Rotational modulation and flares on RS Canum Venaticorum and BY Draconis-type stars. XV - Observations of Proxima Centauri and solar calibration data

التفاصيل البيبلوغرافية
العنوان: Rotational modulation and flares on RS Canum Venaticorum and BY Draconis-type stars. XV - Observations of Proxima Centauri and solar calibration data
المؤلفون: Haisch, B. M, Butler, C. J, Foing, B, Rodono, M, Giampapa, M. S
المصدر: Astronomy and Astrophysics. 232(2 Ju)
بيانات النشر: United States: NASA Center for Aerospace Information (CASI), 1990.
سنة النشر: 1990
مصطلحات موضوعية: Astrophysics
الوصف: Results are reported from simultaneous Exosat and IUE observations of flaring in Proxima Cen on March 2, 1985. The data are presented in extensive tables and sample spectra and discussed in detail. The peak emission of the soft-X-ray flare is found to be about 3 x 10 to the 27th erg/sec, with energy about 3 x 10 to the 30th erg and an associated increase in Mg II flux to 17,000-67,000 erg/sq cm sec, or about an order of magnitude lower than the solar value. The presence of flare- and microflare-related processes heating the corona is inferred.
نوع الوثيقة: Report
اللغة: English
تدمد: 0004-6361
URL الوصول: https://ntrs.nasa.gov/citations/19900064823
ملاحظات: NAS5-28720

NASA ORDER H-85057-B
رقم الأكسشن: edsnas.19900064823
قاعدة البيانات: NASA Technical Reports