Academic Journal

PRIME — A Passive Radar Sounding Concept for Io

التفاصيل البيبلوغرافية
العنوان: PRIME — A Passive Radar Sounding Concept for Io
المؤلفون: Steinbrüegge, Gregor, Romero-Wolf, A., Peters, S., Schroeder, D. M., Carrer, L., Hamilton, C. W., Carter, L., Bierson, C. J., Blankenship, D. D., Chan, K., Fanara, L., Grima, C., Hay, H., Hussmann, H., Keane, J. T., Maurice, M., Nikolaou, A., Rosas-Ortiz, Y., Scanlan, K. M., Soderlund, K. M., Stark, A., Varatharajan, I., Voigt, J. R. C., Young, D. A.
المساهمون: Steinbrüegge, Gregor, Romero-Wolf, A., Peters, S., Schroeder, D. M., Carrer, L., Hamilton, C. W., Carter, L., Bierson, C. J., Blankenship, D. D., Chan, K., Fanara, L., Grima, C., Hay, H., Hussmann, H., Keane, J. T., Maurice, M., Nikolaou, A., Rosas-Ortiz, Y., Scanlan, K. M., Soderlund, K. M., Stark, A., Varatharajan, I., Voigt, J. R. C., Young, D. A.
بيانات النشر: USA
سنة النشر: 2021
المجموعة: Università degli Studi di Trento: CINECA IRIS
الوصف: In this white paper, we argue for a Passive Radar Io Magma Explorer (PRIME) to study Jupiter’s moon Io as one of the priority targets of the in the next decade1,2. Jupiter is the second strongest source of radio noise within our Solar System, after the Sun itself. As passive radar sounding has the potential to operate with low power consumption and robust hardware, which is crucial in an environment like Jupiter, PRIME can also address major outstanding scientific questions regarding the crustal structure of Io.
نوع الوثيقة: article in journal/newspaper
اللغة: English
Relation: volume:53; issue:4; firstpage:1; lastpage:8; numberofpages:8; journal:BULLETIN OF THE AMERICAN ASTRONOMICAL SOCIETY; http://hdl.handle.net/11572/315738; https://baas.aas.org/pub/2021n4i271/release/1
DOI: 10.3847/25c2cfeb.49659984
الاتاحة: http://hdl.handle.net/11572/315738
https://doi.org/10.3847/25c2cfeb.49659984
https://baas.aas.org/pub/2021n4i271/release/1
Rights: info:eu-repo/semantics/openAccess
رقم الانضمام: edsbas.BDBC5247
قاعدة البيانات: BASE
الوصف
DOI:10.3847/25c2cfeb.49659984