Nội dung được dịch bởi AI, chỉ mang tính chất tham khảo
Gia tốc hạt và động học trong vụ phun trào mặt trời – Một sự tổng hợp của các quan sát và khái niệm lý thuyết gần đây (Bài tổng quan mời)
Tóm tắt
Chúng tôi xem xét các quá trình vật lý của sự gia tốc hạt, bơm hạt, sự lan truyền, giam giữ và mất năng lượng trong điều kiện vụ phun trào mặt trời. Việc hiểu các quá trình vật lý cơ bản này là điều không thể thiếu để giải thích chi tiết sự tiến triển về thời gian và quang phổ của các dấu hiệu phát xạ gây ra bởi các hạt không nhiệt trong các tia X cường độ cao, các tia gamma và băng tần vô tuyến. Ngược lại với các bài tổng quan khác có định hướng lý thuyết hơn về các quá trình gia tốc hạt, chúng tôi hướng tới việc khai thác các quan sát phong phú từ các sứ mệnh tàu vũ trụ gần đây, chẳng hạn như từ Đài quan sát Tia gamma Compton (CGRO), Kính viễn vọng Tia X cường độ cao Yohkoh (HXT) và Kính viễn vọng Tia X mềm (SXT), và Khám phá Vùng Chuyển tiếp và Vành đai (TRACE). Các đo lường độ trễ thời gian phụ thuộc vào năng lượng với độ chính xác cao từ CGRO và hình ảnh không gian từ Yohkoh và TRACE cung cấp các ràng buộc quan sát quý giá về hình thái của khu vực gia tốc, sự tái tạo các quá trình kết nối từ tính, các trường điện từ kết quả, và động học của các hạt được kích thích (không nhiệt).
Từ khóa
#gia tốc hạt #động học #vụ phun trào mặt trời #tia X #tia gamma #quan sát vũ trụ #kết nối từ tínhTài liệu tham khảo
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