谷歌浏览器插件
订阅小程序
在清言上使用
VIPCreated with Sketch.

Study of solar brightness profiles in the 18-26 GHz frequency range with INAF radio telescopes II. Evidence of coronal emission (vol 684, A123, 2024)

M. Marongiu,A. Pellizzoni,S. Righini,S. Mulas,R. Nesti,A. Burtovoi,M. Romoli,G. Serra,G. Valente,E. Egron,G. Murtas,M. N. Iacolina, A. Melis,S. L. Guglielmino,S. Loru,P. Zucca,A. Zanichelli,M. Bachetti,A. Bemporad,F. Buffa,R. Concu,G. L. Deiana, C. Karakotia,A. Ladu,A. Maccaferri,P. Marongiu,M. Messerotti,A. Navarrini,A. Orfei,P. Ortu,M. Pili,T. Pisanu,G. Pupillo,P. Romano,A. Saba,L. Schirru,C. Tiburzi,L. Abbo,F. Frassati,M. Giarrusso,G. Jerse,F. Landini,M. Pancrazzi,G. Russano,C. Sasso,R. Susino

ASTRONOMY & ASTROPHYSICS（2024）

引用 0|浏览17
关键词
methods: data analysis,Sun: atmosphere,Sun: chromosphere,Sun: corona,Sun: photosphere,errata, addenda
AI 理解论文
溯源树
样例
生成溯源树，研究论文发展脉络
Chat Paper
正在生成论文摘要