منابع مشابه
Hydrostatic Modeling of the Integrated Soft X-Ray and EUV Emission in Solar Active Regions
Many studies of the solar corona have shown that the observed X-ray luminosity is well correlated with the total unsigned magnetic flux. In this paper we present results from the extensive numerical modeling of active regions observed with the Solar and Heliospheric Observatory (SOHO) Extreme Ultraviolet Telescope (EIT), the Yohkoh Soft X-ray Telescope (SXT), and the SOHO Michelson Doppler Imag...
متن کاملBayesian 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 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 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 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...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1985
ISSN: 0074-1809
DOI: 10.1017/s0074180900075665