搜索结果: 1-5 共查到“理学 chromosphere”相关记录5条 . 查询时间(0.086 秒)
Simultaneous Observations of the Chromosphere with TRACE and SUMER
Simultaneous Observations Chromosphere TRACE SUMER
font style='font-size:12px;'>
2011/1/10
Using mainly the 1600 angstrom continuum channel, and also the 1216 angstrom Lyman-alpha channel (which includes some UV continuum and C IV emission), aboard the TRACE satellite, we observed the compl...
Wave Heating of the Solar Chromosphere
Sun chromosphere oscillations heating and dynamics acoustic waves magnetic waves
font style='font-size:12px;'>
2010/9/15
The nonmagnetic interior of supergranulation cells has been thought since the 1940s to be heated by the dissipation of acoustic waves.But all attempts to measure the acoustic flux have failed to show ...
Wave Heating of the Solar Chromosphere
Sun: chromosphere, oscillations heating and dynamics acoustic waves magnetic waves
font style='font-size:12px;'>
2009/5/6
The nonmagnetic interior of supergranulation cells has been
thought since the 1940s to be heated by the dissipation of acoustic waves.
But all attempts to measure the acoustic flux have failed to sh...
MUTUAL RELATIONSHIP OF OSCILLATIONS IN THE FREQUENCY RANGE 3.6 mHz TO 22 mHz IN THE SOLAR CHROMOSPHERE
Sun chromosphere-Sun oscillations
font style='font-size:12px;'>
2009/2/20
High frequency acoustic oscillations were suggested as the source
of mechanical heating in the chromosphere. In this work the radial component of
the oscillations in the frequency interval 3 mHz to ...
Exploration of Solar Chromosphere Using High Resolution Spectroscopic Observations
Solar Chromosphere High Resolution Spectroscopic Observations
font style='font-size:12px;'>
2010/10/26
Brazilian Solar Spectroscope (BSS), operating in the frequency range of (1000 ¡ 2500) MHz with high time and frequency resolutions, has observed various fine structures showing intensity variati...