID: /0000-0002-8416-1375/work/106342030; ORCID: /0000-0002-4921-4208/work/106342072; 28067319-7ad2-4ea0-a337-015a194fbfb3; http://hdl.handle.net/10138/341025Test; 000730246400033

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    المساهمون: Department of Physics, Space Physics Research Group

    وصف الملف: application/pdf

    العلاقة: We acknowledge the use of ACE data from the ACE Science Center and of SOHO/ERNE data from sepem.eu and of the SEPEM Reference Data Set version 2.00, European Space Agency (2016). N.W. acknowledges funding from the Research Foundation -Flanders (FWO -Vlaanderen, fellowship no. 1184319N). A.A. and B.S. acknowledge the support by the Spanish Ministerio de Ciencia e Innovacion (MICINN) under grant PID2019-105510GB-C31 and through the "Centre of Excellence Maria de Maeztu 2020-2023" award to the ICCUB (CEX2019-000918-M). C.S. acknowledges the NASA Living With a Star Jack Eddy Postdoctoral Fellowship Program, administered by UCAR's Cooperative Programs for the Advancement of Earth System Science (CPAESS) under award no. NNX16AK22G. D.L. acknowledges support from NASA Living With a Star (LWS) programs NNH17ZDA001N-LWS and NNH19ZDA001NLWS, and the Goddard Space Flight Center Heliophysics Innovation Fund (HIF) program. The work in the University of Turku was performed under the umbrella of Finnish Centre of Excellence in Research of Sustainable Space. This project has received funding from the European Union's Horizon 2020 research and innovation programs under grant agreement No. 870405 (EUHFORIA 2.0). These results were also obtained in the framework of the ESA project "Heliospheric modelling techniques" (Contract No. 4000133080/20/NL/CRS). Computational resources and services used in this work were provided by the VSC (Flemish Supercomputer Centre), funded by the FWO and the Flemish Government-Department EWI.; Wijsen , N , Aran , A , Scolini , C , Lario , D , Afanasiev , A , Vainio , R , Sanahuja , B , Pomoell , J & Poedts , S 2022 , ' Observation-based modelling of the energetic storm particle event of 14 July 2012 ' , Astronomy & Astrophysics , vol. 659 , 187 . https://doi.org/10.1051/0004-6361/202142698Test; ORCID: /0000-0003-1175-7124/work/111518680; f2b0e2b9-0e57-4c86-87f2-0843849c69ba; http://hdl.handle.net/10138/344390Test; 000773023600005

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    المؤلفون: Cao,Zhen, Aharonian,F., An,Q., Axikegu, Bai,Y. X., Bao,Y. W., Bastieri,D., Bi,X. J., Bi,Y. J., Cai,J. T., Cao,Q., Cao,W. Y., Cao,Zhe, Chang,J., Chang,J. F., Chen,A. M., Chen,E. S., Chen,Liang, Chen,Lin, Chen,Long, Chen,M. J., Chen,M. L., Chen,Q. H., Chen,S. H., Chen,S. Z., Chen,T. L., Chen,Y., Cheng,N., Cheng,Y. D., Cui,M. Y., Cui,S. W., Cui,X. H., Cui,Y. D., Dai,B. Z., Dai,H. L., Dai,Z. G., Danzengluobu, della Volpe,D., Dong,X. Q., Duan,K. K., Fan,J. H., Fan,Y. Z., Fang,J., Fang,K., Feng,C. F., Feng,L., Feng,S. H., Feng,X. T., Feng,Y. L., Gabici,S., Gao,B., Gao,C. D., Gao,L. Q., Gao,Q., Gao,W., Gao,W. K., Ge,M. M., Geng,L. S., Giacinti,G., Gong,G. H., Gou,Q. B., Gu,M. H., Guo,F. L., Guo,X. L., Guo,Y. Q., Guo,Y. Y., Han,Y. A., He,H. H., He,H. N., He,J. Y., He,X. B., He,Y., Heller,M., Hor,Y. K., Hou,B. W., Hou,C., Hou,X., Hu,H. B., Hu,Q., Hu,S. C., Huang,D. H., Huang,T. Q., Huang,W. J., Huang,X. T., Huang,X. Y., Huang,Y., Huang,Z. C., Ji,X. L., Jia,H. Y., Jia,K., Jiang,K., Jiang,X. W., Jiang,Z. J., Jin,M., Kang,M. M., Ke,T., Kuleshov,D., Kurinov,K., Li,B. B., Li,Cheng, Li,Cong, Li,D., Li,F., Li,H. B., Li,H. C., Li,H. Y., Li,J., Li,Jian, Li,Jie, Li,K., Li,W. L., Li,X. R., Li,Xin, Li,Y. Z., Li,Zhe, Li,Zhuo, Liang,E. W., Liang,Y. F., Lin,S. J., Liu,B., Liu,C., Liu,D., Liu,H., Liu,H. D., Liu,J., Liu,J. L., Liu,J. Y., Liu,M. Y., Liu,R. Y., Liu,S. M., Liu,W., Liu,Y., Liu,Y. N., Lu,R., Luo,Q., Lv,H. K., Ma,B. Q., Ma,L. L., Ma,X. H., Mao,J. R., Min,Z., Mitthumsiri,W., Mu,H. J., Nan,Y. C., Neronov,A., Ou,Z. W., Pang,B. Y., Pattarakijwanich,P., Pei,Z. Y., Qi,M. Y., Qi,Y. Q., Qiao,B. Q., Qin,J. J., Ruffolo,D., Sáiz,A., Semikoz,D., Shao,C. Y., Shao,L., Shchegolev,O., Sheng,X. D., Shu,F. W., Song,H. C., Stenkin,Yu. V., Stepanov,V., Su,Y., Sun,Q. N., Sun,X. N., Sun,Z. B., Tam,P. H. T., Tang,Q. W., Tang,Z. B., Tian,W. W., Wang,C., Wang,C. B., Wang,G. W., Wang,H. G., Wang,H. H., Wang,J. C., Wang,K., Wang,L. P., Wang,L. Y., Wang,P. H., Wang,R., Wang,W., Wang,X. G., Wang,X. Y., Wang,Y., Wang,Y. D., Wang,Y. J., Wang,Z. H., Wang,Z. X., Wang,Zhen, Wang,Zheng, Wei,D. M., Wei,J. J., Wei,Y. J., Wen,T., Wu,C. Y., Wu,H. R., Wu,S., Wu,X. F., Wu,Y. S., Xi,S. Q., Xia,J., Xia,J. J., Xiang,G. M., Xiao,D. X., Xiao,G., Xin,G. G., Xin,Y. L., Xing,Y., Xiong,Z., Xu,D. L., Xu,R. F., Xu,R. X., Xu,W. L., Xue,L., Yan,D. H., Yan,J. Z., Yan,T., Yang,C. W., Yang,F., Yang,F. F., Yang,H. W., Yang,J. Y., Yang,L. L., Yang,M. J., Yang,R. Z., Yang,S. B., Yao,Y. H., Yao,Z. G., Ye,Y. M., Yin,L. Q., Yin,N., You,X. H., You,Z. Y., Yu,Y. H., Yuan,Q., Yue,H., Zeng,H. D., Zeng,T. X., Zeng,W., Zha,M., Zhang,B. B., Zhang,F., Zhang,H. M., Zhang,H. Y., Zhang,J. L., Zhang,L. X., Zhang,Li, Zhang,P. F., Zhang,P. P., Zhang,R., Zhang,S. B., Zhang,S. R., Zhang,S. S., Zhang,X., Zhang,X. P., Zhang,Y. F., Zhang,Yi, Zhang,Yong, Zhao,B., Zhao,J., Zhao,L., Zhao,L. Z., Zhao,S. P., Zheng,F., Zhou,B., Zhou,H., Zhou,J. N., Zhou,M., Zhou,P., Zhou,R., Zhou,X. X., Zhu,C. G., Zhu,F. R., Zhu,H., Zhu,K. J., Zuo,X.