EMISSION MEASURE DISTRIBUTION FOR DIFFUSE REGIONS IN SOLAR ACTIVE REGIONS
نویسندگان
چکیده
منابع مشابه
Bayesian Inference for Identifying Solar Active Regions
The solar chromosphere consists of three classes plage, network, background which contribute differently to ultraviolet radiation reachina thn am-th ~.nl~r nhv&-iota cama intmwatd in --a “Y” U-V.&. Y”*yYJ”.“‘uY” .“A.8 .Y”YIVY”VU IY relating plage area and intensity to UV irradiante, as well as understanding the spatial and temporal evolution of plage shapes. We describe a data set of solar imag...
متن کاملThe Magnetic Classification of Solar Active Regions
The purpose of this letter is to address a blind-spot in our knowledge of solar active region statistics. To the best of our knowledge there are no published results showing the variation of the Mount Wilson magnetic classifications as a function of solar cycle based on modern observations. We show statistics for all active regions reported in the daily Solar Region Summary from 1992 January 1 ...
متن کاملSolar Irradiance Modulation by Active Regions From
Recent satellite measurements of the solar total irradiance (S) indicate that on time scales of days to months the solar constant varies by a few tenths of a percent. The predominant part of these variations can be explained by blocking of the upward solar flux by sunspots. The observations are consistent with current theoretical models of energy storage in which the energy blocked by the sunsp...
متن کاملThe Transparency of Solar Coronal Active Regions
Resonance scattering has often been invoked to explain the disagreement between the observed and predicted line ratios of Fe XVII λ15.01 to Fe XVII λ15.26 (the “3C/3D” ratio). In this process photons of λ15.01, with its much higher oscillator strength, are preferentially scattered out of the line of sight, thus reducing the observed line ratio. Recent laboratory measurements, however, have foun...
متن کاملStatistical Models for Solar Flare Interval Distribution in Individual Active Regions
This article discusses statistical models for solar flare interval distribution in individual active regions. We analyzed solar flare data in 55 active regions that are listed in the Geosynchronous Operational Environmental Satellite (GOES) soft X-ray flare catalog for the years from 1981 to 2005. We discuss some problems with a conventional procedure to derive probability density functions fro...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2014
ISSN: 1538-4357
DOI: 10.1088/0004-637x/795/1/76